Astronomy:HD 27245

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Short description: Star in the constellation Camelopardalis
HD 27245
Camelopardalis constellation map.svg
Red circle.svg
Location of HD 27245 on the map (circled)
Observation data
Epoch J2000.0   Equinox (celestial coordinates)
Constellation Camelopardalis
Right ascension  04h 21m 47.64917s[1]
Declination +60° 44′ 08.2461″[1]
Apparent magnitude (V) 5.40±0.01[2]
Characteristics
Spectral type M0 III[3]
B−V color index +1.50[4]
Variable type suspected[5]
Astrometry
Radial velocity (Rv)+25.2±0.3[6] km/s
Proper motion (μ) RA: +55.890[1] mas/yr
Dec.: −114.046[1] mas/yr
Parallax (π)5.3716 ± 0.0848[1] mas
Distance607 ± 10 ly
(186 ± 3 pc)
Absolute magnitude (MV)−0.27[7]
Details
Mass1.18[8] M☉
Radius52.8±2.7[9] R☉
Luminosity570±16[10] L☉
Surface gravity (log g)1.29[11] cgs
Temperature4,033±122[12] K
Metallicity [Fe/H]+0.11[8] dex
Other designations
25 H. Camelopardalis,[13] NSV 1558, BD+60°800, FK5 2317, GC 5244, HD 27245, HIP 20736, HR 1335, SAO 13113[14]
Database references
SIMBADdata

HD 27245, also known as HR 1335 or rarely 25 H. Camelopardalis is a solitary red-hued star[15] located in the northern circumpolar constellation Camelopardalis. It has an apparent magnitude of 5.4,[2] making it faintly visible to the naked eye. Gaia DR3 Parallax measurements place it approximately 607 light years[1] away from it the Solar System and is drifting further away with a heliocentric radial velocity of 25.2 km/s.[6] At its current distance, HD 27245's brightness is diminished by 0.36 magnitudes due to extinction from interstellar dust.[16] It has an absolute magnitude of −0.27.[7]

HD 27245 is an aging red giant with a stellar classification of M0 III.[3] It has 118% the mass of the Sun[8] but has expanded to a radius of 52.8 R☉.[11] It radiates 570 times the luminosity of the Sun[10] from its enlarged photosphere at an effective temperature of 4,033 K.[12] HD 27245's iron abundance is 129% that of the Sun's,[8] making it metal enriched.

HD 27245 is a suspected variable star with an amplitude of 0.05 magnitudes.[5] Its variability was first observed in 1930 by Joel Stebbins.[17] However, Eggen (1967) instead lists it as an ordinary M-type giant and used the object for comparison.[18] In 1978-9, HD 28245 was again listed as a variable star but did not provide further insight.[19] As of 2017, the star has not been confirmed to be variable.[5]

