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March 28
Melting point of graphite: Lower in Japan?
This article says that graphite plugs in the Kukushima Daichi reactors "start to melt" at 350 C. That seems implausible, since graphite is used in various applications in a solid state at much higher temperatures, as in arc lights. Could graphite really melt at 350 Celsius? The Graphite article does not appear to state a melting temperature. Edison (talk) 00:05, 28 March 2011 (UTC)
- That article actually says 350°F, which is even lower (177°C). That does seem to be a mistake. According to this article: [1], graphite melts (technically it sublimes, or turns to vapor) at around 3652-3697°C. This assumes normal atmospheric pressure though, could that be the difference ? StuRat (talk) 00:29, 28 March 2011 (UTC)
- My guess is the "graphite plugs" are not made of pure graphite, but have something else in them which is what does the melting. Our carbon article says that carbon in normal atmospheric pressures doesn't even HAVE a melting point as it sublimates at about 3900 K. Even given that, 177 deg C still sounds wrong. Vespine (talk) 00:36, 28 March 2011 (UTC)
- Another thought, could the plugs come loose, due to contraction and/or expansion ? They wouldn't need gravity to pull them out, if water can then get underneath them and turn to steam. This certainly isn't "melting", but some reporter could possible get confused and call it that. StuRat (talk) 01:24, 28 March 2011 (UTC)
Yep. my book (columbia enc.) gives carbon (12 that is)melt.pt 3550 C. gas off 4827 C. definitely sounds like journalistic error or typo.Phalcor (talk) 04:01, 28 March 2011 (UTC)
- Carbon-graphite impregnated epoxy resin sealing rings are widely used in industry and the epoxy breaks down around 350 deg... and a few degrees less if it is wet heat. They don't melt, they become soft and crumbly and start to smell very unpleasant. Fairwinds (oh the irony) have posted a diagram of the projected radioactive leak path.--Aspro (talk) 10:11, 28 March 2011 (UTC)
- Is that 350° F or 350° C ? In either case, it seems rather reckless to use a material so poorly suited to withstand the maximum temperature. StuRat (talk) 20:57, 28 March 2011 (UTC)
- 350F. In a boiling-water reactor, it is theoretically impossible for the temperature to get above 212F, so a hundred-degree safety margin would be plenty. Unfortunately, theory and practice are busy disagreeing right now... --Carnildo (talk) 22:49, 29 March 2011 (UTC)
- Only at atmospheric pressure. At around 3.5 atmospheres, the boiling temp goes up to 350° F (do reactors explode before they reach that pressure ?). Not allowing for the possibility of water leaking out and/or becoming pressurized in the reactor core seems rather negligent. Their "theory" appears to be that nothing will ever go wrong. StuRat (talk) 23:03, 29 March 2011 (UTC)
car (celebrities registration of)
can i register a car under a fake name like celebrities do? — Preceding unsigned comment added by Wdk789 (talk • contribs) 05:43, 28 March 2011 (UTC)
- What country are you in? Anyway, do celebrities do this, or register the car under their agent's name? I've made the title more descriptive. CS Miller (talk) 06:11, 28 March 2011 (UTC)
us — Preceding unsigned comment added by Wdk789 (talk • contribs) 07:15, 28 March 2011 (UTC)
If you're in the U.S. no. you need identification proof/documentation.190.148.135.138 (talk) 07:25, 28 March 2011 (UTC) reformatted last response. Richard Avery (talk) 08:01, 28 March 2011 (UTC)
- As of a decade ago (last time I had to care), it was possible in California for someone other than the legal owner of a car to submit the registration paperwork provided that the legal owner signed the forms and all other necessary documentation was provided. You have to show up in person to get a driver's license, but someone else could submit registration paperwork. Not sure if that is still the case, or whether different rules apply in different states. Dragons flight (talk) 08:51, 28 March 2011 (UTC)
- In the UK a vehicle is registered at the DVLA in the name of its "Registered Keeper", who need not be the owner, but is responsible for paying the Vehicle Excise Duty on it, ensuring it's ensured, etc. AndrewWTaylor (talk) 19:45, 28 March 2011 (UTC)
- Do you really need the driver's license? What if you don't drive your own car yourself? Can a car be registered at the name of company? 212.169.184.189 (talk) 02:18, 29 March 2011 (UTC)
Pressurized storage of liquids
Suppose we have a 1 litre container of water (or any other drinkable liquid). Is it theoretically possible to pressurize the container to, say, 300 ml capacity so that this smaller container would still be able to contain 1 litre of water (something like black hole)? Specifically, is there any material capable to withstand the associated water pressure while being flexible enough to allow the needed external pressure?--89.76.224.253 (talk) 10:05, 28 March 2011 (UTC)
- It's doubtful. You would need a pressure of at least 7.333×10^9 Pa (Hope I did the math right.) Which is a pretty immense pressure. But since the bulk modulus of water is non-linear with pressure, the real pressure is probably much much higher. I can't find info on how non-linear. Ariel. (talk) 10:57, 28 March 2011 (UTC)
- I remember seeing an old film clip about what must have been the Bathysphere or Benthoscope returning from the deeps after a test run. When its hatch bolts were gingerly loosened, a huge quanity of water gushed out under pressure, seemingly several times the volume of the sphere. So, yes. In fact anyone could do this - throw a 1l weighted plastic bottle of water into the deep ocean, and when it eventually reaches the bottom it should be considerably crushed. 92.15.14.99 (talk) 11:56, 28 March 2011 (UTC)
- Nah, that's incorrect. Even at the bottom of the ocean water density increases by just a few percent. Dauto (talk) 14:46, 28 March 2011 (UTC)
- Got any evidence for that please? 92.15.14.99 (talk) 15:10, 28 March 2011 (UTC)
- I saw what I saw. The Challenger Deep is about 11km deep. 92.15.14.4 (talk) 20:24, 28 March 2011 (UTC)
- You saw what you saw and you don't know what you saw. At that depth the density will still be only a few percent higher. Dauto (talk) 20:44, 28 March 2011 (UTC)
- Probably an optical illusion. A thin curtain of water mixed with air to form bubbles might look like a lot more than it really is. StuRat (talk) 20:54, 28 March 2011 (UTC)
- On reflection it may have been the air inside that became very compressed and forced the water out, and the sphere wall could have been thinner than I expected. 92.29.126.172 (talk) 13:41, 29 March 2011 (UTC)
- Now you're making sense. Dauto (talk) 13:56, 30 March 2011 (UTC)
- On reflection it may have been the air inside that became very compressed and forced the water out, and the sphere wall could have been thinner than I expected. 92.29.126.172 (talk) 13:41, 29 March 2011 (UTC)
Methanopropylenes
Hi. I recently had a dream about "methanopropylene" (I know, I'm so weird). The name could refer to either a propylene plastic impermeable to polar methano-molecules such as methanol in gaseous or liquid form and to chemicals produced by methanogens, or polymers derived from methanols. The only Google item I could find relavent to my topic, in fact the only website in existance remotely related was this, but any idea what type of chemical methanopropylenes would constitute and what potential they have? Thanks. ~AH1(TCU) 11:46, 28 March 2011 (UTC)
- School time lays long in the past and probably they also changed the way to name things, but when I hear of methanopropylene I think of H2C=C(CH3)-CH3, that is propylene where the middle H is substituted by CH3. I know the CH3 would be in the middle for otherwise the longest unforked C-chain would consist of 4 C-atoms and the basic name would be derived from butan and it would be butylene. 77.3.138.240 (talk) 13:17, 28 March 2011 (UTC)
- That would be methylpropylene (IUPAC name methylpropene); the methano- prefix isn't very common, but it does show up in the names of some amino acids, like 2,4-methanoproline and 2,4-methanoglutamic acid, see [2]. In these cases, methano- refers to a bicyclo system with a cyclopropane ring as part of it; "methano-" means you have bonded one carbon to two neighboring carbons in the main, named chain or molecule. Under that derivation, methanopropylene would likely be an alternate name for Methylcyclopropane. --Jayron32 14:19, 28 March 2011 (UTC)
- So that methano-ethane would be equivalent to cyclopropane? 77.3.138.240 (talk) 14:42, 28 March 2011 (UTC)
- Actually, probably methanoethylene, as the compound would be formed from ethylene (IUPAC name ethene) rather than ethane, which is pretty much unreactive. As I said above, the methano- prefix is non standard, and you wouldn't find the term in any IUPAC-standard name, AFAIK. --Jayron32 00:07, 29 March 2011 (UTC)
time 2
in my March 26 question about "time", most of the answers talk about watching a distant clock move (pass time) at some multiple of my clock. Wouldn't that mean that as I approach the clock the light is getting to me faster than c? —Preceding unsigned comment added by 165.212.189.187 (talk) 13:45, 28 March 2011 (UTC)
- The light is not approaching you (i.e. as measured in your frame) faster than c. However, if there is another observer who sees you moving toward the light source, then because in his frame the speed of light is also c (no contradiction here because time is not absolute), he would see that the distance between where in his frame the light front is, and where you are, is shriking faster than c, however this is not a relative speed, so there is no contradiction with relativity here.
- I think it would be a good exercise for you to work out this in detail and derive the Lorentz transform equations, it is quite easy to do. Count Iblis (talk) 14:17, 28 March 2011 (UTC)
So what explains me observing the minute hand of the distant clock move faster than mine, does mine slow down? —Preceding unsigned comment added by 165.212.189.187 (talk) 15:13, 28 March 2011 (UTC)
- Dominant effect: As you are approaching the clock, the time needed for the light to travel from the clock to your eyes is becoming less. So, the time delay diminshes as a function of time, making the clock look like moving faster. This is just the classical doppler effect. There is then a small relativistic correction to this because of time dilation. Count Iblis (talk) 16:21, 28 March 2011 (UTC)
Cow dung to absorb gamma rays
A leading newspaper from India, quoting a physics professor, says that "Cow dung, in fact, can absorb all the three rays -- alpha, beta and gamma... If the outer walls of houses are coated with thick layers of cow dung, it will absorb the gamma rays and in turn people would be safe". Does anyone know how thick should be be this cow dung coating to make people inside the house safe(in the context of a radiation accident). 14.139.128.14 (talk) 13:46, 28 March 2011 (UTC)
- Dung consists mostly of water and carbon of some form. I estimate that about 10cm would be sufficient to protect from neutron radiation (as long as you can keep the dung from drying). As for alpha and beta radiation, I cannot imagine any building wall, be it concrete, wood, glass or plastic that can be thin enough to not also protect from this kind of radiation. The best protection from gamma rays is dense matter with heavy nuclei. I doubt heavily that dung can protect from it, unless several meters thick. Any shielding whatsoever could not protect from radioactive materials coming in with air, food and water. To put it short: I think that's plain nonsense. If you would use pig dung instead, you could at least assure that no one gets hurt by radiation inside the building because everyone would have left due to the smell. 77.3.138.240 (talk) 14:27, 28 March 2011 (UTC)
- Concur with the above, cow dung would not offer more protection then soil of the same thickness against gamma radiation. I smell BS. Googlemeister (talk) 16:20, 28 March 2011 (UTC)
- Very, very literally BS. SDY (talk) 19:12, 28 March 2011 (UTC)
- Also bogus/nonsense claims? DMacks (talk) 16:25, 28 March 2011 (UTC)
- Concur with the above, cow dung would not offer more protection then soil of the same thickness against gamma radiation. I smell BS. Googlemeister (talk) 16:20, 28 March 2011 (UTC)
- The article is nonsense. And on top of that direct radiation is not something anyone needs to worry about unless they are building (or working in) a reactor. Even if cow dung was a miracle shield, and blocked radiation 100% it would be worthless. The problem is ingesting radioactive elements - the resulting radiation is internal, not external. Ariel. (talk) 21:47, 28 March 2011 (UTC)
Psychology of spending
I wonder if there's a name for the thing I'm thinking about. I see a small one-serving pack of M&M's on the shelf at the store selling for $1.35 and could easily imagine people having no problem with that and buying it. But if I imagine myself trying to sell that pack for that much as an individual or even buying the same from another individual, that price feels too high. But it's the same exact product. It's not that it's used- I get that there's probably an association between individuals and used objects, but I still get this feeling if it's still sealed. Is there a name for the feeling that if it's a real business doing the selling, the higher prices than what I'd ever pay an individual are OK? 20.137.18.50 (talk) 14:29, 28 March 2011 (UTC)
- In the same vein, some people (i.e. me) prefer buying electronics or appliances at a large retail supplier to buying them at a small independent one (unless the price premium is TOO great), despite the fact that the products are identical and would be under the same warranty from the same manufacturer. It's the same for brick-and-mortar vs online stores. I'd be interested to read the replies. Zunaid 15:13, 28 March 2011 (UTC)
- If what you describe amounts to "I'd pay $1.35 for these M&M's from a reliable retailer like MegaLoMart, but if I were buying them off a dodgy geezer like 20.137.18.50 I'd expect they're either rubbish or hooky, so I'd want a major discount" then that would be Halo effect. Similarly one can buy stuff from Fortnum and Mason that's much the same as you'd get from Tesco, but at a significantly higher price, which I think is called "brand premium". -- Finlay McWalter ☻ Talk 15:14, 28 March 2011 (UTC)
- Expanding on that, I'd also point to information asymmetry, The Market for Lemons, and the notion of "the bad driving out the good" in a market. If a random stranger offers to sell me candy, I don't know anything about him, his storage practices, his inventory turnover, or his approach to hygiene. He may or may not have an incentive to keep me happy as a customer; is he interested in repeat business, and is there any way for me to assess that? Because I don't have access to all that information – whereas I can make (better) guesses about it for a regular retailer – I am apt to discount the perceived value of the candy. TenOfAllTrades(talk) 16:43, 28 March 2011 (UTC)
- The stuff you can buy in Harrods is the same as what you can buy elsewhere at cheaper prices. Same with many other shops. 92.15.14.4 (talk) 20:10, 28 March 2011 (UTC)
Physics of insect wings
Can someone can translate the equations from here to math equations (you know, <math>) on Wikipedia so I can include them in the article, Wing (insect)? Bugboy52.4 ¦ =-= 17:04, 28 March 2011 (UTC)
- and are what the first two say, but surely it doesn't mean that? I think Δt is intended in the second one.
(I'm also not sure how to do bigger brackets than one line's worth.)Changed. Grandiose (me, talk, contribs) 17:16, 28 March 2011 (UTC)- You're right. The units are inconsistent. The equation should read . Dauto (talk) 17:38, 28 March 2011 (UTC)
- Thank you! And one more thing, if you can, there are a few mentioned after about elasticity, can you do those two? Bugboy52.4 ¦ =-= 17:41, 28 March 2011 (UTC)
- Which page? Looks like it might be on 78 or 79, which aren't available on that preview (for me, at least). [The first two equations are straightforward rearrangements of each other; might not both be useful depending on context.]Grandiose (me, talk, contribs) 17:53, 28 March 2011 (UTC)
- Thank you! And one more thing, if you can, there are a few mentioned after about elasticity, can you do those two? Bugboy52.4 ¦ =-= 17:41, 28 March 2011 (UTC)
- You're right. The units are inconsistent. The equation should read . Dauto (talk) 17:38, 28 March 2011 (UTC)
79 I believe. Bugboy52.4 ¦ =-= 18:05, 28 March 2011 (UTC)
- I wasn't able to access page 79 in that edition using Google Books (too many people tried, perhaps?), but I was able to access the second edition of that book on Amazon, and searching for "elasticity" led to this equation (eq. 6.11, in section 6.5 "Elasticity of Wings") for the energy E stored in the stretched resilin:
- Is that what you needed? -- Scray (talk) 00:15, 29 March 2011 (UTC)
- Wonderful, what pages can you get with Amazon, I'm going to look more to find those pages. Bugboy52.4 ¦ =-= 01:36, 29 March 2011 (UTC)
- Just search for the book, then "Look inside", and search for a term. You can choose the hit you want to view and you'll see a couple of adjacent pages. No doubt they'll be on to you if you access too many... -- Scray (talk) 01:59, 29 March 2011 (UTC)
- Wonderful, what pages can you get with Amazon, I'm going to look more to find those pages. Bugboy52.4 ¦ =-= 01:36, 29 March 2011 (UTC)
Headlights of a spaceship if turned on relative to two different observers
Lat a spaceship with its remote controlled headlights is moving with 0.9c relative to observer on asteroid who is not co-moving.
