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Kepler-421b

From Wikipedia, the free encyclopedia
Kepler-421b
Discovery
Discovery siteKepler telescope
Discovery date2014
Transit
Orbital characteristics
1.219 AU (182,400,000 km)
704.1984 d
Inclination89.965
StarKepler-421
Physical characteristics
4.16 R🜨
Mass16.1 M🜨

Kepler-421b is an exoplanet that, as of July 2014,[1] has the longest known year of any transiting planet (704 days),[2] although not as long as the planets that have been directly imaged, or many of the planets found by the radial-velocity method, or as long as some transiting planet candidates which are listed as planets in the Extrasolar Planets Encyclopaedia (KIC 5010054 b etc.).[3] It is the first transiting-planet found near the snow-line.

Normally, at least three transits are required to confirm a planet. Due to very high signal to noise ratio, only two transits were sufficient to validate Kepler-421b to be a real planet without additional confirmation methods.

Kepler-421b is slightly larger than Uranus, and having a mass 16.1 times[4] that of Earth, typical of an ice giant.

References

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  1. Kipping, D. M.; Torres, G.; Buchhave, L. A.; Kenyon, S. J.; Henze, C.; Isaacson, H.; Kolbl, R.; Marcy, G. W.; Bryson, S. T.; Stassun, K.; Bastien, F. (2014), "Discovery of a Transiting Planet Near the Snow-Line", The Astrophysical Journal, 795 (1): 25, arXiv:1407.4807, Bibcode:2014ApJ...795...25K, doi:10.1088/0004-637X/795/1/25, S2CID 119240746
  2. Johnson, Michele (July 21, 2014). "Astronomers Discover Transiting Exoplanet with Longest Known Year". NASA. Archived from the original on April 17, 2018. Retrieved July 25, 2014.
  3. "The Extrasolar Planet Encyclopaedia — Catalog Listing". Extrasolar Planets Encyclopaedia.
  4. "Kepler-421 b - NASA Science". science.nasa.gov. Retrieved 2024-12-19.

Further reading

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