B-type main-sequence star; Triangulum
HD 10390Location of HD 10390 on the map (circled)
Observation dataEpoch J2000.0 Equinox J2000.0 (ICRS ) Constellation Triangulum Right ascension 01h 42m 03.48964s [ 1] Declination +35° 14′ 44.5389″[ 1] Apparent magnitude (V)5.64[ 2] Characteristics Evolutionary stage main sequence star [ 3] Spectral type B9 IV-V[ 4] or B9 V[ 5] U−Bcolor index −0.20[ 2] B−Vcolor index −0.07[ 2] Astrometry Radial velocity (Rv )−1.9± 2.0[ 6] km/s Proper motion (μ)RA: +48.763mas /yr [ 1] Dec.: −25.418mas /yr [ 1] Parallax (π)11.1882± 0.164 mas [ 1] Distance 292 ± 4 ly (89 ± 1 pc ) Absolute magnitude (MV )+1.00[ 7] Details Mass 2.62[ 8] M ☉ Radius 2.14± 0.11[ 9] R ☉ Luminosity 51.5+2.4 −2.3 [ 3] L ☉ Surface gravity (log g )4.23+0.08 −0.04 [ 10] cgs Temperature 11,076± 139[ 11] K Metallicity [Fe/H]−0.20[ 12] dex Rotational velocity (v sin i )45[ 13] km/s Age 50+81 −31 [ 14] Myr Other designations 6 H. Trianguli ,[ 15] AG +34°163 ,BD +34°297 ,FK5 1047 ,GC 2064 ,HD 10390 ,HIP 7943 ,HR 490 ,SAO 54912 ,TIC 61524043[ 16] Database references SIMBAD data
HD 10390 (HR 490; 51 H. Trinaguli ) is a solitarystar [ 17] located in the northernconstellation Triangulum . It is faintly visible to thenaked eye as a bluish-white hued point of light with anapparent magnitude of 5.64.[ 2] The object is located relatively close at a distance of 292light-years based onGaia DR3 parallax measurements[ 1] and it is drifting closer with a heliocentricradial velocity of −1.9 km/s .[ 6] At its current distance, HD 10390's brightness is diminished by aninterstellar extinction of only five-hundredths of amagnitude [ 18] and it has anabsolute magnitude of +1.00.[ 7]
HD 10390 has astellar classification of B9 IV-V,[ 4] indicating that it is a slightlyevolved B-type star with aluminosity class intermediate between asubgiant and amain sequence star . Osawa (1959) gave a class of B9 V,[ 5] instead indicating that it is an ordinaryB-type main-sequence star that is generating energy viahydrogen fusion at itscore . It has 2.62 times themass of the Sun [ 8] and 2.14 times theradius of the Sun .[ 9] It radiates 51.5 times theluminosity of the Sun [ 3] from itsphotosphere at aneffective temperature of 11,076 K .[ 11] HD 10390 is metal defecient with aniron abundance of [Fe/H] = −0.2 or 63.1% of theSun 's[ 12] and it spins modestly with aprojected rotational velocity of 45 km/s ,[ 13] well below itsbreakup velocity of 355 km/s.[ 19] Despite the first classification, HD 10390 has only completed 16.8% of itsmain sequence lifetime[ 3] at the age of approximately 50million years .[ 14]
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(November 1972)."Spectral classification of the bright B8 stars" .The Astronomical Journal .77 : 750.Bibcode :1972AJ.....77..750C .doi :10.1086/111348 .ISSN 0004-6256 . ^a b Osawa, Kiyoteru (July 1959)."Spectral Classification of 533 B8-A2 Stars and the Mean Absolute Magnitude of A0 V Stars" .The Astrophysical Journal .130 . American Astronomical Society: 159.Bibcode :1959ApJ...130..159O .doi :10.1086/146706 .ISSN 0004-637X .S2CID 120004061 . ^a b Wilson, Ralph Elmer (1953). "General catalogue of stellar radial velocities".Carnegie Institute Washington D.C. Publication : 0.Bibcode :1953GCRV..C......0W .S2CID 120000732 . ^a b Anderson, E.; Francis, Ch. (May 2012). "XHIP: An extended hipparcos compilation".Astronomy Letters .38 (5):331– 346.arXiv :1108.4971 .Bibcode :2012AstL...38..331A .doi :10.1134/S1063773712050015 .eISSN 1562-6873 .ISSN 1063-7737 .S2CID 119257644 . ^a b David, Trevor J.; Hillenbrand, Lynne A. 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