HD 16175

Last updated
HD 16175 / Buna
Observation data
Epoch J2000.0       Equinox J2000.0
Constellation Andromeda
Right ascension 02h 37m 01.91118s [1]
Declination +42° 03′ 45.4685″ [1]
Apparent magnitude  (V)7.28 [2]
Characteristics
Spectral type F8 IV [3]
B−V color index 0.64 [2]
Astrometry
Radial velocity (Rv)21.83±0.14 [1]  km/s
Proper motion (μ)RA: −38.864  mas/yr [1]
Dec.: −41.234  mas/yr [1]
Parallax (π)16.6670 ± 0.0279  mas [1]
Distance 195.7 ± 0.3  ly
(60.0 ± 0.1  pc)
Absolute magnitude  (MV)3.40 [4]
Details
Mass 1.34 ± 0.01 [5]   M☉
Radius 1.66 ± 0.04 [5]   R☉
Luminosity 3.3 ± 0.01 [5]   L☉
Surface gravity (log g)4.12 ± 0.03 [5]   cgs
Temperature 6048 ± 35 [5]   K
Age 3.2 ± 0.2 [5]   Gyr
Other designations
BD+41°496, HIP 12191, SAO 38170
Database references
SIMBAD data

HD 16175 is a 7th magnitude G-type star with temperature about 6000 K located 196 light-years (60 parsecs ) away [1] in the Andromeda constellation. This star is only visible through binoculars or better equipment; it is also 3.3 times more luminous, is 1.34 times more massive, and has a radius 1.66 times bigger than our local star. [5]

Contents

The star HD 16175 is named Buna. The name was selected in the NameExoWorlds campaign by Ethiopia, during the 100th anniversary of the IAU. Buna is the commonly used word for coffee in Ethiopia. [6] [7]

Planetary system

The discovery of the exoplanet HD 16175 b was published in the June 2009 issue of the Publications of the Astronomical Society of the Pacific . [4] The planetary parameters were updated in 2016. [8] In 2023, the inclination and true mass of HD 16175 b were determined via astrometry. [9]

The HD 16175 planetary system [9]
Companion
(in order from star)		 Mass Semimajor axis
(AU)		 Orbital period
(years)		 Eccentricity Inclination Radius
b / Abol 5.9+1.8
−1.0  MJ 		2.13+0.075
−0.08		2.686+0.031
−0.039		0.675±0.02659+20
−19 or 121+19
−20 ° 		—

See also

Related Research Articles

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HD 16175 b is an exoplanet located approximately 195.7 light-years away in the constellation of Andromeda, orbiting the star HD 16175. This planet has a minimum mass 4.8 times that of Jupiter; the true mass was initially unknown since the inclination of the orbit was unknown. This planet orbits at about 2.2 astronomical units, taking 2.73 years to revolve around the star. The orbit of the planet is highly elliptical with an eccentricity of 0.64. In 2023, the inclination and true mass of HD 16175 b were determined via astrometry.

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References

  1. 1 2 3 4 5 6 7 Vallenari, A.; et al. (Gaia Collaboration) (2022). "Gaia Data Release 3. Summary of the content and survey properties". Astronomy & Astrophysics . arXiv: 2208.00211 . doi: 10.1051/0004-6361/202243940 . Gaia DR3 record for this source at VizieR.
  2. 1 2 Høg, E.; Fabricius, C.; Makarov, V. V.; Urban, S.; Corbin, T.; Wycoff, G.; Bastian, U.; Schwekendiek, P.; Wicenec, A. (2000), "The Tycho-2 catalogue of the 2.5 million brightest stars", Astronomy & Astrophysics, 355: L27–L30, Bibcode:2000A&A...355L..27H.
  3. ↑ Van Belle, Gerard T.; von Braun, Kaspar (2009). "Directly Determined Linear Radii and Effective Temperatures of Exoplanet Host Stars". The Astrophysical Journal. 694 (2): 1085–1098. arXiv: 0901.1206 . Bibcode:2009ApJ...694.1085V. doi:10.1088/0004-637X/694/2/1085. S2CID   18370219.
  4. 1 2 Peek, Kathryn M. G.; et al. (2009). "Old, rich, and eccentric: two jovian planets orbiting evolved metal-rich stars". Publications of the Astronomical Society of the Pacific. 121 (880): 613–620. arXiv: 0904.2786 . Bibcode:2009PASP..121..613P. doi:10.1086/599862. S2CID   12042779.
  5. 1 2 3 4 5 6 7 Bonfanti, A.; et al. (2015). "Revising the ages of planet-hosting stars". Astronomy and Astrophysics. 575. A18. arXiv: 1411.4302 . Bibcode:2015A&A...575A..18B. doi:10.1051/0004-6361/201424951. S2CID   54555839.
  6. ↑ "Approved names". NameExoworlds. Retrieved 2020-01-02.
  7. ↑ "International Astronomical Union | IAU". www.iau.org. Retrieved 2020-01-02.
  8. ↑ Díaz, Rodrigo F.; Rey, Javiera; Demangeon, Olivier D. S.; Hébrard, Guillaume; Boisse, Isabelle; Arnold, Luc; Astudillo-Defru, Nicola; Beuzit, Jean-Luc; Bonfils, Xavier; Borgniet, Simon; Bouchy, François; Bourrier, Vincent; Courcol, Bastien; Deleuil, Magali; Delfosse, Xavier; Ehrenreich, David; Forveille, Thierry; Lagrange, Anne-Marie; Mayor, Michel; Moutou, Claire; Pepe, Francesco; Queloz, Didier; Santerne, Alexandre; Santos, Nuno C.; Sahlmann, Johannes; Ségransan, Damien; Udry, Stéphane; Wilson, Paul A. (2016). "The SOPHIE search for northern extrasolar planets XI. Three new companions and an orbit update: Giant planets in the habitable zone". Astronomy & Astrophysics. 591: A146. arXiv: 1604.07610 . Bibcode:2016A&A...591A.146D. doi:10.1051/0004-6361/201628331. S2CID   3282336.
  9. 1 2 Xiao, Guang-Yao; Liu, Yu-Juan; et al. (May 2023). "The Masses of a Sample of Radial-Velocity Exoplanets with Astrometric Measurements". Research in Astronomy and Astrophysics . 23 (5): 055022. arXiv: 2303.12409 . Bibcode:2023RAA....23e5022X. doi:10.1088/1674-4527/accb7e.
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