Rho1 Cephei

Star in the constellation Cepheus From Wikipedia, the free encyclopedia

Rho1 Cephei is a double star located in the northern constellation of Cepheus. Its name is a Bayer designation that is Latinized from ρ1 Cephei, and abbreviated Rho1 Cep or ρ1 Cep. As of 2014, the pair had an angular separation of 0.29 arc seconds along a position angle of 211.1°. This corresponds to a projected separation of 18.1 AU.[3] Rho1 Cephei is faintly visible to the naked eye with an apparent visual magnitude of 5.84,[2] and it forms an optical pair with the brighter star Rho2 Cephei. Based upon an annual parallax shift of 16.26 mas as seen from the Earth,[1] Rho1 Cephei is located approximately 201 light-years (62 pc) from the Sun.

Quick facts Constellation, Right ascension ...
Rho1 Cephei
Location of ρ1 Cephei (circled in red)
Observation data
Epoch J2000.0      Equinox J2000.0 (ICRS)
Constellation Cepheus
Right ascension 22h 26m 42.434s[1]
Declination +78° 47 09.144[1]
Apparent magnitude (V) 5.84[2]
Characteristics
Spectral type A2m[3]
B−V color index −0.16[2]
Astrometry
Proper motion (μ) RA: −18.440 mas/yr[1]
Dec.: −48.707 mas/yr[1]
Parallax (π)16.2606±0.0414 mas[1]
Distance200.6 ± 0.5 ly
(61.5 ± 0.2 pc)
Details
ρ1 Cep A
Mass2.00 M[3]
1.82±0.04 M
Radius1.870±0.038[1] R
Luminosity13.89±0.08[1] L
Surface gravity (log g)3.8997+0.003
0.005
 cgs
Temperature7,600+9
7
[1] K
Rotational velocity (v sin i)81[4] km/s
Age320 Myr[3]
683±165[1] Myr
ρ1 Cep B
Mass0.51[3] M
Other designations
ρ1 Cep, 28 Cep, BD+78°796, HD 213403, HIP 110787, HR 8578, SAO 10375, WDS J22267+7847AB[5]
Database references
SIMBADdata
Close

The primary component is a chemically peculiar Am star with a stellar classification of A2m.[3] It has twice the mass of the Sun and is around 320 million years old.[3] The smaller companion may be the source of the X-ray emission from this location, as stars similar to the primary component do not generally produce detectable levels of X-rays.[6]

References

Related Articles

Wikiwand AI