Kepler-20b: Difference between revisions
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{{Short description|Mini-Neptune orbiting Kepler-20}} |
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{{Planetbox begin |
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{{Infobox planet |
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| name = Kepler-20b |
| name = Kepler-20b |
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| discoverer = Kepler team |
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| apsis = astron |
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| mean_radius = {{val|1.868|+0.066|-0.034}} {{Earth radius|link=y}} |
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| mass = {{val|9.7|+1.41|-1.44}} <ref>{{cite journal |arxiv=1608.06836 |doi=10.3847/0004-6256/152/6/160 |title=A 1.9 Earth Radius Rocky Planet and the Discovery of a Non-Transiting Planet in the Kepler-20 System |year=2016 |last1=Buchhave |first1=Lars A. |last2=Dressing |first2=Courtney D. |last3=Dumusque |first3=Xavier |last4=Rice |first4=Ken |last5=Vanderburg |first5=Andrew |last6=Mortier |first6=Annelies |last7=Lopez-Morales |first7=Mercedes |last8=Lopez |first8=Eric |last9=Lundkvist |first9=Mia S. |last10=Kjeldsen |first10=Hans |last11=Affer |first11=Laura |last12=Bonomo |first12=Aldo S. |last13=Charbonneau |first13=David |last14=Cameron |first14=Andrew Collier |last15=Cosentino |first15=Rosario |last16=Figueira |first16=Pedro |last17=Fiorenzano |first17=Aldo F. M. |last18=Harutyunyan |first18=Avet |last19=Haywood |first19=Raphaëlle D. |last20=Johnson |first20=John Asher |last21=Latham |first21=David W. |last22=Lovis |first22=Christophe |last23=Malavolta |first23=Luca |last24=Mayor |first24=Michel |last25=Micela |first25=Giusi |last26=Molinari |first26=Emilio |last27=Motalebi |first27=Fatemeh |last28=Nascimbeni |first28=Valerio |last29=Pepe |first29=Francesco |last30=Phillips |first30=David F. |s2cid=216077870 |journal=The Astronomical Journal |volume=152 |issue=6 |page=160 |bibcode=2016AJ....152..160B |display-authors=29 |doi-access=free }}</ref> {{Earth mass|link=y}} |
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| density = {{val|8.2|+2.0|-2.7}} [[gram|g]] [[cubic centimetre|cm<sup>−3</sup>]] |
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| single_temperature = {{convert|1014|K|C F}} |
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}} |
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'''Kepler-20b''' is an [[Extrasolar planet|exoplanet]] orbiting [[Kepler-20]] in a system 922 light years from Earth.<ref>{{Cite web|title=Exoplanet-catalog|url=https://exoplanets.nasa.gov/exoplanet-catalog/1594/kepler-20-b/|access-date=2021-10-05|website=Exoplanet Exploration: Planets Beyond our Solar System}}</ref> It is classified as a [[Super-Earth]], as it has a radius and mass greater than that of [[Earth]]. At about 1.87 {{Earth radius}}, it would most likely be a [[Mini-Neptune]], but its high mass of 9.7 {{Earth mass}} implies that it is an iron-rich rocky world. Along with the other four planets in the system, Kepler-20b was announced on 20 December 2011. |
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{{Planetbox star |
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==References== |
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| constell = [[Lyra]] |
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{{Reflist|refs= |
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| RA = {{RA|19|10|47.524}} |
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| DEC = {{DEC|+42|20|19.30}} |
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| dist_pc = {{val|290|30}} |
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| app_mag = 12.51 |
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| mass = {{val|0.912|0.035}} |
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| radius = {{val|0.944|+0.06|-0.095}} |
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| temperature = {{val|5466|93}} |
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| metallicity = {{val|0.02|0.04}} |
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| age = {{val|8.8|+4.7|-2.7}} |
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}} |
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{{Planetbox character |
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| radius_earth = {{val|1.868|+0.066|-0.034}} |
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| mass_earth = {{val|8.7|+2.1|-2.2}} |
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| density_cgs = {{val|8.2|+2.0|-2.7}} |
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| temperature = {{val|1014}} |
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}} |
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{{Planetbox orbit |
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{{Planetbox discovery |
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| discoverers = Kepler team |
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| detection_methods = Radial velocity |
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| discovery_status = Conference announcement |
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}} |
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{{Planetbox end}} |
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'''Kepler-20b''' is an [[Extrasolar planet|exoplanet]] orbiting [[Kepler-20]]. Its radius is about twice that of [[Earth]], with a mass around 9.7 [[Earth mass]]es. It has a higher density compared to earth. Along with the other four planets in the system, Kepler-20b was announced on 20 December 2011. |
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{{Kepler-20|state=uncollapsed}} |
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[[Category:Exoplanets discovered in 2011]] |
[[Category:Exoplanets discovered in 2011]] |
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[[Category: |
[[Category:Kepler-20|B]] |
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[[Category:Exoplanets discovered by the Kepler space telescope|20b]] |
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[[Category:Super-Earths]] |
[[Category:Super-Earths]] |
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{{Extrasolar-planet-stub}} |
{{Extrasolar-planet-stub}} |
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http://arxiv.org/pdf/1608.06836v1.pdf |
Latest revision as of 17:16, 29 October 2023
Discovery | |
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Discovered by | Kepler team |
Discovery date | 20 December 2011 |
Transit (Kepler Mission) | |
Orbital characteristics | |
0.04537 AU | |
Eccentricity | <0.32 |
3.6961219 d | |
Inclination | 86.50+0.36 −0.31 |
Star | Kepler-20 (KOI-070) |
Physical characteristics | |
1.868+0.066 −0.034 R🜨 | |
Mass | 9.7+1.41 −1.44 [1] ME |
Mean density | 8.2+2.0 −2.7 g cm−3 |
Temperature | 1,014 K (741 °C; 1,366 °F) |
Kepler-20b is an exoplanet orbiting Kepler-20 in a system 922 light years from Earth.[2] It is classified as a Super-Earth, as it has a radius and mass greater than that of Earth. At about 1.87 R🜨, it would most likely be a Mini-Neptune, but its high mass of 9.7 ME implies that it is an iron-rich rocky world. Along with the other four planets in the system, Kepler-20b was announced on 20 December 2011.
References
[edit]- ^ Buchhave, Lars A.; Dressing, Courtney D.; Dumusque, Xavier; Rice, Ken; Vanderburg, Andrew; Mortier, Annelies; Lopez-Morales, Mercedes; Lopez, Eric; Lundkvist, Mia S.; Kjeldsen, Hans; Affer, Laura; Bonomo, Aldo S.; Charbonneau, David; Cameron, Andrew Collier; Cosentino, Rosario; Figueira, Pedro; Fiorenzano, Aldo F. M.; Harutyunyan, Avet; Haywood, Raphaëlle D.; Johnson, John Asher; Latham, David W.; Lovis, Christophe; Malavolta, Luca; Mayor, Michel; Micela, Giusi; Molinari, Emilio; Motalebi, Fatemeh; Nascimbeni, Valerio; Pepe, Francesco; et al. (2016). "A 1.9 Earth Radius Rocky Planet and the Discovery of a Non-Transiting Planet in the Kepler-20 System". The Astronomical Journal. 152 (6): 160. arXiv:1608.06836. Bibcode:2016AJ....152..160B. doi:10.3847/0004-6256/152/6/160. S2CID 216077870.
- ^ "Exoplanet-catalog". Exoplanet Exploration: Planets Beyond our Solar System. Retrieved 2021-10-05.