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I do not think that this is correct. The center of the Milky Way lies in the direction of Sagittarius (see Sgr A*). Could use more location information (local neighborhood, maybe?) and something less colloquial than "spin up".
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Because the companion to PSR J1719-1438 is planet sized, made primarily of carbon (with an unknown amount of oxygen), and is very dense, it may be similar to a very large diamond. In the science press, the object has been called the [[Carbon planet|"Diamond Planet"]]<ref name=UniverseToday>{{cite web|title=Star Transforms Into A Diamond Planet|url=http://www.universetoday.com/88449/star-transforms-into-a-diamond-planet|work=Universe Today|accessdate=8/26/2011}}</ref><ref name=Space.com>{{cite web|title=Surprise! Alien Planet Made of Diamond Discovered|url=http://www.space.com/12731-diamond-alien-planet-discovered-neutron-star.html|work=Space.com|accessdate=8/25/2011}}</ref><ref name= MaxPlanck>{{cite web|title=A Planet made of Diamond|url=http://www.mpifr-bonn.mpg.de/public/pr/pr-pulsar-august2011-en.html|work=Max Planck Institut for Radio Astronomy|accessdate=8/26/2011}}</ref>.
Because the companion to PSR J1719-1438 is planet sized, made primarily of carbon (with an unknown amount of oxygen), and is very dense, it may be similar to a very large diamond. In the science press, the object has been called the [[Carbon planet|"Diamond Planet"]]<ref name=UniverseToday>{{cite web|title=Star Transforms Into A Diamond Planet|url=http://www.universetoday.com/88449/star-transforms-into-a-diamond-planet|work=Universe Today|accessdate=8/26/2011}}</ref><ref name=Space.com>{{cite web|title=Surprise! Alien Planet Made of Diamond Discovered|url=http://www.space.com/12731-diamond-alien-planet-discovered-neutron-star.html|work=Space.com|accessdate=8/25/2011}}</ref><ref name= MaxPlanck>{{cite web|title=A Planet made of Diamond|url=http://www.mpifr-bonn.mpg.de/public/pr/pr-pulsar-august2011-en.html|work=Max Planck Institut for Radio Astronomy|accessdate=8/26/2011}}</ref>.

==See also==
* [[EF Eridani]], a star system with a compact star and a degraded planetary-mass former star


==References==
==References==

Revision as of 04:43, 30 August 2011

PSR J1719-1438 is a millisecond pulsar with a spin period of 5.7 ms located about 4000 ly from Earth in the direction of Serpens.[1][2] Millisecond pulsars are generally thought to begin as normal pulsars and then spin up by accreting matter from a binary companion.

Diamond planet

Timing measurements of PSR J1719-1438 show that it has a low-mass companion: PSR J1719-1438 b. The companion has a mass similar to that of Jupiter, but at about 40% of the diameter. It orbits the pulsar with a period of 2.17 hours at a distance of around 600,000 km (0.89 solar radii).[1] The companion is likely the remnants of a star whose outer layers were siphoned off by the more massive pulsar. Calculations show the companion has a minimum density of 23 grams per cubic centimeter and is probably a ultra-low mass carbon-oxygen white dwarf.[1]

Because the companion to PSR J1719-1438 is planet sized, made primarily of carbon (with an unknown amount of oxygen), and is very dense, it may be similar to a very large diamond. In the science press, the object has been called the "Diamond Planet"[2][3][4].

See also

  • EF Eridani, a star system with a compact star and a degraded planetary-mass former star

References

  1. ^ a b c Bailes, M. " Transformation of a Star into a Planet in a Millisecond Pulsar Binary". Science. doi:10.1126/science.1208890. {{cite journal}}: Unknown parameter |coauthors= ignored (|author= suggested) (help)
  2. ^ a b "Star Transforms Into A Diamond Planet". Universe Today. Retrieved 8/26/2011. {{cite web}}: Check date values in: |accessdate= (help)
  3. ^ "Surprise! Alien Planet Made of Diamond Discovered". Space.com. Retrieved 8/25/2011. {{cite web}}: Check date values in: |accessdate= (help)
  4. ^ "A Planet made of Diamond". Max Planck Institut for Radio Astronomy. Retrieved 8/26/2011. {{cite web}}: Check date values in: |accessdate= (help)