1- Onboard observer turned on the headlights of his spaceship with the help of a remote control device by sending a signal (pulse) from the back of ship to it's front
2- While due to the high speed of ship a signal (pulse) will still be moving inside the ship relative to asteroid observer.
Thus would the headlights be turned on at the same time for both onboard and asteroid observers if the perception distances are ignorable
Perception distances: The distance travelled by headlight
b/w headlights and onboard observers AND b/w headlights and asteroid observer 68.147.41.231 (talk) 17:52, 28 March 2011 (UTC)Eccentric Khattak#1-420------[GO]
- See relativity of simultaneity for a discussion about this kind of thing. --Tango (talk) 22:17, 28 March 2011 (UTC)
I asked above in regard to sub section " The train and the platform thought eperiment" of the article. I got unsatisfactory answers from forums therefore still its difficult for me to the fathom.
The same senario but the other way
Let aforementioned remotely control spaceship is moving with 0.9c relative to stationary observer on asteroid. Onboard observer sends a stoping signal (pulse) from the back of ship to it's front with the help of a remote control device.
1- For onboard observer: A pulse would hit the front and thus stopped the ship earlier than asteroid's observer
2- While due to the high speed of ship a pulse will still be moving inside the ship relative to asteroid observer
Since a pulse would arrived the front at two different timing relative to aforementioned observers therefore would the ship be stopped at the same time at the front of asteroid for both observers.
The purpose of this post is to share knowledge and shouldn’t be considered offensive.68.147.41.231 (talk) 00:15, 31 March 2011 (UTC)Eccentric Khattak#1-420
Vanadium oxidation
Does it make the pentoxide or vanadium(IV) oxide? --98.221.179.18 (talk) 18:35, 28 March 2011 (UTC)
- Vanadium oxide indicates both the (4+) and (5+) oxides, along with several others, as well as the possibility of non-stoichiometric oxides, indicating multiple oxidation states within a single crystal lattice. --Jayron32 00:03, 29 March 2011 (UTC)
Game theory: paying ransom
Imagine that something worth $1000 has been stolen. The thief demands $900 from you. You thing: OK, I pay, it's still $100 on my favor. After you pay, the thief demands $900 again. Do you pay again? It's still $100 cheaper than buying anew. (the first $900 are now sunk costs). Quest09 (talk) 18:45, 28 March 2011 (UTC)
- If your country takes your taxes but still refuses to protect your property rights then you should consider hiring Juri Kalashnikov instead of paying indefinite ransom . (Millions for defense, but not one cent for tribute) 77.3.138.240 (talk) 19:22, 28 March 2011 (UTC)
- What's missing from this apparent paradox is an assessment of risk. That resolves the paradox.
- In the first scenario, let's say you were 95% certain that the ransom would be honored. That puts you at a $950 'expected' payout on your $900 investment.
- During the second ransom, you know that your original assessment of the risk was wrong. Now you're much less sure that the ransom will be honored. Let's say now you're only 25% certain that they'll honor the second random after not honoring the first ransom. That gives you a $250 'expected' payout on a $900 investment. Clearly you should walk away.
- In other words, the sunk-cost doesn't carry over from one 'round' to the next, but previous 'rounds' do change your expectations of how the other party will act.
- (This all assumes that there's no better options available. For example, If you believe that there's a 50% chance that law enforcement can retrieve your item at no cost to you, then that is the correct choice because it offers an expected $500 profit.) APL (talk) 19:39, 28 March 2011 (UTC)
- (ec) 50 percent chance of law enforcement? "Har Har Har" Excuse me, from what I personally experienced in Germany, my advice is: forget about it. 77.3.138.240 (talk) 19:50, 28 March 2011 (UTC)
- As an alternative, the money that would have been spent on the ransom could also be spent in hiring private detectives and/or posting a reward. If the payment is contingent upon the item being recovered, then you are guaranteed that some effort will be made to recover the object, unlike with police, who may not much care about such a tiny item, since they won't get a share. StuRat (talk) 22:30, 28 March 2011 (UTC)
- I wouldn't say your assessment of the risk was wrong. If you had thought there was a 100% chance they would give you your money, then you would have been wrong, but just because the 1 in 20 chance happened doesn't mean it was more likely than 1 in 20. We're not talking about a random occurance, anyway, we're talking about a definite thing (either they are planning to give you your money or they aren't - they aren't going to toss a coin to decide), just one that you have incomplete information about. Getting additional information doesn't mean you made a mistake before. --Tango (talk) 22:26, 28 March 2011 (UTC)
- If you were aware of the idea of sunk costs then you could, but the kidnappers refusal to return the goods the first time would give you a lot of information about them, so you would probably think they would repeat the same trick again, and refuse. A clever thief would ask for a lesser amount the second time, to tempt you. I think J. Paul Getty was probably right about refusing to pay a ransom for John Paul Getty III. 92.15.14.4 (talk) 20:01, 28 March 2011 (UTC)
- Isn't the original theft already a "sunk cost"? Would you trust a random person, who admits that he is a thief, who offers to sell you $1000 worth of goods for $900? Additionally, of course, one worries that by doing business with a scam artist, he is branded as a sucker - just like buying something from a spammer. Conversely, an attack on the thief that succeeds has substantial prestige value. Wnt (talk) 01:44, 29 March 2011 (UTC)
- "Conversely, an attack on the thief that succeeds has substantial prestige value." What kind of attack did you have in mind? How would this help you get your stuff back? Its usual to do the paying of the ransom secretly, so being seen as a sucker or gaining prestige would not apply. 92.29.126.172 (talk) 13:51, 29 March 2011 (UTC)
- The secret might get out, or that same thief might target you again, or tell one of his thief friends about it, who then target you. So, the cost of the increased future likelihood of theft must be considered in the equation. The original theft could even be a test case, to see how you react to ransom demands, so the thief will know whether to go ahead with kidnapping your kids, as planned. StuRat (talk) 18:19, 29 March 2011 (UTC)
- In a law-abiding society one might pay the thief with an exploding dye-pack and a police pursuit, or in a less lawful one, with a pipe bomb; either way, the ensuing damage to the thief is apt to become known and dissuade further attacks. Wnt (talk) 03:43, 30 March 2011 (UTC)
- Never heard of revenge or vendetta? 92.15.1.33 (talk) 16:20, 30 March 2011 (UTC)
- Smart kidnappers know not to return "the goods" (if at all) until they have completely gotten away, by telling you where to go pick it up. They might also use an innocent "patsy" to pick up "a package somebody left for me". StuRat (talk) 05:05, 30 March 2011 (UTC)
- You learnt that off the movies. 92.15.1.33 (talk) 16:20, 30 March 2011 (UTC)
- And so did the smart kidnappers. StuRat (talk) 16:24, 30 March 2011 (UTC)
Question regarding extraterrestrial radio pulses
I was watching an interview with Arthur C. Clarke (co-writer of 2001: A Space Odyssey) before the movie's 1968 premier in which he said:
- "In the last few weeks there has been tremendous excitement among the astronomers over the extraordinarily precise and rhythmic radio pulses coming from the direction of a point between Vega and Altair. Which may yet turn out to have a natural explanation, but its periodicity and characteristics are so extraordinary that no explanation as yet seems very feasible."
I'm picking up some references to 1967 signals picked up from Vega and Altair...but whatever happened? Have these been explained? Thanks. WordyGirl90 19:44, 28 March 2011 (UTC)
- The timing and location look right for it to refer to the first pulsar to be discovered. AndrewWTaylor (talk) 19:49, 28 March 2011 (UTC)
- There was the Wow! signal But that was in 1977, not in 1967. Googlemeister (talk) 19:50, 28 March 2011 (UTC)
- The LGM-1 was from 1967 and is probably what Clarke was talking about. Googlemeister (talk) 19:56, 28 March 2011 (UTC)
- That would have to be it...correct constellation, too. Thanks :) WordyGirl90 20:19, 28 March 2011 (UTC)
- The LGM-1 was from 1967 and is probably what Clarke was talking about. Googlemeister (talk) 19:56, 28 March 2011 (UTC)
- There was the Wow! signal But that was in 1977, not in 1967. Googlemeister (talk) 19:50, 28 March 2011 (UTC)
- The timing and location look right for it to refer to the first pulsar to be discovered. AndrewWTaylor (talk) 19:49, 28 March 2011 (UTC)
Interface for communicating with blind people
Hi all. I'm writing a short novel where the protagonist, who is blind, uses a technological device that accurately scans his surroundings and sends this information back to him. The problem is that I can't imagine exactly how I would transmit this information to the blind user. Using a synthetic voice would interfere with 'real', useful sounds. Maybe using a pad in the hand with vibrations/pressure/heat that conveys this information? Please, help me with my brainstorming! Thank you very much. --Bliviinc (talk) 21:49, 28 March 2011 (UTC)
- There were experiments that had a head-mounted grayscale camera. It converted the image to sound by scanning a line at time. Left-to-right was represented by low tones to the left, and high tones to the right; black was quiet for that frequency, white was loud. I'm not sure how the start of each frame was represented; lets say a click.
- Thus
- A vertical line white line on a black background is a solid tone; lower in tone to the left
- A horizontal line is sudden burst of white noise, the rest is silence. The closer to the click the higher up the line is.
- A top-left to bottom-right line is a rising tone
- A top-right to bottom-left line is a descending tone.
- From memory, the experiments were successful enough for the subjects to navigate using the device. I'm not sure if there were different sounds (views) for each ear or not. It probably started with the same tones to each ear if there was eventually two cameras/tones. CS Miller (talk) 22:08, 28 March 2011 (UTC)
- How about a device that has little bumps that raise up to form the equivalent of a black and white image of the room ? There already exists a device which raises bumps to form Braille letters. As an alternative, instead of the bumps being raised based on the darkness/lightness of the object, they could be raised or lowered based on distance from the device, to created a 3D image of the room, at perhaps 1/1000th the depth of the room (it would be nice if this ratio was adjustable for large and small rooms). Since the blind person would be constantly running their hand over it, it should be washable, as it would accumulate oils and dirt. Perhaps a removable flexible surface on top could be washed or replaced, as needed, with the expensive "guts" remaining dry. StuRat (talk) 22:20, 28 March 2011 (UTC)
- I recall a TV show featuring someone blind from birth who had developed his own sense of echo location, making his own audible clicks. If someone has been blind from birth, their senses have had a longer time to compensate for the loss of sight. PЄTЄRS
JV ►TALK 22:25, 28 March 2011 (UTC)
- I recall a similar TV show. I remember a young boy finding and identifying a fire hydrant by clicking. --Tango (talk) 22:48, 28 March 2011 (UTC)
- Personally, I'd think the smell of dog pee might be a clue. :-) StuRat (talk) 22:53, 28 March 2011 (UTC)
- This site: http://www.seeingwithsound.com/ they have a demo and you can practice playing tic-tac-toe by sound alone. Ariel. (talk) 22:58, 28 March 2011 (UTC)
- That's a heck of a lot less challenging than navigating through a room, though. StuRat (talk) 23:00, 28 March 2011 (UTC)
- The tic-tac-toe is just a demo for sighted people. The device is actually used for navigating rooms. Ariel. (talk) 23:20, 28 March 2011 (UTC)
- That's a heck of a lot less challenging than navigating through a room, though. StuRat (talk) 23:00, 28 March 2011 (UTC)
- A device far cooler then using sound already exists. Vespine (talk) 23:04, 28 March 2011 (UTC)
Great ideas!! I particularly like your idea, StuRat. Apparently, a big problem blind people face and that most "navigating aid" devices can't detect are slopes and steps, instead of massive obstacles. How would you communicate those to the user with your bump-grid? --Bliviinc (talk) 23:40, 28 March 2011 (UTC)
- Well, if the difference in height of the bumps wasn't enough when looking at the whole staircase or slope, perhaps it could be focused on an individual step or section of the ramp, and would automatically scale the depth so that the closest objects in the view had bumps 100% up, and those farthest away in that view would have bumps 100% down. StuRat (talk) 23:54, 28 March 2011 (UTC)
- I think that the main problem is detecting those on the fly, without having to stop and focus on them. Maybe additional, always-zoomed bumps? --Bliviinc (talk) 23:59, 28 March 2011 (UTC)
- Just to be explicit, the bump-grid concept is actually the basis of the device that Vespine pointed to above. Looie496 (talk) 00:01, 29 March 2011 (UTC)
- I also once read about a blind guy who could use echo like a bat, but I suppose that while all people can use echolocation to some extent only chosen few can use it to navigate. How about full body suit that warms or puts pressure on persons skin if it senses an obstecle right in front of that spot and the pressure/warmth varies in strenght depending on how close the object is? Also assuming blindnes isn't caused by brain damage artifical eyes or neural interface could work (we're talking sci-fi short story, right?). ~~Xil (talk) 00:20, 29 March 2011 (UTC)
- Actually, no, they already have that. But it's black-and-white, low res, and requires surgery and training, so not ready for mass-marketing yet. StuRat (talk) 00:31, 29 March 2011 (UTC)
- You mean artifical eye? I am aware, but the technology has only just started to develop and there seems to be some promise in it. OP said it is for a story, but hasn't given any further details on setting of his story, so I am assuming it is sci-fi i.e. that it dosen't need to exist or must be producable with current technology ~~Xil (talk) 01:13, 30 March 2011 (UTC)
- Actually, no, they already have that. But it's black-and-white, low res, and requires surgery and training, so not ready for mass-marketing yet. StuRat (talk) 00:31, 29 March 2011 (UTC)
- Wikipedia has an article about corner reflectors. -- Wavelength (talk) 15:08, 29 March 2011 (UTC)
- How does that relate to the question ? StuRat (talk) 18:16, 29 March 2011 (UTC)
- Radar is a technological device, and staircases have corners. -- Wavelength (talk) 19:25, 29 March 2011 (UTC)
- So you're suggesting use of radar ? I don't think this question is about getting the room shape info into a device, it's about conveying that info to a blind person. That's the tricky bit. StuRat (talk) 20:39, 29 March 2011 (UTC)
- That information can be conveyed by audible signals. (See Geiger counter.)
