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HD 85945

Coordinates:Sky map09h 57m 13.61s, +57° 25′ 05.54″
From Wikipedia, the free encyclopedia
Giant star in the constellation Ursa Major
HD 85945
Observation data
Epoch J2000      Equinox J2000
ConstellationUrsa Major[1]
Right ascension09h 57m 13.61s[2]
Declination+57° 25′ 05.54″[2]
Apparent magnitude (V)5.959±0.009[2]
Characteristics
Evolutionary stageHorizontal branch[3]
Spectral typeG6III:Fe-0.5[2]
Apparent magnitude (B)6.854±0.015[2]
Apparent magnitude (G)5.733[2]
Apparent magnitude (J)4.513±0.028[2]
Apparent magnitude (H)4.141±0.036[2]
Apparent magnitude (K)3.978±0.3[2]
B−Vcolor index0.895[4]
Astrometry
Radial velocity (Rv)−46.55±0.12[5] km/s
Proper motion (μ)RA: 31.347mas/yr[5]
Dec.: -61.766mas/yr[5]
Parallax (π)7.4137±0.024 mas[5]
Distance432.08 ly
(132.54 pc)[5]
Absolute magnitude (MV)0.16[1]
Details
Mass2.5[3] M
Radius10.28±0.14[6] R
Luminosity77.62[7][a] L
Surface gravity (log g)2.6866[5] cgs
Temperature5281±22[6] K
Metallicity[Fe/H]–0.4[7] dex
Rotational velocity (v sin i)7.53[4] km/s
Age660.7[3][b] Myr
Other designations
BD+58 1224,Gaia DR2 1046383298937140864,Gaia DR3 1046383298937140864,HIP 48802,HR 3922,PPM 32387,TIC 377368616,TYC 3817-1649-1,GSC 03817-01649,IRAS 09537+5739
Database references
SIMBADdata

HD 85945 (HR 3922) is a star in the constellationUrsa Major. It is ayellow giant star with aspectral type of G6III:Fe-0.5. Based on information from Gaia DR3, it is located 132.54parsecs (432.3 ly) from Earth and is moving towards Earth at a velocity of 47 km/s. It has anapparent magnitude of 5.96, which makes it faintly visible to thenaked eye.

Characteristics

[edit]

It is an evolvedG-type giant star, based on itsspectral type of G6III:Fe-0.5, which also indicates that it has a [Fe/Hmetallicity of -0.5.[2] HD 85945 is 2.5 times more massive than the Sun and has expanded to 10.28 times the Sun's size.[3][6] It is emitting 78 times thesolar luminosity from its photosphere at aneffective temperature of 5,281 K.[7][6] Currently, the star is located in thehorizontal branch stage ofevolution.[3] The age of HD 85945 is estimated at 660 million years,[3] and it rotates under its axis at a speed of 7.53 km/s.[4] It is slightlymetal-poor compared to the Sun, with an abundance of iron equivalent to 40% of the solar abundance.[7][c]

HD 85945 is located within theUrsa Major constellation. The distance to HD 85945 is of 132.54parsecs (432.3 ly), based on spectra from Gaia DR3.[5] Theapparent magnitude of the star is of 5.96,[2] which is brighter than thelimiting magnitude for naked-eye vision (6.5m), making it faintly visible to thenaked eye.[8] The absolute magnitude, i.e. the brightness of the star if it was seen at a distance of 10 parsecs (32.6 ly), is 0.32.[9] At the current distance, its brightness is diminished by 0.03 magnitudes due tointerstellar extinction between Earth and the star.[6] HD 85945 is moving away from Earth at a velocity of 46.55 km/s.[5] It has a highproper motion in the sky.[6][2]

Notes

[edit]
  1. ^From a logarithm of 1.62.
  2. ^from a logarithm of 8.82.
  3. ^From a logarithm of -0.4

References

[edit]
  1. ^abAnderson, 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.
  2. ^abcdefghijkl"HD 85945".SIMBAD.Centre de données astronomiques de Strasbourg. RetrievedMay 7, 2024.
  3. ^abcdefStock, Stephan; Reffert, Sabine; Quirrenbach, Andreas (2018-08-01)."Precise radial velocities of giant stars. X. Bayesian stellar parameters and evolutionary stages for 372 giant stars from the Lick planet search".Astronomy and Astrophysics.616: A33.arXiv:1805.04094.Bibcode:2018A&A...616A..33S.doi:10.1051/0004-6361/201833111.ISSN 0004-6361. Data about this star is availablehere in VizieR.
  4. ^abcHekker, S.; Meléndez, J. (2007-12-01)."Precise radial velocities of giant stars. III. Spectroscopic stellar parameters".Astronomy and Astrophysics.475 (3):1003–1009.arXiv:0709.1145.Bibcode:2007A&A...475.1003H.doi:10.1051/0004-6361:20078233.ISSN 0004-6361. Data about this star is avalilablehere in VizieR.
  5. ^abcdefgVallenari, 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.
  6. ^abcdefRen, J. -J.; Raddi, R.; Rebassa-Mansergas, A.; Hernandez, M. S.; Parsons, S. G.; Irawati, P.; Rittipruk, P.; Schreiber, M. R.; Gänsicke, B. T.; Torres, S.; Wang, H. -J.; Zhang, J. -B.; Zhao, Y.; Zhou, Y. -T.; Han, Z. -W. (2020-12-01)."The White Dwarf Binary Pathways Survey. V. The Gaia White Dwarf Plus AFGK Binary Sample and the Identification of 23 Close Binaries".The Astrophysical Journal.905 (1): 38.arXiv:2010.02885.Bibcode:2020ApJ...905...38R.doi:10.3847/1538-4357/abc017.ISSN 0004-637X. Data about this star is availablehere in VizieR.
  7. ^abcdCharbonnel, C.; Lagarde, N.; Jasniewicz, G.; North, P. L.; Shetrone, M.; Krugler Hollek, J.; Smith, V. V.; Smiljanic, R.; Palacios, A.; Ottoni, G. (2020-01-01)."Lithium in red giant stars: Constraining non-standard mixing with large surveys in the Gaia era".Astronomy and Astrophysics.633: A34.arXiv:1910.12732.Bibcode:2020A&A...633A..34C.doi:10.1051/0004-6361/201936360.ISSN 0004-6361. Data about this star is availablehere in VizieR.
  8. ^"University Lowbrow Astronomers Naked Eye Observer's Guide".websites.umich.edu. Retrieved2024-05-07.
  9. ^Ford, Dominic."HIP-48802 (Star)".In-The-Sky.org. Retrieved2024-05-07.
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