Binary star system in the constellation Canis Major
For other stars with this Bayer designation , see ν Canis Majoris .
Nu Canis Majoris
Observation dataEpoch J2000.0 Equinox J2000.0 (ICRS )
Constellation
Canis Major
Right ascension
06 36 22.85133
Declination
−18° 39′ 35.6838″
Apparent magnitude (V)
5.704 (5.87 + 7.61)
Characteristics
Spectral type
G8 III + F3 IV-V
B−V color index
+0.815
Astrometry Radial velocity (Rv )+26.13 km/s Proper motion (μ) RA: −10.09 mas /yr Dec.: +13.06 mas /yr Parallax (π)12.3660 ± 0.1985 mas Distance 264 ± 4 ly (81 ± 1 pc ) Absolute magnitude (MV )+1.23
Details ν CMa A Mass 1.41 M ☉ Luminosity 8 L ☉ Surface gravity (log g )3.00 cgs Temperature 6,091±822 K Metallicity −0.06 dex Rotational velocity (v sin i )4.8±0.2 km/s Age 3.07 Gyr
Other designations ν CMa , 6 Canis Majoris , BD −18°1480, GC 8614, HD 47138, HIP 31564, HR 2423, SAO 151694, ADS 5253, CCDM 06364-1840, WDS 06364-1840
Database references SIMBAD data
Nu Canis Majoris (ν Canis Majoris) is a binary star in the constellation Canis Major . It is visible to the naked eye with a combined apparent visual magnitude of 5.7. Based on parallax shift of 12.366 mas as seen from our orbit, this system is approximately 264 light years from the Sun .
As of 2011, the pair had an angular separation of 17.29 arc seconds along a position angle of 264.2°. The yellow hued magnitude 5.87 primary, component A, is an evolved G-type giant star with a stellar classification of G8 III. Its magnitude 7.61 companion, component B, is a yellow-white hued F-type main sequence /subgiant hybrid with a class of F3 IV-V.
References
^ 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 .
^ Luck, R. Earle (September 2015), "Abundances in the Local Region. I. G and K Giants", The Astronomical Journal , 150 (3): 23, arXiv :1507.01466 , Bibcode :2015AJ....150...88L , doi :10.1088/0004-6256/150/3/88 , S2CID 118505114 , 88.
^ 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 .
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 .
^ Ammler-von Eiff, Matthias; Reiners, Ansgar (June 2012), "New measurements of rotation and differential rotation in A-F stars: are there two populations of differentially rotating stars?", Astronomy & Astrophysics , 542 : A116, arXiv :1204.2459 , Bibcode :2012A&A...542A.116A , doi :10.1051/0004-6361/201118724 , S2CID 53666672 .
^ Soubiran, C.; et al. (2008), "Vertical distribution of Galactic disk stars. IV. AMR and AVR from clump giants", Astronomy and Astrophysics , 480 (1): 91–101, arXiv :0712.1370 , Bibcode :2008A&A...480...91S , doi :10.1051/0004-6361:20078788 , S2CID 16602121 .
"nu01 CMa" . SIMBAD . Centre de données astronomiques de Strasbourg . Retrieved 2017-09-05.{{cite web }}
: CS1 maint: postscript (link )
Mason, Brian D.; et al. (May 2012), "Speckle Interferometry at the U.S. Naval Observatory. XVIII" , The Astronomical Journal , 143 (5): 6, Bibcode :2012AJ....143..124M , doi :10.1088/0004-6256/143/5/124 , 124, archived from the original on June 13, 2017.
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