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HD 37320

From Wikipedia, the free encyclopedia
Blue giant star in the constellation Orion

HD 37320 (HR 1920, HIP 26487) is a star located in the constellationOrion.[a] It is an evolvedblue giant star, based on itsspectral type of B8III.[1] The distance to HD 37320 is calculated at 285.5parsecs (931 light-years), based on aparallax fromGaia EDR3.[2] Theapparent magnitude of the star is 5.852,[1] which is above thelimiting magnitude for naked-eye vision (6.5m), making it faintly visible to thenaked eye.[3]

HD 37320
Observation data
Epoch J2000      Equinox J2000
ConstellationOrion[a]
Right ascension05h 38m 01.12s[1]
Declination+07° 32′ 29.1″[1]
Apparent magnitude (V)5.852±0.009[1]
Characteristics
Evolutionary stageBlue giant
Spectral typeB7III[1]
Apparent magnitude (U)5.44[1]
Apparent magnitude (B)5.788[1]
Apparent magnitude (G)5.844[1]
Apparent magnitude (J)5.933[1]
Apparent magnitude (H)5.997[1]
Apparent magnitude (K)5.964[1]
Astrometry
Radial velocity (Rv)20.1±1[4] km/s
Proper motion (μ)RA: 10.602mas/yr[4]
Dec.: -15.499mas/yr[4]
Parallax (π)3.5025±0.0568 mas[2]
Distance930 ± 20 ly
(286 ± 5 pc)
Absolute magnitude (MV)-1.43[5]
Details
Mass5.644±0.282[6] M
Radius4.696[b] R
Luminosity218.78[8] L
Temperature12,303[8] K
Rotational velocity (v sin i)25[9] km/s
Other designations
BD+07 953,Gaia DR2 3334369174165649536,Gaia DR3 3334369174165649536,HIP 26487,HR 1920,SAO 112979,PPM 149251,TIC 144611068,TYC 714-524-1,GSC 00714-00524,2MASS J05380112+0732292
Database references
SIMBADdata

Characteristics

[edit]

It is an evolvedblue giant star with aspectral type of B8III.[1] It radiates about 219 times thesolar luminosity by its photosphere at aneffective temperature of 12,300 K.[8] Its uniform diskangular diameter is measured at 0.153 milliarcseconds.[7] At the estimated distance by Gaia EDR3, it yields a physical size of 4.696 R. The star has a mass of 5.644 M[6] and rotates under its own axis at a speed of 25 km/s.[9]

HD 37320 is located within the constellation Orion, based on itsastronomical coordinates.[a] The distance to the star is 285.5parsecs (931light-years), based on a parallax of3.5025 mas fromGaia EDR3.[2] Theapparent magnitude of the star, i.e. its brightness as seen from Earth, is of 5.852m,[1] which is above the limiting magnitude for naked-eye vision, generally defined as 6.5m, making it faintly visible to thenaked eye.[3] Theabsolute magnitude of HD 37320, i.e. its brightness if it was seen at 10 parsecs (32.6 ly), is -1.43.[5] It is moving away from Earth at a velocity of 20.1 km/s.[4]

HD 37320 is theHenry Draper Catalogue designation for this star. Other designations include HR 1920 from theBright Star Catalogue, HIP 26487 from theHipparcos Catalogue and BD+07 953 from theBonner Durchmusterung catalogue.[1]

Notes

[edit]
  1. ^abcObtained with a right ascension of05h 38m 01.12s and a declination of +07° 32′ 29.1″[1] on thiswebsite.
  2. ^From an angular diameter of 0.153milliarcseconds[7] and a distance of 285.5parsecs.[2]

References

[edit]
  1. ^abcdefghijklmnop"HD 37320".SIMBAD.Centre de données astronomiques de Strasbourg. Retrieved2024-05-05.
  2. ^abcdBrown, A. G. A.; et al. (Gaia collaboration) (2021)."Gaia Early Data Release 3: Summary of the contents and survey properties".Astronomy & Astrophysics.649: A1.arXiv:2012.01533.Bibcode:2021A&A...649A...1G.doi:10.1051/0004-6361/202039657.S2CID 227254300. (Erratum: doi:10.1051/0004-6361/202039657e). Gaia EDR3 record for this source atVizieR.
  3. ^ab"University Lowbrow Astronomers Naked Eye Observer's Guide".websites.umich.edu. Retrieved2024-05-05.
  4. ^abcBrandt, Timothy D. (2021-06-01)."The Hipparcos-Gaia Catalog of Accelerations: Gaia EDR3 Edition".The Astrophysical Journal Supplement Series.254 (2): 42.arXiv:2105.11662.Bibcode:2021ApJS..254...42B.doi:10.3847/1538-4365/abf93c.ISSN 0067-0049. Data about this star is availablehere at VizieR.
  5. ^ab"HIP-26487 (Star)".In-the-sky. Retrieved2024-05-05.
  6. ^abKervella, Pierre; Arenou, Frédéric; Mignard, François; Thévenin, Frédéric (2019-03-01)."Stellar and substellar companions of nearby stars from Gaia DR2. Binarity from proper motion anomaly".Astronomy and Astrophysics.623: A72.arXiv:1811.08902.Bibcode:2019A&A...623A..72K.doi:10.1051/0004-6361/201834371.ISSN 0004-6361. Data about the star is availablehere at VizieR.
  7. ^abChallouf, M.; Nardetto, N.; Mourard, D.; Graczyk, D.; Aroui, H.; Chesneau, O.; Delaa, O.; Pietrzyński, G.; Gieren, W.; Ligi, R.; Meilland, A.; Perraut, K.; Tallon-Bosc, I.; McAlister, H.; Brummelaar, T. ten (2014-10-01)."Improving the surface brightness-color relation for early-type stars using optical interferometry".Astronomy & Astrophysics.570: A104.arXiv:1409.1351.Bibcode:2014A&A...570A.104C.doi:10.1051/0004-6361/201423772.ISSN 0004-6361.
  8. ^abcSimón-Díaz, S.; Godart, M.; Castro, N.; Herrero, A.; Aerts, C.; Puls, J.; Telting, J.; Grassitelli, L. (2017-01-01)."The IACOB project . III. New observational clues to understand macroturbulent broadening in massive O- and B-type stars".Astronomy and Astrophysics.597: A22.arXiv:1608.05508.Bibcode:2017A&A...597A..22S.doi:10.1051/0004-6361/201628541.ISSN 0004-6361. Data about the star is availablehere at VizieR.
  9. ^abAbt, Helmut A.; Levato, Hugo; Grosso, Monica (2002-07-01)."Rotational Velocities of B Stars".The Astrophysical Journal.573 (1):359–365.Bibcode:2002ApJ...573..359A.doi:10.1086/340590.ISSN 0004-637X. Availablehere in VizieR.
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