Categories
  Encyclosphere.org ENCYCLOREADER
  supported by EncyclosphereKSF

List of smallest exoplanets

From Wikipedia - Reading time: 7 min

A size comparison of the planets in the Kepler-37 system and objects in the Solar System

Below is a list of the smallest exoplanets so far discovered, in terms of physical size, ordered by radius.

List

[edit]
This is a dynamic list and may never be able to satisfy particular standards for completeness. You can help by adding missing items with reliable sources.

The sizes are listed in units of Earth radii (R🜨). All planets listed are smaller than Earth and Venus, up to 0.7 Earth radii. The NASA Exoplanet Archive is used as the main data source.[1][2]

Exoplanet Radius (R🜨) Notes and references
SDSS J0845+2257 b 0.01-0.013 Planetesimal, enhanced in iron and silicates. [3]
WD 1145+017 b ~0.03[4] Disintegrating planetesimal, likely one of several orbiting its star. Likely about one-tenth the mass of Ceres and ~200 km in radius.[4]
Ceres 0.0742 Shown for comparison
Pluto 0.1863 Shown for comparison
Moon 0.2725 Shown for comparison
Kepler-37b 0.3098+0.0059
−0.0076 		Smallest known exoplanet.[5][6]
BD+05 4868 Ab ~0.314 Disintegrating planet, radius is just an estimate.[7]
PSR B1257+12 b (Draugr) ~0.338 Least massive known exoplanet, at 0.02 Earth masses. Radius estimated from mass-radius relationship.[8]
Kepler-1520b ≲0.36 Disintegrating planets with poorly known radii, all thought to be smaller than Mercury.[9][10]
KOI-2700b
K2-22b
Mercury 0.3826 Shown for comparison
Kepler-879c 0.4±0.1 [11]
Kepler-444b 0.403+0.016
−0.014 		[12]
Ganymede 0.413 Shown for comparison
Kepler-158d 0.43±0.05 [11]
Kepler-102b 0.460±0.026 [6]
Kepler-444c 0.497+0.021
−0.017 		[12]
Kepler-1971b (KOI-4777.01) 0.51±0.03 [13]
Kepler-1489c 0.51±0.08 [11]
Kepler-1994b 0.51+0.06
−0.05 		[14]
Kepler-1308b 0.52+0.06
−0.05
Kepler-444d 0.530+0.022
−0.019 		[12]
Mars 0.5325 Shown for comparison
Kepler-62c 0.54±0.03
Kepler-444e 0.546+0.017
−0.015 		[12]
Gliese 238 b 0.566±0.014 [15]
Kepler-102c 0.567±0.028 [6]
Kepler-42d 0.57±0.18
Kepler-1583b 0.60+0.09
−0.05
Kepler-1998b 0.6+0.08
−0.04 		[16]
Kepler-963c 0.6±0.2 [11]
Kepler-1087b 0.61+0.17
−0.05
K2-89b 0.615±0.080
Kepler-1877b 0.624
K2-137b 0.64±0.10[17] The discovery paper finds a larger radius of 0.89±0.09 R🜨[18]
Kepler-1371c 0.64+0.07
−0.05
Kepler-138b 0.64±0.02 [19]
Kepler-1130d 0.645
Kepler-1351b 0.65+0.05
−0.04
Kepler-1542c 0.65+0.09
−0.06
Kepler-271d 0.66±0.05
Kepler-431c 0.668
Kepler-1558b 0.68+0.06
−0.04
LHS 1678 b 0.685+0.037
−0.035 		[20]
K2-116b 0.69±0.04
Kepler-141b 0.69±0.05
K2-297b (EPIC 201497682 b) 0.692+0.059
−0.048
Gliese 367 b (Tahay) 0.699±0.024 Smallest known exoplanet within 10 parsecs.[21]
Kepler-2003b (KOI-4978.02) 0.7±0.1 [11]
Kepler-378c 0.70±0.05

Excluded objects

[edit]

Kepler-37e is listed with a radius of 0.37±0.18 R🜨 in the Exoplanet Archive based on KOI data, but the existence of this planet is doubtful,[22] and assuming its existence, a 2023 study found a mass of 8.1±1.7 M🜨, inconsistent with such a small radius.[23]

KOI-6705.01, listed as a potential very small planet in the KOI dataset, was shown to be a false positive in 2016.[24]

Candidate planets

[edit]

Below shows a list candidate planets below 0.7 R🜨. These planets have yet to be confirmed.

