| Observation data Epoch J2000.0 Equinox J2000.0 ( ICRS) | |
|---|---|
| Constellation | Lepus |
| Right ascension | 05h 19m 59.02275s [1] |
| Declination | −12° 18′ 56.1139″ [1] |
| Apparent magnitude (V) | 5.29 [2] |
| Characteristics | |
| Spectral type | B7/8 V [3] or B7 IVnn [4] |
| U−B color index | −0.41 [2] |
| B−V color index | −0.12 [2] |
| Astrometry | |
| Radial velocity (Rv) | +16.0±7.4 [5] km/s |
| Proper motion (μ) |
RA: −13.32
[1]
mas/
yr Dec.: +7.18 [1] mas/ yr |
| Parallax (π) | 9.78 ± 0.37 mas [1] |
| Distance | 330 ± 10
ly (102 ± 4 pc) |
| Absolute magnitude (MV) | +0.25 [6] |
| Details | |
| Mass | 3.28±0.05 [7] M☉ |
| Radius | 3.0 [8] R☉ |
| Luminosity | 138 [7] L☉ |
| Temperature | 12,417 [7] K |
| Rotational velocity (v sin i) | 285 [9] km/s |
| Other designations | |
| Database references | |
| SIMBAD | data |
Nu Leporis, Latinized from ν Leporis, is a probable astrometric binary [11] star system in the constellation Lepus. It is visible to the naked eye as a faint star with an apparent visual magnitude of 5.29. [2] Based upon an annual parallax shift of 7.70 mas as seen from the Earth, [1] it is 420 light years from the Sun.
The visible component is a B-type star with an estimated 3.3 [7] times the mass of the Sun. Lesh (1968) gave a stellar classification of B7 IVnn, [4] which would indicate this is a somewhat evolved subgiant star. The 'nn' notation indicates especially "nebulous" absorption lines caused by rapid rotation. Houk and Smith-Moore (1978) listed it as B7/8 V, [3] suggesting this is instead a B-type main sequence star that has not yet consumed all the hydrogen at its core.
Nu Leporis is spinning rapidly with a projected rotational velocity of 285 km/s. [9] The star has a radius about three [8] times that of the Sun and is radiating 138 times the Sun's luminosity from its photosphere at an effective temperature of 12,417 K. [7]
- ^ 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.
- ^ a b c d Crawford, D. L.; et al. (1971), "Four-color, H-beta, and UBV photometry for bright B-type stars in the northern hemisphere", The Astronomical Journal, 76: 1058, Bibcode: 1971AJ.....76.1058C, doi: 10.1086/111220.
- ^ a b Houk, Nancy; Smith-Moore, M. (1978), Michigan catalogue of two-dimensional spectral types for the HD stars, vol. 4, Ann Arbor: Dept. of Astronomy, University of Michigan, Bibcode: 1988mcts.book.....H.
- ^ a b Lesh, Janet Rountree (December 1968), "The Kinematics of the Gould Belt: an Expanding Group?", Astrophysical Journal Supplement, 17: 371, Bibcode: 1968ApJS...17..371L, doi: 10.1086/190179.
- ^ 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 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 Pasinetti Fracassini, L. E.; et al. (2001), "Catalogue of Apparent Diameters and Absolute Radii of Stars (CADARS)", Astronomy and Astrophysics, 367 (2) (Third ed.): 521, arXiv: astro-ph/0012289, Bibcode: 2001A&A...367..521P, doi: 10.1051/0004-6361:20000451, S2CID 425754.
- ^ a b Abt, Helmut A.; et al. (2002), "Rotational Velocities of B Stars", The Astrophysical Journal, 573 (1): 359–365, Bibcode: 2002ApJ...573..359A, doi: 10.1086/340590.
-
^
"nu. Lep".
SIMBAD.
Centre de données astronomiques de Strasbourg. Retrieved 2017-08-18.
