FK Comae Berenices
Star FK Comae Berenices |
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AladinLite | |||||||||||||||
Observation dates equinox : J2000.0 , epoch : J2000.0 |
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Constellation | Berenike's hair | ||||||||||||||
Right ascension | 13 h 30 m 46.8 s | ||||||||||||||
declination | + 24 ° 13 ′ 57.8 ″ | ||||||||||||||
Apparent brightness | 8.25 mag 8.03 to 8.43 mag |
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Typing | |||||||||||||||
B − V color index | +0.8 | ||||||||||||||
Spectral class | G4 III | ||||||||||||||
Variable star type | FKCOM | ||||||||||||||
Astrometry | |||||||||||||||
Radial velocity | (−21.0 ± 5.8) km / s | ||||||||||||||
parallax | (4.61 ± 0.04) mas | ||||||||||||||
distance | 710 ly 215 pc |
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Proper movement | |||||||||||||||
Rec. Share: | (−51.97 ± 0.09) mas / a | ||||||||||||||
Dec. portion: | (−22.26 ± 0.04) mas / a | ||||||||||||||
Physical Properties | |||||||||||||||
radius | 8.5 R ☉ | ||||||||||||||
Effective temperature | 5080 K | ||||||||||||||
Other names and catalog entries |
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FK Comae Berenices is a spectral class G star at a distance of about 700 light years . It is the prototype of the FK-Comae-Berenices stars , which belong to the rotation variable stars . The star shows what is known as flip-flop behavior.
The apparent brightness of the stars fluctuates between 8.03 and 8.43 with a period of 2.4 days. The variability was noted in 1966.
Individual evidence
- ↑ a b c d e f g FK Com. In: SIMBAD . Center de Données astronomiques de Strasbourg , accessed on August 24, 2018 .
- ↑ a b c FK Com. In: VSX. AAVSO, accessed August 24, 2018 .
- ↑ a b c Klaus G. Strassmeier: Starspots . In: The Astronomy and Astrophysics Review . 17, No. 3, Sep 2009, pp. 251 to 308. bibcode : 2009A & ARv..17..251S . doi : 10.1007 / s00159-009-0020-6 .
- ↑ T. Hackman et al .: Flip-flops of FK Comae Berenices . In: Astronomy & Astrophysics . 553, May 2013. bibcode : 2013A & A ... 553A..40H . doi : 10.1051 / 0004-6361 / 201220690 .
- ↑ PF Chugainov: New Micro variable HD 117555 . In: Information Bulletin on Variable Stars . 17, No. 3, Dec 1966, pp. 251 to 308. bibcode : 1966IBVS..172 .... 1C .