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HD 112410 is a star in the southern constellation of Musca. It has a yellow hue and is too dim to be readily visible to the average sight, having an apparent visual magnitude of 6.86.[2] The distance to this star is 513 light years based on parallax, and it is drifting further away from the Sun with a radial velocity of 73 km/s.[1] It has an absolute magnitude of 1.22.[2]

HD 112410
Observation data
Epoch J2000      Equinox J2000
Constellation Musca
Right ascension 12h 57m 31.95991s[1]
Declination −65° 38′ 47.2594″[1]
Apparent magnitude (V) 6.86[2]
Characteristics
Evolutionary stage red giant branch
Spectral type G8III[3]
B−V color index 1.018±0.008[2]
Astrometry
Radial velocity (Rv)72.82±0.15[1] km/s
Proper motion (μ) RA: −65.486±0.043[1] mas/yr
Dec.: +31.269±0.038[1] mas/yr
Parallax (π)6.3628 ± 0.0284 mas[1]
Distance513 ± 2 ly
(157.2 ± 0.7 pc)
Absolute magnitude (MV)1.22[2]
Details[4]
Mass1.21±0.25[4]
1.54±0.05[5]
2.32±0.23[6] M☉
Radius10.28+0.11
−0.17[1] R☉
Luminosity50.5±0.4[1] L☉
Surface gravity (log g)2.49±0.06 cgs
Temperature4,793±22 K
Metallicity [Fe/H]−0.28±0.05 dex
Rotational velocity (v sin i)3.29±0.47 km/s
Age4.17±2.34 Myr
Other designations
CD−64° 676, GC 17573, HD 112410, HIP 63242, SAO 252106, 2MASS J12573196-6538472[7]
Database references
SIMBADdata

This is an aging giant star with a stellar classification of G8III.[3] It is cooling and expanding along the red giant branch,[5] having evolved off the main sequence after exhausting its core supply of hydrogen fuel. At present it has 10[1] times the Sun's radius. Mass estimates range from 1.21[4] up to 2.32[6] times the mass of the Sun. The star has a lower metallicity the Sun – what astronomers term the abundance of elements with more mass than helium – and it is spinning with a projected rotational velocity of 3.3 km/s.[4] It is radiating 50.5[1] times the luminosity of the Sun from its enlarged photosphere at an effective temperature of 4,793 K.[4]


Planetary system


HD 112410 has a substellar companion calculated to have a mass at least 9.2 times that of Jupiter and an orbital period of 124.6 days at a typical separation of approximately 0.57 astronomical units (AU). As of 2013, this is the nearest exoplanet orbiting around any ascending red giant branch star, and second-closest planet to a giant star after the companion of HIP 13044.[5]

The HD 112410 planetary system
Companion
(in order from star)		 Mass Semimajor axis
(AU)		 Orbital period
(days)		 Eccentricity Inclination Radius
HD 112410 b >9.18 MJ 0.565 124.6 0.23 — —

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. Houk, Nancy (1979). Michigan catalogue of two-dimensional spectral types for the HD stars. Vol. 1. Ann Arbor, Michigan: Department of Astronomy, University of Michigan. Bibcode:1978mcts.book.....H.
  4. Jofré, E.; et al. (2015). "Stellar parameters and chemical abundances of 223 evolved stars with and without planets". Astronomy & Astrophysics. 574: A50. arXiv:1410.6422. Bibcode:2015A&A...574A..50J. doi:10.1051/0004-6361/201424474. S2CID 53666931.
  5. Jones, M. I.; et al. (2013). "Study of the Impact of the Post-MS evolution of the Host Star on the Orbits of Close-in Planets. II. A Giant Planet in a Close-in Orbit around the RGB Star HIP 63242". Astronomy & Astrophysics. 556 (A78): 5. arXiv:1306.3939. Bibcode:2013A&A...556A..78J. doi:10.1051/0004-6361/201321660. S2CID 118618692.
  6. Sousa, S. G.; et al. (November 2018). "SWEET-Cat updated. New homogenous spectroscopic parameters". Astronomy & Astrophysics. 620: 13. arXiv:1810.08108. Bibcode:2018A&A...620A..58S. doi:10.1051/0004-6361/201833350. S2CID 119374557. A58.
  7. "HD 112410". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2020-08-04.

На других языках

- [en] HD 112410

[ru] HD 112410

HD 112410 — звезда жёлтый гигант созвездия Мухи[2]. Звезда находится от нас на расстоянии 513 световых лет, она удаляется от Солнца с лучевой скоростью 73 км/с[1]. Имеет абсолютную звёздную величину 1,22[2].


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