{{ 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.
| Observation data Epoch J2000.0 Equinox J2000.0 ( ICRS) | |
|---|---|
| Constellation | Lepus |
| Right ascension | 05h 19m 59.02275s [1] |
| Declination | −12° 18′ 56.1139″ [1] |
| Apparent magnitude (V) | 5.29 [2] |
| Characteristics | |
| Spectral type | B7/8 V [3] or B7 IVnn [4] |
| U−B color index | −0.41 [2] |
| B−V color index | −0.12 [2] |
| Astrometry | |
| Radial velocity (Rv) | +16.0±7.4 [5] km/s |
| Proper motion (μ) |
RA: −13.32
[1]
mas/
yr Dec.: +7.18 [1] mas/ yr |
| Parallax (π) | 9.78 ± 0.37 mas [1] |
| Distance | 330 ± 10
ly (102 ± 4 pc) |
| Absolute magnitude (MV) | +0.25 [6] |
| Details | |
| Mass | 3.28±0.05 [7] M☉ |
| Radius | 3.0 [8] R☉ |
| Luminosity | 138 [7] L☉ |
| Temperature | 12,417 [7] K |
| Rotational velocity (v sin i) | 285 [9] km/s |
| Other designations | |
| Database references | |
| SIMBAD | data |
Nu Leporis, Latinized from ν Leporis, is a probable astrometric binary [11] star system in the constellation Lepus. It is visible to the naked eye as a faint star with an apparent visual magnitude of 5.29. [2] Based upon an annual parallax shift of 7.70 mas as seen from the Earth, [1] it is 420 light years from the Sun.
The visible component is a B-type star with an estimated 3.3 [7] times the mass of the Sun. Lesh (1968) gave a stellar classification of B7 IVnn, [4] which would indicate this is a somewhat evolved subgiant star. The 'nn' notation indicates especially "nebulous" absorption lines caused by rapid rotation. Houk and Smith-Moore (1978) listed it as B7/8 V, [3] suggesting this is instead a B-type main sequence star that has not yet consumed all the hydrogen at its core.
Nu Leporis is spinning rapidly with a projected rotational velocity of 285 km/s. [9] The star has a radius about three [8] times that of the Sun and is radiating 138 times the Sun's luminosity from its photosphere at an effective temperature of 12,417 K. [7]
- ^ 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.
- ^ a b c d Crawford, D. L.; et al. (1971), "Four-color, H-beta, and UBV photometry for bright B-type stars in the northern hemisphere", The Astronomical Journal, 76: 1058, Bibcode: 1971AJ.....76.1058C, doi: 10.1086/111220.
- ^ a b Houk, Nancy; Smith-Moore, M. (1978), Michigan catalogue of two-dimensional spectral types for the HD stars, vol. 4, Ann Arbor: Dept. of Astronomy, University of Michigan, Bibcode: 1988mcts.book.....H.
- ^ a b Lesh, Janet Rountree (December 1968), "The Kinematics of the Gould Belt: an Expanding Group?", Astrophysical Journal Supplement, 17: 371, Bibcode: 1968ApJS...17..371L, doi: 10.1086/190179.
- ^ 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 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 Pasinetti Fracassini, L. E.; et al. (2001), "Catalogue of Apparent Diameters and Absolute Radii of Stars (CADARS)", Astronomy and Astrophysics, 367 (2) (Third ed.): 521, arXiv: astro-ph/0012289, Bibcode: 2001A&A...367..521P, doi: 10.1051/0004-6361:20000451, S2CID 425754.
- ^ a b Abt, Helmut A.; et al. (2002), "Rotational Velocities of B Stars", The Astrophysical Journal, 573 (1): 359–365, Bibcode: 2002ApJ...573..359A, doi: 10.1086/340590.
-
^
"nu. Lep".
SIMBAD.
Centre de données astronomiques de Strasbourg. Retrieved 2017-08-18.
{{ 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.