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HD 106252 is a star with a brown dwarf[8] companion in the constellation Virgo. An apparent visual magnitude of 7.41[2] means this star is too faint to be visible to the naked eye. It is located at a distance of 210 light years from the Sun based on parallax measurements, and is receding with a radial velocity of 15 km/s.[5]

HD 106252
Observation data
Epoch J2000      Equinox J2000
Constellation Virgo
Right ascension 12h 13m 29.510s[1]
Declination +10° 02′ 29.88″[1]
Apparent magnitude (V) 7.41[2]
Characteristics
Spectral type G0V[3]
B−V color index 0.635±0.007[4]
Astrometry
Radial velocity (Rv)15.44±0.11[5] km/s
Proper motion (μ) RA: 22.863 mas/yr[1]
Dec.: −280.009 mas/yr[1]
Parallax (π)15.533 ± 0.0048 mas[1]
Distance209.98 ± 0.06 ly
(64.38 ± 0.02 pc)
Absolute magnitude (MV)4.53[2]
Details
Mass1.05±0.02[6] M☉
Radius1.096[3] R☉
Luminosity1.328±0.030[6] L☉
Surface gravity (log g)4.40±0.15[4] cgs
Temperature5,890±50[4] K
Metallicity [Fe/H]−0.06±0.04[6] dex
Rotation22.8 d[3]
Rotational velocity (v sin i)1.74±0.25[4] km/s
Age3.00+0.8
−0.6[6] Gyr
Other designations
BD+10° 2392, HD 106252, HIP 59610, SAO 99998, LTT 13402, NLTT 30020[7]
Database references
SIMBADdata
Exoplanet Archivedata

The stellar classification of HD 106252 is G0V,[3] matching an ordinary G-type main-sequence star. It has 5%[6] more mass than the Sun and 10%[3] greater in girth. This star is about three[6] billion years old with a low level of magnetic activity[4] and is spinning with a projected rotational velocity of 2 km/s.[4] It is radiating 1.3[6] times the luminosity of the Sun from its photosphere at an effective temperature of 5,890 K.[4]

In 2001, a massive sub-stellar companion was announced orbiting the star by the European Southern Observatory.[9][4] The discovery was confirmed by a different team using the Lick Telescope.[3] Astrometric observations from Hipparcos in 2011 suggested that its true mass is likely around 30.6 MJ, in the brown dwarf range.[8] More accurate astrometry from Gaia in 2021 revealed a smaller true mass of 10.0 MJ.[6]

The HD 106252 planetary system[6]
Companion
(in order from star)		 Mass Semimajor axis
(AU)		 Orbital period
(years)		 Eccentricity Inclination Radius
b 10.00+0.78
−0.73 MJ		 2.655±0.017 4.202+0.011
−0.010		 0.480±0.010 46.0+4.9
−4.1°		 —

References


  1. 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.
  2. 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.
  3. Fischer, Debra A.; et al. (2002). "Planetary Companions to HD 136118, HD 50554, and HD 106252". Publications of the Astronomical Society of the Pacific. 114 (795): 529–535. Bibcode:2002PASP..114..529F. doi:10.1086/341677.
  4. Perrier, C.; et al. (2003). "The ELODIE survey for northern extra-solar planets. I. Six new extra-solar planet candidates". Astronomy and Astrophysics. 410 (3): 1039–1049. arXiv:astro-ph/0308281. Bibcode:2003A&A...410.1039P. doi:10.1051/0004-6361:20031340. S2CID 6946291.
  5. Nidever, David L.; Marcy, Geoffrey W.; Butler, R. Paul; Fischer, Debra A.; Vogt, Steven S.; McGahee, C. E.; O'Donoghue, A. A.; Knox, E. R. (2002). "Radial Velocities for 889 Late-Type Stars". The Astrophysical Journal Supplement Series. 141 (2): 503–522. arXiv:astro-ph/0112477. Bibcode:2002ApJS..141..503N. doi:10.1086/340570. S2CID 51814894.
  6. Li, Yiting; et al. (2021). "Precise Masses and Orbits for Nine Radial-velocity Exoplanets". The Astronomical Journal. 162 (6): 266. arXiv:2109.10422. Bibcode:2021AJ....162..266L. doi:10.3847/1538-3881/ac27ab. S2CID 237592581.
  7. "HD 106252". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2018-04-12.
  8. Reffert, S.; Quirrenbach, A. (March 2011). "Mass constraints on substellar companion candidates from the re-reduced Hipparcos intermediate astrometric data: nine confirmed planets and two confirmed brown dwarfs". Astronomy & Astrophysics. 527: 22. arXiv:1101.2227. Bibcode:2011A&A...527A.140R. doi:10.1051/0004-6361/201015861. A140.
  9. "Exoplanets: The Hunt Continues!" (Press release). Garching, Germany: European Southern Observatory. April 4, 2001. Retrieved December 27, 2012.



На других языках

[de] HD 106252

HD 106252 ist ein etwa 120 Lichtjahre von der Erde entfernter Gelber Zwerg mit einer Rektaszension von 12h 13m 30s und einer Deklination von +10° 02′ 30″ im Sternbild Virgo. Er besitzt eine scheinbare Helligkeit von rund 7,4 mag. Im Jahre 2002 entdeckten Fischer et al. mit Hilfe der Radialgeschwindigkeitsmethode einen vermutlich substellaren Begleiter, der diesen Stern mit einer Umlaufperiode von rund 1500 Tagen umrundet. Dieser trägt die systematische Bezeichnung HD 106252 b und weist eine Mindestmasse von ungefähr 7 Jupitermassen auf. Nach astrometrischen Abschätzungen der Masse handelt es sich dabei höchstwahrscheinlich um einen Braunen Zwerg.[4]
- [en] HD 106252

[ru] HD 106252

HD 106252 — звезда, которая находится в созвездии Девы на расстоянии около 122 световых года от нас. Вокруг звезды обращается, как минимум, одна планета.


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