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HD 32356

From Wikipedia, the free encyclopedia
Astrometric binary in Camelopardalis
HD 32356
Location of HD 32356 on the map (circled)
Observation data
EpochJ2000.0      EquinoxJ2000.0 (ICRS)
ConstellationCamelopardalis[1]
Right ascension05h 06m 29.70999s[2]
Declination+61° 10′ 11.0995″[2]
Apparent magnitude (V)5.99±0.01[3]
Characteristics
Spectral typeK5 II[4]
B−Vcolor index+1.36[5]
Astrometry
Radial velocity (Rv)−45.2±1.2[6] km/s
Proper motion (μ)RA: +39.428mas/yr[2]
Dec.: −80.907mas/yr[2]
Parallax (π)5.8511±0.0881 mas[2]
Distance557 ± 8 ly
(171 ± 3 pc)
Absolute magnitude (MV)+0.23[1]
Details
Mass1.18[7] M
Radius30.67±1.58[8] R
Luminosity300+9
−8
[2] L
Surface gravity (log g)1.56±0.11[9] cgs
Temperature4,111±13[10] K
Metallicity[Fe/H]−0.30±0.05[10] dex
Rotational velocity (v sin i)<1.0[11] km/s
Age4.27+0.86
−0.72
[9] Gyr
Other designations
AG+61°416,BD+60°857,GC 6202,HD 32356,HIP 23766,HR 1624,SAO 13369,TIC 286710338[12]
Database references
SIMBADdata

HD 32356, also designated asHR 1624, is anastrometric binary[13] located in the northerncircumpolar constellationCamelopardalis, the giraffe, nearβ Camelopardalis. The visible component is faintly visible to thenaked eye as an orange-huedstar with anapparent magnitude of 5.99.[3]Gaia DR3parallax measurements imply a distance of 557light-years[2] and it is currently drifting closer with a heliocentricradial velocity of−45.2 km/s.[6] At its current distance, HD 32356's brightness is diminished by aninterstellar extinction of 0.29magnitudes[14] and it has anabsolute magnitude of +0.23.[1]

The visible component has astellar classification of K5 II,[4] indicating that it is anevolvedK-typebright giant that has ceasedhydrogen fusion at itscore and left themain sequence. It has 1.18 times themass of the Sun[7] but at the age of 4.27billion years,[9] it has expanded to 30.67 times theradius of the Sun.[8] It radiates 300 times theluminosity of the Sun[2] from its enlargedphotosphere at aneffective temperature of4,111 K.[10] HD 32356 A is metal deficient with aniron abundance roughly half of theSun's[10] and it spins too slowly for itsprojected rotational velocity to be measured accurately.[11]

References

[edit]
  1. ^abcAnderson, 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. XHIP record for this object atVizieR.
  2. ^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.
  3. ^abHøg, E.; Fabricius, C.; Makarov, V. V.; Urban, S.; Corbin, T.; Wycoff, G.; Bastian, U.; Schwekendiek, P.; Wicenec, A. (March 2000). "The Tycho-2 catalogue of the 2.5 million brightest stars".Astronomy and Astrophysics.355:L27–L30.Bibcode:2000A&A...355L..27H.ISSN 0004-6361.S2CID 17128864.
  4. ^abBartaya, R. A. (1979). "Catalog of spectral and luminosity classes of 10396 stars in Kapteyn's selected areas NN 2-43".Abastumanskaia Astrofizicheskaia Observatoriia Byulleten.51: 1.Bibcode:1979AbaOB..51....1B.ISSN 0258-7327.
  5. ^Ljunggren, B.; Oja, T. (1965). "Photoelectric measurements of magnitudes and colours for 849 stars".Arkiv för Astronomi.3:439–465.Bibcode:1965ArA.....3..439L.ISSN 0004-2048.
  6. ^abGontcharov, G. A. (November 2006). "Pulkovo Compilation of Radial Velocities for 35,495 Hipparcos stars in a common system".Astronomy Letters.32 (11):759–771.arXiv:1606.08053.Bibcode:2006AstL...32..759G.doi:10.1134/S1063773706110065.eISSN 1562-6873.ISSN 1063-7737.S2CID 119231169.
  7. ^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.
  8. ^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.
  9. ^abcFeuillet, Diane K.; Bovy, Jo; Holtzman, Jon; Girardi, Léo; MacDonald, Nick; Majewski, Steven R.; Nidever, David L. (20 January 2016)."Determining Ages of APOGEE Giants with Known Distances".The Astrophysical Journal.817 (1): 40.arXiv:1511.04088.Bibcode:2016ApJ...817...40F.doi:10.3847/0004-637X/817/1/40.eISSN 1538-4357.S2CID 118675933.
  10. ^abcdWu, Yue; Singh, H. P.; Prugniel, P.; Gupta, R.; Koleva, M. (2 December 2010)."Coudé-feed stellar spectral library – atmospheric parameters".Astronomy & Astrophysics.525: A71.arXiv:1009.1491.Bibcode:2011A&A...525A..71W.doi:10.1051/0004-6361/201015014.eISSN 1432-0746.ISSN 0004-6361.
  11. ^abde Medeiros, J. R.; Mayor, M. (November 1999)."A catalog of rotational and radial velocities for evolved stars".Astronomy and Astrophysics Supplement Series.139 (3):433–460.Bibcode:1999A&AS..139..433D.doi:10.1051/aas:1999401.ISSN 0365-0138.S2CID 54046583.
  12. ^"HD 32356".SIMBAD.Centre de données astronomiques de Strasbourg. RetrievedMay 7, 2024.
  13. ^Frankowski, A.; Jancart, S.; Jorissen, A. (19 December 2006)."Proper-motion binaries in the Hipparcos catalogue: Comparison with radial velocity data".Astronomy & Astrophysics.464 (1):377–392.arXiv:astro-ph/0612449.Bibcode:2007A&A...464..377F.doi:10.1051/0004-6361:20065526.eISSN 1432-0746.ISSN 0004-6361.S2CID 14010423.
  14. ^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.
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