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1 See also  





2 References  














Kepler-298d






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From Wikipedia, the free encyclopedia
 


Kepler-298d
Discovery
Discovered byJason F. Rowe et al.[1]
Discovery siteKepler
Discovery dateFebruary 26, 2014

Detection method

Transit method
Orbital characteristics

Orbital period (sidereal)

77.473633[1] d

Time of periastron

JD 2454985.64156[1]
StarKepler-298
Physical characteristics

Mean radius

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 Kepler-298, 473.69 parsecs away (1545 ly). Kepler-298d was discovered in 2014,[2] it orbits its star in the Habitable zone. Kepler-298d was thought to be an Earth-like planet, further research shows that its atmosphere is +2.11 on the HZA scale, this means the planet may be an ocean planet with a thick gas atmosphere like a gas dwarf.[citation needed]

See also[edit]

References[edit]

  1. ^ 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.

  • Retrieved from "https://en.wikipedia.org/w/index.php?title=Kepler-298d&oldid=1191315348"

    Categories: 
    Exoplanets discovered in 2014
    Super-Earths in the habitable zone
    Exoplanets discovered by the Kepler space telescope
    Transiting exoplanets
    Hidden categories: 
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    Articles with unsourced statements from December 2023
     



    This page was last edited on 22 December 2023, at 20:08 (UTC).

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