References

  1. ↑ 1.0 1.1 1.2 1.3 1.4 Brown, A. G. A. (2021). "Gaia Early Data Release 3: Summary of the contents and survey properties". Astronomy & Astrophysics 649: A1. doi:10.1051/0004-6361/202039657. Bibcode: 2021A&A...649A...1G.  Gaia EDR3 record for this source at VizieR.
  2. ↑ 2.0 2.1 Høg, E.; Fabricius, C.; Makarov, V. V.; Urban, S.; Corbin, T.; Wycoff, G.; Bastian, U.; Schwekendiek, P. et al. (March 2000). "The Tycho-2 catalogue of the 2.5 million brightest stars". Astronomy and Astrophysics 355: L27–L30. ISSN 0004-6361. Bibcode: 2000A&A...355L..27H. 
  3. ↑ 3.0 3.1 Appenzeller, Immo (April 1967). "MK Spectral Types for 185 Bright Stars". Publications of the Astronomical Society of the Pacific 79 (467): 102. doi:10.1086/128449. ISSN 0004-6280. Bibcode: 1967PASP...79..102A. 
  4. ↑ Haggkvist, L.; Oja, T. (1970). "Results of BV photometry 1969-70 (Uppsala refractor)". Private Communication. Bibcode: 1970Priv.........0H. 
  5. ↑ 5.0 5.1 5.2 Samus’, N. N.; Kazarovets, E. V.; Durlevich, O. V.; Kireeva, N. N.; Pastukhova, E. N. (January 2017). "General catalogue of variable stars: Version GCVS 5.1". Astronomy Reports 61 (1): 80–88. doi:10.1134/S1063772917010085. ISSN 1063-7729. Bibcode: 2017ARep...61...80S. 
  6. ↑ 6.0 6.1 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. doi:10.1051/0004-6361:20041272. Bibcode: 2005A&A...430..165F. 
  7. ↑ 7.0 7.1 Anderson, E.; Francis, Ch. (May 2012). "XHIP: An extended hipparcos compilation". Astronomy Letters 38 (5): 331–346. doi:10.1134/S1063773712050015. ISSN 1063-7737. Bibcode: 2012AstL...38..331A. 
  8. ↑ 8.0 8.1 8.2 8.3 Anders, F. et al. (August 2019). "Photo-astrometric distances, extinctions, and astrophysical parameters for Gaia DR2 stars brighter than G = 18". Astronomy & Astrophysics 628: A94. doi:10.1051/0004-6361/201935765. ISSN 0004-6361. Bibcode: 2019A&A...628A..94A. 
  9. ↑ Kervella, P.; Thévenin, F.; Di Folco, E.; Ségransan, D. (October 2004). "The angular sizes of dwarf stars and subgiants". Astronomy & Astrophysics 426 (1): 297–307. doi:10.1051/0004-6361:20035930. ISSN 0004-6361. Bibcode: 2004A&A...426..297K. 
  10. ↑ 10.0 10.1 Brown, A. G. A. (August 2018). "Gaia Data Release 2: Summary of the contents and survey properties". Astronomy & Astrophysics 616: A1. doi:10.1051/0004-6361/201833051. Bibcode: 2018A&A...616A...1G.  Gaia DR2 record for this source at VizieR.
  11. ↑ 11.0 11.1 McDonald, I.; Zijlstra, A. A.; Watson, R. A. (15 June 2017). "Fundamental parameters and infrared excesses of Tycho–Gaia stars". Monthly Notices of the Royal Astronomical Society 471 (1): 770–791. doi:10.1093/mnras/stx1433. ISSN 0035-8711. Bibcode: 2017MNRAS.471..770M. 
  12. ↑ 12.0 12.1 Stassun, Keivan G. et al. (9 September 2019). "The Revised TESS Input Catalog and Candidate Target List". The Astronomical Journal 158 (4): 138. doi:10.3847/1538-3881/ab3467. Bibcode: 2019AJ....158..138S. 
  13. ↑ Verbunt, F.; van Gent, R. H. (June 2010). "The star catalogue of Hevelius". Astronomy and Astrophysics 516: A29. doi:10.1051/0004-6361/201014003. ISSN 0004-6361. Bibcode: 2010A&A...516A..29V. 
  14. ↑ "HD 27245". SIMBAD. Centre de données astronomiques de Strasbourg. http://simbad.u-strasbg.fr/simbad/sim-basic?Ident=HD+27245. 
  15. ↑ 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. doi:10.1111/j.1365-2966.2008.13596.x. ISSN 0035-8711. Bibcode: 2008MNRAS.389..869E. 
  16. ↑ 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. doi:10.1093/mnras/stx2219. ISSN 0035-8711. Bibcode: 2017MNRAS.472.3805G. 
  17. ↑ Stebbins, Joel; Huffer, Charles Morse (1930). "The constancy of the light of red stars". Publications of the Washburn Observatory 15: 140–174. Bibcode: 1930PWasO..15..140S. 
  18. ↑ Eggen, Olin J. (September 1967). "- and Broad-Band Photometry of Red Stars. Northern Giants". The Astrophysical Journal Supplement Series 14: 307. doi:10.1086/190158. ISSN 0067-0049. Bibcode: 1967ApJS...14..307E. 
  19. ↑ Pyl'skaja, O. P.; Zakharova, P. E.; Polushina, T. S. (December 1978). "V-R Colours of Red Variable Stars". Information Bulletin on Variable Stars 1513: 1. ISSN 0374-0676. Bibcode: 1978IBVS.1513....1P. 

External links



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