- —Wavelength (talk) 21:48, 29 March 2011 (UTC)
- [I am correcting my punctuation. -- Wavelength (talk) 21:50, 29 March 2011 (UTC)]
- But how, precisely ? Would you point a beam in various directions and know the distance in that direction from the frequency of the sounds ? Such a system would work, but would also be very slow to use. I have difficulty imagining how a brain not designed for echo-location could use hearing to instantly "see" an entire room in the way that our eyes do. StuRat (talk) 05:02, 30 March 2011 (UTC)
- Our Britches (monkey) article is about a monkey, liberated by the ALF, whose eyes had been sewn shut at birth and he had been made to wear a "substitute sensory device". Comet Tuttle (talk) 18:36, 29 March 2011 (UTC)
- It says "sonar device", sounds like echolocation again, it does though mention the device being version of "sonicguide", I googled it didn't find anything in particular, but it seems to be sound emiting device attached to cane, here's a similar device: [3] ~~Xil (talk) 01:13, 30 March 2011 (UTC)
March 29
Rendering Equations
I've been trying to lean how to render equations instead of having to ask. Why doesn't this render png? On my browser it appears as html.Bugboy52.4 ¦ =-= 03:34, 29 March 2011 (UTC)
- How about this:
- Courtesy of Help:Math#Forced PNG rendering. DMacks (talk) 03:48, 29 March 2011 (UTC)
- What about
Failed to parse (syntax error): {\displaystyle \text {E}=\text {mgh}=0.1\times980\times10^{−2}=0.98\text {erg}}
Its not rendering, what am I doing wrong? Bugboy52.4 ¦ =-= 03:53, 29 March 2011 (UTC)
- The minus sign in your "-2" is not an ordinary minus sign, it is some sort of fancy dash. The math mode parser does not know how to handle it. If you use an ordinary minus sign, it will render:
Someone please copy this to WP:VPT so the developers know about it. 99.2.149.161 (talk) 17:30, 29 March 2011 (UTC)
- The developers will tell you that the TeX parser is fully compliant - and that this behavior is correct. You have entered invalid syntax that is not a valid equation. Unicode (and therefore MediaWiki and its TeX parser) specifies a different interpretation for − and - though the glyphs look similar in most standard Windows, *nix, and Mac fonts. (Consider reading the characters in a hex editor). Read about character duplication in Unicode, which is slightly technical. Nimur (talk) 19:41, 29 March 2011 (UTC)
A test where E. Coli is not exceeding 3/g ???
Under Australian legislation, ready-to-eat meat products must not have E.coli exceeding "3/g"
But it doesn't specify what the unit of measurement is, 3 what???
3 Colony-forming_units?
3 single Bacterium?
I have contacted the Food Authority and they will come back to me within 10 days. I have also contacted laboratories but their sales people don't know.
220.244.35.181 (talk) 05:02, 29 March 2011 (UTC)
- Based on this I think it means 3 single Bacteria (per gram). Ariel. (talk) 07:04, 29 March 2011 (UTC)
- Thanks, I did come across that paper, but I'm afraid it's no clearer - it doesn't state what test it uses - the test could use a different scale altogether. I'm not a food scientist (or any scientist for that matter) but it was impression that meat products can have thousands if not millions of bacteria - it seems absurd to me that you'd only find "3" micro-scopic bacteria of E. coli on a single gram. 220.244.35.181 (talk) 09:27, 29 March 2011 (UTC)
- Reading this [4] report, it seems it may be common to give the number in log10. So "3" actually means "10^3". That's still not a lot though, maybe it just puts a cap on the required measurement sensitivity. If you had say 20 bacteria per gram, you may have had to incubate them for a long time before you could detect them, while a thousand bacteria per gram can be detected just in time to stop a meat shipment. But this is just my speculations. EverGreg (talk) 12:51, 30 March 2011 (UTC)
What percentage of the atoms in our bodies were born in the hearts of dying stars?
Based on this table detailing the Chemical makeup of the human body, what percentage of our atomic composition (not mass) was created as a result of the death of stars? Flaming Ferrari (talk) 06:03, 29 March 2011 (UTC)
- It's almost impossible to speculate. Just about any element lighter than iron can be created by Stellar nucleosynthesis; heavier elements than iron are thought to arise from supernovae. However, given all of the various ways that a star may "die"; even if we just consider supernovae, a large percentage of all elements are likely scattered from them, even small elements like hydrogen, so just about any of the atoms in your body could have come from "dying stars"; and since two atoms of the same element and isotope are literally indistinguishable, there's no telling where they came from. --Jayron32 06:23, 29 March 2011 (UTC)
- This sounds like a homework question to me. I'd guess that the instructor means for you to figure that everything but hydrogen "was created as a result of the death of stars". So, that's 90% of the mass of a human, but you can do the math to figure out the "percentage of our atomic composition" (which I assume means by count of atoms). Since hydrogen is the lightest element, the count of hydrogen atoms should be considerably more than 10% of the body. If you want to do the math here, we'll check your work. StuRat (talk) 07:16, 29 March 2011 (UTC)
- A homework question where the lecturer refers the students to a Wikipedia table? Things have gone downhill since I left academia five years ago! --TammyMoet (talk) 07:57, 29 March 2011 (UTC)
- They may have found that on their own, but don't know how to get the answer to the HW question from it. StuRat (talk) 08:55, 29 March 2011 (UTC)
- Wikipedia has come on a lot in five years. We hope. Itsmejudith (talk) 16:16, 29 March 2011 (UTC)
- They may have found that on their own, but don't know how to get the answer to the HW question from it. StuRat (talk) 08:55, 29 March 2011 (UTC)
- A significant part of the Lithium also originates from BBN. Count Iblis (talk) 14:06, 29 March 2011 (UTC)
- True, but lithium (and helium, the other major non-radioactive elemental product of Big Bang nucleosynthesis) have no known biological function, and are present in the body in negligibly trace amounts. TenOfAllTrades(talk) 14:29, 29 March 2011 (UTC)
- Maybe you should count everything heavier than (or at least as heavy as) lithium and at least as light as iron, because it is hard to think of a supernova's exploding shell as a heart. But then again, most stellar nucleosynthesis takes place when most people would not say the star is dying, but the supernova does, so maybe you should count everything heavier than iron. But don't supernovae synthesize some proportion of light elements, too? Does anyone have a good idea what that proportion may be? 99.2.149.161 (talk) 17:49, 29 March 2011 (UTC)
- There's the issue of when elements are created, and also when they are released. Even if somewhat heavier elements are created before the death of a star, if they languish in the star's core, they aren't available biologically. From my experience with sloppy homework (and test) questions, it wouldn't surprise me a bit if the instructor is conflating those elements created by a star's death with those released by it. Unfortunately, with such sloppy questions, figuring out what the instructor really meant to ask is often the most difficult part of the problem. StuRat (talk) 18:09, 29 March 2011 (UTC)
part 2
A.mohammadzade let me ask this again ,as all know the huge part of our body contains water and the protein which made our meat is made of hydro carbon .Calcium element is about 15 percent and iron is in our blood and so zinc and Natherium ,... The first interstellar cloud which made sun and solar system might had hydrogen and helium so the last effects of dust came from novas and supernovae mixed to this cloud and the nebula had some thermodynamic conditions to made water and chemical matters , hydrocarbons made in earth specially condition which made the life .and first nebula did not be able to produce carbon and oxygen , which made 23percent of earth mass and 21%of air ,and several metals and silicates in earth crust are oxidized .
I want you my friends not to say died star for super novae they made life and they are absent in sky and send pulses and notice: Some body used to say something about the black holes but I prefer to say about super novas , the first one shows death and being mystery the second one is about the life and being alive .it had send oxygen and carbon ,so calcium and iron here to made our life(akbar mohammadzade)
:--78.38.28.3 (talk) 04:08, 30 March 2011 (UTC)
- I moved this from your new post on the same topic. It should all be kept together. StuRat (talk) 04:21, 30 March 2011 (UTC)
gas heat
my furnace is AC ready but has no AC hooked up to it. my repair guy said i have to clean that part too. how do i do that? — Preceding unsigned comment added by Wdk789 (talk • contribs) 07:03, 29 March 2011 (UTC)
- When you say AC do you mean Air Conditioning or AC electricity? Ariel. (talk) 07:08, 29 March 2011 (UTC)
Air Conditioning — Preceding unsigned comment added by Wdk789 (talk • contribs) 07:17, 29 March 2011 (UTC)
- So you have a point where the A/C unit will tie in to the duct-work of a forced-air gas furnace, and need it cleaned ? If it's a matter of cleaning out a duct, I'd use some kind of a mop in the open end. I'd use it dry to get the dust out. Wear work clothes and a dust mask while you do this, or you may be in for a coughing fit. Also, turn the furnace off shortly before you do this, as the duct-work might be hot where it connects. Note that there are companies that clean ducts, if you don't want to do it yourself. StuRat (talk) 07:22, 29 March 2011 (UTC)
Could you fit a model V12 or W16 onto a motor scooter and make it really work?
See, this is a real-working model V12: http://www.youtube.com/watch?v=0V_2v-ol1EU
And this is a W16, intended to be a 1/5th scale model of the Bugatti Veyron engine: http://www.youtube.com/watch?v=-DijdisWkAE
Are the horsepowers divided by their scales? Therefore, if the W16 has 1001 HP, would the fully-working 1/5th scale model have 200.2 HP? If so, how well would a 200.2 HP engine work on your everyday commuter motor scooter?
Regardless, what kind of ride would you get by putting those miniature versions of the Über engines into a motor scooter? What would your top speed be from there on out, as well as the acceleration, noise and fuel mileage? --70.179.169.115 (talk) 07:54, 29 March 2011 (UTC)
- I don't know if the simplistic approach to working out the horsepower is right, but even if it is, since the engine is three-dimensional you'd want the inverse cube, which is 1/5th times 1/5th, making 1/25th the horsepower. Wait, or do I mean 1/5th times 1/5th times 1/5th (1/125). It will be disappointing, anyway. 213.122.57.127 (talk) 08:31, 29 March 2011 (UTC)
- It would be the cube of 1/5, since the engine displacement volume is related to horsepower. So that would be 1/125th of 1001 HP, or approximately 8 HP, if it worked. However, internal combustion engines aren't very scalable (unless you change the number of cylinders along with the scale). So, while a 3 cylinder engine with that displacement might work well, a 16 cylinder engine would probably barely run, because all those moving cylinders would increase friction relative to the 3 cylinder engine, but without the displacement needed to overcome it. Of course, there are other things to change, too, such as the compression ratio and revs per minute, to get better performance out of the smaller engine. StuRat (talk) 08:47, 29 March 2011 (UTC)
Neutron star matter, on Earth
So let's say some Star Trek like genius, in the 53rd century AD, creates a technology that can grab neutron star matter without it decaying in any way. So the United Federation of Planets decides to go grab some, and transport it back to Earth.
Once at Earth, the matter is released as-is into the Earth's atmosphere. What would the reaction be? of:
- The Quark-gluon plasma at the center (density: ~6-8 trillion pounds per teaspoon)
- The crust (density: ~10 thousand pounds per teaspoon, and ten billion times stronger than steal, at least at the immense pressure on the neutron star itself).
Magog the Ogre (talk) 17:16, 29 March 2011 (UTC)
- Some potentially useful discussion along similar lines was discussed not too long ago, though it doesn't address your question directly. --Mr.98 (talk) 19:09, 29 March 2011 (UTC)
Oh, neat. From what I can see, regarding the thickest of the matter:
- If it were to remain in this neat sci-fi vessel we have, and not explode, it would barrel a whole to the center of the earth, sucking massive amounts of matter in its wake, and surely causing earthquakes, volcanic eruptions, and all sorts of other havoc.
- If it were released suddenly into the air, it would be the equivalent of a nasty nuclear bomb; however, given that it would keep exploding for a good time, it quite likely could destroy all life on Earth.
For the less dense stuff: maybe just a really big explosion that could kill a lot of people? Magog the Ogre (talk) 20:47, 29 March 2011 (UTC)
- At STP, what is the predicted density of a neutron gas. Does a neutron gas have a theoretical triple point? Plasmic Physics (talk) 03:23, 30 March 2011 (UTC)
- There isn't any predicted information like that. Neutronium is a term which was coined, conjecturally, for such standard conditions neutron-based matter, but no known substances exist, and there isn't a lot of reliable prediction for what it would look like if it did. The Wikipedia article actually covers this well, at least in noting that no one seriously considers it a likely form of matter, except in some very exotic conditions. The other type of neutron matter, known as Neutron-degenerate matter literally cannot exist at STP, as it requires the literally astronomical pressures in a neutron star to exist. If that matter were to be brought to STP, it would rapidly convert to normal (proton-electron-neutron) matter of some sort, likely mostly hydrogen, deuterium, and helium. --Jayron32 05:21, 30 March 2011 (UTC)
- At STP, what is the predicted density of a neutron gas. Does a neutron gas have a theoretical triple point? Plasmic Physics (talk) 03:23, 30 March 2011 (UTC)
- I don't really know what ot make of your answer - I googled "neutron gas", and one result described a low density neutron gas produced for the purposes of a projectile target for a particle physics experiment. For clarification, I'm not refering to degenerate states of matter, but simply a bulk sample of neutrons in a closed container with movable walls. The result did't answer my questions, if you were going to ask. Plasmic Physics (talk) 12:08, 30 March 2011 (UTC)
- While I'm at it, here's another one: since neutrons have no atomic orbitals, is there any substance that can contain such a hypothetical gas of neutrons, wouldn't the gas simply diffuse through the walls of the container within a matter of hours? Plasmic Physics (talk) 12:13, 30 March 2011 (UTC)
- Hypothetically, neutrons would not be subject to intermolecular forces, since they are both neutral and extremely hard (i.e. nonpolarizable). In other words, they aren't subject to even London dispersion forces, generally held to be the weakest of the common Van der Waals forces regulating the formation of non-gasseous phases of matter. If we were to consider a bulk gas composed of nothing but neutrons which was also at atmospheric densities, there are literally no forces at all which could act, at any temperature, even infinitessimally close to absolute zero, which could cause the neutrons to form a condensed phase. So, there would literally be no triple point, because there are no forces acting to cause neutrons to attract to one another. Collecting low-temperature neutrons like this to even make such a gas is likely impossible; but even if you could it would never be anything but a gas. --Jayron32 13:02, 30 March 2011 (UTC)
- The neutrons are made of quarks, right? Quarks have charges, right? Would that make the neutrons slightly polar? So, if the temperature brought within a picokelvin above absolute zero, wouldn't they form transient atractions to one another? Plasmic Physics (talk) 13:12, 30 March 2011 (UTC)
- I was about to say no, but reviewing Neutron#Structure_and_geometry_of_charge_distribution_within_the_neutron, it seems that very recent research suggests that there is a non-uniform charge distribution within a neutron, implying that they would be subject to something akin to London dispersion forces, so perhaps at such tiny temperatures (femtokelvin? attokelvin) there may be some time when induced charge seperation could generate a condensed, low-energy, low-pressure form of neutron matter; akin to a neutron liquid or neutron solid. The problem is, we have no reliable way to predict behavior at that level; at the distances that would be required for such tiny forces to work, the electromagnetic force, which would be responsible for solid or liquid formation, is actually much weaker than the nuclear forces which regulate things like quark interactions and internucleon interactions. In other words, at the distance you would need to bring many neutrons together in order to have them be attracted enough to form anything like a condensed phase of normal atomic matter, the situation is so drastically different than even for the smallest atoms. Consider that Hydrogen has a van Der Waals radius of 120 pm; this is the roughly scale of the minimum interatomic distances present in a condensed phase. The Wikipedia article on the neutron doesn't contain any information on its size, but this document calculates a radius of about 1 femtometer, or roughly 1/100,000 the radius of a hydrogen atom. So your hypothetical neutron solid would, once again, be under the influence of forces other than the electromagnetic force, which is sorta the definition of degenerate matter in the first place. In other words, low-temperature neutronium solid wouldn't be a solid under the normal definition of a solid, insofar as it obeys the odd laws of physics regulating degenerate matter rather than that of normal matter. So, once again, there is no hypothetical "normal matter" condensed phase substance composed of neutrons alone. There may be a neutron gas, but it will not condense to form solids or liquids which resemble, in any meaningful way, a real solid or liquid. --Jayron32 14:02, 30 March 2011 (UTC)
- The neutrons are made of quarks, right? Quarks have charges, right? Would that make the neutrons slightly polar? So, if the temperature brought within a picokelvin above absolute zero, wouldn't they form transient atractions to one another? Plasmic Physics (talk) 13:12, 30 March 2011 (UTC)
- The neutron is "supposed" to have a Neutron electric dipole moment according with theoretical models, but that moment is so small that no experiment has ever been able to detect it. Dauto (talk) 19:21, 30 March 2011 (UTC)
- Ok, I believe you, there is only one phase in the classical sense for a neutron gas due to the lack of interaction taking place however, interneucleon forces may or may not cause a condensate like phase to form (degenerate matter). What about my other question, concerning its diffusuability through solids? Plasmic Physics (talk) 23:47, 30 March 2011 (UTC)
- There is such a thing as a neutron reflector but their efficiency has limitations. Dauto (talk) 01:01, 31 March 2011 (UTC)
- Ok, I believe you, there is only one phase in the classical sense for a neutron gas due to the lack of interaction taking place however, interneucleon forces may or may not cause a condensate like phase to form (degenerate matter). What about my other question, concerning its diffusuability through solids? Plasmic Physics (talk) 23:47, 30 March 2011 (UTC)
What did the retired US Air Force nuclear missile commanders tell the National Press Club?
