Back كبلر-296e Arabic Kepler-296e German Kepler-296e Spanish Kepler-296e Finnish Kepler-296 e French Kepler-296e ID Kepler-296 e Italian ケプラー296e Japanese Kepler-296e Polish Kepler-296e Portuguese
| Discovery | |
|---|---|
| Discovery site | Kepler Space Observatory |
| Discovery date | 2014 |
| Transit | |
| Orbital characteristics | |
| 0.17400 AU (26,030,000 km) | |
| Eccentricity | <0.33[4] |
| 34.14234700 d | |
| Inclination | 89.950 |
| Star | Kepler-296 |
| Physical characteristics | |
| 1.530 R🜨 [4] | |
| Temperature | 267 K (−6 °C; 21 °F) |
Kepler-296e (also known by its Kepler Object of Interest designation KOI-1422.05) is a confirmed super-Earth exoplanet orbiting within the habitable zone of Kepler-296. The planet was discovered by NASA's Kepler spacecraft using the transit method, in which the dimming effect that a planet causes as it crosses in front of its star is measured. NASA announced the discovery of the exoplanet on 26 February 2014.[1]
- ^ a b Staff (26 February 2014). "715 Newly Verified Planets More Than Triples the Number of Confirmed Kepler Planets". NASA. Archived from the original on 4 March 2014. Retrieved 8 January 2015.
- ^ Lissauer, Jack J.; et al. (25 February 2014). "Validation of Kepler's Multiple Planet Candidates. II: Refined Statistical Framework and Descriptions of Systems of Special Interest". The Astrophysical Journal. 784 (1): 44. arXiv:1402.6352. Bibcode:2014ApJ...784...44L. doi:10.1088/0004-637X/784/1/44. S2CID 119108651.
- ^ Rowe, Jason F. (2014). "Validation of Kepler's Multiple Planet Candidates. III: Light Curve Analysis & Announcement of Hundreds of New Multi-planet Systems". The Astrophysical Journal. 784 (1): 45. arXiv:1402.6534. Bibcode:2014ApJ...784...45R. doi:10.1088/0004-637X/784/1/45. S2CID 119118620.
- ^ a b Cite error: The named reference
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