Astronomy:HD 187085

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Short description: Star in the constellation Sagittarius
HD 187085
Observation data
Equinox J2000.0]] (ICRS)
Constellation Sagittarius
Right ascension  19h 49m 33.9667s[1]
Declination −37° 46′ 49.981″[1]
Apparent magnitude (V) +7.225[2]
Characteristics
Spectral type G0V[3]
B−V color index 0.622±0.007[2]
Astrometry
Radial velocity (Rv)+17.70±0.59[4] km/s
Proper motion (μ) RA: −2.853±0.344[1] mas/yr
Dec.: +8.514±0.363[1] mas/yr
Parallax (π)3.2263 ± 0.1847[1] mas
Distance1,010 ± 60 ly
(310 ± 20 pc)
Absolute magnitude (MV)4.00[4]
Details[2]
Mass1.189±0.023 M☉
Radius1.270±0.066 R☉
Luminosity2.298+0.007
−0.006
[1] L☉
Surface gravity (log g)4.279±0.041 cgs
Temperature6,117±27 K
Metallicity [Fe/H]+0.12±0.04 dex
Rotation~21 days
Age2.747±0.838 Myr
Other designations
CD–38°13701, GC 27415, HD 187085, HIP 97546, SAO 211579[5]
Database references
SIMBADdata

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]

The HD 187085 planetary system[2]
Companion
(in order from star)
Mass Semimajor axis
(AU)
Orbital period
(days)
Eccentricity Inclination Radius
b ≥0.836±0.011 MJ 2.100±0.032 1,019.74+21.29
−22.58
0.251+0.221
−0.191
— —

See also

References

  1. ↑ 1.0 1.1 1.2 1.3 1.4 1.5 1.6 1.7 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. Bibcode: 2018A&A...616A...1G.  Gaia DR2 record for this source at VizieR.
  2. ↑ 2.0 2.1 2.2 2.3 2.4 2.5 2.6 Barbato, D. et al. (August 2018), "Exploring the realm of scaled solar system analogues with HARPS", Astronomy & Astrophysics 615: 21, doi:10.1051/0004-6361/201832791, A175, Bibcode: 2018A&A...615A.175B. 
  3. ↑ 3.0 3.1 Houk, Nancy (1979), Michigan catalogue of two-dimensional spectral types for the HD stars, 3, Ann Arbor, Michigan: Department of Astronomy, University of Michigan, Bibcode: 1982mcts.book.....H. 
  4. ↑ 4.0 4.1 4.2 Anderson, E.; Francis, Ch. (2012), "XHIP: An extended hipparcos compilation", Astronomy Letters 38 (5): 331, doi:10.1134/S1063773712050015, Bibcode: 2012AstL...38..331A. 
  5. ↑ "HD 187085". SIMBAD. Centre de données astronomiques de Strasbourg. http://simbad.u-strasbg.fr/simbad/sim-basic?Ident=HD+187085. 
  6. ↑ 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, doi:10.1111/j.1365-2966.2006.10298.x, Bibcode: 2006MNRAS.369..249J, https://academic.oup.com/mnras/article/369/1/249/1053642. 
  7. ↑ 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, doi:10.1093/mnras/stx1449, Bibcode: 2017MNRAS.471.4494A. 
  8. ↑ Kóspál, Ágnes et al. (August 2009), "On the Relationship Between Debris Disks and Planets", The Astrophysical Journal Letters 700 (2): L73–L77, doi:10.1088/0004-637X/700/2/L73, Bibcode: 2009ApJ...700L..73K.