What's the most reliable summary of this? Specifically I am looking for something with the number of retired officials confirming the incidents, whether there are any incidents reported that vary substantially from the typical report, and the date ranges for each of the incidents. 99.2.149.161 (talk) 17:36, 29 March 2011 (UTC)
- That article describes a book, written by a space alien enthusiast. It seems he read about, or attended, a September 2010 press conference, where a retired Air Force officer did make explicit reference to extra-terrestrial life.
- But overall, this is just a space-alien enthusiast, who read about, and then created a mangled and contorted version of, a much more benign press version of reality; and then added several generic, probably totally-fictional stock-descriptions about extra-terrestrial encounters. In the 1940s and 1950s, as the threat of nuclear war became real, military brass set up loads of early warning systems: RADARs and other aerial surveillance systems. The plan, part of the Mutually Assured Destruction strategy, was to monitor the sky for anything that looked like an incoming bomber or missile - and if we saw one, we'd blow away the Soviet Union with a full-scale missile strike. (Obviously, this was a bad idea)..
- Now, as anyone who has ever used technology of any kind can tell you, electronics have "glitches" sometimes. RADARs often report false-positives - "glitches" - noise, due to electronics and atmospheric effects. (When a RADAR picks displays an unknown dot, it is an "unidentified flying object", right?) So, as the NORAD and SAC commanders and strategists realized that their RADARs had glitches, they realized that they couldn't sustain a "fire all missiles" response to every little static-noise burst.
- Our space-alien enthusiasts gladly pick up on Project Blue Book: the Air Force systematically studied UFOs, and then decided to close all further investigations - well, let's step back and read that one more time. After years of policy that required escalating every static noise burst to the President so he could decide whether to nuke the Russians, the Air Force finally realized that there was such a thing as electronic noise, and that not every RADAR pulse was actually an enemy aircraft or missile (or extraterrestrial space-ship). The presence of "UFOs" required bringing our nuclear response to a reasonable level. Nimur (talk) 14:32, 30 March 2011 (UTC)
- Is that a fair characterization of what took place at the National Press Club? Is it true or not that "several" retired USAF officials said that they had personally witnessed nuclear ICBMs deactivating at the same time that UFOs were being reported above ground at the same facilities? If so, exactly how many officials and how many separate incidents were there? Over what time period did these incidents occur? Is it true that such incidents have also been reported by former USSR officials? I am baffled that even UFO enthusiasts do not seem to be following this story as closely as I'd expect them to. I just want a reliable summary. 99.2.149.161 (talk) 21:19, 30 March 2011 (UTC)
- Here are some more links of interest: video, Socio-Economics History Blog, VeteransToday.com. And [5] might be excerpts from one of the organizers of the National Press Club event. 99.2.149.161 (talk) 02:03, 31 March 2011 (UTC)
What experimental recreational drug am I thinking of?
I remember reading a news article a year or two ago (I think) about a company that was trying to create a recreational drug that would get you high, but without side-effects, and with an antidote that you could take should you need to become sober quickly. Does anyone know what I'm thinking of? A Quest For Knowledge (talk) 17:41, 29 March 2011 (UTC)
- Nevermind. I found it.[6] A Quest For Knowledge (talk) 20:03, 29 March 2011 (UTC)
Identify my skull
Could anyone help to identify this skull (assuming it is a skull). It was found in rocky hills in Oman; the absence of obvious front-facing eyes is puzzling; it's very light and has what look like air pockets, so possibly a bird? Thanks for any help! HenryFlower 18:07, 29 March 2011 (UTC)
-
side view
-
bottom view
-
rear view
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eye socket remnant?
-
brain case
-
the nose
- If it lacks eye holes, are you sure it's a skull, as opposed to some other bone ? StuRat (talk) 18:12, 29 March 2011 (UTC)
Not at all sure, no. :) On the other hand, I have no idea what other bone it could be; it is basically round and hollow, with a hole at the back which looks like a spinal cord would go through it; and there might have been an eye socket in the broken part (though then the eyes would have been looking to the side and slightly backwards. HenryFlower 18:17, 29 March 2011 (UTC)
- Yes, it's a skull (you can see the distinctive suture lines), but we'd need more pictures to be sure of what exactly it came from. Based on the general roundness, size, and the area it was found, I'm thinking it's a species of monkey. Matt Deres (talk) 18:57, 29 March 2011 (UTC)
- (EC)I can't help with ID, but I think you're on the wrong track with the "lack of eyes" idea. Keep in mind that your specimen is highly damaged, whatever it is. Look at this raccoon skull:[7], and this gerbil skull [8]. Basically, these animals' eyes are well outside the main brain-case enclosure. It could be that what you have is a similarly shaped skull, and the thin bits of bone arch that surround the eye socket have broken off. It's hard to tell from your pictures, but I think the side view may show remnants of such bones. SemanticMantis (talk) 18:59, 29 March 2011 (UTC)
- Yes, it's definitely a skull, and definitely very badly damaged -- you really only have a small part of it. It looks to me to be a mammal skull, from a pretty good-sized mammal. One possibility may be a dog. Looie496 (talk) 19:09, 29 March 2011 (UTC)
- If there are any teeth left, a close shot of those might be very helpful. Googlemeister (talk) 19:41, 29 March 2011 (UTC)
- The round hole at the front made me think of some sort of anteater, something like this doesn't look too dissimilar, has a similar "lack" of obvious eye holes. Having a quick look it seems like there are anteaters in Oman. Vespine (talk) 23:11, 29 March 2011 (UTC)
- Hmm well, ok, i'm wrong about the anteater in Oman, seems like they're only in south america.. How about armadillos ? Vespine (talk) 23:21, 29 March 2011 (UTC)
- The round hole at the front made me think of some sort of anteater, something like this doesn't look too dissimilar, has a similar "lack" of obvious eye holes. Having a quick look it seems like there are anteaters in Oman. Vespine (talk) 23:11, 29 March 2011 (UTC)
- That's the back, so the hole is for the spinal cord. StuRat (talk) 23:18, 29 March 2011 (UTC)
- Aaah! Yes, i was looking at it wrong, sorry... but anyway the links I posted show that lack of "obvious" eye holes are not necessarily a problem. Vespine (talk) 23:22, 29 March 2011 (UTC)
- I'm really curious now! I don't think it looks rodent, canine or rabbit, what other "common" animals are there in Oman? Vespine (talk) 23:25, 29 March 2011 (UTC)
- Aaah! Yes, i was looking at it wrong, sorry... but anyway the links I posted show that lack of "obvious" eye holes are not necessarily a problem. Vespine (talk) 23:22, 29 March 2011 (UTC)
- That's the back, so the hole is for the spinal cord. StuRat (talk) 23:18, 29 March 2011 (UTC)
- It would help to know what kind of soil or rock strata it was found in. then we might have an idea whether we're trying to match with a modern (familiar) animal or something else. Also does it seem to be actual bone or rock,as in fossil?190.148.134.128 (talk) 00:32, 30 March 2011 (UTC)
also what is front or back seems at this point to be conjecture.190.148.134.128 (talk) 00:56, 30 March 2011 (UTC)
- It's light and has air pockets, i think it's obviously bone, not a fossil. The main problem I think is the OP has not given a good frontal photo showing the nasal area and the jaw structure on the underside photo is badly out of focus, these areas in particular would probably reveal a lot more unique detail. Vespine (talk) 01:02, 30 March 2011 (UTC)
- I'm trying to find fauna local to the region but not much luck. There's an awesome feline called a caracal but the skull looks very different, as does a local wolf, hyena and several antelope or goat like animals. I don't think it's a bird or a a lizard, or a rodent, my guess is some sort of mammal but I'm really stumped without some better photos. Just for clarification, you do mean Oman the country on the Arabian peninsula, not some other town somewhere like Paris Texas or something. Vespine (talk) 01:18, 30 March 2011 (UTC)
- The nasal area is missing, as is most of the upper jaw. This is really just the back of the skull, and not even all of that. Looie496 (talk) 03:07, 30 March 2011 (UTC)
- I'm trying to find fauna local to the region but not much luck. There's an awesome feline called a caracal but the skull looks very different, as does a local wolf, hyena and several antelope or goat like animals. I don't think it's a bird or a a lizard, or a rodent, my guess is some sort of mammal but I'm really stumped without some better photos. Just for clarification, you do mean Oman the country on the Arabian peninsula, not some other town somewhere like Paris Texas or something. Vespine (talk) 01:18, 30 March 2011 (UTC)
- It's light and has air pockets, i think it's obviously bone, not a fossil. The main problem I think is the OP has not given a good frontal photo showing the nasal area and the jaw structure on the underside photo is badly out of focus, these areas in particular would probably reveal a lot more unique detail. Vespine (talk) 01:02, 30 March 2011 (UTC)
Thanks for all the ideas! In answer to a few points:
- SemanticMantis, your point about the eyes seems to be along the right lines - the racoon skull is quite similar. Presumably not an actual racoon here in Oman, though there must be something similar.
- I've added a few more photos showing the (probable) remnants of the eye sockets, inside, and what's left of the front/nasal area.
- For what it's worth, this page has photos of various animals from the author's travels (mostly in Oman).
- It's definitely bone, not a fossil. It was in a rocky desert area, altitude about 500m.
Even if we can't identify it for certain, at least is slightly less of a mystery to me now. :) HenryFlower 03:24, 30 March 2011 (UTC)
- AH, I see now. In the first out of focus photo I actually thought those might be tooth socket remnants but it's obvious that whole upper jaw area is worn away.. I take back what I said about it not being a rabbit or rodent, in fact, if you use your imagination, it could be a rabbit, or maybe more likely a hare, if you look at a picture like this and use your imagination to deteriorate the missing parts, it's not extremely dissimilar. Vespine (talk) 04:54, 30 March 2011 (UTC)
- My guess would be a Mustelid but without an indication of size it's very hard to be more specific. If it is clearly too big to be a Mustelid I would change my "vote" to Canid. Roger (talk) 12:51, 30 March 2011 (UTC)
I don't think it's a rabbit: the spinal cord hole in the rabbit skulls I've seen is in the base (the head sitting on top of the body); I imagine a hare is the same. This one has the hole in the rear of the skull, which would seem to imply a more horizontal body posture, which in turn would fit with the idea of a weasel-type thing. The skull (or rather the bit I have) is about 7-8cm, so maybe something a bit bigger than a pine marten. HenryFlower 16:46, 30 March 2011 (UTC)
- If I can get a bit nosy: what in the world were you doing in Oman? I can't think of any reason whatsoever to be a tourist in that country. Unless you live there, which also seems unlikely to me. Magog the Ogre (talk) 17:02, 30 March 2011 (UTC)
- See Tourism in Oman. Are you confusing Oman with Yemen perhaps? Looie496 (talk) 17:20, 30 March 2011 (UTC)
- Didn't they used to be the same country? Regardless, I can't imagine traveling halfway around the world to a part of the world quite hostile to westerners (of which I am one), to go touring in the middle of the desert. Then again, I live in the US, so maybe that will cause some differences. And to each his own (maybe Oman has a great industry I don't know), but I still don't understand why someone else would do it. Magog the Ogre (talk) 19:54, 30 March 2011 (UTC)
- We're way off topic here, but the two are quite different. Oman is a country with 2.7 million inhabitants and a per-capita GDP of about $14,000. Yemen is a country with about 22 million inhabitants and a per-capita GDP of less than $1000 -- i.e., one of the poorest countries on earth. Oman is politically stable and welcoming to westerners. Yemen is a hotbed of turmoil and a dangerous place to visit. Looie496 (talk) 20:50, 30 March 2011 (UTC)
- If I can get a bit nosy: what in the world were you doing in Oman? I can't think of any reason whatsoever to be a tourist in that country. Unless you live there, which also seems unlikely to me. Magog the Ogre (talk) 17:02, 30 March 2011 (UTC)
What a strange turn the discussion's taking! Looie of course is entirely right. I'm off for the Muslim weekend now, but will be back on Saturday in case there are more thoughts. HenryFlower 03:35, 31 March 2011 (UTC)
carbon-dioxide atmosphere
I have a long list of questions for an idea that I've been thinking about. But I will stick with the first because it may negate the rest. I only mention this because this question surely seems nonsensical... Assume that a lot of carbon dioxide was added to the Earth's atmosphere. Along with this, there would be extensive global warming. So, it is safe to assume sulfer dioxide would be be produced in excess. Is there a point at which excessive heavy gasses (ie: carbon dioxide and sulfer dioxide) would settle to the lower elevations on Earth and the lighter atmosphere consisting of oxygen and nitrogen would float above that? Obviously, there would be a mixed area. I'm really asking if oxygen can be pushed up higher than it is now due to heavier gasses in the atmosphere - or, will the oxygen remain where it is and just mix with the heavier gasses? -- kainaw™ 19:51, 29 March 2011 (UTC)
- We have many different gases in the atmosphere now, and they generally seem to mix rather than form distinct layers. Yes, the concentrations of the various gases does vary a bit by altitude, but, other than the pressure differences, the air on the top of Everest is basically the same as at sea level, because winds continuously mix them up. I'd suspect that winds would be even stronger on a hotter Earth, since heat differences drive winds, so this "mixing bowl" effect would remain. StuRat (talk) 20:32, 29 March 2011 (UTC)
- It's because the atmosphere is clear to a lot of radiation, which is then absorbed by the ground thus bottom heating the atmosphere and preventing stable stratification. If the atmosphere was opaque to most radiation, stable stratification could be a possibility. —Preceding unsigned comment added by 92.20.201.71 (talk) 20:57, 29 March 2011 (UTC)
- Well, the atmosphere does show quasi-stable stratification, but the strata are relatively thick: troposphere, stratosphere, ionosphere, etc. Within the troposphere there is very extensive mixing due to the fact that solar radiation heats it from the bottom -- this mixing rapidly undoes any separation that may start to arise from differences in density. Note that there have been epochs of geological history when CO2 concentrations were up to 100 or more times higher than today. Looie496 (talk) 21:26, 29 March 2011 (UTC)
- One might consider that even with all the lower level mixing there is a surprising degree of stratification.for example ozone being triatomic oxygen O3 is way up there, in the mesosphere if I remember correctly.and we all know how important that is. I don't know what you're theory is but you might pursue it further.190.148.134.128 (talk) 01:21, 30 March 2011 (UTC)
- Hi there, i just fixed up 128's reply, please don't manually indent your replies but instead use : at the start of your contribution (have a look at the other replies to see how it works). A manual indent has a different function in wiki formatting. Vespine (talk) 01:27, 30 March 2011 (UTC)
- Thank you "vespine". I must explain that I am a really old guy and the computer is a new tool to me. I have no idea what "manual indent" means because I don't speak computorese. you're probably quite young and can't imagine how this can be possible because you probably have grown up with a computor. It sounds to me that you're saying I must read the other entries and agree with them, but I can't believe that. I'm not trying to be a smart ass. please tell me what I did wrong in plain english.190.148.134.128 (talk) 02:22, 30 March 2011 (UTC)
- "Manual indent" means starting a line with spaces. If you want a line to be indented in Wikipedia, you should start it with a series of colons, such as "::::::". (I have fixed your previous line.) Looie496 (talk) 03:02, 30 March 2011 (UTC)
- And, just to demonstrate:
this is a manual indent.
