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Kepler-24d 
Summary
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]
| Discovery | |
|---|---|
| Discovered by | Jason F. Rowe et al.[1] |
| Discovery date | 26 February 2014 |
| Transit method | |
| Orbital characteristics | |
| 0.051 AU (7.6 million km)[1] | |
| 4.24437621(2426)[2] d | |
| Star | Kepler-24 |
| Physical characteristics | |
Mean radius | 0.149 ± 0.035[1] RJ |
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.