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HD 30442

From Wikipedia, the free encyclopedia
Star in the constellation Camelopardalis
HD 30442
Observation data
Epoch J2000      Equinox J2000
ConstellationCamelopardalis[1]
Right ascension04h 52m 05.2195s[2]
Declination+63° 30′ 19.5173″[2]
Apparent magnitude (V)5.47±0.01[3]
Characteristics
Evolutionary stageAGB[4]
Spectral typeM3 IIIab[5]
U−Bcolor index+1.76[6]
B−Vcolor index+1.55[6]
Astrometry
Radial velocity (Rv)−37±0.3[7] km/s
Proper motion (μ)RA: +38.424mas/yr[2]
Dec.: −94.026mas/yr[2]
Parallax (π)8.098±0.1027 mas[2]
Distance403 ± 5 ly
(123 ± 2 pc)
Absolute magnitude (MV)−0.44[1]
Details
Mass1.09[8] M
Radius70.85[9] R
Luminosity1,096+106
−96
[10] L
Surface gravity (log g)0.92[8] cgs
Temperature3,500±150[10] K
Metallicity[Fe/H]0.00[10] dex
Other designations
BD+63°543,FK5 2362,GC 5881,HD 30442,HIP 22626,HR 1527,SAO 13291,WDS J04521+6330A[11]
Database references
SIMBADdata

HD 30442 (HR 1527) is a solitary[12]star in the northerncircumpolar constellationCamelopardalis. It is faintly visible to thenaked eye with anapparent magnitude of 5.47[3] and is estimated to be 403light years away from theSolar System.[2] The object has a heliocentricradial velocity of−37 km/s, indicating that it is drifting closer.[7]

HD 30442 has astellar classification of M3 IIIab,[5] indicating that it is ared giant. It is anasymptotic giant branch[4] star currently generating energy usinghydrogen andhelium shells around an inertcarboncore. It has 109% themass of the Sun[8] and has an enlargedradius of70.8 R[9] due to its evolved state. It radiates at almost 1,100 times theluminosity of the Sun from itsphotosphere at aneffective temperature of3,500 K,[10] giving a red hue. HD 30442 is estimated to have a solarmetallicity,[8] with an abundance ofiron equivalent to that of theSun.

HD 30442 has a companion120 away along aposition angle of350°.[13] It shares a commonproper motion with HD 30442, suggesting physical relation, but itsparallax indicates otherwise.[14]

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. XHIP record for this object atVizieR.
  2. ^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.
  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.
  4. ^abEggen, Olin J. (July 1992). "Asymptotic giant branch stars near the sun".The Astronomical Journal.104: 275.Bibcode:1992AJ....104..275E.doi:10.1086/116239.ISSN 0004-6256.
  5. ^abYamashita, Y. (1967). "MK Spectral Types of Bright M-Type Stars".Publications of the Dominion Astrophysical Observatory Victoria.13: 44.Bibcode:1967PDAO...13...47Y.ISSN 0078-6950.
  6. ^abMermilliod, J.-C. (1986), "Compilation of Eggen's UBV data, transformed to UBV (unpublished)",Catalogue of Eggen's UBV Data. SIMBAD,Bibcode:1986EgUBV........0M
  7. ^abFamaey, B.; Jorissen, A.; Luri, X.; Mayor, M.; Udry, S.; Dejonghe, H.; Turon, C. (January 2005)."Local kinematics of K and M giants from CORAVEL/Hipparcos/Tycho-2 data. Revisiting the concept of superclusters".Astronomy and Astrophysics.430: 165.arXiv:astro-ph/0409579.Bibcode:2005A&A...430..165F.doi:10.1051/0004-6361:20041272.S2CID 17804304.
  8. ^abcdAnders, F.; et al. (August 2019)."Photo-astrometric distances, extinctions, and astrophysical parameters for Gaia DR2 stars brighter than G = 18".Astronomy & Astrophysics.628: A94.arXiv:1904.11302.Bibcode:2019A&A...628A..94A.doi:10.1051/0004-6361/201935765.ISSN 0004-6361.
  9. ^abKervella, Pierre; Arenou, Frédéric; Thévenin, Frédéric (2022)."Stellar and substellar companions fromGaia EDR3".Astronomy & Astrophysics.657: A7.arXiv:2109.10912.Bibcode:2022A&A...657A...7K.doi:10.1051/0004-6361/202142146.eISSN 1432-0746.ISSN 0004-6361.
  10. ^abcdCharbonnel, C.; Lagarde, N.; Jasniewicz, G.; North, P. L.; Shetrone, M.; Krugler Hollek, J.; Smith, V. V.; Smiljanic, R.; Palacios, A.; Ottoni, G. (January 2020)."Lithium in red giant stars: Constraining non-standard mixing with large surveys in theGaia era".Astronomy & Astrophysics.633: A34.arXiv:1910.12732.Bibcode:2020A&A...633A..34C.doi:10.1051/0004-6361/201936360.eISSN 1432-0746.ISSN 0004-6361.
  11. ^"HD 30442".SIMBAD.Centre de données astronomiques de Strasbourg. RetrievedJune 22, 2022.
  12. ^Eggleton, P. P.; Tokovinin, A. A. (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,S2CID 14878976
  13. ^Mason, Brian D.; Wycoff, Gary L.; Hartkopf, William I.; Douglass, Geoffrey G.; Worley, Charles E. (December 2001)."The 2001 US Naval Observatory Double Star CD-ROM. I. The Washington Double Star Catalog".The Astronomical Journal.122 (6):3466–3471.Bibcode:2001AJ....122.3466M.doi:10.1086/323920.ISSN 0004-6256.
  14. ^Vallenari, 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.

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