Astronomy:HD 10939

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Short description: Star in the constellation Eridanus
HD 10939
Observation data
Equinox J2000.0]] (ICRS)
Constellation Eridanus[1]
Right ascension  01h 46m 06.3s[2]
Declination −53° 31′ 19″[2]
Apparent magnitude (V) 5.03[3]
Characteristics
Evolutionary stage main sequence[2]
Spectral type A1V[4]
U−B color index 0.05[5][6]
B−V color index 0.04[5][6]
Astrometry
Proper motion (μ) RA: +126.534[2] mas/yr
Dec.: +59.909[2] mas/yr
Parallax (π)16.0575 ± 0.0693[2] mas
Distance203.1 ± 0.9 ly
(62.3 ± 0.3 pc)
Absolute magnitude (MV)+1.08[1]
Details
Mass2.3[7] M☉
Radius2.27[7] R☉
Luminosity32[7] L☉
Surface gravity (log g)4.09[7] cgs
Temperature9,110[7] K
Rotation0.69 days[8]
Rotational velocity (v sin i)72.8[8] km/s
Age346[9] Myr
Other designations
CPD−54°377, SAO 232520, HD 10939, HR 520, q2 Eridani[5]
Database references
SIMBADdata

HD 10939 is a star[5][6] with an apparent magnitude of 5.03, making it visible to the naked eye. It glows white with a spectral type of A1V, and has a surface temperature of around 7,500 to 10,000 K.

References

  1. ↑ 1.0 1.1 Anderson, E.; Francis, Ch. (2012). "XHIP: An extended hipparcos compilation". Astronomy Letters 38 (5): 331. doi:10.1134/S1063773712050015. Bibcode: 2012AstL...38..331A  XHIP record for this object at VizieR.
  2. ↑ 2.0 2.1 2.2 2.3 2.4 Vallenari, A. et al. (2022). "Gaia Data Release 3. Summary of the content and survey properties". Astronomy & Astrophysics. doi:10.1051/0004-6361/202243940  Gaia DR3 record for this source at VizieR.
  3. ↑ Høg, E.; Fabricius, C.; Makarov, V. V.; Urban, S.; Corbin, T.; Wycoff, G.; Bastian, U.; Schwekendiek, P. et al. (2000). "The Tycho-2 catalogue of the 2.5 million brightest stars". Astronomy and Astrophysics 355. Bibcode: 2000A&A...355L..27H. 
  4. ↑ Houk, N.; Cowley, A. P. (1975). University of Michigan Catalogue of two-dimensional spectral types for the HD stars. Volume I. Declinations -90_ to -53_ƒ0. Bibcode: 1975mcts.book.....H. 
  5. ↑ 5.0 5.1 5.2 5.3 "HD 10939". SIMBAD. Centre de données astronomiques de Strasbourg. http://simbad.u-strasbg.fr/simbad/sim-basic?Ident=HD+10939. 
  6. ↑ 6.0 6.1 6.2 "VizieR Detailed Page". http://vizier.u-strasbg.fr/viz-bin/VizieR-5?-out.add=.&-source=5050&-corr=PK=HR&-out.max=9999&HR=520. Retrieved 2012-07-13. 
  7. ↑ 7.0 7.1 7.2 7.3 7.4 Stassun, Keivan G. et al. (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. 
  8. ↑ 8.0 8.1 Balona, L. A. (2019). "Evidence for spots on hot stars suggests major revision of stellar physics". Monthly Notices of the Royal Astronomical Society 490 (2): 2112. doi:10.1093/mnras/stz2808. Bibcode: 2019MNRAS.490.2112B. 
  9. ↑ Meshkat, Tiffany; Mawet, Dimitri; Bryan, Marta L.; Hinkley, Sasha; Bowler, Brendan P.; Stapelfeldt, Karl R.; Batygin, Konstantin; Padgett, Deborah et al. (2017). "A Direct Imaging Survey of Spitzer-detected Debris Disks: Occurrence of Giant Planets in Dusty Systems". The Astronomical Journal 154 (6): 245. doi:10.3847/1538-3881/aa8e9a. Bibcode: 2017AJ....154..245M.