Astronomy:Kepler-409b

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Short description: Exoplanet
Kepler-409b
Discovery
Discovered byKepler space telescope
Discovery date2014
Transit
Orbital characteristics[1]
0.3192 AU
Eccentricity<0.69
Orbital period68.9583216±0.0000039 d
Inclination86.30±0.13
StarKepler-409
Physical characteristics
Mean radius1.199 R
Mass<6 M
Mean density<19 g/cm3
Physics438±7


Kepler-409b is a super-Earth orbiting Kepler-409, a G-type main-sequence star. Its orbital period around the star is 69 days. Kepler-409b has a radius that is 1.199 that of Earth and a mass of 6 that of Earth. Its discovery in 2014 was made through the use of the transit detection method. The transit method was performed by the Kepler space telescope.[2]

Possible exomoon

In 2020, a possible exomoon was discovered from transit timing variations.[3] Follow-up observations deemed it unlikely.[4]

References

  1. Bonomo, A. S.; Dumusque, X.; Massa, A.; Mortier, A.; Bongiolatti, R.; Malavolta, L.; Sozzetti, A.; Buchhave, L. A. 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. ISSN 0004-6361. https://www.aanda.org/10.1051/0004-6361/202346211. 
  2. "The Extrasolar Planet Encyclopaedia — Kepler-409b". Extrasolar Planets Encyclopaedia. 1995. https://exoplanet.eu/catalog/kepler_409_b--2542/. 
  3. Fox, Chris; Wiegert, Paul (23 November 2020). "Exomoon Candidates from Transit Timing Variations: Eight Kepler systems with TTVs explainable by photometrically unseen exomoons". Monthly Notices of the Royal Astronomical Society 501 (2): 2378–2393. doi:10.1093/mnras/staa3743. Bibcode2021MNRAS.501.2378F. 
  4. Kipping, David (8 August 2020). "An Independent Analysis of the Six Recently Claimed Exomoon Candidates". The Astrophysical Journal 900 (2): L44. doi:10.3847/2041-8213/abafa9. Bibcode2020ApJ...900L..44K.