Astronomy:Kappa Coronae Borealis b

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Short description: Extrasolar planet in the constellation Corona Borealis
Kappa Coronae Borealis b
Discovery[1]
Discovered byJohnson et al.
Discovery siteLick Observatory
Discovery date2007
Doppler spectroscopy
Orbital characteristics[2]
2.65±0.13 astronomical unit|AU
Eccentricity0.167±0.032
Orbital period1285±14 d
|{{{apsis}}}|helion}}2456830±51 JD
194±14 º
Semi-amplitude26.18±0.86 m/s
StarKappa Coronae Borealis
Physical characteristics[2]
Mass≥1.811±0.057 Jupiter mass


Kappa Coronae Borealis b is an extrasolar planet approximately 98 light-years away[3] in the constellation of Corona Borealis. This planet was discovered by Johnson et al., who used the radial velocity method to detect wobbling of the star caused by a planet move around by its tug of gravity. It was first discovered in September 2007 and was published in November.[1]

The planet is 1.8 Jupiter masses, or 570 Earth masses, although only the minimum mass is known since the inclination is not known. It orbits at a distance of 2.7 astronomical units, or 400 gigameters, and takes 1,208 days, or 3.307 years, to orbit around Kappa Coronae Borealis.

See also

References

  1. 1.0 1.1 Johnson, John Asher et al. (2008). "Retired A Stars and Their Companions. II. Jovian Planets Orbiting κ CrB and HD 167042". The Astrophysical Journal 675 (1): 784–789. doi:10.1086/526453. Bibcode2008ApJ...675..784J. 
  2. 2.0 2.1 Luhn, Jacob K. et al. (2019). "Retired A Stars and Their Companions. VIII. 15 New Planetary Signals around Subgiants and Transit Parameters for California Planet Search Planets with Subgiant Hosts". The Astronomical Journal 157 (4): 149. doi:10.3847/1538-3881/aaf5d0. Bibcode2019AJ....157..149L. 
  3. Brown, A. G. A. (August 2018). "Gaia Data Release 2: Summary of the contents and survey properties". Astronomy & Astrophysics 616: A1. doi:10.1051/0004-6361/201833051. Bibcode2018A&A...616A...1G.  Gaia DR2 record for this source at VizieR.

es:Kappa Coronae Borealis#Sistema planetario