2 Lupi

2 Lupi
Location of 2 Lupi (circled in red)
Observation data
Epoch J2000      Equinox ICRS
Constellation Lupus
Right ascension 15h 17m 49.83809s
Declination −30° 08′ 55.2165″
Apparent magnitude (V) 4.33
Characteristics
Evolutionary stage giant
Spectral type K0 IIIa CH-1
B−V color index 1.100±0.004
Variable type none
Astrometry
Radial velocity (Rv)−2.91±0.15 km/s
Proper motion (μ) RA: −10.16 mas/yr
Dec.: −3.66 mas/yr
Parallax (π)10.01±0.21 mas
Distance326 ± 7 ly
(100 ± 2 pc)
Absolute magnitude (MV)−0.65
Details
Radius11.0+0.7
−0.8
 R☉
Luminosity65.6±0.8 L☉
Surface gravity (log g)2.84 cgs
Temperature4,953+197
−148
 K
Metallicity [Fe/H]0.11 dex
Other designations
f Lupi, 2 Lup, NSV 7012, CD−29°11630, FK5 3207, HD 135758, HIP 74857, HR 5686, SAO 183346
Database references
SIMBADdata

2 Lupi, also known by its Bayer designation f Lupi, is a solitarystar in the southern constellation of Lupus, situated approximately 326 light-years away from the Sun. It has the Bayer designation f Lupi; 2 Lupi is the Flamsteed designation. It is visible to the naked eye as a faint, orange-hued star with an apparent visual magnitude of 4.33. It is moving closer to the Earth with a heliocentric radial velocity of −3 km/s.

This is an aging giant star with a stellar classification of K0 IIIa CH-1. The suffix notation indicates abnormally weak lines of carbyne. Having exhausted the hydrogen at its core, the star evolved away from the main sequence by expanding to 11 times the Sun's radius. The star is radiating 65.6 times the luminosity of the Sun from its enlarged photosphere at an effective temperature of 4,953 K.

2 Lupi is also moving steadily toward our solar system at a rate of roughly –3 km/s. This slow approach is observable through its measured radial velocity.

References

  1. 1 2 3 4 5 6 van Leeuwen, F. (2007), "Validation of the new Hipparcos reduction", Astronomy and Astrophysics, 474 (2): 653–664, arXiv:0708.1752, Bibcode:2007A&A...474..653V, doi:10.1051/0004-6361:20078357, S2CID 18759600.
  2. 1 2 3 4 McWilliam, Andrew (December 1990), "High-resolution spectroscopic survey of 671 GK giants. I - Stellar atmosphere parameters and abundances", Astrophysical Journal Supplement Series, 74: 1075–1128, Bibcode:1990ApJS...74.1075M, doi:10.1086/191527
  3. 1 2 Keenan, Philip C.; McNeil, Raymond C. (1989), "The Perkins catalog of revised MK types for the cooler stars", Astrophysical Journal Supplement Series, 71: 245, Bibcode:1989ApJS...71..245K, doi:10.1086/191373
  4. 1 2 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, S2CID 119257644.
  5. ↑ Samus, N. N.; et al. (2017), "General Catalogue of Variable Stars", Astronomy Reports, 5.1, 61 (1): 80–88, Bibcode:2017ARep...61...80S, doi:10.1134/S1063772917010085, S2CID 125853869.
  6. 1 2 3 4 5 6 7 8 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.
  7. 1 2 "2 Boo". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2019-04-06.
  8. ↑ Eggleton, P. P.; Tokovinin, A. A. (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, S2CID 14878976.
  9. ↑ "2 Lupi - Star in Lupus | TheSkyLive". theskylive.com. Retrieved 2025-08-19.