NR Canis Majoris
Appearance
Observation data J2000
| |
---|---|
Constellation | Canis Major |
Right ascension | 07h 27m 07.99012s[2] |
Declination | −17° 51′ 53.5058″[2] |
Apparent magnitude (V) | 5.60[3] (5.66 + 9.23)[4] |
Characteristics | |
Spectral type | F2V[5] |
B−V color index | +0.314±0.002[3] |
Variable type | δ Sct[6] |
Absolute magnitude (MV) | 0.78[3] |
Details | |
A | |
Gyr | |
Database references | |
SIMBAD | data |
NR Canis Majoris is a
light years from the Sun based on parallax.[2] The system is drifting closer to the Sun with a radial velocity of −29 km/s,[3] and in about three million years it is predicted to approach within 14.1+4.7
−4.0 ly.[12] At that time, the star will become the brightest in the night sky, potentially reaching magnitude −0.88.[13]
−4.0 ly.[12] At that time, the star will become the brightest in the night sky, potentially reaching magnitude −0.88.[13]
The magnitude 5.66projected rotational velocity of 185 km/s, which is giving the star an equatorial bulge that is estimated to be 8% larger than the polar radius.[9]
The secondary companion is magnitude 9.23 and lies at an
″ along a position angle of 39°, as of 2005.[4]
References
- ^ "MAST: Barbara A. Mikulski Archive for Space Telescopes". Space Telescope Science Institute. Retrieved 8 December 2021.
- ^ .
- ^ S2CID 119257644.
- ^ doi:10.1086/323920. Retrieved 2015-07-22.
- ^ Bibcode:1988mcts.book.....H.
- ^ S2CID 125853869.
- ^ S2CID 33401607.
- S2CID 55586789.
- ^ S2CID 119273474.
- ^ "NR CMa". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 12 February 2017.
- S2CID 14878976.
- S2CID 59039482. A35.
- Bibcode:1998S&T....95d..59T.
- ^ Watson, Christopher (4 January 2010). "LS Canis Majoris". AAVSO Website. American Association of Variable Star Observers. Retrieved 12 July 2014.