Kepler object of interest Radius (R🜨) Notes and references
SDSS J1228+1040 b
(SDSS J122859.92+104033.0 b, WD 1226+110 b) 		0.010+0.0504
−0.0085[25][26] 		Extrasolar planetesimal. Likely a remnant iron core. Radius is in the range of 1.2 – 120 km.[25] Has been disputed in a 2023 publication.[27]
KOI-4582.01 0.35[28]
KOI-2298.03 0.36[28]
KIC 1718360.01 0.366[29]
KOI-2169.04 0.37[28]
KOI-7174.01 0.37[28]
KOI-8012.01 0.42[28]
KOI-6860.01 0.43[28]
KOI-2059.02 0.44[28]
KOI-304.02 0.46[28]
KOI-7793.01 0.46[28]
KOI-2678.02 0.48[28]
KOI-6631.01 0.48[28]
KOI-2421.02 0.48[28]
KOI-5974.01 0.49[28]
KOI-3444.03 0.5[28]
KOI-2295.01 0.52[28]
KOI-7863.01 0.52[28]
KOI-2612.02 0.53[28]
KOI-4657.01 0.54[28]
KOI-8257.01 0.54[28]
KOI-115.03 (Kepler-105d) 0.55+0.08
−0.07 		[30]
KOI-2421.01 0.55[28]
KOI-4097.02 0.55[28]
KOI-7645.01 0.55[28]
KOI-3208.01 0.56[28]
KOI-6763.01 0.56[28]
KOI-2859.03 0.57[28]
KOI-4146.02 0.57[28]
KOI-2859.04 0.57[28]
KOI-7873.01 0.57[28]
TOI-4307.02 0.57±0.14[31]
KOI-2657.01 0.58[28]
KOI-8277.01 0.58[28]
KOI-4296.01 0.59[28]
KOI-3196.01 0.59[28]
KOI-5692.01 0.59[28]
KOI-1964.01 0.6[28]
KOI-4407.01 0.6[28]
KOI-4871.01 0.6[28]
KOI-5211.01 0.6[28]
KOI-7888.01 0.6[28]
KOI-3184.03 0.6[28]
KOI-8183.01 0.6[28]
KOI-3083.02 0.61[28]
KOI-4421.01 0.61[28]
KOI-4716.01 0.61[28]
KOI-3102.01 0.61[28]
KOI-7032.01 0.61[28]
KOI-1843.03 0.61+0.12
−0.08 		[32]
KOI-1499.02 0.62[28]
KOI-605.02 0.62[28]
KOI-7676.01 0.62[28]
KOI-4849.01 0.62[28]
KOI-365.02 0.62[28]
KOI-7116.01 0.62[28]
KOI-4421.02 0.62[28]
KOI-7949.01 0.62[28]
KOI-2029.04 0.63[28]
KOI-6889.01 0.63[28]
KOI-2636.02 0.63[28]
KOI-3248.01 0.64[28]
KOI-5213.01 0.64[28]
KOI-6276.01 0.64[28]
KOI-7617.01 0.64[28]
KOI-7903.01 0.64[28]
KOI-7925.01 0.64[28]
KOI-8174.01 0.64[28]
KOI-3083.03 0.65[28]
KOI-4875.01 0.65[28]
KOI-4808.01 0.65[28]
KOI-6568.01 0.65[28]
KOI-1619.01 0.66[28]
KOI-3111.02 0.66[28]
KOI-2859.05 0.66[28]
KOI-3017.01 0.67[28]
KOI-4907.01 0.67[28]
KOI-1616.02 0.67[28]
KOI-6299.01 0.67[28]
KOI-8211.01 0.67[28]
KOI-2593.02 0.68[28]
KOI-4605.01 0.68[28]
KOI-7832.01 0.68[28]
KOI-7483.01 0.68[28]
KOI-2623.02 0.68[28]
KOI-7924.01 0.68[28]
KOI-7628.01 0.69[28]
KOI-4129.01 0.69[28]
KOI-4822.01 0.69[28]
KOI-6600.01 0.69[28]

See also

[edit]

