V509 Cassiopeiae

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Stern
V509 Cassiopeiae (HR 8752)
AladinLite
Observation
dates equinoxJ2000.0 , epoch : J2000.0
Constellation Cassiopeia
Right ascension 23 h 00 m 5.1 s
declination + 56 ° 56 ′ 43.3 ″
Apparent brightness 5.1 (4.75 to 5.5) mag
Typing
B − V color index +1.42 
U − B color index +1.16 
R − I index +0.85 
Spectral class G0 Ia
Variable star type SRD 
Astrometry
Radial velocity (−50.2 ± 0.7) km / s
distance > 7800  ly
> 2400  pc
Proper movement 
Rec. Share: (−2.79 ± 0.16)  mas / a
Dec. portion: (−2.05 ± 0.14)  mas / a
Physical Properties
Dimensions 25  M
radius 910  R
Luminosity

350000  L

Effective temperature 5550  K
Rotation time 202 days
Other names
and catalog entries
Bonn survey BD + 56 ° 2923
Bright Star Catalog HR 8752 [1]
Henry Draper Catalog HD 217476 [2]
Hipparcos catalog HIP 113561 [3]
SAO catalog SAO 35039 [4]
Tycho catalog TYC 3993-2269-1 [5]Template: Infobox star / maintenance / specification of the TYC catalog
2MASS catalog 2MASS J23000509 + 5656433 [6]
Other names V509 Cassiopeiae, FK5 3839

V509 Cassiopeiae ( V509 Cas for short ), also known as HR 8752 , is a star in the Cassiopeia constellation .

V509 Cassiopeiae is a yellow Tallstar from the type G with a mean apparent brightness of +5.10. Its distance from Earth is at least 7800 light years . It is classified as a semi-regularly variable star . Its brightness fluctuates from magnitude +4.75 to +5.5. According to RW Cephei , V509 Cassiopeiae is the brightest star in the stellar association Cep OB1 .
The exact nature of V509 Cassiopeiae and its fluctuations in brightness is not yet understood; among other things, it is assumed that a possible companion star could also play a certain role.

Web links

Individual evidence

  1. a b V509 Cas. In: SIMBAD . Center de Données astronomiques de Strasbourg , accessed on November 12, 2018 .
  2. a b Hipparcos catalog (ESA 1997)
  3. a b V509 Cas. In: VSX. AAVSO, accessed November 12, 2018 .
  4. a b c Bright Star Catalog
  5. Pulkovo radial velocities for 35493 HIP stars