Kepler-24d explained
| Kepler-24d |
| Discoverer: | Jason F. Rowe et al. |
| Discovered: | 26 February 2014 |
| Apsis: | astron |
| Semimajor: | 0.051AU[1] |
| Period: | 4.24437621(2426)[2] d |
| Star: | Kepler-24 |
| Mean Radius: | 0.149 ± 0.035 |
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]
Notes and References
- 2014ApJ...784...45R. 10.1088/0004-637X/784/1/45. 1402.6534. etal. Validation of Kepler's Multiple Planet Candidates. III. Light Curve Analysis and Announcement of Hundreds of New Multi-planet Systems. Rowe. Jason F.. The Astrophysical Journal. 784. 1. 45. 20. 2014. 119118620.
- 2016ApJ...822...86M. 1605.02825. 10.3847/0004-637X/822/2/86. False Positive Probabilities for All Kepler objects of Interest: 1284 Newly Validated Planets and 428 Likely False Positives. The Astrophysical Journal. 822. 2. 86. 2016. Morton. Timothy D.. Bryson. Stephen T.. Coughlin. Jeffrey L.. Rowe. Jason F.. Ravichandran. Ganesh. Petigura. Erik A.. Haas. Michael R.. Batalha. Natalie M.. 20832201. 1 . free .
