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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
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] Radii listed in italics are estimates.
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 predicted 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-974c (KOI-1843.03)
0.61+0.12 −0.08
Candidate.[ 17] As of 2025[update] , the Exoplanet Archive lists it as confirmed.[ 2]
Kepler-1087b
0.61+0.17 −0.05
K2-89b
0.615± 0.080
Kepler-1877b
0.624
Barnard's Star e
~0.637
Radius predicted from mass-radius relationship.[ 2] Least massive exoplanet detected by radial velocity and possibly smallest known within 10 parsecs .[ 18]
K2-137b
0.64± 0.10[ 19]
The discovery paper finds a larger radius of 0.89± 0.09 R 🜨 [ 20]
Kepler-1371c
0.64+0.07 −0.05
Kepler-138b
0.64± 0.02
[ 21]
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
[ 22]
K2-116b
0.69± 0.04
Kepler-141b
0.69± 0.05
K2-297b (EPIC 201497682 b)
0.692+0.059 −0.048
Proxima Centauri d
~0.692
Radius predicted from mass-radius relationship.[ 2] [ 23]
Barnard's Star d
~0.694
Radius predicted from mass-radius relationship.[ 2] [ 18]
Gliese 367 b (Tahay)
0.699± 0.024
Smallest exoplanet within 10 parsecs with a measured radius.[ 24]
Kepler-2003b (KOI-4978.02)
0.7± 0.1
[ 11]
Kepler-378c
0.70± 0.05
Excluded objects
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,[ 25] and assuming its existence, a 2023 study found a mass of 8.1± 1.7 M 🜨 , inconsistent with such a small radius.[ 26]
KOI-6705.01, listed as a potential very small planet in the KOI dataset, was shown to be a false positive in 2016.[ 27]
Candidate planets
Below is a list of 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 [ 28] [ 29]
TRAPPIST-1i
0.228+0.025 −0.032 [ 30]
KOI-4582.01
0.35[ 31]
KOI-2298.03
0.36[ 31]
KOI-2169.04
0.37[ 31]
KOI-7174.01
0.37[ 31]
KOI-8012.01
0.42[ 31]
KOI-6860.01
0.43[ 31]
KOI-2059.02
0.44[ 31]
KOI-304.02
0.46[ 31]
KOI-7793.01
0.46[ 31]
KOI-2678.02
0.48[ 31]
KOI-6631.01
0.48[ 31]
KOI-2421.02
0.48[ 31]
KOI-5974.01
0.49[ 31]
KOI-3444.03
0.5[ 31]
KOI-2295.01
0.52[ 31]
KOI-7863.01
0.52[ 31]
KOI-2612.02
0.53[ 31]
KOI-4657.01
0.54[ 31]
KOI-8257.01
0.54[ 31]
KOI-115.03 (Kepler-105d)
0.55+0.08 −0.07
[ 32]
KOI-2421.01
0.55[ 31]
KOI-4097.02
0.55[ 31]
KOI-7645.01
0.55[ 31]
KOI-3208.01
0.56[ 31]
KOI-6763.01
0.56[ 31]
KOI-2859.03
0.57[ 31]
KOI-4146.02
0.57[ 31]
KOI-2859.04
0.57[ 31]
KOI-7873.01
0.57[ 31]
TOI-4307.02
0.57± 0.14[ 33]
KOI-2657.01
0.58[ 31]
KOI-8277.01
0.58[ 31]
KOI-4296.01
0.59[ 31]
KOI-3196.01
0.59[ 31]
KOI-5692.01
0.59[ 31]
KOI-1964.01
0.6[ 31]
KOI-4407.01
0.6[ 31]
KOI-4871.01
0.6[ 31]
KOI-5211.01
0.6[ 31]
KOI-7888.01
0.6[ 31]
KOI-3184.03
0.6[ 31]
KOI-8183.01
0.6[ 31]
KOI-3083.02
0.61[ 31]
KOI-4421.01
0.61[ 31]
KOI-4716.01
0.61[ 31]
KOI-3102.01
0.61[ 31]
KOI-7032.01
0.61[ 31]
KOI-1499.02
0.62[ 31]
KOI-605.02
0.62[ 31]
KOI-7676.01
0.62[ 31]
KOI-4849.01
0.62[ 31]
KOI-365.02
0.62[ 31]
KOI-7116.01
0.62[ 31]
KOI-4421.02
0.62[ 31]
KOI-7949.01
0.62[ 31]
KOI-2029.04
0.63[ 31]
KOI-6889.01
0.63[ 31]
KOI-2636.02
0.63[ 31]
KOI-3248.01
0.64[ 31]
KOI-5213.01
0.64[ 31]
KOI-6276.01
0.64[ 31]
KOI-7617.01
0.64[ 31]
KOI-7903.01
0.64[ 31]
KOI-7925.01
0.64[ 31]
KOI-8174.01
0.64[ 31]
KOI-3083.03
0.65[ 31]
KOI-4875.01
0.65[ 31]
KOI-4808.01
0.65[ 31]
KOI-6568.01
0.65[ 31]
KOI-1619.01
0.66[ 31]
KOI-3111.02
0.66[ 31]
KOI-2859.05
0.66[ 31]
KOI-3017.01
0.67[ 31]
KOI-4907.01
0.67[ 31]
KOI-1616.02
0.67[ 31]
KOI-6299.01
0.67[ 31]
KOI-8211.01
0.67[ 31]
KOI-2593.02
0.68[ 31]
KOI-4605.01
0.68[ 31]
KOI-7832.01
0.68[ 31]
KOI-7483.01
0.68[ 31]
KOI-2623.02
0.68[ 31]
KOI-7924.01
0.68[ 31]
KOI-7628.01
0.69[ 31]
KOI-4129.01
0.69[ 31]
KOI-4822.01
0.69[ 31]
KOI-6600.01
0.69[ 31]
See also
References
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↑ 2.0 2.1 2.2 2.3 2.4 "Planetary Systems Composite Data" . https://exoplanetarchive.ipac.caltech.edu/cgi-bin/TblView/nph-tblView?app=ExoTbls&config=PSCompPars . Retrieved 13 March 2025 .