- We do use that, but not when we just want regular text, it's reserved for special things. For example, it's sometimes used to make diagrams. StuRat (talk) 03:19, 30 March 2011 (UTC)
- It should be noted that in high enough concentrations, carbon dioxide does settle, see Lake_Nyos#The_1986_disaster for an example of what happens when it does. However, this is quite a different scenario from atmospheric carbon dioxide. Essentially what happened at Lake Nyos was a bubble of pure carbon dioxide was "burped" out of the earth; this CO2 had very little mixing with the atmosphere, and so it suffocated the entire region. Atmospheric CO2 accounts for less than one part per thousand (see Atmosphere_of_Earth#Composition). According to Hypercapnia (the medical term for too much CO2), severe effects on humans don't set in until 10 kPa, or about 10% of the air, though minor effects set it at lower concentrations. Even assuming that some medical problems set in at 1% CO2, that would still require there to be 30X as much CO2 in the atmosphere as there is now. Even at those concentrations, there is sufficient circulation in the troposphere to assure complete mixing, even in the face of gravitational seperation. --Jayron32 03:33, 30 March 2011 (UTC)
- According to scale height, each gas has its own scale height above 100 km due to diffusion. Wnt (talk) 03:39, 30 March 2011 (UTC)
- Yes, but there is a big difference between what happens way up at 100 km and what happens in the much denser, and much more well mixed, troposphere... --Jayron32 03:45, 30 March 2011 (UTC)
- According to scale height, each gas has its own scale height above 100 km due to diffusion. Wnt (talk) 03:39, 30 March 2011 (UTC)
- Thanks for the answers. It appears that stratification is inhibited by heat that radiates from the planet surface. So, to get stratification to work well, radiant heat must be limited. Low-level greenhouse gasses will assist in two ways. First, they will reflect much of the solar radiation before it reaches the surface. Then, they will absorb and reflect heat before it reaches very high into the atmosphere. I think that studying temperatures on Venus will help me get a good idea of how well that will work. -- kainaw™ 12:15, 30 March 2011 (UTC)
Superallowed beta decay.
Superallowed transitions seems to be defined as those between members of an isotopic spin multiplet.
How could a beta decay not be between members of an isotopic spin multiplet? Since it is a weak interaction surely the number of quarks and hence total isospin will be conserved? So what is the difference between allowed and superallowed transitions? —Preceding unsigned comment added by 92.20.201.71 (talk) 20:29, 29 March 2011 (UTC)
- OP: Is it just that nuclear spin doesn't change? In which case how is a superallowed transition different from a pure fermi transition? —Preceding unsigned comment added by 92.20.201.71 (talk) 20:46, 29 March 2011 (UTC)
You stated "the number of quarks and hence total isospin will be conserved?". That's not true. The total isospin can change. Dauto (talk) 21:00, 29 March 2011 (UTC)
- up and down quarks both have I=1/2. I don't understand. —Preceding unsigned comment added by 92.20.201.71 (talk) 21:05, 29 March 2011 (UTC)
- What don't you understand? We might be able to explain if you let us know. Dauto (talk) 02:14, 30 March 2011 (UTC)
- Ok so my understanding was that nuclear isospin multiplets all had the same I and different values of I3. And that beta decay acted essentially as the creation/annihilation operator I±. And that since the operator I± cant get you out of the spin multiplet, all beta decay must be between isospin multiplet states. This appears to be in contradiction with the above statement I was troubled by about superallowed states, and your statement that I can change. So I'd be glad if you could help me grasp the nature of my misunderstanding. Thanks. —Preceding unsigned comment added by 92.20.201.71 (talk) 02:34, 30 March 2011 (UTC)
- Let me state upfront that my specialty is with particle physics, not nuclear physics. Your understanding is approximately correct and that's why beta-decays that violate the principle you describe must pay a penalty and will be less probable than naively expected. You must keep in mind that unlike weak isospin, isospin is not an exact symmetry. Dauto (talk) 04:08, 30 March 2011 (UTC)
- What kind of beta decays are the ones that break the symmetry? Is it just beta decay which changes a quantum number other than I3, such as when the neutrino and beta particle make a spin triplet and nuclear spin changes? Sorry, I may be asking tedious questions as I only started nuclear and particle this year so I do not have a condensed understanding of the subjects. —Preceding unsigned comment added by 92.20.201.71 (talk) 20:05, 30 March 2011 (UTC)
- I don't remember the answer to that specific question off the top of my head and solving it right now feels too much like homework. You need to get a good book about nuclear physics. As I said, my specialty is high energy physics. But I can explain to you without going into too many details why superallowed decays are favored. Basically, in a superallowed decay the nucleons in the parent and daughter nuclei have similar wave functions so there is a lot of overlap between their wavefunctions and all that needs to happen is the transition between a proton and a neutron or vice-versa. In a non-superallowed decay the form of the nucleon wavefunctions of the parent and daughter nuclei are different and their overlap may be quite small suppressing these decays. Dauto (talk) 00:56, 31 March 2011 (UTC)
- What kind of beta decays are the ones that break the symmetry? Is it just beta decay which changes a quantum number other than I3, such as when the neutrino and beta particle make a spin triplet and nuclear spin changes? Sorry, I may be asking tedious questions as I only started nuclear and particle this year so I do not have a condensed understanding of the subjects. —Preceding unsigned comment added by 92.20.201.71 (talk) 20:05, 30 March 2011 (UTC)
- Let me state upfront that my specialty is with particle physics, not nuclear physics. Your understanding is approximately correct and that's why beta-decays that violate the principle you describe must pay a penalty and will be less probable than naively expected. You must keep in mind that unlike weak isospin, isospin is not an exact symmetry. Dauto (talk) 04:08, 30 March 2011 (UTC)
- Ok so my understanding was that nuclear isospin multiplets all had the same I and different values of I3. And that beta decay acted essentially as the creation/annihilation operator I±. And that since the operator I± cant get you out of the spin multiplet, all beta decay must be between isospin multiplet states. This appears to be in contradiction with the above statement I was troubled by about superallowed states, and your statement that I can change. So I'd be glad if you could help me grasp the nature of my misunderstanding. Thanks. —Preceding unsigned comment added by 92.20.201.71 (talk) 02:34, 30 March 2011 (UTC)
- What don't you understand? We might be able to explain if you let us know. Dauto (talk) 02:14, 30 March 2011 (UTC)
ingesting radiation
I am confused as to the reporting concerning the dangers of the current Japanese Radiation problem.
To my very basic knowledge it will be really bad to ingest any radioactive substance even on a small scale as it will spit out beta,gamma or alpha for a lifetime which would harm the body's cells . Hence absorption into the body is the real danger, this will occur via the food chain or inhalation.
I am not sure if the media reporting is referring to "safe" levels of radiation as "safe if you do not ingest/breath it in" in other words the level is safe "at a distance" outside of the body.
In a similar way you can say that Americium in a smoke detector is at a perfectly safe level but if you ate it it would be very bad for you as you are then having a permanent amount of Americium absorbed into your body. —Preceding unsigned comment added by 2.97.155.22 (talk) 21:32, 29 March 2011 (UTC)
- It is important to distinguish between "radiation" and "radioactive substances". Radiation reduces very quickly with distance so the radiation being emitted by the reactors in Japan is only potentially harmful for the people working on them. The big risks are associated with radioactive particles escaping, since they can travel great distances and, as you say, be ingested. The big fears at the moment are with water outside the reactors that has been found to contain radioactive particles. As for the media, they usually don't know what they are talking about. They talk about both radiation and radioactivity, but don't always distinguish between them. --Tango (talk) 21:55, 29 March 2011 (UTC)
- EC, See Sievert and Gray (unit). Your understanding comes from the fact that ionising radiation has zero risk when the source is at a sufficient distance. However, a suitably small amount of even a potent alpha source, can still be safely consumed. Basically when the scientists say it is safe, it is safe. —Preceding unsigned comment added by 92.20.201.71 (talk) 22:03, 29 March 2011 (UTC)
- What happens to you if a radioactive substance gets into your body depends on a lot of things, not just its nuclear properties but also its chemical and biological ones, and mode of administration. For example a very tiny amount of plutonium in your lung is very likely to give you lung cancer. However it might not harm you if you ate it, because it's poorly absorbed (no warranty on this! I will not be responsible for anything that happens to you). See plutonium#toxicity.
- Similarly iodine-131 is extra dangerous because of its tendency to concentrate in the thyroid gland, and strontium-90 because it is chemically similar to calcium and is incorporated into bone. --Trovatore (talk) 22:05, 29 March 2011 (UTC)
- You are correct that most descriptions of "safe" radiation are about acute exposure, not chronic. Acute exposure is the kind of radiation that'll give you radiation sickness — it's most of what this chart is about. Unfortunately, for 99% of the people concerned, this is not the kind of radiation hazard they are going to be exposed to, because very high levels of radiation are quite rare and usually quite localized (e.g. right around the reactor). The chronic risks are from elements with long half-lives and corresponding low energy radiation, but when ingested can cause a lot of internal damage over time.
- Why is this distinction not usually made? Ignorance, probably. Mixed with that lovely impulse by the scientists and engineers to assert that the general public is worried about nothing. But also because discussing chronic exposure requires a lot more specificity about the particular risks you've got in mind, and frankly even the experts are often very poor at breaking these down into separate issues. As Trovatore points out, it really depends on the substances in question and how they get into you. Some radioactive substances through some pathways flush out of the body with no harm. Some deposit themselves in your bones or thyroid or what have you, and can do a lot of damage.
- I would not be comfortable if it was just the media telling me it was safe — it is clear that most journalists do not even begin the know what "safe" and "dangerous" means in the context of radiation. I would parse very closely the statements by officials and engineers — they often will say things like, it is safe for you to be in an area, but don't eat anything that grows there. There are also complicating factors — being exposed to radon gas by itself, for example, will have very little effect on your long term lung cancer risk. But if you smoke a cigarette in an area with high amounts of radon, you end up with all sorts of compounding factors and your risk goes up by a huge amount. --Mr.98 (talk) 22:21, 29 March 2011 (UTC)
March 30
Spreading mineral matters on earth
The general oxidation of earth crust might be after the time once the earth surface was molten ,the outer crust material complex and the location of mines such as aluminum and Ferro and copper in Alp -Himalaya belt shows us that thoroughly it was our earth surface molten for about 800 million years , and when any asteroid with mineral matters hinted our earth it had to be molten and spread on earth surface.(A. mohammadzade ) --78.38.28.3 (talk) 05:15, 30 March 2011 (UTC)
- Is there a question here ? StuRat (talk) 05:23, 30 March 2011 (UTC)
- Also, let me suggest that you also post in your native language (and tell us what it is), as we might be able to translate it better than you. Your English is barely readable. For example, "Coeur" isn't an English word. It means heart in French, but that seems wrong in this context. Did you mean copper ? StuRat (talk) 05:26, 30 March 2011 (UTC)
- I can't find a question, but the OP may find useful information on the cooling of the earth at History of the Earth and Hadean Eon. The asteroid impacts he is talking about occuring during Earth's molten phase happened during the Late Heavy Bombardment period. The ancient cores of continents, believed to date from the Hadean, are called Cratons. The location of ore deposits and how they formed are complex geochemical processes known as Ore genesis. All of the links I provided here should answer any questions the OP may have, given the various statements he made. --Jayron32 05:29, 30 March 2011 (UTC)
the continues spreading shows the question about the subject late heavy bombardment say me about this ,and first earth creation .--78.38.28.3 (talk) 05:36, 30 March 2011 (UTC)a. mohammadzade THANK YOU
- Please post your question in your own language as your English, which I suspect is a machine translation, is unintelligible. Roger (talk) 13:19, 30 March 2011 (UTC)
- His IP suggests he is from Iran. At any rate my guess is that he wants to know is if meteorite strikes have any relation to current composition of Earth's crust (i.e. have they changed location of minerals and metals in it) ~~Xil (talk) 15:37, 30 March 2011 (UTC)
- If so, he might be interested in our article on the Sudbury Basin. Matt Deres (talk) 18:35, 30 March 2011 (UTC)
- How do you ask him to post in Farsi, in Farsi? 92.15.1.33 (talk) 16:17, 30 March 2011 (UTC)
- I will post a request for assistance at the Language RefDesk. Roger (talk) 16:32, 30 March 2011 (UTC)
با در نظر گرفتن جایگری معادن در رگه هایی که به صورت تقریبا پیوسته مابین قاره ها امتداد یافته اند برای مثال معادن آهن و الومینیوم و مس به صورت تقریبا خطی بر روی کره زمین گسترده شده اند دو نتیجه می توانیم بگیریم .یک اینکه این معادن اقفاقی در یک خط قرار گرفته اند ودوم اینکه زمین در هنگام اختلاط هریک از این معادن با خاکش به صورت مذاب بوده است و هر سنگ اسمانی حاوی این عناصر را ذوب و در یک امتداد مثلا طولی یا عرضی کشیده است و با انشقاق قاره هابه شکل کنونی در امده است . اگر در یک دوره سطح زمین به صورت گسترده مورد بمباران شهاب سنگ ها قرار گرفته و هریک دارای عناصر معدنی بوده با فرض جامد بودن جبه زمین در زمان یاد شده به این نتیجه می رسیم که معادن نباید این گستردگی خطی را داشته باشند این تناقض را چگونه حل می کنید ؟
—Preceding unsigned comment added by 78.38.28.3 (talk) 03:39, 31 March 2011 (UTC)
Here's its translation: knowing that mines are located almost continuously along veins across continents, e.g. iron, aluminium, or copper mines are located almost linearly on the surface of the Earth, we can get two results. First, mines were accidentally located in a line; and second, when earth was mixing with these minerals, it was in a molten state, and it melted every meteorite containing these ingredients and pulled them in a latitudinal or longitudinal line, and present forms appeared when continents took shape by splitting. But if Earth was solid when those meteorites fell, this linearity of mines could not be formed. How do you explain this contradiction? (I myself don't see any contradiction here though! I don't understand him clearly --Omidinist (talk) 05:48, 31 March 2011 (UTC))
- Most minerals are found in veins, which are roughly tabular in shape, and therefore appear linear where they intersect the surface. They are mostly located along fault of fracture surfaces, that are generally of one or two distinct orientations in an area, relating to the stress field at the time of formation. Stress fields are often fairly constant in orientation over large areas, meaning that the faults/fracture and their associated veins are sub-parallel. If the stress-state changes, further mineralisation will occur along different lines, an example is the so-called 'cross-courses' in SW England associated with the cornubian batholith granitic intrusion, which run mainly north-south, cutting the earlier west-east main course veins. Mikenorton (talk) 07:37, 31 March 2011 (UTC)
- If you are interested in reading about metal deposits that are forming right now and being mined have a look for the one on Lihir Island, "Ladolam", in Papua New Guinea. Sean.hoyland - talk 08:55, 31 March 2011 (UTC)
برای مثال به معادن مس و خاکهای حاوی مس دقت کنید که می توانیم آنها را به صورت رگه باریک از شمال غرب ایران تا جنوب شرق از منطقه سونگون آذربایجان تا سرچشمه کرمان مشاهده کنیم یا معادن آهن از زنگولداک ترکیه تا چغارت ایران در یک باریکه خطی قرار گرفته اند —Preceding unsigned comment added by 78.38.28.3 (talk) 09:26, 31 March 2011 (UTC)
- OK 78, if google translate hasn't completely misled me, you are talking specifically about the porphyry copper deposits within the Urumieh-Dokhtar magmatic belt, formed as part of the Kerman arc during the collision between the Arabian Plate and Eurasian Plate. This is linear because it marks the location of a past subduction zone along that convergent boundary. Mikenorton (talk) 09:41, 31 March 2011 (UTC)
Milligram scale
We cannot offer you instructions on compounding pharmaceutical products. Please speak with your doctor or pharmacist if you would like to be able to safely adjust the dosages of your medication. TenOfAllTrades(talk) 22:44, 30 March 2011 (UTC) |
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The following discussion has been closed. Please do not modify it. |
This question is a bit unorthodox, I realize, but: where can I get a scale that will accurately measure within 1mg? I am willing to pay no more than $100, $150 if I get really desperate. I looked on Amazon and found a lot of cheap ones that aren't precise at the 1mg level, which is unacceptable for me. And I see some more expensive ones but they don't have enough reviews for me to tell how well they'll work. I am willing to buy online, although buying locally would be even more ideal. Magog the Ogre (talk) 16:59, 30 March 2011 (UTC)
Ugh, it turns out I have misread! I need it to be accurate to .01 mg, which I know is ridiculously precise, and probably not something I could find easily on the market. But to answer your question: no more than a few milligrams. Magog the Ogre (talk) 18:32, 30 March 2011 (UTC)
Re: Aspro: I am trying to measure my prescribed medication which I am splitting (the minimum dosage is .25mg, and I am cutting it in fourths, leaving ~.06 mg/dose; if I am off by even about 25%, I suffer undesirable side effects until my next dosage; my body is amazingly sensitive to tiny changes in chemistry... I can get pretty buzzed off just one beer for example). You will note I am not asking for medical advice (I've already talked to my doctor); I am asking about a scale. Magog the Ogre (talk) 19:58, 30 March 2011 (UTC)
Re: 50.*: a good idea; i have local contacts in a very large university chemistry department. Doesn't mean I'll get it though!
