GD 61
GD 61 is a white dwarf star. It is 150 light-years from Earth in the constellation Perseus.[1] [2][3] The star has a planetary system. It may once have been a main sequence star of spectral type A0V with around three times the mass of the Sun. It has aged and passed through a red giant phase. What was left is a dense hot remnant. This remnant has around 70% of the Sun's mass and a surface temperature of 17280 K. It is thought to be around 600 million years old. This age includes both its life as a main sequence star, and as a white dwarf stellar remnant.[4] It has an apparent magnitude of 14.8.[1] GD 61 was first noted as a potential degenerate star in 1965. This was done in a survey of white dwarf suspects by astronomers from the Lowell Observatory in Arizona.[5]
An asteroid in the system was detected in 2013 that contains water. This was the first finding of solid or liquid water on an extrasolar body. The asteroid, the first extrasolar asteroid detected, is 26% water by mass, close to the water content of Ceres. This means that a planet, with a rocky surface similar to Earth's, may have existed in the past. The asteroid could be an artifact from this period. It is now possibly part of a debris field from that planet's breakup. Such a planet would have had both a rocky surface and water. These are two key ingredients for life.[6][7][8] The researchers used the Cosmic Origins Spectrograph on the Hubble Space Telescope to determine what it is made of. The elements magnesium, silicon, iron and oxygen were detected. These are all components of rocky planets. However, the amount of oxygen is much higher than what was expected. There was also less carbon than expected. This meant there was one possible reason for the extra oxygen. There had to be water there.[7]
Related pages
change- 24 Themis, the first Solar System asteroid found to have liquid water
References
change- ↑ 1.0 1.1 S. Xu (许偲艺) and M. Jura (2012). "Spitzer Observations of White Dwarfs: The Missing Planetary Debris around DZ Stars". The Astrophysical Journal. 745 (1): 88–102. arXiv:1109.4207. Bibcode:2012ApJ...745...88X. doi:10.1088/0004-637X/745/1/88. S2CID 118755550.
- ↑ "GD 61 -- White Dwarf". SIMBAD Astronomical Database. Centre de Données astronomiques de Strasbourg. Retrieved 20 October 2013.[permanent dead link]
- ↑ Rosen, Meghan (13 October 2013). "Water seen in rubble around star". ScienceNews. Retrieved 14 October 2013.
- ↑ Farihi, J.; Brinkworth, C. S.; Gänsicke, B. T.; Marsh, T. R.; Girven, J.; Hoard, D. W.; Klein, B.; Koester, D. (2011). "Possible Signs of Water and Differentiation in a Rocky Exoplanetary Body". The Astrophysical Journal Letters. 728 (1): L8–L13. arXiv:1101.0158. Bibcode:2011ApJ...728L...8F. doi:10.1088/2041-8205/728/1/L8. S2CID 46224877.
{{cite journal}}: CS1 maint: multiple names: authors list (link) - ↑ Giclas, Henry L.; Burnham, Robert; Thomas, Norman Gene (1965). "A list of white dwarf suspects I : special objects of small proper motion from the Lowell survey" (PDF). Bulletin / Lowell Observatory. 6 (6): 155–64. Bibcode:1965LowOB...6..155G.
{{cite journal}}: CS1 maint: multiple names: authors list (link) - ↑ Sterling, Nate (12 October 2013). "Scientists discover water-rich asteroid orbiting dead star GD 61 outside our solar system". Pentagon Post. Archived from the original on 13 October 2013. Retrieved 12 October 2013.
- ↑ 7.0 7.1 "Watery asteroid discovered in dying star points to habitable exoplanets". Phys.org. 10 October 2013. Retrieved 12 October 2013.
- ↑ Mack, Eric (17 October 2011). "Newly spotted wet asteroids point to far-flung Earth-like planets | Crave - CNET". News.cnet.com. Retrieved 12 October 2013.