Article · Wikipedia archive · Last revised Jul 1, 2026

Kepler-453b

Kepler-453b is a transiting circumbinary exoplanet in the binary-star system Kepler-453. It orbits the binary system in the habitable zone every 240.5 days. The orbit of the planet is inclined relative to the binary orbit therefore precession of the orbit leads to it spending most of its time in a non-transiting configuration. By the time the TESS and PLATO spacecraft are available for follow up observations it will no longer be transiting.

Last revised
Jul 1, 2026
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≈ 1 min
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Source
Kepler-453b
Discovery
Discovery siteKepler Space Observatory
Discovery date2015
Transit
Orbital characteristics
0.7903 ± 0.0028 AU (118,230,000 ± 420,000 km)1
Eccentricity0.0359±0.00881
240.503±0.0531 d
Inclination89.4429±0.0091 1
StarKepler-453
Physical characteristics
6.204±0.0391 R🜨

Kepler-453b is a transiting circumbinary exoplanet in the binary-star system Kepler-453. It orbits the binary system in the habitable zone every 240.5 days.12 The orbit of the planet is inclined relative to the binary orbit therefore precession of the orbit leads to it spending most of its time in a non-transiting configuration. By the time the TESS and PLATO spacecraft are available for follow up observations it will no longer be transiting.3

References

References

  1. "Kepler-453 b Confirmed Planet Overview Page". NASA Exoplanet Archive. Retrieved 2015-10-08.
  2. Welsh, William F.; et al. (2015). "Kepler 453 b - The 10th Kepler Transiting Circumbinary Planet". The Astrophysical Journal. 809 (1). 26. arXiv:1409.1605. Bibcode:2015ApJ...809...26W. doi:10.1088/0004-637X/809/1/26. S2CID 55158342.
  3. Martin, David V. (2017). "Circumbinary planets - II. When transits come and go". Monthly Notices of the Royal Astronomical Society. 465 (3): 3235–3253. arXiv:1611.00526. Bibcode:2017MNRAS.465.3235M. doi:10.1093/mnras/stw2851. S2CID 119187045.