HD 34255

Last updated
HD 34255
Observation data
Epoch J2000.0        Equinox J2000.0 (ICRS)
Constellation Camelopardalis [1]
Right ascension 05h 20m 22.61066s [2]
Declination +62° 39′ 13.3608″ [2]
Apparent magnitude  (V)5.60±0.01 [3]
Characteristics
Spectral type K4 I [4]
U−B color index +2.00 [5]
B−V color index +1.75 [5]
Astrometry
Radial velocity (Rv)−7.7±0.15 [6] km/s
Proper motion (μ)RA: −3.105 mas/yr [2]
Dec.: −2.373 mas/yr [2]
Parallax (π)1.9726±0.0788  mas [2]
Distance 1,650 ± 70  ly
(510 ± 20  pc)
Absolute bolometric
magnitude  (Mbol)		−4.40±0.24 [7]
Details
Mass 6.9±0.9 [8]   M☉
Radius 145 [7]   R☉
Luminosity 6,101 [9]   L☉
Surface gravity (log g)1.14 [10]   cgs
Temperature 3,927±170 [7]   K
Metallicity [Fe/H]−0.01±0.05 [10]   dex
Age 46±6 [8]   Myr
Other designations
AG+62°410, BD+62°742, FK5 2397, GC 6496, HD 34255, HIP 24914, HR 1720, SAO 13460 [11]
Database references
SIMBAD data

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, [3] allowing it to be faintly visible to the naked eye. The object is located relatively far at a distance of about 1.65 kly [2] but is approaching the Solar System with a heliocentric radial velocity of −7.7  km/s . [6]

This is a solitary, [12] evolved red supergiant with a stellar classification of K4 I. [4] It has 6.9 times the mass of the Sun and is said to be 46 million years old. [8] Despite the young age, it has already ceased hydrogen fusion at its core and now has an enlarged radius of 145  R☉. [7] HD 34255 radiates a bolometric luminosity over 6,000 times that of the Sun [9] from its photosphere at an effective temperature of 3,927  K , [7] giving it an orange glow. The star's metallicity – what astronomers dub as elements heavier than helium – is around solar level. [10]

References

  1. ↑ Roman, Nancy G. (1987). "Identification of a constellation from a position". Publications of the Astronomical Society of the Pacific . 99 (617): 695. Bibcode:1987PASP...99..695R. doi: 10.1086/132034 . Constellation record for this object at VizieR.
  2. 1 2 3 4 5 6 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.
  3. 1 2 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.
  4. 1 2 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.
  5. 1 2 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.
  6. 1 2 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.
  7. 1 2 3 4 5 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.
  8. 1 2 3 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. 410 (1). Oxford University Press (OUP): 190–200. arXiv: 1007.4883 . Bibcode:2011MNRAS.410..190T. doi: 10.1111/j.1365-2966.2010.17434.x . ISSN   0035-8711.
  9. 1 2 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.
  10. 1 2 3 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.
  11. ↑ "HD 34255". SIMBAD . Centre de données astronomiques de Strasbourg . Retrieved 21 September 2022.
  12. ↑ 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.
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