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HD 204941 b

HD 204941 b is an exoplanet of the star HD 204941 in the constellation Capricorn [1] . The planet is removed from the Earth at a distance of 88 light years [1] .

HD 204941 b
Exoplanet
Parent star
StarHD 204941
ConstellationCapricorn
Right Ascension ( α )21 h 32 m 23.5 s
Declination ( δ )−20 ° 57 ′ 26.7 ″
Visible magnitude ( m V )8.45
Distance88 St. years
(27 pc )
Spectral classK2V
Elements of the orbit
Semimajor axis ( a )2.56 a. e.
Eccentricity ( e )0.37
Orbital Period ( P )1733 d.
physical characteristics
Minimum Weight ( m sin i )84 M ⊕
Radius ( r )? R j
Discovery Information
opening date2011
Detection methodDoppler Method
Opening placeHarps
Opening statusPosted by

The parent star is an orange dwarf of the spectral class K2V [2] .

Planet HD 204941 b has a mass of 0.266 mass of Jupiter , is an example of a gas giant [3] [2] . It is very far from the star, at a distance of 2.56 AU The eccentricity of the orbit is 0.37 [3] . The planet was discovered in 2011 by a group of astronomers working with the HARPS spectrograph by the Doppler method [3] .

Notes

  1. ↑ 1 2 The Extrasolar Planet Encyclopaedia - HD 204941 b (neopr.) . exoplanet.eu. Date of treatment July 28, 2019.
  2. ↑ 1 2 Open Exoplanet Catalog - HD 204941 b (neopr.) . openexoplanetcatalogue.com. Date of treatment July 28, 2019.
  3. ↑ 1 2 3 HD 204941, HIP 106353 (neopr.) . www.allplanets.ru. Date of treatment July 28, 2019.
Source - https://ru.wikipedia.org/w/index.php?title=HD_204941_b&oldid=102153412


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Clever Geek | 2019