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HD 106252

Coordinates: Sky map 12h 13m 29.5093s, +10° 02′ 29.898″
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HD 106252
Observation data
Epoch J2000Ā Ā Ā Ā Ā Ā Equinox ICRS
Constellation Virgo[1]
Right ascension 12h 13m 29.510s[2]
Declination +10° 02′ 29.89″[2]
ApparentĀ magnitudeĀ (V) 7.41[1]
Characteristics
EvolutionaryĀ stage main sequence[2]
SpectralĀ type G0V[3]
Bāˆ’V color index 0.635±0.007[4]
Astrometry
Radial velocity (Rv)15.44±0.11[5] km/s
Proper motion (μ) RA: +23.315 mas/yr[2]
Dec.:Ā āˆ’279.896 mas/yr[2]
Parallax (Ļ€)15.2484±0.00268Ā mas[2]
Distance213.90 ± 0.04 ly
(65.58 ± 0.01 pc)
AbsoluteĀ magnitudeĀ (MV)4.53[1]
Details
Mass1.05±0.02[6]Ā Mā˜‰
Radius1.096[3]Ā Rā˜‰
Luminosity1.328±0.030[6]Ā Lā˜‰
Surface gravity (log g)4.40±0.15[4] cgs
Temperature5,890±50[4] K
Metallicity [Fe/H]āˆ’0.06±0.04[6]Ā dex
Rotation22.8 d[3]
Rotational velocity (v sin i)1.74±0.25[4] km/s
Age3.00+0.8
āˆ’0.6
[6]Ā Gyr
Other designations
BD+10°2392, HD 106252, HIP 59610, SAO 99998, LTT 13402, NLTT 30020[7]
Database references
SIMBADdata
Exoplanet Archivedata

HD 106252 is a star with a brown dwarf[8] companion in the constellation Virgo. An apparent visual magnitude of 7.41[1] means this star is too faint to be visible to the naked eye. It is located at a distance of 210Ā light years from the Sun based on parallax measurements, and is receding with a radial velocity of 15Ā km/s.[5]

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 2Ā km/s.[4] It is radiating 1.3[6] times the luminosity of the Sun from its photosphere at an effective temperature of 5,890Ā 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 30.6Ā MJ, in the brown dwarf range.[8] More accurate astrometry from Gaia in 2021 revealed a smaller true mass of 10.0Ā 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
āˆ’0.73
Ā MJ
2.655±0.017 4.202+0.011
āˆ’0.010
0.480±0.010 46.0+4.9
āˆ’4.1
—

References

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  1. 1 2 3 4 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. S2CIDĀ 119257644.
  2. 1 2 3 4 5 6 Vallenari, A.; etĀ al. (Gaia collaboration) (2023). "Gaia Data Release 3. Summary of the content and survey properties". Astronomy and Astrophysics. 674: A1. arXiv:2208.00211. Bibcode:2023A&A...674A...1G. doi:10.1051/0004-6361/202243940. S2CIDĀ 244398875. Gaia DR3 record for this source at VizieR.
  3. 1 2 3 4 5 6 Fischer, Debra A.; etĀ 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. 1 2 3 4 5 6 7 8 Perrier, C.; etĀ 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. S2CIDĀ 6946291.
  5. 1 2 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. S2CIDĀ 51814894.
  6. 1 2 3 4 5 6 7 8 9 Li, Yiting; etĀ 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. S2CIDĀ 237592581.
  7. ↑ "HD 106252". SIMBAD. Centre de donnĆ©es astronomiques de Strasbourg. Retrieved 2018-04-12.
  8. 1 2 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. S2CIDĀ 54986291. A140.
  9. ↑ "Exoplanets: The Hunt Continues!" (Press release). Garching, Germany: European Southern Observatory. April 4, 2001. Retrieved December 27, 2012.
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