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I can't be bothered with the elaborate brown rice recipes.
Is it still worthwhile to eat brown rice when I can't be bothered to cook it for a long time? 12.40.220.253 (talk) 17:21, 30 March 2011 (UTC)
- It sounds like you are asking if it's OK to eat raw rice. Dauto (talk) 18:54, 30 March 2011 (UTC)
- If you can be bothered to walk round the supermarket you can find it ready cooked – just needs two minutes in the microwave.--Aspro (talk) 18:55, 30 March 2011 (UTC)
- Yes it is, the fibre is very good for you. The way I make rice is: add half a cup of rice and a full cup of boiling water to a saucepan. Bring back to the boil, then reduce the heat and simmer for 20-25 minutes (depends on the rice - could be 25mins for wholemeal, but down to only 15 for white or easy-cook rice - follow packet instructions). Check the saucepan from time to time to make sure it is not boiling dry. I use a timer to measure the time, as it is essential to remove the saucepan before it gets too dry and starts to burn. You can add chopped vegetables at the beginning, but this can introduce more moisture which may need draining off five minutes or so before the end. Best to be watching the saucepan for the last 5 minutes so that you can get the rice as dry as you wish, without burning. I prefer moist fairly soft rice. I use an open saucepan lid, so that all the interior is moist but which allows the steam to escape. I think you could alternately make rice with more boiling water and then drain and dry it after cooking. 92.15.1.33 (talk) 20:47, 30 March 2011 (UTC)
- I was surprised when I had some Chinese and Malaysian borders at my place a couple of years ago, when they told me that NO ASIANS these days cook rice as described above. They ALL use rice cookers. And when I bought one, I could see why. They cost about nothing (say $20). you just put the rice in, cover it with water by a couple of fingers, put the glass top on, and turn it on. It will cook the rice perfectly, then switch off to "keep warm" mode. There is nothing to do at all, and the rice is ALWAYS perfect! I never use anything else now. No chance for burning or undercooking, and the cooker keeps the rice warm for hours. Try it. All the Asians use it, and they are the canniest buyers I know. Myles325a (talk) 00:12, 31 March 2011 (UTC)
- But the rice in Asian cooking is usually sticky white rice. I think that some rice cookers won't work properly with other types of rice, so you should check that before buying. -- BenRG (talk) 04:27, 31 March 2011 (UTC)
- And, the other part of the "is it worth it" calculation is based on how good it is for you. Take a look at the nutrition here: [11]. The good points are that lack of fat, saturated fat, cholesterol, sugar, and sodium (unless you need to add those things to make it palatable). It also has a moderate glycemic index (less than white rice). It's a mixed bag as far as vitamins and minerals, having lots of some (like manganese), and very little of others. On the bad side, it's also fairly high in calories (almost all of them from starch), low in protein (although it is almost complete in amino acids), and somewhat inflammatory. StuRat (talk) 04:25, 31 March 2011 (UTC)
- You've forgotten the fibre, which most people do not get enough of. It is very much better than filling up on junk food such as "french fries" or pizza. 92.29.119.112 (talk) 10:43, 31 March 2011 (UTC)
Protein subunit names vs gene names?
Hi, I had a question about how it is that protein subunits get their names. I was under the impression that if an operon had the structure (for example, in the case of the perchlorate reductase enzyme) pcrABCD, the subunits would be alpha, beta, gamma, and delta (respectively). However, I just noticed that in the case of another enzyme, methane monooxygenase, the pmoCAB operon encodes gamma, beta, and alpha, respectively. So, how is it that biochemists name subunits? Is it not supposed to correlate with the genes (i.e., why is "A" not the alpha subunit?) Thanks for your help. Ccarlst (talk) 22:05, 30 March 2011 (UTC)
Acceleration and relativity
So using the Newtonian a = F/m it would seem an object could be accelerated to any speed. What is the relativistic equation that is asymptotic at the speed of light? jorgenev (talk) 22:05, 30 March 2011
- Four-force —Preceding unsigned comment added by 92.20.201.71 (talk) 22:51, 30 March 2011 (UTC)
- (edit conflict):Our article Mass in special relativity explains that the apparent mass M at speed v is given by (though this equation is not the best way to look at the situation). The acceleration is thus and gradually reduces towards zero as the speed approaches that of light. Dbfirs 23:00, 30 March 2011 (UTC)
- That is totally wrong, and the article you linked to even includes a quote from einstein about the total vacancy of introducing the quantity . Infact
- —Preceding unsigned comment added by 92.20.201.71 (talk) 00:31, 31 March 2011 (UTC)
- I agree, that's why I said it's not the best way of looking at the situation. I thought that the OP was looking for a simplistic explanation (and first approximation) of why an object cannot accelerate to infinite speed. My equation provides an approximate first improvement on Newton's approximation. Your link provides a better view and your equation is more accurate as v approaches c. Dbfirs 12:47, 31 March 2011 (UTC)
- No, for parallel acceleration and velocity you are out by two powers of gamma. Thus even to a first order correction in power series your correction is out by a factor of 3. That is big, that is like me responding to a question "what is pi?" with the answer "3" and claiming I thought they just wanted an approximation. Besides this your answer also does not support your claim that you were merely intending to provide a first approximation (never mind discussion as to in what way this is a first approximation), if you were providing an approximate answer you should have stated this. There is no benefit in proliferating some kind of lie on some assumed and awkward notion that the OP couldn't handle the truth. —Preceding unsigned comment added by 92.20.201.71 (talk) 02:19, 1 April 2011 (UTC)
- I agree, that's why I said it's not the best way of looking at the situation. I thought that the OP was looking for a simplistic explanation (and first approximation) of why an object cannot accelerate to infinite speed. My equation provides an approximate first improvement on Newton's approximation. Your link provides a better view and your equation is more accurate as v approaches c. Dbfirs 12:47, 31 March 2011 (UTC)
Antimatter, antigravity, spacetime, retrocausality, and antispace
Warning: Risk of cosmological brain spasms or nonexistent headaches
Hi. Does antimatter have positive or negative mass? Assuming it has negative mass, we could depict its effect on the curvature of spacetime as a flat sheet as an object causing an upward dent in this fabric from antigravity, rather than a downward dent produced by normal matter. Using this representation, could we conclude that the collision of a piece of matter and antimatter represents the overlapping of a positive and a negative dent, therby causing the two warping areas to collide and annihilate? Would this be similar to standing waves cancelling out each other, in this case each respective object's mass/antimass, and would this send out gravitational waves? Or, would the idea of each having the other object's respective antigravity cause some kind of gravitational repulsion?
Since spacetime is the modern interpretation for interwoven space and time, would antimatter cause negative time to occur in addition to causing a negative gravitational "space-dent"? Could antimatter fuel thus have the capacity for time travel alongside massive propulsion? Also, considering that antimatter produces antigravity as an assumption, would the graviton theory apply to "negative gravitons" or regular gravitons going inward? If a negative and positive graviton were to intersect, what would ensue?
Creating negative time from antimatter would enable backward flow of time, and in fact there is some preliminary laboratory evidence of retrocausality. In this scenario, do the occurence of future events cause past events, or do the un-occurrence of future events un-cause past events to un-materialize? When a forward-time-flowing mass of matter and a negative-time-flowing negative mass of antimatter collide, do their respective time reflections cause the collision to un-occur, or does time stop before each object collides into the other?
From the relativistic view of one object, it would take an infinite amount of time for the other object to approach whereas it takes very little time to an outside observer. Would this be similar to the theory that time stops for objects entering black holes, which is also proposed by the varying speed of light hypothesis? Or, would this mean that in a quantum mechanics sense, the objects have both simultaneously annihilated and stopped their annhilation but neither outcome has taken place due to the lack of an observer? Does that mean that black holes are the unity of matter and antimatter confined so that their produced energy are converted to mass as time stops the explosive reaction and release of rest energy from taking place? Similarly, could this explain the paradox of an object entering a black hole and coming out in the past in a different trajectory as to knock the original object away from the black hole's path so that the original event could never have taken place, by realizing the past post-entrance object as one quantum half of the original object so that they merge and two digressional paths occur?
Could any event in the universe, even for a fraction of Plank time, cause the black hole-type dent in spacetime to reach so infinitely deep that it comes around on the other side ("around" the ultra-dimensions of the universe, even if flat) and connects into itself like an infinite regression wormhole? Finally, would a "dent" made in space by antimatter cause the object to take up negative space, so that its dimensions are, say, -2 cm in diameter (and would this also cause "in" to be an infinite directional dimension similar to "out", which does not end until the edge of space is reached)? Does this potential for anti-spacetime have any potential implications, or does this hypothetical description reduce relevance to cosmological nonsense? Thanks. ~AH1(TCU) 23:33, 30 March 2011 (UTC)
- Replace "article" with "thread": {{Sub-sections}} Magog the Ogre (talk) 00:16, 31 March 2011 (UTC)
- Unfortunately, none of what you said has any bearing on reality, since as noted in the Antiparticle article, antiparticles (the constituents of antimatter) have the same mass as normal particles, not negative mass. Truthforitsownsake (talk) 00:18, 31 March 2011 (UTC)
- Negative mass (if it existed) would not cause an upward dent in space. An upward dent is the same as a downward dent, because only the intrinsic shape (curvature) matters. Rather, negative mass would cause there to be less space in the middle, instead of more. If you add material in the middle of a sheet, it bulges (up or down). If you remove material, it "pinches". That would be the negative-mass version of those bulgy GR images.
- There is nothing physically "anti" about antimatter. Every kind of particle in nature has a mirror image under a certain symmetry (CPT symmetry), and sometimes one particle of these mirror-image pairs is named "anti-" followed by the name of the other. By analogy, the shapes F and ꟻ are mirror images of each other under ordinary mirror symmetry, and we could call the second one "reversed F" (that is its name in Unicode). But "reversedness" is not a property of the shape itself. It just happens that F is more commonly encountered in everyday life, so it gets the simpler name.
- I'm not aware of any relationship between VSL cosmology and the idea that time stops near a black hole. -- BenRG (talk) 03:31, 31 March 2011 (UTC)
- Also, there's no preliminary laboratory evidence of retrocausality. -- BenRG (talk) 04:35, 31 March 2011 (UTC)
- Hmmm... to be clear, in order for negative mass to be possible, you'd have to be able to draw a line that is straighter than straight? Wnt (talk) 04:55, 31 March 2011 (UTC)
- No, there's no such thing as a line that's straighter than straight, but there is such a thing as spacetime curvature corresponding to negative mass.
- A way to make a crude model of the usual "bulge" is to take a circle of paper, cut out (and discard) a wedge, tape the cut edges together to get a cone, then tape that cone to another piece of paper with a circular hole cut in it (as shown here, but I wouldn't necessarily believe any of the text on that page). To get a model of negative mass you could do the same thing, but adding a wedge instead of removing it. That is, make a radial cut in the circle, insert the wedge you removed from the other circle, tape it at both sides, then try to tape the edge of that to a circular hole in another piece of paper. This doesn't work nearly as well as the cone, and it's not clear that the concept of negative mass actually makes sense, but I think that those two facts are unrelated.
- (It may seem like you're "removing space" when you make the cone and "adding it" when you make the anti-cone, but it's actually the other way around, in the following sense: if you draw a circle on the flat paper around the cone, the area of the paper inside the circle is larger than you'd expect from the circumference; and in the case of the anti-cone it's smaller.) -- BenRG (talk) 08:33, 31 March 2011 (UTC)
- The connection between VSL and time stopping at the event horizon in addition to the experimental evidence of retrocausality are both found in Discover magazine. Perhaps an ultra-straight line would be an anti-geodesic? ~AH1(TCU) 13:07, 31 March 2011 (UTC)
- There's no such thing as an ultra-straight line or an anti-geodesic.
- The retrocausality article is this one, I guess, which describes some sort of delayed-choice experiment. These are old news, and aren't evidence of retrocausality. The VSL article is this one, I guess, from which I learned that João Magueijo does believe that black holes are frozen stars, so I stand corrected. But João Magueijo is not a reliable source of information about the real world.
