Beta Comae Berenices
Appearance
Observation data Epoch J2000 Equinox J2000 | |
---|---|
Constellation | Coma Berenices |
Right ascension | 13h 11m 52.39379s[1] |
Declination | +27° 52′ 41.4535″[1] |
Apparent magnitude (V) | 4.26[2] |
Characteristics | |
Spectral type | G0 V[3] |
U−B color index | +0.08[2] |
B−V color index | +0.58[4] |
Absolute magnitude (MV) | 4.46[7] |
Details | |
Gyr | |
Database references | |
SIMBAD | data |
![](http://upload.wikimedia.org/wikipedia/commons/thumb/1/13/Beta_Comae_Berenices.jpg/220px-Beta_Comae_Berenices.jpg)
Beta Comae Berenices (β Comae Berenices, β Com) is a
too dim
to be viewed from a built-up urban area.
The star is similar to the Sun, being only slightly larger and brighter in absolute magnitude. It has a stellar classification of G0 V,[3] compared to G2 V for the Sun. The effective temperature of the outer envelope is 5,936 K,[9] giving it a yellow hue of a G-type star.[14] In terms of age it is younger than the Sun, being about 3 billion years old.[12]
Observations of short term variations in the chromatic activity suggest that the star undergoes differential rotation,dusty disk.
The
AU, where 1 AU is the average distance from the Earth to the Sun.[17]
See also
References
- ^ .
- ^ Bibcode:1966CoLPL...4...99J
- ^ doi:10.1086/319956
- ^ Bibcode:1998A&A...338..623M.
- Bibcode:1953GCRV..C......0W.
- ^ .
- S2CID 118577511.
- S2CID 18775378. Note: see VizieR catalogue J/ApJS/168/297.
- ^ S2CID 18993744. See Table 10.
- ^ Brandenburg, Axel; et al. (August 2017), "Evolution of Co-existing Long and Short Period Stellar Activity Cycles", The Astrophysical Journal, 845 (1): 79,
- ^ doi:10.1086/303522
- ^ S2CID 27151456.
- Centre de Données astronomiques de Strasbourg, retrieved 2012-02-04
- Commonwealth Scientific and Industrial Research Organisation, December 21, 2004, archived from the originalon 2012-03-18, retrieved 2012-01-16
- doi:10.1086/186452
- doi:10.1086/175072See appendix A.
- S2CID 44208180