From Wikipedia, the free encyclopedia
Exoplanet
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 1.199 times that of
Earth and a
mass 6 times 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 .
[1]
Possible exomoon
In 2020, a possible
exomoon was discovered from transit timing variations.
[3] Follow-up observations deemed it unlikely.
[4]
References
^
a
b
"The Extrasolar Planet Encyclopaedia — Kepler-409b" .
Extrasolar Planets Encyclopaedia . 1995. Retrieved 11 September 2023 .
^ Bonomo, A. S.; Dumusque, X.; Massa, A.; Mortier, A.; Bongiolatti, R.; Malavolta, L.; Sozzetti, A.; Buchhave, L. A.; Damasso, M.; Haywood, R. D.; Morbidelli, A.; Latham, D. W.; Molinari, E.; Pepe, F.; Poretti, E. (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 .
doi :
10.1051/0004-6361/202346211 .
ISSN
0004-6361 .
^ 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.
arXiv :
2006.12997 .
Bibcode :
2021MNRAS.501.2378F .
doi :
10.1093/mnras/staa3743 .
S2CID
219980961 .
^ Kipping, David (8 August 2020).
"An Independent Analysis of the Six Recently Claimed Exomoon Candidates" . The Astrophysical Journal . 900 (2): L44.
arXiv :
2008.03613 .
Bibcode :
2020ApJ...900L..44K .
doi :
10.3847/2041-8213/abafa9 .
S2CID
225253170 .