- Please understand that Discover has to come up with something to entice its readers every single month. When there's no real news about cosmology or quantum mechanics—which there usually isn't—they have to manufacture something. Real evidence for retrocausality or VSL cosmology would change the whole course of theoretical physics. Anything that appears solely in Discover isn't news. -- BenRG (talk) 01:24, 1 April 2011 (UTC)
March 31
Space and matter shortly after the Big Bang
Hi
1. In the early Universe, just after the Big Bang, was there "as much space" as there is now but compressed into a smaller volume, or was there actually "less space"? If there was "as much space" then in what sense was the Universe "smaller"?
2. In the time shortly after the Big Bang, were particles and atoms in some sense actually "smaller" than they are now? Or did the formation of matter have to wait until enough space had been created to contain it?
86.177.108.189 (talk) 00:19, 31 March 2011 (UTC)
- What's the difference?
- There were no atoms. Only a subatomic particle soup. Dauto (talk) 00:33, 31 March 2011 (UTC)
- If there was "as much space" then "as much stuff" could fit into it (e.g. all the atoms that now exist), yet that stuff would be "smaller" in some sense that I do not understand. If there was "less space" then "less stuff" could fit into it. In the latter case, as we get smaller and smaller, eventually there would be no room for the particles in your soup. Then what? Just energy in some other form? 86.177.108.189 (talk) 00:53, 31 March 2011 (UTC)
- (edit conflict) I think I see what you are getting at. There was actually less space; in the sense that the stuff that was not space (matter and energy) was all closer together. The big bang and inflation created the space in which matter and energy organized itself into its current state. See Metric expansion of space and Timeline of the Big Bang and Inflationary epoch and Inflation (cosmology). Your sense is correct; all the "stuff" in the universe was compressed so there was a lot less room, even down to a singularity at the moment of genesis. --Jayron32 03:49, 31 March 2011 (UTC)
- In simple terms, yes. The universe was much, much smaller, and all of the mass-energy was compressed into that very small space. I say mass-energy because at that density it's practically impossible for particles as we know them to exist, and it was all pretty much just high-energy photons. After a while, as the universe expanded, the energy density dropped, and particles started to condense out - starting with the really small ones like quarks and leptons. Check out Timeline of the Big Bang for more info. Confusing Manifestation(Say hi!) 03:45, 31 March 2011 (UTC)
- Atoms were never smaller. But atoms only exist at low temperatures, because it doesn't take much energy to knock the electrons off, and it doesn't take much more than that to knock the nuclei apart. So physics is effectively different at higher temperatures, though the laws are the same. At even higher temperatures, the Higgs field gets knocked out of its nonzero vacuum state, and concepts like "electron" and "photon" break down, though the laws of physics are still the same. At even higher temperatures, nobody has any idea what happens (but I suppose the laws of physics are the same even then, by definition...)
- Generally, things can be smaller at higher temperatures because there are more accessible fermion states. Ordinary matter is hard to compress because all of the low-energy electron states are occupied, and you aren't strong enough to push a substantial fraction of the electrons into higher energy states. But far more compact configurations of matter are physically possible when the energy is available.
- I don't agree with ConMan's response. At high enough temperatures you can pair-produce arbitrary Standard Model particles, so all of the particle types are equally represented in the soup. (And, as I said, at even higher energies the low-energy particle types are meaningless.) I'm also unhappy with the idea that small things condense out first. Things condense out when there's insufficient energy to knock them apart.
- I think the "Timeline of the Big Bang" article is of rather poor quality right now. The "inflationary epoch" is certainly misplaced; it should have no start time, since (1) A.B.B. times only make sense post-inflation, and (2) nobody has the slightest idea how long inflation lasted, nor what the pre-inflationary state might have been. I don't want to rewrite the article, though, because I don't really know very much about high energy physics. -- BenRG (talk) 05:56, 31 March 2011 (UTC)
- Thanks for the replies. I'm still a little confused about how we actually measure the size of things when space is not constant. In principle, could we take a 30cm ruler back to the time when the Universe was 30cm across and find that the ruler only just fitted (ignoring practical complications such as the conditions being too extreme for the ruler to survive)? Let's assume the answer is "yes". Then, over billions of years, space has expanded, but the ruler has stayed the same size? How does that work? Space must be expanding in all places, right, so why isn't it expanding "inside" the ruler, thereby stretching it? (Imagine the ruler is a drawing on the surface of a balloon. As the balloon inflates -- as space expands -- the ruler gets bigger.) This is what I don't understand. Thank you! 86.179.115.14 (talk) 12:58, 31 March 2011 (UTC)
- I will say "yes" to your first question, although most solids vary in size with temperature and no solid can exist at those temperatures. A better answer is that the laws of the Standard Model haven't changed (it's thought) and various length scales can be derived from that. For example, the confinement scale of the strong force is about a femtometer, and that was the same back then. This is how the size of space is defined, essentially—it's the amount of space you'd need now to reproduce similar conditions in the lab. If the physical laws were different, there would be some fuzziness in how much the universe had expanded.
- The reason rulers don't lengthen as the universe expands is the same as the reason they don't lengthen in other circumstances. Rulers are bound together by forces that, for complicated reasons, prefer a certain separation between particles and resist attempts to increase or decrease the separation. The laws of physics don't change, so the preferred separation doesn't change. There's nothing special about the recessional motion associated with the expansion of the universe; it is the same as any other recessional motion as far as the laws of physics are concerned.
- Self-gravitation does act on rulers; it's constantly squeezing them. They don't collapse into black holes because the forces binding the ruler resist compression with a force that roughly follows Hooke's law (everything is like a spring under small enough deformations). Self-gravitation compresses the ruler until the opposing force matches the compression force, and the ruler remains permanently in that equilibrium state. It's slightly smaller than it would be without gravity, but it doesn't get smaller over time. If the cosmological constant is real then it also acts on rulers, trying to pull them apart, but because rulers resist pulling also, the effect is again just a slight change in the equilibrium size (much smaller than the effect of self-gravitation, which is already very small). If there were a pushing/pulling force directly associated with the expansion of the universe (which, I want to stress, there is not—Aristotle was wrong about that), it also would simply change the equilibrium size. -- BenRG (talk) 18:38, 31 March 2011 (UTC)
- Ben, thank you for your very helpful answer. If I could prevail upon you again: At the time when the 30cm ruler only just fitted into the Universe, did it only just fit because it hit a boundary, or "edge", of available space? I'm guessing the answer to this is "no", but if there is no boundary or edge stopping the ruler extending further, then what would prevent us placing a longer ruler in the same Universe, thereby contradicting the proposition that the 30cm ruler only just fitted? 86.179.117.213 (talk) 01:04, 1 April 2011 (UTC)
Shrinking Sun
According to the article Formation and evolution of the Solar System and Future of the Earth, the Sun is getting warmer and brighter by around 10% every 1 billion years because of the helium build-up at its core (nearly half the hydrogen has been consumed). This will wipe out Earth's life even before the time of the Red Giant. Now what the young-earth creationist use as evidence for their young Earth is the proof that the Sun is shrinking at 5 feet/hour. Try googling shrinking Sun. Is it really true? The two statements above seem contradictory. Please tell me which one is right. Aquitania (talk) 00:35, 31 March 2011 (UTC)
- The evidence that the sun is shrinking is not very good, but I think the idea is that the sun is contacting, and therefore getting warmer in its core (since the extra density causes fusion to happen faster). Although like you I would have expected a warmer sun means a bigger sun, I think that's impossible: A bigger core (of the same mass) means lower energy production, so the core can't be any bigger than it is now. (In a red giant the core is small, but the outer layers are large.) Ariel. (talk) 01:11, 31 March 2011 (UTC)
- Each Helium nuclei has half the electric charge and a quarter of the particles of the four protons it replaces. Therefore Sol has less volume (and higher density) and very slightly less mass. Hcobb (talk) 01:34, 31 March 2011 (UTC)
- "...half the electric charge..." yes, but only because you have ignored the 2 positrons released when each of two proton pairs fuses into a deuterium nucleus - there is no overall loss of charge (obviously). "... a quarter of the particles ..." - I don't follow this at all - there are 4 nucleons both before and after fusion. Gandalf61 (talk) 09:24, 31 March 2011 (UTC)
- Gandalf, Hcobb is talking about reducing the number of nuclei which is the number that appears at the ideal gas law PV=nRT, that governs pressure in non-degenerate matter. Dauto (talk) 12:28, 31 March 2011 (UTC)
- And does the core of a star behave like an ideal gas ? As it is a plasma, I would have thought its equation of state would be much more complex. Gandalf61 (talk) 13:02, 31 March 2011 (UTC)
- Gandalf, Hcobb is talking about reducing the number of nuclei which is the number that appears at the ideal gas law PV=nRT, that governs pressure in non-degenerate matter. Dauto (talk) 12:28, 31 March 2011 (UTC)
- "...half the electric charge..." yes, but only because you have ignored the 2 positrons released when each of two proton pairs fuses into a deuterium nucleus - there is no overall loss of charge (obviously). "... a quarter of the particles ..." - I don't follow this at all - there are 4 nucleons both before and after fusion. Gandalf61 (talk) 09:24, 31 March 2011 (UTC)
- Each Helium nuclei has half the electric charge and a quarter of the particles of the four protons it replaces. Therefore Sol has less volume (and higher density) and very slightly less mass. Hcobb (talk) 01:34, 31 March 2011 (UTC)
- Yes, the core of a main sequence star does behave like an ideal gas. where is proportional to the number of particles per molecular weight . The quantities , , and are the hydrogen, helium, and metalicity mass fraction respectively. So hydrogen contributes two particles (a proton and an electron) per nuclei (which has a molecular mass equal to one): , helium contributes three particles (a nucleus and two electrons) per nuclei (which has a molecular mass equal to 4): , and metals contribute (n+1) particles (a nucleus and n electrons) per nuclei (which has a molecular mass equal to 2n): . Dauto (talk) 15:17, 31 March 2011 (UTC)
- When was the last time young earth creationist were right about anything? Dauto (talk) 03:27, 31 March 2011 (UTC)
- The problem with that arguement, is that young earth creationists assume that that trend can be extended indefinitely backwards in time. This kind of error is sadly not uncommon. Plasmic Physics (talk) 07:32, 31 March 2011 (UTC)
Size of the universe
How big is the universe? — Preceding unsigned comment added by JoshuaDonald (talk • contribs) 04:36, 31 March 2011 (UTC)
- We don't know. It could be infinitely large, or perhaps has finite limits but which the laws of physics do not allow us to probe. See Universe#Size.2C_age.2C_contents.2C_structure.2C_and_laws and Shape of the universe and Observable universe for some extended content on this matter. --Jayron32 04:39, 31 March 2011 (UTC)
Would I be able to donate extra skin and fat cells for $?
As I was in Germany as a toddler, I can't donate blood. (After over 20 years of not being in Europe, I clearly don't have CJD, but it'll take a lot to get that through the FDA's thick heads.)
As I'm 11-13 lbs. overweight, and aware of how organs are sold for money, what about donating my extra skin and fat cells to anyone who may need it? Where do I go to get this to happen, and how much $ would I earn per lb.?
Other than that, what CAN I donate (that will replenish/regenerate, so no kidneys, for example) that will still net me some funds? --70.179.169.115 (talk) 11:26, 31 March 2011 (UTC)
- I think you're out of luck. Dauto (talk) 12:24, 31 March 2011 (UTC)
- Doesn't somebody need skin grafts at any point in time? Also, if fat tissue has been burned, that would need replacement too, right? --70.179.169.115 (talk) 13:18, 31 March 2011 (UTC)
- For your second question you might be able to sell blood plasma and gametes (the second is easier for males then females). Googlemeister (talk) 13:15, 31 March 2011 (UTC)
- Gametes? Okay then, where is the closest gamete donation center to 66502, please? --70.179.169.115 (talk) 13:18, 31 March 2011 (UTC)
- As an aside, I will note that the latent period of CJD infection can run into multiple decades, with some speculation that it may take up to 50 years for symptoms to appear. TenOfAllTrades(talk) 15:13, 31 March 2011 (UTC)
- The restrictions on donors with vCJD are borderline paranoia, given that the number of total cases is vanishingly small and the impending epidemic never happened. The restrictions on blood donation are restrictive because people are still paranoid about disease risks, and it leads them to refuse life-saving treatments. Better to deal with their fears ahead of time. I'm not aware of adipose tissue donation. Skin donation is almost entirely either autografts (i.e. from one spot on the patient to another) or from cadavers, and has the same restriction on European residence anyway. Semen/oocyte donation, as of 2005, now has the same restriction unlesss you're giving for someone that knows you and they're notified of the potential risk up front. You can't donate a kidney for money in the US anyway. There's a blood test for vCJD which has been proven on paper, but it'll probably be at least several years before it's commercially available, since getting it to work is one thing, nailing down specificity and sensitivity to a decent level is another entirely. For the record, routine blood donors are not paid (again, volunteers are felt to be safer). Plasma donation is paid in the US, even though the World Health Organization frowns on that practice. SDY (talk) 16:52, 31 March 2011 (UTC)
- Out of interest here are the precautions taken in the UK against transmission of CJD in donated blood. A far worse disaster in the UK was the use of blood imported from US prisons in the 1980s. Alansplodge (talk) 18:32, 31 March 2011 (UTC)
- We have an article on that topic, though it looks like the UK-specific article is yet to be written. People got scared for a reason. What's sad is that some of this same issue was repeated in China, but there it was shared needles resulting in something like a quarter of a million HIV infections (again, shortcuts for economic reasons). There it was the donors, haven't heard anything about the recipients. Modern processing techniques are fairly thorough, but I wouldn't be surprised if some slipped through. SDY (talk) 19:18, 31 March 2011 (UTC)
- Out of interest here are the precautions taken in the UK against transmission of CJD in donated blood. A far worse disaster in the UK was the use of blood imported from US prisons in the 1980s. Alansplodge (talk) 18:32, 31 March 2011 (UTC)
- The restrictions on donors with vCJD are borderline paranoia, given that the number of total cases is vanishingly small and the impending epidemic never happened. The restrictions on blood donation are restrictive because people are still paranoid about disease risks, and it leads them to refuse life-saving treatments. Better to deal with their fears ahead of time. I'm not aware of adipose tissue donation. Skin donation is almost entirely either autografts (i.e. from one spot on the patient to another) or from cadavers, and has the same restriction on European residence anyway. Semen/oocyte donation, as of 2005, now has the same restriction unlesss you're giving for someone that knows you and they're notified of the potential risk up front. You can't donate a kidney for money in the US anyway. There's a blood test for vCJD which has been proven on paper, but it'll probably be at least several years before it's commercially available, since getting it to work is one thing, nailing down specificity and sensitivity to a decent level is another entirely. For the record, routine blood donors are not paid (again, volunteers are felt to be safer). Plasma donation is paid in the US, even though the World Health Organization frowns on that practice. SDY (talk) 16:52, 31 March 2011 (UTC)
Obsolete or speculative physical theories
Are speculative physical theories that don't make any predictions that can easily be tested still considered to be "scientific"? Are obsolete physical theories considered to be unscientific? I ask because in this thread an editor is convinced that Einstein-Cartan theory is some combination of "wildly speculative", "not science", and "pseudoscience". In the end, he says it's mathematics, not physics. To me, that doesn't seem fair to established speculative physical theories (e.g., Brans-Dicke theory, string theory, quantum gravity). But I'm a mathematician, not an empirical scientist. I'd like a broader view on this question. Sławomir Biały (talk) 12:25, 31 March 2011 (UTC)
- It is relevant to point out that our definition of hypothesis says "For a hypothesis to be put forward as a scientific hypothesis, the scientific method requires that one can test it." Even our article on theory says "Such theories are preferably described in such a way that any scientist in the field is in a position to understand, verify, and challenge (or "falsify") it." Keep in mind these are fairly narrow definitions, and alternate formulations end up being more about philosophy of science than about science per se.