References

[edit]
  1. ^ Staff (10 July 2017). "Exoplanet Catalog". Extrasolar Planets Encyclopaedia. Retrieved 10 July 2017.
  2. ^ "Planetary Systems Composite Data". NASA Exoplanet Archive. Retrieved 16 July 2023.
  3. ^ Wilson, D. J.; Gänsicke, B. T.; Koester, D.; Toloza, O.; Pala, A. F.; Breedt, E.; Parsons, S. G. (2015). "The composition of a disrupted extrasolar planetesimal at SDSS J0845+2257 (Ton 345)". Monthly Notices of the Royal Astronomical Society. 451 (3): 3237–3248. arXiv:1505.07466. doi:10.1093/mnras/stv1201.
  4. ^ a b Rappaport, S.; Gary, B. L. (June 2016). "Drifting asteroid fragments around WD 1145+017". Monthly Notices of the Royal Astronomical Society. 458 (4): 3904–3917. arXiv:1602.00740. Bibcode:2016MNRAS.458.3904R. doi:10.1093/mnras/stw612.
  5. ^ Simukoff, E.; et al. (2013). "Below One Earth Mass: The Detection, Formation, and Properties of Subterrestrial Worlds". Space Science Reviews. 180 (1–4): 71. arXiv:1308.6308. Bibcode:2013SSRv..180...71S. doi:10.1007/s11214-013-0019-1. S2CID 118597064.
  6. ^ a b c Bonomo, A. S.; Dumusque, X.; et al. (September 2023). "Cold Jupiters and improved masses in 38 Kepler and K2 small planet systems from 3661 HARPS-N radial velocities. No excess of cold Jupiters in small planet systems". Astronomy & Astrophysics. 677: A33. arXiv:2304.05773. Bibcode:2023A&A...677A..33B. doi:10.1051/0004-6361/202346211. S2CID 258078829.
  7. ^ Hon, Marc; Rappaport, Saul; Shporer, Avi; Vanderburg, Andrew; Collins, Karen A.; Watkins, Cristilyn N.; Schwarz, Richard P.; Barkaoui, Khalid; Yee, Samuel W. (2025-01-09). "A Disintegrating Rocky Planet with Prominent Comet-like Tails Around a Bright Star". arXiv:2501.05431.
  8. ^ "Exoplanet-catalog".
  9. ^ Ansdell, M.; Hirano, T.; Gaidos, E. (2019). "Monitoring of the D doublet of neutral sodium during transits of two 'evaporating' planets". Monthly Notices of the Royal Astronomical Society. 485 (3): 3876–3886. arXiv:1903.06217. Bibcode:2019MNRAS.485.3876G. doi:10.1093/mnras/stz693. [...]the radii are not known but are thought to be smaller than Mercury (0.36R⊕).
  10. ^ Garai, Z. (2018). "Light-curve analysis of KOI 2700b: The second extrasolar planet with a comet-like tail". Astronomy & Astrophysics. 611: A63. arXiv:1712.07461. Bibcode:2018A&A...611A..63G. doi:10.1051/0004-6361/201629676. S2CID 118885868. We confirmed the disintegrating-planet scenario of KOI 2700b.
  11. ^ a b c d e Wang, Kaitlyn; Ge, Jian; et al. (November 2024). "Discovery of small ultra-short-period planets orbiting Kepler KG dwarfs with GPU phase folding and deep learning". Monthly Notices of the Royal Astronomical Society. 534 (3): 1913–1927. arXiv:2312.17382. Bibcode:2024MNRAS.534.1913W. doi:10.1093/mnras/stae2155.
  12. ^ a b c d Campante, T.; et al. (2015). "KOI-3158: The oldest known system of terrestrial-size planets". EPJ Web of Conferences. 101: 02004. arXiv:1501.07869. Bibcode:2015EPJWC.10102004C. doi:10.1051/epjconf/201510102004. S2CID 16191462.
  13. ^ 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, GuÄ‘mundur (2022). "A Hot Mars-sized Exoplanet Transiting an M Dwarf". The Astronomical Journal. 163 (1): 3. arXiv:2112.03958. Bibcode:2022AJ....163....3C. doi:10.3847/1538-3881/ac3088. S2CID 244954104.
  14. ^ "Kepler-1994". NASA Exoplanet Archive. Retrieved 16 June 2023.
  15. ^ Tey, Evan; Shporer, Avi; et al. (May 2024). "GJ 238 b: A 0.57 Earth Radius Planet Orbiting an M2.5 Dwarf Star at 15.2 pc". The Astronomical Journal. 167 (6): 283. arXiv:2407.18199. Bibcode:2024AJ....167..283T. doi:10.3847/1538-3881/ad3df1.
  16. ^ "Kepler-1998". NASA Exoplanet Archive. Retrieved 16 June 2023.
