Article · Wikipedia archive · Last revised Jul 8, 2026

Kepler-23c

Kepler-23c is a Neptune-sized exoplanet orbiting the star Kepler-23, located in the constellation Cygnus. The planet is 3.12 times wider than the Earth and is 0.189 Jupiter masses. The planet was discovered using data taken from the Kepler space telescope. It is likely a gas giant. The planets Kepler-23b and d both reside in the same planetary system.

Last revised
Jul 8, 2026
Read time
≈ 1 min
Length
243 w
Citations
10
Source
Kepler-23c
Discovery
Discovered byEric B. Ford et al.1
Discovery date25 January 2012
Transit method
Orbital characteristics
0.099 AU (14,800,000 km)1
Eccentricity0.02+0.39
−0.02
2
10.742434(39)2 d
StarKepler-23
Physical characteristics
3.12 ± 0.102 R🜨
Mass0.189+0.033
−0.036
3 MJ
Comparative sizes of Earth, Kepler-23 c and Jupiter.
Comparative sizes of Earth, Kepler-23 c and Jupiter. source ↗

Kepler-23c is a Neptune-sized exoplanet orbiting the star Kepler-23, located in the constellation Cygnus.3 The planet is 3.12 times wider than the Earth2 and is 0.189 Jupiter masses.3 The planet was discovered using data taken from the Kepler space telescope.1 It is likely a gas giant. The planets Kepler-23b and d both reside in the same planetary system.

References

References

  1. Ford, Eric B.; Fabrycky, Daniel C.; Steffen, Jason H.; Carter, Joshua A.; Fressin, Francois; Holman, Matthew J.; Lissauer, Jack J.; Moorhead, Althea V.; Morehead, Robert C.; Ragozzine, Darin; Rowe, Jason F.; Welsh, William F.; Allen, Christopher; Batalha, Natalie M.; Borucki, William J.; Bryson, Stephen T.; Buchhave, Lars A.; Burke, Christopher J.; Caldwell, Douglas A.; Charbonneau, David; Clarke, Bruce D.; Cochran, William D.; Désert, Jean-Michel; Endl, Michael; Everett, Mark E.; Fischer, Debra A.; Gautier, Thomas N.; Gilliland, Ron L.; Jenkins, Jon M.; et al. (2012). "Transit Timing Observations Fromkepler. Ii. Confirmation of Two Multiplanet Systems Via a Non-Parametric Correlation Analysis". The Astrophysical Journal. 750 (2): 113. arXiv:1201.5409. Bibcode:2012ApJ...750..113F. doi:10.1088/0004-637X/750/2/113. S2CID 4528963.
  2. Van Eylen, Vincent; Albrecht, Simon (2015). "Eccentricity from Transit Photometry: Small Planets in Kepler Multi-Planet Systems Have Low Eccentricities". The Astrophysical Journal. 808 (2): 126. arXiv:1505.02814. Bibcode:2015ApJ...808..126V. doi:10.1088/0004-637X/808/2/126. S2CID 14405731.
  3. "Kepler-23 c". Extrasolar Planets Encyclopaedia. Retrieved 26 June 2017.