- The work of applied mathematicians, theoretical physicists and their ilk often falls through the cracks of easy-to-formulate definitions of science. Certainly marking string theory as 'pseudoscience' would be perverse. Though I am not that familiar with this notion of Torsion field physics, some of the views at the talk page constitute extremely hard-line bias towards empiricism as the only valid form of science. Consider this: lack of obvious testable predictions does not mean a proposition or theory is not falsifiable. If a case can be made for falsifiability, then you have a good claim that the theory is scientific under the Popperian scheme of science. SemanticMantis (talk) 15:22, 31 March 2011 (UTC)
- Slightly off-topic, but: In general relativity you can think of continuous mass distributions (the stuff that appears in the stress-energy tensor) as a continuum limit of a bunch of tiny nonrotating black holes in vacuum. If they're rotating, the continuum limit has torsion. So it's easy to argue that Einstein–Cartan theory is more natural than general relativity, since it doesn't impose an arbitrary constraint on black holes in the continuum limit. The difference between Einstein–Cartan theory and GR is too small to be tested, but neither theory is to blame for that. If you wanted to discard one theory, it would have to be on the basis of Occam's razor. GR has simpler math, but E–C appears to me to have fewer arbitrary assumptions. Newtonian gravity has simpler math than GR, but GR has fewer arbitrary assumptions. So this argument would seem to favor E–C gravity. I suppose the broader point is that the testability of a theory depends somewhat on what alternatives are available. Every theory makes many predictions that aren't testable (because we don't have any labs on distant planets, for example). That doesn't matter until a rival theory comes along that predicts the same result in a lab on Earth but a different result on another planet. Suddenly the untestability of the distant-planet prediction becomes a problem. It's not fair to blame the new theory for that just because it was invented later. -- BenRG (talk) 23:20, 31 March 2011 (UTC)
Temperature induced nuclear fission
How do I calculate the theoretical ratio of free nucleons to nuclei in a nuclear plasma, as a function of temperature, pressure, and muclear binding energy? Plasmic Physics (talk) 12:56, 31 March 2011 (UTC)
- I don't understand your question. could you elaborate? Dauto (talk) 00:49, 1 April 2011 (UTC)
At the temperature increases for a electromagnetic plasma gas, a new type of plasma develops. I say plasma gas, because a plasma is not a distinct phase like a solid or liquid, as a table salt is considered a solid example of a plasma. This plasma is a nuclear plasma gas - in a nuclear plasma gas, nuclear fission of normally stable nuclei is induced. In this process, the binding energy is overcome by the thermal energy. Since temperature is equivalent to the average thermal energy of a bulk sample, not all nuclei would have energies over the threshold required for nulear fission to be induced. In addition to this, there is a continueum of discrete fission products ranging from no fission, to individual nucleons. So, it is fair to say that across a change in temperature, a gradient of proportion should exist for a specific fission product. Plasmic Physics (talk) 01:37, 1 April 2011 (UTC)
Isn't there an anti-hunger pill anywhere?
This question has been removed. Per the reference desk guidelines, the reference desk is not an appropriate place to request medical, legal or other professional advice, including any kind of medical diagnosis or prognosis, or treatment recommendations. For such advice, please see a qualified professional. If you don't believe this is such a request, please explain what you meant to ask, either here or on the talk page discussion (if a link has been provided). --TenOfAllTrades(talk) 01:03, 1 April 2011 (UTC)
Green Laser
I have one 20mW green laser pointer. It does not burn matches (as I daydreamed) yet gives a slight sensation of heat on skin. It works on 3 AAA batteries (alkaline). My question is that if I add more voltage will it increase in power, say burn paper etc. Jon Ascton (talk) 14:10, 31 March 2011 (UTC)
- No. Excessive voltage will simply destroy the laser diode. Roger (talk) 17:00, 31 March 2011 (UTC)
- Not something that personally interests me but since it's something I've seen in sites I visit I believe red lasers tend to be far more cost effective if you just want something that will light matches. I believe you can get random Chinese laser of indeterminate power that will nevertheless light matches for around US$30 presuming it can get thru customs. While you can get green and other colour lasers that will do the job, their primary advantage to the hobbyist would be for looks. I presume you're already aware such a laser as yours is very dangerous (probably (3B) and could easily blind anyone who views the light directly and already have appropriate safety goggles. Nil Einne (talk) 17:24, 31 March 2011 (UTC)
- Avoid using Class III and Class IV lasers in your home! Your basic assumptions about safety are Just Not Good Enough! Powerful lasers can scintillate, reflect obliquely, and behave in nonintuitive ways. A proper optical laboratory will take much more precaution far beyond just "don't look into the laser beam." You need the laser to be firmly mounted on an optical bench where it can not shine anywhere unexpected. You need the work area (and the rest of the room) to be totally nonreflective; avoid specular reflective surfaces, avoid certain materials in the furniture and walls, and so forth. Even diffuse reflection of powerful laser light can cause permanent eye damage. By definition, Class III and Class IV lasers can cause you physical harm - and most can cause permanent damage faster than it takes you to blink or avert your eyes. Playing with lasers is like juggling knives - fun for a while, but your first "minor accident" will cause permanent and irreparable injury/damage. If you like powerful lasers, get involved with an optical research laboratory and learn the safety procedures, just like the experts do. Nimur (talk) 20:56, 31 March 2011 (UTC)
- You can also use a laser from a DVD burner. Instructions here. — DanielLC 20:27, 31 March 2011 (UTC)
Identifying an old timey flying machine
I'm trying to find the identity or history of what I believe is a (failed) pre-Wright flying machine. It's well known to pop culture because it appears as stock footage in many, many movies and television shows, but I know nothing about it so I can only describe it visually.
It appears as though someone has taken an old car and attached a giant parasol to a vertical shaft through the center of the car. There's some sort of engine 'pumping' the parasol up and down. Apparently the principle is that air will be pushed to the sides during the up-stroke but downwards during the down-stroke.
Of course, in the familiar stock footage, the car does not fly. It just sort of bounces up and down on its shocks. I don't think its wheels even leave the ground.
Thanks APL (talk) 16:53, 31 March 2011 (UTC)
- Was it the Flugan? --Jayron32 17:21, 31 March 2011 (UTC)
- Or is it the first machine in this clip? Alansplodge (talk) 17:44, 31 March 2011 (UTC)
- Here is some video of the machine in question. It is called the "John Pitts Skycar". This is the patent for its unique form of "flight". --Sean 17:43, 31 March 2011 (UTC)
- Well done sir! A different movie clip of the same beast (with sound) here. On the upstroke the 60 vanes making up the "parasol" opened and on the downstroke they closed, hopefully creating downforce. Not enough apparently. It appears on our List of aircraft (P-Q) but there is no article yet. Alansplodge (talk) 17:45, 31 March 2011 (UTC)
- Wow. Thank you. That's exactly what I was looking for.
- I didn't even realize that the parasol "propeller" actually rotated as well as oscillated up and down. APL (talk) 18:16, 31 March 2011 (UTC)
- That's a big engine under the thing. If they'd just hit on the standard helicopter rotor, I wonder if it could have taken off. (no comment on what would come afterward...) Wnt (talk) 20:01, 31 March 2011 (UTC)
- That device probably had a poor power to weight ratio. I wonder if a modern engine could get that contraption to work? Googlemeister (talk) 21:11, 31 March 2011 (UTC)
- That's a big engine under the thing. If they'd just hit on the standard helicopter rotor, I wonder if it could have taken off. (no comment on what would come afterward...) Wnt (talk) 20:01, 31 March 2011 (UTC)
What is fertilising the blossoming shrubs in England?
I have not seen any bees around, or any other insects for that matter, at this time of year. So what is fertilizing all the blossoms please? Thanks 92.29.127.125 (talk) 19:21, 31 March 2011 (UTC)
- Just because you haven't noticed any bees or other insects doesn't mean they aren't around. Also, just because there are blossoms doesn't mean anything has been fertilised. The blossoms attract the insects to fertilise them so the plant can produce seeds. It's seeds that are proof of fertilisation, not blossoms (and even then some plants can produce seeds without being fertilised by insects). --Tango (talk) 19:28, 31 March 2011 (UTC)
- Surely bees pollinate, not fertilize? APL (talk) 20:21, 31 March 2011 (UTC)
- The terminology is fine: fertilisation "is the fusion of gametes to produce a new organism." Bees are the vector of fertilization for many plants. "Fertilizing" in the sense of supplying nutrients to a plant is the spurious usage. SemanticMantis (talk) 20:26, 31 March 2011 (UTC)
- Surely bees pollinate, not fertilize? APL (talk) 20:21, 31 March 2011 (UTC)
- Plenty of bumblebees up here in Edinburgh. I assume if it's warm enough for them in Scotland, it's warm enough in England. 86.135.222.99 (talk) 21:59, 31 March 2011 (UTC)
- We have an article on Pollination which explains quite a bit. There are some plants which don't even require other organisms to pollinate them, but also many other creatures other then bees can pollinate, including butterflies, moths, wasps, flies and beetles, even ants. Vespine (talk) 22:17, 31 March 2011 (UTC)
April 1
milk
will putting milk thru a coffee filter remove radioactive iodine — Preceding unsigned comment added by Wdk789 (talk • contribs) 00:59, 1 April 2011 (UTC)
why not — Preceding unsigned comment added by Wdk789 (talk • contribs) 01:29, 1 April 2011 (UTC)
- Because iodine in milk doesn't form into large particles the size of coffee grounds. StuRat (talk) 01:36, 1 April 2011 (UTC)
- The idea is that you can't separate radioactive iodine from normal iodine whithout the use of some very expensive equipment. Secondly, iodine is removed by chemical means which essentialy ruins the milk, rendering it undrinkable in any case. Plasmic Physics (talk) 01:41, 1 April 2011 (UTC)
what about a laboratory filter? — Preceding unsigned comment added by Wdk789 (talk • contribs) 01:45, 1 April 2011 (UTC)
- I asked this here, and apparently it's hard to filter iodine. You could freeze the milk for about 2 months and 99.5% of the radioactive iodine will be gone by then. 70% will be gone after 2 weeks. Ariel. (talk) 01:54, 1 April 2011 (UTC)
- To give an idea, as I've just added to the article, coffee filters pass particles under about 10 to 15 micrometers. Now by comparison iodine has a Van der Waals radius of 198 picometers (1.98 Angstroms). 1 micrometer = 1000 nanometers = 1 000 000 picometers, so the holes in a coffee filter are about 76,000 times larger than an iodine atom. Wnt (talk) 02:04, 1 April 2011 (UTC)
- As stued rat says, the iodine in milk is not present as crystals that can be filtered, it is dissolved. Similiarly, you can't filter table salt out of solution. Be carefull with your understanding of what filtration is. Plasmic Physics (talk) 02:13, 1 April 2011 (UTC)
- Perhaps I should offer a bit more background for clarity. It's very common in research to encounter a .22 micron (220 nanometer) filter, which is still 1000 times larger than the iodine atom. By that point it gets quite hard to pass large amounts of fluid (depending of course on the amount of sediment). At smaller sizes molecular sieves are used, but generally in a different way - because it's no longer practical to wait for everything to pass through, instead they delay the molecules that can pass through them as they're dripped through in chromatography. When you get down to that scale, you generally rate them by the size of the molecule that can go through, such as 1000 daltons. Iodine is smaller than even that! Animals are equipped with gap junctions that work more like traditional filters though, because the cells with them are only 4 nm apart, the time delay isn't a big deal. (There are also tight junctions between cells that work like filters with a size that sometimes can be regulated).
- But when you get down the the size of atoms, materials made out of atoms are weird to filter with. You can see ion channels set to pass specific sizes, but which won't pass anything larger or smaller than what they're set for. There's even a specific iodide channel in the thyroid,[12] but alas we don't have an article for it. And if you go smaller than that - well, a filter that passes half of one of the smaller atoms won't pass anything; besides, any two surfaces half an atom apart are either going to spread out and accept solvent between them, or stick together and be held by Van der Waals forces.
- The talk of biological channels suggests a possible practical solution, though I don't know if it works: live kelp and other seaweeds absorb iodide into themselves with great avidity, and one could hope that they might suck up radioactive iodide if left in milk for some time (before, presumably, dying) ... unfortunately you have to have a source of clean, live seaweed to start with! Wnt (talk) 02:50, 1 April 2011 (UTC)
Our nearest neighbouring solar system
What is the nearest solar system to our own, and based on present technologies, how long would it take for us to send astronauts there? Flaming Ferrari (talk) 01:13, 1 April 2011 (UTC)
- About 40,000 years with our currently fastest spaceships, if I recall correctly. --Belchman (talk) 01:32, 1 April 2011 (UTC)
- According to this 2006 article, Epsilon Eridani is the next stop for the most intrepid real estate agent, a mere 10.5 light years away. However, our article states that the planet is "unconfirmed". Clarityfiend (talk) 01:31, 1 April 2011 (UTC)
- The Proxima Centauri system is closest, but we have no way, with our current technology, to send astronauts there (alive). Also, we don't know if planets are present there. StuRat (talk) 01:34, 1 April 2011 (UTC)
- I'm not an expert, but doesn't a solar system require a system of orbiting bodies, not just a star(s). Ergo, does a triple star with no suspected planets (Proxima Centauri) qualify? Plasmic Physics (talk) 01:45, 1 April 2011 (UTC)
- I don't think we would be able to detect small planets. And how about asteroids, comets, etc ? What precisely is required to be a solar system ? StuRat (talk) 03:26, 1 April 2011 (UTC)
amount of carbon created in the early universe
There's a 12-year-old prodigy who's got doubts about an aspect of big bang theory (check Google news today). Can anybody suggest what he means by this? (particularly the last two paragraphs -- the first grafs are fairly common):
"There are two different types of when stars end. When the little stars die, it's just like a small poof. They just turn into a planetary nebula. But the big ones, above 1.4 solar masses, blow up in one giant explosion, a supernova," Jake said. "What it does, is, in larger stars there is a larger mass, and it can fuse higher elements because it's more dense."
"So you get all the elements, all the different materials, from those bigger stars. The little stars, they just make hydrogen and helium, and when they blow up, all the carbon that remains in them is just in the white dwarf; it never really comes off.
"So, um, in the big-bang theory, what they do is, there is this big explosion and there is all this temperature going off and the temperature decreases really rapidly because it's really big. The other day I calculated, they have this period where they suppose the hydrogen and helium were created, and, um, I don't care about the hydrogen and helium, but I thought, wouldn't there have to be some sort of carbon?"
"Otherwise, the carbon would have to be coming out of the stars and hence the Earth, made mostly of carbon, we wouldn't be here. So I calculated, the time it would take to create 2 percent of the carbon in the universe, it would actually have to be several micro-seconds. Or a couple of nano-seconds, or something like that. An extremely small period of time. Like faster than a snap. That isn't gonna happen."
"Because of that," he continued, "that means that the world would have never been created because none of the carbon would have been given 7 billion years to fuse together. We'd have to be 21 billion years old . . . and that would just screw everything up."63.17.54.2 (talk) 03:33, 1 April 2011 (UTC)