Talk:Drake equation
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This article in the press
This article is linked to in this press article: Man Uses Math to Explain Girlfriend Woes Samboy (talk) 05:22, 14 January 2010 (UTC)
So this is just a guess? —Preceding unsigned comment added by AdbMonkey (talk • contribs) 13:22, 26 October 2010 (UTC)
Wrong equation for R*
The equation
ignores the fact that all stars have a finite lifespan, as they will either undergo a supernova or become a white dwarf. In fact, our Galaxy is known to have multiple generations of stars, and not a single "first-generation" star (i.e. population III) has yet been discovered. Furthermore, assigning an age to a galaxy is rather ambiguous, since it is now known that galaxies (especially large ones) have undergone many mergers with other galaxies. Thus it can said that the age of all galaxies is (nearly) the age of the Universe.
Wrong statement for L
RM below about L to talk. If L is the length of time such civilizations release detectable signals into space then Grote Reber and radio astronomy have nothing to do with this value, his antenna was a receiver, not a transmitter. Maybe the example should date back to the Invention of radio. Fountains of Bryn Mawr (talk) 00:23, 4 March 2010 (UTC)
- The value of L can be estimated from the lifetime of our current civilization from the advent of radio astronomy in 1938 (dated from Grote Reber's parabolic dish radio telescope) to the current date. In 2009, this gives an L of 71 years. However such an assumption would be erroneous. 71 for the value of L would be an artificial minimum based on Earth's broadcasting history to date and would make unlikely the possibility of other civilizations existing. 10,000 for L is still the most popular estimate.
Current estimate of fl
In the "Current estimates of the parameters" section, it says that Drake estimated fl to be 1, whereas a couple other guys more recently estimated it to be 0.13. However, in the two sections that calculate N based on the current estimates (both at the bottom of the "Historical estimates" section and the bottom of the "Current estimates" section), a value of 0.33 is used for fl. Where did 0.33 come from? Should an explanation should be added regarding how 0.33 was derived, or should we be using 0.13 in our current estimate calculation of N? SnottyWong talk 21:29, 19 April 2010 (UTC)
Mayr vs Sagan out? Michael Crichton in?
Hello
The late Ernst Mayr was the most famous biologist at our times, especially in the theory of evolution which is most relevant here, and he criticised the SETI project in various occasions. I find the discussion he had with Carl Sagan, one of the fathers of SETI especially enlightening and that is why I added it. Now the current section about critics of the SETI project contains a cite of Michael Crichton, a science fiction writer and removed the Mayr link. With all due respect to Mr. Crichton but I think the critics of Ernst Mayr is far more relevant. One of his arguments, which he clearly emphasised as being speculative is based on the fact that of the many species on earth, which might be in the billions, only one developed intelligence. Now the wording of the paragraph I added can be changed of course and rephrased, but leaving Crichton in and Mayr out, seems to me sort of ridiculous. Oub (talk) 12:52, 28 April 2010 (UTC):
- Mayr's argument is actually fallacious. The reason only one species on Earth developed a technological intelligence is that there is only one niche per planet for such a species. Reflect on the fate of the Neanderthals. WolfmanSF (talk) 22:57, 2 October 2010 (UTC)
factor missing in the equation?
In the equation appear the factors
:fc = the fraction of civilizations that develop a technology that releases detectable signs of their existence into space :L = the length of time such civilizations release detectable signals into space.
It might be, that such civilization existed for 1 million years, that would produce a good result of calculation for N.
But if that happened 100 million years ago, and 99 million years ago that civilization disappeared, we cannot communicate. Should a "factor of same time" be added to the equation? Is there anything in the literature? --Hans W (talk) 15:14, 14 August 2010 (UTC)
εEarth is not obtainable from Drake equation parameters
It is not true that εEarth = fp x ne (where εEarth is the the fraction of stars with Earth-like planets). Consider an extreme but illustrative example. If fp = 0.01 (only 1% of stars have planets) and ne = 100 (each of those stars has 100 Earthlike planets), then εEarth = 0.01, but fp x ne = 1.0. You need to know the statistical distribution of ne to calculate εEarth. WolfmanSF (talk) 23:13, 2 October 2010 (UTC)
R* is the number of stars in the galaxy?
