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最小的系外行星列表

维基百科，自由的百科全书
开普勒-37系统中的行星和太阳系中天体的大小比较。

以下是迄今为止发现的最小的 系外行星列表，就有形的大小，按半径排序。但其中一些未经证实和/或仍有争议。

列表

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 本表是动态列表，或许永远不会完结。欢迎您参考可靠来源来查漏补缺。

以地球半径为单位列出行星半径（R地球）。所有列出的系外行星都小于地球，最大为0.7地球半径。NASA系外行星档案（英语：NASA Exoplanet Archive）是最主要的数据来源[1][2]。

系外行星 半径 （R地球） 注解和参考资料
SDSS J1228+1040 b
(SDSS J122859.92+104033.0 b, WD 1226+110 b) 		0.0101+0.0504
−0.0085 		Extrasolar planetesimal. Remnant iron core.[3]
PSR B1828-11 b 0.016 Unconfirmed, controversial[1]
Ceres 0.07466 Shown for comparison
WD 1145+017 b ~0.15 Extrasolar planetesimal.[4]
Pluto 0.1825 Shown for comparison
Moon 0.2739 Shown for comparison
Kepler-37b 0.296±0.037 Smallest known exoplanet.[5]
Kepler-1520b ~0.3 Disintegrating planets with poorly known radii, all thought to be smaller than Mercury.[6][7]
KOI-2700b
K2-22b
PSR B1257+12 b (Draugr) ~0.338 Least massive known exoplanet, at 0.02 Earth masses. Radius estimated from mass-radius relationship.[8]
Kepler-37e 0.37±0.18 Dubious[9]
Mercury 0.3825 Shown for comparison
Kepler-444b 0.403+0.016
−0.014 		[10]
Kepler-102b 0.47±0.02
Kepler-444c 0.497+0.021
−0.017 		[10]
Kepler-1971b (KOI-4777.01) 0.51±0.03 [11]
Kepler-1308b 0.52+0.06
−0.05
Kepler-138b 0.522±0.032
Kepler-444d 0.530+0.022
−0.019 		[10]
Mars 0.5314 Shown for comparison
Kepler-62c 0.54±0.03
Kepler-444e 0.546+0.017
−0.015 		[10]
KOI-115.03 (Kepler-105d) 0.55+0.08
−0.07 		Unconfirmed[12]
Kepler-42d 0.57±0.18
Kepler-102c 0.58±0.02
KOI-1843.03 0.59 Unconfirmed
Kepler-1583b 0.60+0.09
−0.05
Kepler-1087b 0.61+0.17
−0.05
K2-89b 0.615±0.080
Kepler-1877b 0.624
Kepler-1371c 0.64+0.07
−0.05
UCF-1.02 0.64 Dubious[13][14]
Kepler-1130d 0.645
Kepler-1351b 0.65+0.05
−0.04
Kepler-1542c 0.65+0.09
−0.06
UCF-1.01 0.65 Dubious[13][14]
Kepler-271d 0.66±0.05
Kepler-431c 0.668
Kepler-1558b 0.68+0.06
−0.04
K2-116b 0.69±0.04
Kepler-141b 0.69±0.05
K2-297b (EPIC 201497682 b) 0.692+0.059
−0.048
LHS 1678 b 0.696±0.044
Kepler-1349b 0.700+0.630
−0.110
Kepler-378c 0.70±0.05
K2-266c 0.705+0.096
−0.085
Kepler-1339b 0.71+0.06
−0.04
Gliese 367 b 0.718±0.054 Smallest known exoplanet within 10 parsecs.

