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Lambda Pictoris
Observation data
Epoch J2000.0       Equinox J2000.0 ( ICRS)
Constellation Pictor
Right ascension 04h 42m 46.42350s [1]
Declination −50° 28′ 52.8050″ [1]
Apparent magnitude (V) +5.29 [2]
Characteristics
Spectral type K0/1 III [3]
U−B color index +0.74 [2]
B−V color index +0.98 [2]
Astrometry
Radial velocity (Rv)+4.60 [4] km/s
Proper motion (μ) RA: −36.02 [1]  mas/ yr
Dec.:   mas/ yr
Parallax (π)8.71 ± 0.18  mas [1]
Distance374 ± 8  ly
(115 ± 2  pc)
Details
Mass2.20 [4]  M
Luminosity112 [4]  L
Surface gravity (log g)2.77±0.09 [5]  cgs
Temperature4,851±45 [4]  K
Metallicity [Fe/H]−0.13±0.03 [5]  dex
Age2.24 [4]  Gyr
Other designations
λ Pic, CD−50° 1471, FK5 2351, HD 30185, HIP 21914, HR 1516, SAO 233638 [6]
Database references
SIMBAD data

λ Pictoris, Latinised as Lambda Pictoris, is a solitary, [7] orange-hued star in the southern constellation of Pictor. It is visible to the naked eye, having an apparent visual magnitude of +5.29. [2] With an annual parallax shift of 8.71 [1]  mas as seen from the Earth, it is located around 374  light-years from the Sun. At the estimated age of 2.24 [4] billion years old, it is an evolved K-type giant star with a stellar classification of K0/1 III. [3] Lambda Pictoris has 2.2 times the mass of the Sun and is radiating 112 times the Sun's luminosity from its photosphere at an effective temperature of 4,581  K. [4]

References

  1. ^ a b c d e 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. ^ a b c d Cousins, A. W. J.; et al. (1969), "Comparison Stars for Long Period Variables", Monthly Notes of the Astronomical Society of Southern Africa, 28: 63, Bibcode: 1969MNSSA..28...63C.
  3. ^ a b Houk, Nancy (1978), "Michigan catalogue of two-dimensional spectral types for the HD stars", Ann Arbor: Dept. Of Astronomy, 2, Ann Arbor: Dept. of Astronomy, University of Michigan, Bibcode: 1978mcts.book.....H.
  4. ^ a b c d e f g Luck, R. Earle (2015), "Abundances in the Local Region. I. G and K Giants", Astronomical Journal, 150 (3): 88, arXiv: 1507.01466, Bibcode: 2015AJ....150...88L, doi: 10.1088/0004-6256/150/3/88, S2CID  118505114.
  5. ^ a b Alves, S.; et al. (April 2015), "Determination of the spectroscopic stellar parameters for 257 field giant stars", Monthly Notices of the Royal Astronomical Society, 448 (3): 2749–2765, arXiv: 1503.02556, Bibcode: 2015MNRAS.448.2749A, doi: 10.1093/mnras/stv189.
  6. ^ "lam Pic". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2017-06-21.{{ cite web}}: CS1 maint: postscript ( link)
  7. ^ 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.