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HD 34255

From Wikipedia, the free encyclopedia

HD 34255
Observation data
Epoch J2000.0      Equinox J2000.0 (ICRS)
Constellation Camelopardalis
Right ascension 05h 20m 22.61066s[1]
Declination +62° 39′ 13.3608″[1]
Apparent magnitude (V) 5.60±0.01[2]
Characteristics
Spectral type K4 I[3]
U−B color index +2.00[4]
B−V color index +1.75[4]
Astrometry
Radial velocity (Rv)−7.7±0.15[5] km/s
Proper motion (μ) RA: −3.105 mas/yr[1]
Dec.: −2.373 mas/yr[1]
Parallax (π)1.9726 ± 0.0788 mas[1]
Distance1,650 ± 70 ly
(510 ± 20 pc)
Absolute bolometric
magnitude (Mbol)		−4.40±0.24[6]
Details
Mass6.9±0.9[7] M☉
Radius145[6] R☉
Luminosity6,101[8] L☉
Surface gravity (log g)1.14[9] cgs
Temperature3,927±170[6] K
Metallicity [Fe/H]−0.01±0.05[9] dex
Age46±6[7] Myr
Other designations
AG+62°410, BD+62°742, FK5 2397, GC 6496, HD 34255, HIP 24914, HR 1720, SAO 13460[10]
Database references
SIMBADdata

HD 34255, also known HR 1720, is a star located in the northern circumpolar constellation Camelopardalis, the giraffe. It has an apparent magnitude of 5.60,[2] allowing it to be faintly visible to the naked eye. The object is located relatively far at a distance of about 1.65 kly[1] but is approaching the Solar System with a heliocentric radial velocity of −7.7 km/s.[5]

This is a solitary,[11] evolved red supergiant with a stellar classification of K4 I.[3] It has 6.9 times the mass of the Sun and is said to be 46 million years old.[7] Despite the young age, it has already ceased hydrogen fusion at its core and now has an enlarged radius of 145 R☉.[6] HD 34255 radiates a bolometric luminosity over 6,000 times that of the Sun[8] from its photosphere at an effective temperature of 3,927 K,[6] giving it an orange glow. The star's metallicity – what astronomers dub as elements heavier than helium – is around solar level.[9]

References

  1. ^ a b c d e 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 at VizieR.
  2. ^ a b Høg, 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.
  3. ^ a b Adams, Walter S.; Joy, Alfred H.; Humason, Milton L.; Brayton, Ada Margaret (April 1935). "The Spectroscopic Absolute Magnitudes and Parallaxes of 4179 Stars". The Astrophysical Journal. 81: 187. Bibcode:1935ApJ....81..187A. doi:10.1086/143628. eISSN 1538-4357. ISSN 0004-637X.
  4. ^ a b Argue, A. N. (1 September 1966). "UBV Photometry of 550 F, G and K Type Stars". Monthly Notices of the Royal Astronomical Society. 133 (4): 475–493. Bibcode:1966MNRAS.133..475A. doi:10.1093/mnras/133.4.475. eISSN 1365-2966. ISSN 0035-8711.
  5. ^ a b Famaey, 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.
  6. ^ a b c d e Messineo, M.; Brown, A. G. A. (18 June 2019). "A Catalog of Known Galactic K-M Stars of Class I Candidate Red Supergiants in Gaia DR2". The Astronomical Journal. 158 (1): 20. arXiv:1905.03744. Bibcode:2019AJ....158...20M. doi:10.3847/1538-3881/ab1cbd. eISSN 1538-3881.
  7. ^ a b c Tetzlaff, N.; Neuhäuser, R.; Hohle, M. M. (October 12, 2010). "A catalogue of young runaway Hipparcos stars within 3 kpc from the Sun". Monthly Notices of the Royal Astronomical Society. Oxford University Press (OUP). 410 (1): 190–200. arXiv:1007.4883. Bibcode:2011MNRAS.410..190T. doi:10.1111/j.1365-2966.2010.17434.x. ISSN 0035-8711.
  8. ^ a b McDonald, I.; Zijlstra, A. A.; Boyer, M. L. (21 November 2012). "Fundamental parameters and infrared excesses of Hipparcos stars: Parameters and IR excesses from Hipparcos". Monthly Notices of the Royal Astronomical Society. 427 (1): 343–357. arXiv:1208.2037. Bibcode:2012MNRAS.427..343M. doi:10.1111/j.1365-2966.2012.21873.x. eISSN 1365-2966. ISSN 0035-8711.
  9. ^ a b c Wu, 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.
  10. ^ "HD 34255". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 21 September 2022.
  11. ^ 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.
This page was last edited on 9 January 2024, at 00:26
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