HD_106252 Latitude and Longitude:

Sky map 12h 13m 29.5093s, +10° 02′ 29.898″
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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
SIMBAD data
Exoplanet Archive data

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]

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. ^ a b c d 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. ^ 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.
  3. ^ a b c d e f 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. ^ a b c d e f g h 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. ^ a b 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. ^ a b c d e f g h i 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. ^ a b 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. S2CID  54986291. A140.
  9. ^ "Exoplanets: The Hunt Continues!" (Press release). Garching, Germany: European Southern Observatory. April 4, 2001. Retrieved December 27, 2012.

External links