Gliese 581 d: Difference between revisions
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| period = | | period = 66.8 ± 0.14<ref name="mayor" /><ref name="udry">{{cite journal|url=http://cdsads.u-strasbg.fr/cgi-bin/nph-bib_query?2007A%26A...469L..43U&db_key=AST&nosetcookie=1|title=The HARPS search for southern extra-solar planets. XI. Super-Earths (5 and 8 M<sub>⊕</sub>) in a 3-planet system|author=Udry, S.; Bonfils, X.; Delfosse, X.; Forveille, T.; Mayor, M.; Perrier, C.; Bouchy, F.; Lovis, C.; Pepe, F.; Queloz, D.; Bertaux, J.-L.|journal=[[Astronomy and Astrophysics]]|volume=469|issue=3|year=2007|pages=L43 – L47|doi=10.1051/0004-6361:20077612|accessdate=2008-08-18}}</ref> | ||
| semimajor = 0. | | semimajor = 0.22<ref name="mayor" /> | ||
| eccentricity = 0. | | eccentricity = 0.38 ± 0.09<ref name="mayor" /> | ||
| arg_peri = 295 ± 28<ref name="udry" /> | | arg_peri = 295 ± 28<ref name="udry" /> | ||
| semi_amp = 2.52 ± 0.17<ref name="udry" /> | | semi_amp = 2.52 ± 0.17<ref name="udry" /> | ||
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| minimum_mass_earth = 7. | | minimum_mass_earth = 7.09<ref name="mayor" /> | ||
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{{Planetbox discovery | {{Planetbox discovery | ||
Revision as of 22:54, 21 April 2009
Template:Planetbox begin Template:Planetbox image Template:Planetbox star Template:Planetbox orbit Template:Planetbox character Template:Planetbox discovery Template:Planetbox reference Template:Planetbox end
Gliese 581 d (Template:Pron-en) is an extrasolar planet approximately 20 light-years away in the constellation of Libra. Because of its mass, the planet is classified as a super-Earth planet. In late April 2009 new observations by the original discovery team concluded that the planet is within the habitable zone where liquid water could exist.
Discovery
The planet was discovered by the team of Stéphane Udry of the Geneva Observatory in Switzerland using the HARPS instrument on the European Southern Observatory 3.6 meter telescope in La Silla, Chile on 24 April 2007. Udry's team employed the radial velocity technique, in which the size and mass of a planet are determined based on the small perturbations it induces in its parent star’s orbit via gravity.[1]
The team is confident that the planet exists but recognizes that unlikely events could mimic its existence. They believe the issue will be settled by upcoming studies.
Dynamical simulations of the Gliese 581 system assuming that the orbits of the three planets are coplanar show that the system becomes unstable if its component masses are so high as to correspond to an overall inclination angle of 10° or less.[2] For Gliese 581 d, the upper bound of its mass must be half that of 581 b; that is, 581 d's maximum is 44 Earth masses.[3] At this mass it must be held together with a central heavy-element core like Saturn and maybe even HD 149026 b.
Climate and habitability
It was originally thought that Gliese 581 d orbits outside the theoretical habitable zone of its star. However, further studies released in April of 2009 confirmed that the planet is within the habitable zone where liquid water could exist. According to Stephan Udry " d could be covered by a deep ocean, it is the first serious waterworld candidate."“Gliese 581 d is probably too massive to be made only of rocky material, but we can speculate that it is an icy planet that has migrated closer to the star,” .[4][5] Scientists originally believed that Gliese 581 d would be too cold for liquid water to exist, and therefore could not support life in forms as existing on Earth. However, since Earth's temperature would be about -18°C[6] without any greenhouse gases, and due to a theorized greenhouse effect of Gliese 581 d, research now suggests that atmospheric conditions on the planet could create temperatures at which liquid water can exist, and therefore the planet may be capable of supporting life.[7][8][9]
On 21 April 2009, ESO announced, together with the discovery of Gliese 581 e, that they had refined the models of Gliese 581 d's orbit, discovering it lay well within the habitable zone.[10][11]
References
- ↑ Cite error: Invalid
<ref>tag; no text was provided for refs namedudry - ↑ Beust, H. et al. (2008). "Dynamical evolution of the Gliese 581 planetary system". Astronomy and Astrophysics 479 (1): 277–282. doi:. http://cdsads.u-strasbg.fr/cgi-bin/nph-bib_query?2008A%26A...479..277B&db_key=AST&nosetcookie=1. Retrieved on 2008-08-20.
- ↑ Dividing the m sin i by "Sin(10/180 * PI)" on a radian-configured processor.
- ↑ SPACE.com - Hopes Dashed for Life on Distant Planet
- ↑ von Bloh, W.; Bounama, C.; Cuntz, M.; Franck, S. (2007). "The Habitability of Super-Earths in Gliese 581". Astronomy & Astrophysics 476: 1365 – 1371. doi:. http://cdsads.u-strasbg.fr/cgi-bin/nph-bib_query?2007A%26A...476.1365V&db_key=AST&nosetcookie=1. Retrieved on 2008-08-18.
- ↑ "Global Warming Frequently Asked Questions". Lwf.ncdc.noaa.gov. 2008-05-08. http://lwf.ncdc.noaa.gov/oa/climate/globalwarming.html#q1. Retrieved on 2009-01-18.
- ↑ http://arxiv.org/abs/0712.3219v4
- ↑ "Centauri Dreams » Blog Archive » Gliese 581d: A Habitable World After All?". Centauri-dreams.org. 2007-12-13. http://www.centauri-dreams.org/?p=1625. Retrieved on 2009-01-18.
- ↑ Posted at 12:06 AM in Space Exploration (2007-06-15). "New 'Super Earth 2' Discovered in Constellation Libra". Dailygalaxy.com. http://www.dailygalaxy.com/my_weblog/2007/06/another_super_e.html. Retrieved on 2009-01-18.
- ↑ "Lightest exoplanet yet discovered". eso.org. 2009-04-21. http://www.eso.org/public/outreach/press-rel/pr-2009/pr-15-09.html. Retrieved on 2009-04-21.
- ↑ Mayor et al. (2009). "The HARPS search for southern extra-solar planets,XVIII. An Earth-mass planet in the GJ 581 planetary system". Astronomy and Astrophysics. http://obswww.unige.ch/~udry/Gl581_preprint.pdf.
External links
Template:Gliese 581 Template:Sky
ca:Gliese 581 d cy:Gliese 581 d de:Gliese 581 d es:Gliese 581 d fr:Gliese 581 d ko:글리제 581 d id:Gliese 581 d it:Gliese 581 d lt:Gliese 581 d nl:Gliese 581 d ja:グリーゼ581d no:Gliese 581#Gliese 581 d pl:Gliese 581 d pt:Gliese 581 d ru:Глизе 581 d fi:Gliese 581 d sv:Gliese 581 d