↑ 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. doi :10.1093/mnras/stv1201 . Bibcode : 2015MNRAS.451.3237W . https://academic.oup.com/mnras/article/451/3/3237/1197266?login=false .
↑ 4.0 4.1 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. doi :10.1093/mnras/stw612 . Bibcode : 2016MNRAS.458.3904R .
↑ Simukoff, E. et al . (2013). "Below One Earth Mass: The Detection, Formation, and Properties of Subterrestrial Worlds". Space Science Reviews 180 (1–4): 71. doi :10.1007/s11214-013-0019-1 . Bibcode : 2013SSRv..180...71S .
↑ 6.0 6.1 6.2 Bonomo, A. S. 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. doi :10.1051/0004-6361/202346211 . Bibcode : 2023A&A...677A..33B .
↑ Hon, Marc; Rappaport, Saul; Shporer, Avi; Vanderburg, Andrew; Collins, Karen A.; Watkins, Cristilyn N.; Schwarz, Richard P.; Barkaoui, Khalid et al . (2025-01-09). "A Disintegrating Rocky Planet with Prominent Comet-like Tails Around a Bright Star". The Astrophysical Journal 984 (1): L3. doi :10.3847/2041-8213/adbf21 . Bibcode : 2025ApJ...984L...3H .
↑ "Exoplanet-catalog" . 22 April 2019. https://exoplanets.nasa.gov/exoplanet-catalog/7134/psr-b125712-b/ .
↑ 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. doi :10.1093/mnras/stz693 . Bibcode : 2019MNRAS.485.3876G . "[...]the radii are not known but are thought to be smaller than Mercury (0.36R⊕).".
↑ Garai, Z. (2018). "Light-curve analysis of KOI 2700b: The second extrasolar planet with a comet-like tail". Astronomy & Astrophysics 611 : A63. doi :10.1051/0004-6361/201629676 . Bibcode : 2018A&A...611A..63G . "We confirmed the disintegrating-planet scenario of KOI 2700b.".
↑ 11.0 11.1 11.2 11.3 11.4 Wang, Kaitlyn 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. doi :10.1093/mnras/stae2155 . Bibcode : 2024MNRAS.534.1913W .
↑ 12.0 12.1 12.2 12.3 Campante, T. et al . (2015). "KOI-3158: The oldest known system of terrestrial-size planets". EPJ Web of Conferences 101 : 02004. doi :10.1051/epjconf/201510102004 . Bibcode : 2015EPJWC.10102004C .
↑ Cañas, Caleb I.; Mahadevan, Suvrath; Cochran, William D.; Bender, Chad F.; Feigelson, Eric D.; Harman, C. E.; Kopparapu, Ravi Kumar; Caceres, Gabriel A. et al . (2022). "A Hot Mars-sized Exoplanet Transiting an M Dwarf". The Astronomical Journal 163 (1): 3. doi :10.3847/1538-3881/ac3088 . Bibcode : 2022AJ....163....3C .
↑ "Kepler-1994" . https://exoplanetarchive.ipac.caltech.edu/overview/Kepler-1994%20b . Retrieved 16 June 2023 .
↑ Tey, Evan 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. doi :10.3847/1538-3881/ad3df1 . Bibcode : 2024AJ....167..283T .
↑ "Kepler-1998" . https://exoplanetarchive.ipac.caltech.edu/overview/Kepler-1998%20b . Retrieved 16 June 2023 .