相关条目

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参考资料

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  1. ^ 1.0 1.1 Staff. Exoplanet Catalog. Extrasolar Planets Encyclopaedia. 10 July 2017 [10 July 2017]. （原始内容存档于2012-07-05）. 
  2. ^ Planetary Systems Composite Data. NASA Exoplanet Archive. [12 December 2021]. （原始内容存档于2020-10-07）. 
  3. ^ Planet SDSS J1228+1040 b. exoplanet.eu. [2019-08-05]. （原始内容存档于2019-10-19）. 
  4. ^ Vanderburg, Andrew; John Asher Johnson; Rappaport, Saul; Bieryla, Allyson; Irwin, Jonathan; John Arban Lewis; Kipping, David; Brown, Warren R.; Dufour, Patrick; Ciardi, David R.; Angus, Ruth; Schaefer, Laura; Latham, David W.; Charbonneau, David; Beichman, Charles; Eastman, Jason; McCrady, Nate; Wittenmyer, Robert A.; Wright, Jason T. A disintegrating minor planet transiting a white dwarf. Nature. 2015, 526 (7574): 546–549. Bibcode:2015Natur.526..546V. PMID 26490620. S2CID 4451207. arXiv:1510.06387 可免费查阅. doi:10.1038/nature15527. 
  5. ^ Simukoff, E.; et al. Below One Earth Mass: The Detection, Formation, and Properties of Subterrestrial Worlds. Space Science Reviews. 2013, 180 (1–4): 71. Bibcode:2013SSRv..180...71S. S2CID 118597064. arXiv:1308.6308 可免费查阅. doi:10.1007/s11214-013-0019-1. 
  6. ^ Ansdell, M.; Hirano, T.; Gaidos, E. Monitoring of the D doublet of neutral sodium during transits of two 'evaporating' planets. Monthly Notices of the Royal Astronomical Society. 2019, 485 (3): 3876–3886. arXiv:1903.06217 可免费查阅. doi:10.1093/mnras/stz693. [...]the radii are not known but are thought to be smaller than Mercury (0.36R⊕). 
  7. ^ Garai, Z. Light-curve analysis of KOI 2700b: The second extrasolar planet with a comet-like tail. Astronomy & Astrophysics. 2018, 611: A63. Bibcode:2018A&A...611A..63G. S2CID 118885868. arXiv:1712.07461 可免费查阅. doi:10.1051/0004-6361/201629676. We confirmed the disintegrating-planet scenario of KOI 2700b. 
  8. ^ Exoplanet-catalog. [2022-11-28]. （原始内容存档于2022-02-10）. 
  9. ^ Rajpaul, V. M.; Buchhave, L. A.; Lacedelli, G.; Rice, K.; Mortier, A.; Malavolta, L.; Aigrain, S.; Borsato, L.; Mayo, A. W.; Charbonneau, D.; Damasso, M.; Dumusque, X.; Ghedina, A.; Latham, D. W.; López-Morales, M.; Magazzù, A.; Micela, G.; Molinari, E.; Pepe, F.; Piotto, G.; Poretti, E.; Rowther, S.; Sozzetti, A.; Udry, S.; Watson, C. A., A HARPS-N mass for the elusive Kepler-37d: A case study in disentangling stellar activity and planetary signals, Monthly Notices of the Royal Astronomical Society, 2021, 507 (2): 1847–1868, arXiv:2107.13900 可免费查阅, doi:10.1093/mnras/stab2192 
  10. ^ 10.0 10.1 10.2 10.3 Campante, T.; et al. KOI-3158: The oldest known system of terrestrial-size planets. EPJ Web of Conferences. 2015, 101: 02004. Bibcode:2015EPJWC.10102004C. S2CID 16191462. arXiv:1501.07869 可免费查阅. doi:10.1051/epjconf/201510102004. 
  11. ^ Cañas, Caleb I.; Mahadevan, Suvrath; Cochran, William D.; Bender, Chad F.; Feigelson, Eric D.; Harman, C. E.; Kopparapu, Ravi Kumar; Caceres, Gabriel A.; Diddams, Scott A.; Endl, Michael; Ford, Eric B.; Halverson, Samuel; Hearty, Fred; Jones, Sinclaire; Kanodia, Shubham; Lin, Andrea S. J.; Metcalf, Andrew J.; Monson, Andrew; Ninan, Joe P.; Ramsey, Lawrence W.; Robertson, Paul; Roy, Arpita; Schwab, Christian; Stefánsson, Guđmundur. A Hot Mars-sized Exoplanet Transiting an M Dwarf. The Astronomical Journal. 2022, 163 (1): 3. Bibcode:2022AJ....163....3C. S2CID 244954104. arXiv:2112.03958 可免费查阅. doi:10.3847/1538-3881/ac3088. 
  12. ^ Kepler-105. NASA Exoplanet Archive. [12 December 2021]. 
  13. ^ 13.0 13.1 Stevenson, Kevin B.; et al. A Hubble Space Telescope Search for a Sub-Earth-sized Exoplanet in the GJ 436 System. The Astrophysical Journal. 2014, 796 (1). 32. Bibcode:2014ApJ...796...32S. S2CID 118412895. arXiv:1410.0002 可免费查阅. doi:10.1088/0004-637X/796/1/32. 
  14. ^ 14.0 14.1 Lanotte, A. A.; et al. A global analysis of Spitzer and new HARPS data confirms the loneliness and metal-richness of GJ 436 b. Astronomy and Astrophysics. 2014, 572. A73 [2022-11-28]. Bibcode:2014A&A...572A..73L. S2CID 55405647. arXiv:1409.4038 可免费查阅. doi:10.1051/0004-6361/201424373. （原始内容存档于2022-10-06）. 
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