  17. ^ Adams, Elisabeth R.; Jackson, Brian; et al. (August 2021). "Ultra-short-period Planets in K2. III. Neighbors are Common with 13 New Multiplanet Systems and 10 Newly Validated Planets in Campaigns 0-8 and 10". The Planetary Science Journal. 2 (4): 152. arXiv:2011.11698. Bibcode:2021PSJ.....2..152A. doi:10.3847/PSJ/ac0ea0.
  18. ^ Smith, A. M. S.; Cabrera, J.; et al. (March 2018). "K2-137 b: an Earth-sized planet in a 4.3-h orbit around an M-dwarf". Monthly Notices of the Royal Astronomical Society. 474 (4): 5523–5533. arXiv:1707.04549. Bibcode:2018MNRAS.474.5523S. doi:10.1093/mnras/stx2891.
  19. ^ Piaulet, Caroline; Benneke, Björn; et al. (15 December 2022). "Evidence for the volatile-rich composition of a 1.5-Earth-radius planet". Nature Astronomy. 7: 206. arXiv:2212.08477. Bibcode:2023NatAs...7..206P. doi:10.1038/s41550-022-01835-4. S2CID 254764810.
  20. ^ Silverstein, Michele L.; Barclay, Thomas; et al. (May 2024). "Validation of a Third Planet in the LHS 1678 System". The Astronomical Journal. 167 (6): 255. arXiv:2403.00110. Bibcode:2024AJ....167..255S. doi:10.3847/1538-3881/ad3040.
  21. ^ Goffo, Elisa; Gandolfi, Davide; et al. (September 2023). "Company for the ultra-high density, ultra-short period sub-Earth GJ 367 b: discovery of two additional low-mass planets at 11.5 and 34 days". The Astrophysical Journal Letters. 955 (1): L3. arXiv:2307.09181. Bibcode:2023ApJ...955L...3G. doi:10.3847/2041-8213/ace0c7.
  22. ^ 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. (2021), "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, 507 (2): 1847–1868, arXiv:2107.13900, Bibcode:2021MNRAS.507.1847R, doi:10.1093/mnras/stab2192
  23. ^ Weiss, Lauren M.; et al. (2024-01-01). "The Kepler Giant Planet Search. I. A Decade of Kepler Planet-host Radial Velocities from W. M. Keck Observatory". The Astrophysical Journal Supplement Series. 270 (1) 8. arXiv:2304.00071. Bibcode:2024ApJS..270....8W. doi:10.3847/1538-4365/ad0cab.
  24. ^ Gaidos, Eric; Mann, Andrew W.; Ansdell, Megan (January 2016). "The Enigmatic and Ephemeral M Dwarf System KOI 6705: Cheshire Cat or Wild Goose?". The Astrophysical Journal. 817 (1): 50. arXiv:1511.06471. Bibcode:2016ApJ...817...50G. doi:10.3847/0004-637X/817/1/50.
  25. ^ a b Manser, Christopher J.; et al. (5 April 2019). "A planetesimal orbiting within the debris disc around a white dwarf star". Science. 364 (6435): 66–69. arXiv:1904.02163. Bibcode:2019Sci...364...66M. doi:10.1126/science.aat5330. ISSN 0036-8075. PMID 30948547. S2CID 96434522.
  26. ^ "Planet SDSS J1228+1040 b". Extrasolar Planets Encyclopaedia. Retrieved 2019-08-05.
  27. ^ Ates Goksu, Olcay; Kutra, Taylor; Wu, Yanqin (2023-08-01), Eccentric Gas Disk Orbiting the White Dwarf SDSS J1228+1040, arXiv:2308.01234, retrieved 2024-04-15
  28. ^ a b c d e f g h i j k l m n o p q r s t u v w x y z aa ab ac ad ae af ag ah ai aj ak al am an ao ap aq ar as at au av aw ax ay az ba bb bc bd be bf bg bh bi bj bk bl bm bn bo bp bq br bs bt bu bv bw bx by bz ca cb cc cd ce cf cg "NASA Exoplanet Archive". NASA Exoplanet Archive. Retrieved 16 June 2023.
  29. ^ Roche, Jakob (2024-06-07). "The Detection of KIC 1718360, A Rotating Variable with a Possible Companion, Using Machine Learning". arXiv:2405.05282 [astro-ph.EP].
  30. ^ "Kepler-105". NASA Exoplanet Archive. Retrieved 12 December 2021.
  31. ^ "NASA Exoplanet Archive". NASA Exoplanet Archive. Retrieved 16 June 2023.
  32. ^ Price, Ellen M.; Rogers, Leslie A. (May 2020). "Tidally Distorted, Iron-enhanced Exoplanets Closely Orbiting Their Stars". The Astrophysical Journal. 894 (1): 8. arXiv:1901.10666. Bibcode:2020ApJ...894....8P. doi:10.3847/1538-4357/ab7c67.
Licensed under CC BY-SA 3.0 | Source: https://en.wikipedia.org/wiki/List_of_smallest_exoplanets
25 views |
↧ Download as ZWI file
Encyclosphere.org EncycloReader is supported by the EncyclosphereKSF