Star in the constellation Sagittarius
HD 187085 is a yellow–hued star in the southern constellation of Sagittarius . It is too faint to be visible to the naked eye, having an apparent visual magnitude of +7.225.[ 2] The star is located at a distance of approximately 1,010 light years from the Sun based on parallax ,[ 1] and is drifting further away with a radial velocity of +18 km/s.[ 4]
This is an ordinary G-type main-sequence star with a stellar classification of G0V,[ 3] which means it is generating energy through core hydrogen fusion . It is younger than the Sun with an estimated age of 2.7 billion years and is spinning with a leisurely rotation period of around 21 days. The star is 27% larger and 19% more massive than the Sun.[ 2] It is radiating 2.3[ 1] times the luminosity of the Sun from its photosphere at an effective temperature of 6,117 K.[ 2]
In 2006, an extrasolar planet was announced orbiting HD 187085, with a minimum mass slightly below that of the planet Jupiter . It is orbiting the host star with a period of around 2.8 years.[ 6] The orbit overlaps the habitable zone of this star.[ 7] In 2009, the presence of an infrared excess was announced, suggesting a debris disk orbits the star.[ 8]
See also
References
^ a b c d e f g h Brown, A. G. A. ; et al. (Gaia collaboration) (August 2018). "Gaia Data Release 2: Summary of the contents and survey properties" . Astronomy & Astrophysics . 616 . A1. arXiv :1804.09365 . Bibcode :2018A&A...616A...1G . doi :10.1051/0004-6361/201833051 . Gaia DR2 record for this source at VizieR .
^ a b c d e f g Barbato, D.; et al. (August 2018), "Exploring the realm of scaled solar system analogues with HARPS", Astronomy & Astrophysics , 615 : 21, arXiv :1804.08329 , Bibcode :2018A&A...615A.175B , doi :10.1051/0004-6361/201832791 , S2CID 119099721 , A175.
^ a b Houk, Nancy (1979), Michigan catalogue of two-dimensional spectral types for the HD stars , vol. 3, Ann Arbor, Michigan: Department of Astronomy, University of Michigan, Bibcode :1982mcts.book.....H .
^ a b c Anderson, E.; Francis, Ch. (2012), "XHIP: An extended hipparcos compilation", Astronomy Letters , 38 (5): 331, arXiv :1108.4971 , Bibcode :2012AstL...38..331A , doi :10.1134/S1063773712050015 , S2CID 119257644 .
^ "HD 187085" . SIMBAD . Centre de données astronomiques de Strasbourg . Retrieved 2018-07-09 .
^ Jones, Hugh R. A.; et al. (2006), "High-eccentricity planets from the Anglo-Australian Planet Search", Monthly Notices of the Royal Astronomical Society , 369 (1): 249– 256, arXiv :astro-ph/0603335 , Bibcode :2006MNRAS.369..249J , doi :10.1111/j.1365-2966.2006.10298.x , S2CID 15452372 .
^ Agnew, Matthew T.; et al. (November 2017), "Stable habitable zones of single Jovian planet systems", Monthly Notices of the Royal Astronomical Society , 471 (4): 4494– 4507, arXiv :1706.05805 , Bibcode :2017MNRAS.471.4494A , doi :10.1093/mnras/stx1449 , S2CID 119227856 .
^ Kóspál, Ágnes; et al. (August 2009), "On the Relationship Between Debris Disks and Planets", The Astrophysical Journal Letters , 700 (2): L73 – L77 , arXiv :0907.0028 , Bibcode :2009ApJ...700L..73K , doi :10.1088/0004-637X/700/2/L73 , S2CID 16636256 .
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