Movatterモバイル変換


[0]ホーム

URL:


Jump to content
WikipediaThe Free Encyclopedia
Search

HD 10390

From Wikipedia, the free encyclopedia
B-type main-sequence star; Triangulum
HD 10390
Location of HD 10390 on the map (circled)
Observation data
EpochJ2000.0      EquinoxJ2000.0 (ICRS)
ConstellationTriangulum
Right ascension01h 42m 03.48964s[1]
Declination+35° 14′ 44.5389″[1]
Apparent magnitude (V)5.64[2]
Characteristics
Evolutionary stagemain sequence star[3]
Spectral typeB9 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]
Distance292 ± 4 ly
(89 ± 1 pc)
Absolute magnitude (MV)+1.00[7]
Details
Mass2.62[8] M
Radius2.14±0.11[9] R
Luminosity51.5+2.4
−2.3
[3] L
Surface gravity (log g)4.23+0.08
−0.04
[10] cgs
Temperature11,076±139[11] K
Metallicity [Fe/H]−0.20[12] dex
Rotational velocity (v sin i)45[13] km/s
Age50+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
SIMBADdata

HD 10390 (HR 490; 51 H. Trinaguli) is a solitarystar[17] located in the northernconstellationTriangulum. 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 DR3parallax 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 slightlyevolvedB-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 of11,076 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 of45 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]

References

[edit]
  1. ^abcdeVallenari, A.; et 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.S2CID 244398875. Gaia DR3 record for this source atVizieR.
  2. ^abcdDucati, J. R. (2002). "VizieR Online Data Catalog: Catalogue of Stellar Photometry in Johnson's 11-color system".VizieR Online Data Catalog.2237.Bibcode:2002yCat.2237....0D.
  3. ^abcdZorec, J.; Royer, F. (January 2012)."Rotational velocities of A-type stars IV: Evolution of rotational velocities".Astronomy & Astrophysics.537: A120.arXiv:1201.2052.Bibcode:2012A&A...537A.120Z.doi:10.1051/0004-6361/201117691.eISSN 1432-0746.ISSN 0004-6361.S2CID 55586789.
  4. ^abCowley, A. (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.
  5. ^abOsawa, 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.
  6. ^abWilson, Ralph Elmer (1953). "General catalogue of stellar radial velocities".Carnegie Institute Washington D.C. Publication: 0.Bibcode:1953GCRV..C......0W.S2CID 120000732.
  7. ^abAnderson, 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.
  8. ^abDavid, Trevor J.; Hillenbrand, Lynne A. (12 May 2015)."The Ages of Early-type Stars: Strömgren Photometric Methods Calibrated, Validated, Tested, and Applied to Hosts and Prospective Hosts of Directly Imaged Exoplanets".The Astrophysical Journal.804 (2): 146.arXiv:1501.03154.Bibcode:2015ApJ...804..146D.doi:10.1088/0004-637X/804/2/146.eISSN 1538-4357.S2CID 33401607.
  9. ^abKervella, P.; Thévenin, F.; Di Folco, E.; Ségransan, D. (April 8, 2004)."The angular sizes of dwarf stars and subgiants: Surface brightness relations calibrated by interferometry".Astronomy & Astrophysics.426 (1):297–307.arXiv:astro-ph/0404180.Bibcode:2004A&A...426..297K.doi:10.1051/0004-6361:20035930.eISSN 1432-0746.ISSN 0004-6361.S2CID 6077801.
  10. ^Stassun, Keivan G.; et al. (9 September 2019)."The RevisedTESS Input Catalog and Candidate Target List".The Astronomical Journal.158 (4): 138.arXiv:1905.10694.Bibcode:2019AJ....158..138S.doi:10.3847/1538-3881/ab3467.eISSN 1538-3881.hdl:1721.1/124721.S2CID 166227927.
  11. ^abPaunzen, E.; Schnell, A.; Maitzen, H. M. (December 2005)."An empirical temperature calibration for the Δa photometric system I: The B-type stars".Astronomy & Astrophysics.444 (3):941–946.arXiv:astro-ph/0509049.Bibcode:2005A&A...444..941P.doi:10.1051/0004-6361:20053546.eISSN 1432-0746.ISSN 0004-6361.
  12. ^abAnders, F.; et al. (August 2019)."Photo-astrometric distances, extinctions, and astrophysical parameters forGaia DR2 stars brighter thanG = 18".Astronomy & Astrophysics.628: A94.arXiv:1904.11302.Bibcode:2019A&A...628A..94A.doi:10.1051/0004-6361/201935765.eISSN 1432-0746.ISSN 0004-6361.S2CID 131780028.
  13. ^abAbt, Helmut A.; Levato, Hugo; Grosso, Monica (July 2002)."Rotational Velocities of B Stars".The Astrophysical Journal.573 (1):359–365.Bibcode:2002ApJ...573..359A.doi:10.1086/340590.ISSN 0004-637X.
  14. ^abGrosbol, P. J. (June 1978). "Space velocities and ages of nearby early-type stars".Astronomy and Astrophysics Supplement Series.32:409–421.Bibcode:1978A&AS...32..409G.ISSN 0365-0138.
  15. ^Verbunt, F.; van Gent, R. H. (June 2010)."The star catalogue of Hevelius: Machine-readable version and comparison with the modern Hipparcos Catalogue".Astronomy and Astrophysics.516: A29.Bibcode:2010A&A...516A..29V.doi:10.1051/0004-6361/201014003.eISSN 1432-0746.ISSN 0004-6361.S2CID 54171435.
  16. ^"HD 10390".SIMBAD.Centre de données astronomiques de Strasbourg. RetrievedDecember 15, 2023.
  17. ^Eggleton, P. P.; Tokovinin, A. A. (11 September 2008)."A catalogue of multiplicity among bright stellar systems".Monthly Notices of the Royal Astronomical Society.389 (2):869–879.arXiv:0806.2878.Bibcode:2008MNRAS.389..869E.doi:10.1111/j.1365-2966.2008.13596.x.eISSN 1365-2966.ISSN 0035-8711.S2CID 14878976.
  18. ^Gontcharov, George A.; Mosenkov, Aleksandr V. (28 September 2017)."Verifying reddening and extinction for Gaia DR1 TGAS main sequence stars".Monthly Notices of the Royal Astronomical Society.472 (4):3805–3820.arXiv:1709.01160.Bibcode:2017MNRAS.472.3805G.doi:10.1093/mnras/stx2219.eISSN 1365-2966.ISSN 0035-8711.S2CID 118879856.
  19. ^Huang, Wenjin; Gies, D. R.; McSwain, M. V. (22 September 2010)."A Stellar Rotation Census of B Stars: From ZAMS to TAMS".The Astrophysical Journal.722 (1):605–619.arXiv:1008.1761.Bibcode:2010ApJ...722..605H.doi:10.1088/0004-637X/722/1/605.eISSN 1538-4357.ISSN 0004-637X.
Stars
Bayer
Flamsteed
Variable
HR
HD
Other
Exoplanets
Nebulae
Galaxies
NGC
Numbered
Other
Retrieved from "https://en.wikipedia.org/w/index.php?title=HD_10390&oldid=1266528251"
Categories:
Hidden categories:

[8]ページ先頭

©2009-2025 Movatter.jp