In Evidence
Other stars in Coma Berenices
- Ī² Comae Berenices
- Ī³ Comae Berenices
- 11 Comae Berenices
- 36 Comae Berenices
- 41 Comae Berenices
- 12 Comae Berenices
- 23 Comae Berenices
- 35 Comae Berenices
- 37 Comae Berenices
- 31 Comae Berenices
- 14 Comae Berenices
- 7 Comae Berenices
- HR4668
- 16 Comae Berenices
- 24 Comae Berenices
- 6 Comae Berenices
- 27 Comae Berenices
- 13 Comae Berenices
- Ī± Comae Berenices
- Diadem
- 17 Comae Berenices
- 21 Comae Berenices
- 26 Comae Berenices
- 18 Comae Berenices
- HR4693
- 5 Comae Berenices
- 40 Comae Berenices
- 4 Comae Berenices
- 25 Comae Berenices
- 20 Comae Berenices
- HR4673
- 29 Comae Berenices
- HR5057
- 30 Comae Berenices
- HR4793
- 2 Comae Berenices
- HR4962
- 38 Comae Berenices
- 39 Comae Berenices
- HR4633
- HR4725
- HR4992
- HR5102
- HR4694
- HR4705
- HR4956
- HR4926
- HR4680
- 8 Comae Berenices
- 22 Comae Berenices
- HR4886
- HR4864
- 32 Comae Berenices
- HR4984
- 9 Comae Berenices
- HR4676
- HR4812
- 3 Comae Berenices
- HR4719
- HR4873
- HR5007
- HR5010
- HR4684
- HR4642
- HR4987
- HR4948
- HR4750
- 28 Comae Berenices
- HR4751
- HR4698
5 Comae Berenices
5 Comae Berenices is a hypergiant star of spectral class K0 in the constellation of Coma Berenices.
5 Comae Berenices visual magnitude is 5.57. Because of its faintness, 5 Comae Berenices is visible to the naked eye only from locations with very dark skies, while it is not visible at all from skies affected by light pollution.
Celestial Coordinates
Apparent
J2000
Galactic Coordinates
Finder Chart
Magnitude, Color, Spectral Class
The red dot in the diagram below shows where 5 Comae Berenices is situated in the HertzsprungāRussell diagram.
Distance, Radial Speed, Proper Motion
5 Comae Berenices is distant 484.40 light years from the Sun and it is moving towards the Sun at the speed of 25 kilometers per second.
Alternative Designations
Visibility from Your Location
Today's 5 Comae Berenices rise, transit and set times from Greenwich, UK are the following (all times relative to the local timezone Europe/London):