Star in the constellation Lepus
Kappa Leporis Observation dataEpoch J2000.0 Equinox J2000.0 (ICRS ) Constellation Lepus Right ascension 05h 13m 13.87761s [ 1] Declination −12° 56′ 28.6463″[ 1] Apparent magnitude (V)4.43 + 7.00[ 2] Characteristics Spectral type B9 V[ 3] U−Bcolor index −0.34[ 4] B−Vcolor index −0.10[ 4] Astrometry Radial velocity (Rv ) +20.8± 1.0[ 5] km/s Proper motion (μ)RA: −12.29 [ 1] mas /yr Dec.: −0.79 [ 1] mas /yr Parallax (π)4.48± 0.58 mas [ 1] Distance approx. 730 ly (approx. 220 pc ) Absolute magnitude (MV )−2.34[ 6] Details[ 3] κ Lep A Mass 4.86± 0.39 M ☉ Radius 2.6[ 7] R ☉ Luminosity 1,346 L ☉ Surface gravity (log g )3.44[ 8] cgs Temperature 11,588 K Metallicity [Fe/H]−0.07[ 8] dex Rotational velocity (v sin i )135 km/s Other designations κ Lep ,4 Lep ,BD −13° 1092 ,GC 6387 ,HD 33949 ,HIP 24327 ,HR 1705 ,SAO 150239 ,CCDM J05132-1256AB[ 9] Database references SIMBAD data
Kappa Leporis ,Latinized from κ Leporis, is abinary star [ 10] system in the southernconstellation ofLepus . The pair haveapparent visual magnitudes of 4.43 and 7.00, with the former being bright enough to be seen with the naked eye. As of 2000, they had anangular separation of 2.179 arc seconds along aposition angle of 357.3°. Based upon an annualparallax shift of 4.48 mas as measured from Earth,[ 1] the system is located roughly 730 light years from theSun . The system is travelling away from the Sun with aradial velocity of +20.8 km/s.[ 5]
The brighter, blue-white hued member of the system, component A, is aB-type main-sequence star with astellar classification of B9 V.[ 3] It has nearly five[ 3] times themass of the Sun and around 2.6[ 7] times theSun's radius . The star is radiating 1,346 times theSun's luminosity from itsphotosphere at aneffective temperature of 11,588 K.[ 3] It displays aninfrared excess at a wavelength of 12μm , making it a candidate host for a circumstellardebris disk .[ 11]
^a b c d e f 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 . ^ Fabricius, C.; Makarov, V. V. (April 2000), "Two-colour photometry for 9473 components of close Hipparcos double and multiple stars",Astronomy and Astrophysics ,356 :141– 145,Bibcode :2000A&A...356..141F . ^a b c d e Zorec, J.; Royer, F. (January 2012), "Rotational velocities of A-type stars. IV. Evolution of rotational velocities",Astronomy & Astrophysics ,537 : A120,arXiv :1201.2052 ,Bibcode :2012A&A...537A.120Z ,doi :10.1051/0004-6361/201117691 ,S2CID 55586789 . ^a b Johnson, H. L.; et al. (1966), "UBVRIJKL photometry of the bright stars",Communications of the Lunar and Planetary Laboratory ,4 (99): 99,Bibcode :1966CoLPL...4...99J . ^a b 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. ^ 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 . ^a b Pasinetti Fracassini, L. E.; et al. (February 2001), "Catalogue of Apparent Diameters and Absolute Radii of Stars (CADARS)",Astronomy and Astrophysics ,367 (Third ed.):521– 24,arXiv :astro-ph/0012289 ,Bibcode :2001A&A...367..521P ,doi :10.1051/0004-6361:20000451 ,S2CID 425754 . ^a b Saffe, C.; Gómez, M.; Pintado, O.; González, E. (October 2008), "Spectroscopic metallicities of Vega-like stars",Astronomy and Astrophysics ,490 (1):297– 305,arXiv :0805.3936 ,Bibcode :2008A&A...490..297S ,doi :10.1051/0004-6361:200810260 ,S2CID 15059920 . ^ "kap Lep" .SIMBAD .Centre de données astronomiques de Strasbourg . Retrieved2017-08-18 .{{cite web }}
: CS1 maint: postscript (link )^ 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 . ^ Mannings, Vincent; et al. (1998), "Candidate Main-Sequence Stars with Debris Disks: A New Sample of Vega-like Sources",The Astrophysical Journal ,497 (1):330– 341,Bibcode :1998ApJ...497..330M ,CiteSeerX 10.1.1.502.7594 ,doi :10.1086/305432 ,S2CID 122421281 .