Kepler-298d
| Discovery | |
|---|---|
| Discovered by | Jason F. Rowe et al.[1] |
| Discovery site | Kepler |
| Discovery date | February 26, 2014 |
| Transit method | |
| Orbital characteristics | |
| 77.473633[1] d | |
| JD 2454985.64156[1] | |
| Star | Kepler-298 |
| Physical characteristics | |
| 2.50 ± 0.20[1] R🜨 | |
Mean density | 2.8203 ± 4.0164 g/cm3 (0.10189 ± 0.14510 lb/cu in)[1] |
Kepler-298d is an exoplanet orbiting within the habitable zone of the orange dwarf star Kepler-298, located 1545 light years (473.69 parsecs) away from Earth. It was discovered in 2014 via the transit method.[2] The planet was originally considered to be potentially habitable,[3] but further research places its atmosphere at +2.11 on the HZA scale,[jargon] meaning it may be an ocean planet with a thick gas atmosphere like a gas dwarf.[citation needed]
See also
[edit]References
[edit]- ^ a b c d e 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.
- ^ "Planet Kepler-298 d". Extrasolar Planets Encyclopaedia. Retrieved 26 April 2018.
- ^ Safonova, M.; Murthy, J.; Shchekinov, Yu. A. (27 August 2018). "Age Aspects of Habitability": 10. Retrieved 17 January 2025.
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