● Home ● Random ● Nearby ● Log in ● Settings ● Donate ● About Wikipedia ● Disclaimers

Kepler-24d

● Article ● Talk ● Language ● Watch ● Edit

Kepler-24d is a transiting exoplanet orbiting the star Kepler-24, located in the constellation Lyra. It was discovered by the Kepler telescope in February 2014. It orbits its parent star at only 0.051 astronomical units away, and at its distance it completes an orbit once every 4.244384 days.^[1]

Kepler-24d
Discovery
Discovered by	Jason F. Rowe et al.^[1]
Discovery date	26 February 2014
Detection method	Transit method
Orbital characteristics
Semi-major axis	0.051 AU (7.6 million km)^[1]
Orbital period (sidereal)	4.24437621(2426)^[2] d
Star	Kepler-24
Physical characteristics
Mean radius	0.149 ± 0.035^[1] `R`_J

References

edit

^ ^a ^b ^c ^d Rowe, Jason F.; et al. (2014). "Validation of Kepler's Multiple Planet Candidates. III. Light Curve Analysis and Announcement of Hundreds of New Multi-planet Systems". The Astrophysical Journal. 784 (1): 20. arXiv:1402.6534. Bibcode:2014ApJ...784...45R. doi:10.1088/0004-637X/784/1/45. S2CID 119118620. 45.

^ Morton, Timothy D.; et al. (2016). "False Positive Probabilities for All Kepler objects of Interest: 1284 Newly Validated Planets and 428 Likely False Positives". The Astrophysical Journal. 822 (2): 86. arXiv:1605.02825. Bibcode:2016ApJ...822...86M. doi:10.3847/0004-637X/822/2/86. S2CID 20832201.

This extrasolar-planet-related article is a stub. You can help Wikipedia by expanding it.

Retrieved from "https://en.wikipedia.org/w/index.php?title=Kepler-24d&oldid=1177271202" Last edited on 27 September 2023, at 00:29

Languages

●Español ●Bahasa Indonesia

●This page was last edited on 27 September 2023, at 00:29 (UTC). ●Content is available under CC BY-SA 4.0 unless otherwise noted. ●Privacy policy ●About Wikipedia ●Disclaimers ●Contact Wikipedia ●Code of Conduct ●Developers ●Statistics ●Cookie statement ●Terms of Use ●Desktop