↑ Price, Ellen M.; Rogers, Leslie A. (May 2020). "Tidally Distorted, Iron-enhanced Exoplanets Closely Orbiting Their Stars". The Astrophysical Journal 894 (1): 8. doi :10.3847/1538-4357/ab7c67 . Bibcode : 2020ApJ...894....8P .
↑ 18.0 18.1 Basant, Ritvik et al . (March 2025). "Four Sub-Earth Planets Orbiting Barnard's Star from MAROON-X and ESPRESSO". The Astrophysical Journal Letters 982 (1): L1. doi :10.3847/2041-8213/adb8d5 . Bibcode : 2025ApJ...982L...1B .
↑ Adams, Elisabeth R. 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. doi :10.3847/PSJ/ac0ea0 . Bibcode : 2021PSJ.....2..152A .
↑ Smith, A. M. S. 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. doi :10.1093/mnras/stx2891 . Bibcode : 2018MNRAS.474.5523S .
↑ Piaulet, Caroline et al . (15 December 2022). "Evidence for the volatile-rich composition of a 1.5-Earth-radius planet". Nature Astronomy 7 : 206. doi :10.1038/s41550-022-01835-4 . Bibcode : 2023NatAs...7..206P .
↑ Silverstein, Michele L. et al . (May 2024). "Validation of a Third Planet in the LHS 1678 System". The Astronomical Journal 167 (6): 255. doi :10.3847/1538-3881/ad3040 . Bibcode : 2024AJ....167..255S .
↑ Suárez Mascareño, Alejandro et al . (29 July 2025). "Diving into the planetary system of Proxima with NIRPS: Breaking the metre per second barrier in the infrared". Astronomy & Astrophysics 700 : A11. doi :10.1051/0004-6361/202553728 . Bibcode : 2025A&A...700A..11S .
↑ Goffo, Elisa 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. doi :10.3847/2041-8213/ace0c7 . Bibcode : 2023ApJ...955L...3G .
↑ Rajpaul, V. M.; Buchhave, L. A.; Lacedelli, G.; Rice, K.; Mortier, A.; Malavolta, L.; Aigrain, S.; Borsato, L. et al . (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, doi :10.1093/mnras/stab2192 , Bibcode : 2021MNRAS.507.1847R
↑ 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). doi :10.3847/1538-4365/ad0cab . Bibcode : 2024ApJS..270....8W .
↑ 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. doi :10.3847/0004-637X/817/1/50 . Bibcode : 2016ApJ...817...50G .
↑ Manser, Christopher J. (5 April 2019). "A planetesimal orbiting within the debris disc around a white dwarf star" . Science 364 (6435): 66–69. doi :10.1126/science.aat5330 . ISSN 0036-8075 . PMID 30948547 . Bibcode : 2019Sci...364...66M . https://www.science.org/doi/10.1126/science.aat5330 .
↑ "Planet SDSS J1228+1040 b" . Extrasolar Planets Encyclopaedia . https://exoplanet.eu/catalog/sdss_j1228_1040_b--7079/ . Retrieved 2019-08-05 .
↑ "First JWST thermal phase curves of temperate terrestrial exoplanets reveal no thick atmosphere around TRAPPIST-1 b and c". 2 September 2025. arXiv :2509.02128 [astro-ph.EP ].
↑ 31.00 31.01 31.02 31.03 31.04 31.05 31.06 31.07 31.08 31.09 31.10 31.11 31.12 31.13 31.14 31.15 31.16 31.17 31.18 31.19 31.20 31.21 31.22 31.23 31.24 31.25 31.26 31.27 31.28 31.29 31.30 31.31 31.32 31.33 31.34 31.35 31.36 31.37 31.38 31.39 31.40 31.41 31.42 31.43 31.44 31.45 31.46 31.47 31.48 31.49 31.50 31.51 31.52 31.53 31.54 31.55 31.56 31.57 31.58 31.59 31.60 31.61 31.62 31.63 31.64 31.65 31.66 31.67 31.68 31.69 31.70 31.71 31.72 31.73 31.74 31.75 31.76 31.77 31.78 31.79 31.80 31.81 31.82 31.83 31.84 "NASA Exoplanet Archive" . https://exoplanetarchive.ipac.caltech.edu/cgi-bin/TblView/nph-tblView?app=ExoTbls&config=cumulative . Retrieved 16 June 2023 .
↑ "Kepler-105" . https://exoplanetarchive.ipac.caltech.edu/overview/KOI-115 . Retrieved 12 December 2021 .
↑ "NASA Exoplanet Archive" . https://exoplanetarchive.ipac.caltech.edu/cgi-bin/TblView/nph-tblView?app=ExoTbls&config=TOI . Retrieved 16 June 2023 .
Original source: https://en.wikipedia.org/wiki/List of smallest exoplanets. Read more