HD 137058

HD 137058
Location of HD 137058 (circled in red)
Observation data
Epoch J2000      Equinox ICRS
Constellation Lupus
Right ascension 15h 25m 20.20923s
Declination −38° 44′ 00.8803″
Apparent magnitude (V) 4.60
Characteristics
Evolutionary stage main sequence
Spectral type A0 V
B−V color index 0.000±0.015
Astrometry
Radial velocity (Rv)−3.0±2.8 km/s
Proper motion (μ) RA: −41.573 mas/yr
Dec.: −24.603 mas/yr
Parallax (π)13.6178±0.4759 mas
Distance240 ± 8 ly
(73 ± 3 pc)
Absolute magnitude (MV)−0.76
Details
Mass2.4 M☉
Radius3.3 R☉
Luminosity72 L☉
Surface gravity (log g)3.78 cgs
Temperature9,283 K
Rotational velocity (v sin i)300.0 km/s
Age267 Myr
Other designations
k Lup, CD−38°10289, HD 137058, HIP 75501, HR 5724, SAO 206616
Database references
SIMBADdata

HD 137058 is a star in the southern constellation of Lupus. Eggleton and Tokovinin (2008) list it as a single star, although Nitschelm and David (2011) suggested it may be a double-lined spectroscopic binary. Its apparent visual magnitude is 4.60, making it bright enough to be visible to the naked eye. Based on an annual parallax shift of 13.6 mas, it is located approximately 240 light years away.

The primary component has a stellar classification of A0 V, indicating it is an A-type main-sequence star. It rotates rapidly, with a projected rotational velocity of 300 km/s, resulting in an oblate shape with an equatorial radius 22% larger than its polar radius. The star radiates 72 times the Sun's luminosity from its photosphere at an effective temperature of 9,283 K.

References

  1. 1 2 3 4 5 Anderson, 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 at VizieR.
  2. 1 2 3 4 5 6 Brown, A. G. A.; et al. (Gaia collaboration) (August 2018). "Gaia Data Release 2: Summary of the contents and survey properties". Astronomy & Astrophysics. 616. A1. arXiv:1804.09365. Bibcode:2018A&A...616A...1G. doi:10.1051/0004-6361/201833051. Gaia DR2 record for this source at VizieR.
  3. ↑ Patten, B. M.; Willson, L. A. (1991). "An IRAS Survey of Main-Sequence B,A, and F Stars". The Astronomical Journal. 102: 323. Bibcode:1991AJ....102..323P. doi:10.1086/115879.
  4. 1 2 Houk, Nancy (1978). Michigan catalogue of two-dimensional spectral types for the HD stars. Vol. 2. Ann Arbor: Dept. of Astronomy, University of Michigan. Bibcode:1978mcts.book.....H.
  5. ↑ de Bruijne, J. H. J.; Eilers, A.-C. (October 2012). "Radial velocities for the HIPPARCOS-Gaia Hundred-Thousand-Proper-Motion project". Astronomy & Astrophysics. 546: 14. arXiv:1208.3048. Bibcode:2012A&A...546A..61D. doi:10.1051/0004-6361/201219219. S2CID 59451347. A61.
  6. 1 2 3 4 5 6 Stassun, Keivan G.; et al. (2019). "The Revised TESS Input Catalog and Candidate Target List". The Astronomical Journal. 158 (4): 138. arXiv:1905.10694. Bibcode:2019AJ....158..138S. doi:10.3847/1538-3881/ab3467.
  7. 1 2 van Belle, Gerard T. (March 2012). "Interferometric observations of rapidly rotating stars". The Astronomy and Astrophysics Review. 20 (1): 51. arXiv:1204.2572. Bibcode:2012A&ARv..20...51V. doi:10.1007/s00159-012-0051-2. S2CID 119273474.
  8. ↑ Gontcharov, G. A. (2012). "Dependence of kinematics on the age of stars in the solar neighborhood". Astronomy Letters. 38 (12): 771. arXiv:1606.08814. Bibcode:2012AstL...38..771G. doi:10.1134/S1063773712120031.
  9. ↑ "HD 137058". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2018-07-29.
  10. ↑ Eggleton, P. P.; Tokovinin, A. A. (2008). "A catalogue of multiplicity among bright stellar systems". Monthly Notices of the Royal Astronomical Society. 389 (2): 869. arXiv:0806.2878. Bibcode:2008MNRAS.389..869E. doi:10.1111/j.1365-2966.2008.13596.x. S2CID 14878976.
  11. ↑ Nitschelm, C.; David, M. (2011). "An Investigation on Close Binaries in the Sco-Cen Complex". Evolution of Compact Binaries. 447: 75. Bibcode:2011ASPC..447...75N.