I'm not sure why this article emphasizes the number of stars formed per year, without multiplying that number by the number of years the galaxy has been forming stars! This matter is explained somewhat in the subsection "Alternative expression" but later ignored in the "Current estimates of the parameters" section. The result is that the first three terms of the right hand side give the number of earth-like planets formed per year. The end result, 2.31 civilizations, is an absurdly low estimate. The original Drake equation was: where the first term on the right-hand side is the number of stars in the galaxy. is on the order of 200 to 400 billion, not 7. I have edited the "Current estimates" section with the estimates made by James Kasting in his book "How To Find A Habitable Planet". 70.112.186.143 (talk) 03:23, 10 October 2010 (UTC) Eric
offensive anthropocentrism
I'm taking issue with the text
- fi = the fraction of the above that actually go on to develop intelligent life. Estimated by Drake as 0.01 based on little or no evidence. This value remains particularly controversial. Pessimists such as Ernst Mayr point out that of the billions of species that have existed on Earth, only one has become intelligent[18] and infer a tiny value for fi.
the view that Earth has only one intelligent species is ridiculous and offensive. in fact it harbours several very intelligent species. this aspect of the controversy has not been exposed in the article. some versions of the drake equation, however, do make the distinction between intelligence and technological advancement as different factors. -- 99.233.186.4 (talk) 01:43, 13 November 2010 (UTC)
- Hm, please name another intelligence species on this planet! In order to prevent a fight over the word intelligence, the basic motivation of the Drake equations is to communicate. So instead of looking for an intelligent species one could say a species which posses a language with a full developed grammar, so I am curious which species do you have in mind? Oub (talk) 17:45, 16 November 2010 (UTC):
Current estimates of the parameters: Mayr (POV)
The actual subsection the fraction of the above that actually go on to develop intelligent life reads
- Estimated by Drake as 0.01 based on little or no evidence. This value remains particularly controversial. Pessimists such as Ernst Mayr point out that of the billions of species that have existed on Earth, only one has become intelligent[18] and infer a tiny value for fi. Optimists note the generally increasing complexity of life and conclude that the eventual appearance of intelligence might be inevitable, meaning fi=1.[19]
several remarks:
- Mayr was a very famous biologist that should be mentioned.
- He is denoted as a pessimist, that is clearly POV , it would be more accurate to call him realist but I think it is best to drop any label.
- Now [19] is cited presenting a counterargument. first of all it is written by enrico , is this any known or even famous biologist? Besides in this article it not claimed that fi=1.
Given all that I suggest to drop pessimist for Mayr and drop the link to enrico. Oub (talk) 22:01, 18 November 2010 (UTC):
- Famous is true, but irrelevant. Especially in this field, where little is known for sure, famous does not guarantee anything. (Einstein, clearly a famous physicist, said God does not play games with dice, but the consensus now is that he was wrong...).
- Also, I provided a very solid reference to "Generally increasing complexity of life". Even if you object to some other reference, please do not remove this one. There is no doubt that many SETI folks have set the probability to 1 (that's what Meyr is objecting to....), based on (among others) this argument. So adding a "citation needed" is as far as you should go in this area.
- Finally, it's not POV to summarize the two conclusions and the arguments behind them. Even though you, personally, may feel one is much stronger than the other, both have been used in the field, so they should remain. Removing, or minimizing, one of them only, is quite POV by itself. LouScheffer (talk) 19:14, 21 November 2010 (UTC)
- Re: LouScheffer thanks for your answer. To make this clear: Both estimates about the value of fi should be mentioned. I only objected to the version Mayr vs Enrico. The second reference you inserted is solid enough, however I would prefer to leave out the first one, but I don' want to make a war about it. The formulation which I feel uneasy about it, is the word pessimist, that in my opinion is too strong and too biased, what's about skeptic instead of pessimist. Oub (talk) 11:24, 22 November 2010 (UTC):
- The current meaning of 'pessimist' is someone who is pessimistic about making contact (for any one of a number of reasons). In this sense Mayr is definitely a pessimist, as I think he would agree. Similarly, 'optimists' are those who are optimistic about the chances of making contact, or at least about intelligence evolving. I personally think 'skeptic' is better reserved for those who believe all such calculations are unreliable at best, as opposed to those who are skeptical of making contact. Maybe we could say 'Contact pessimists' and 'contact optimists' or just replace it with the more bland 'some' and 'others'. LouScheffer (talk) 03:22, 23 November 2010 (UTC)
- Re: LouScheffer hm Mayr is dead, so we can't ask him. I strongly recommend not to use pessimist or optimist but some and others. Oub (talk) 14:21, 23 November 2010 (UTC):