RW Cephei

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RW Cephei
Cepheus constellation map.svg
Red circle.svg

Position of RW Cephei
Observation data
Epoch J2000.0      Equinox J2000.0
Constellation Cepheus
Right ascension 22h 23m 07.01657s[1]
Declination +55° 57′ 47.6262″[1]
Apparent magnitude (V) +6.59[2]
Characteristics
Spectral type K20-Ia[3]
Apparent magnitude (K) 1.88[4]
U−B color index 2.38[4]
B−V color index 2.22[4]
Variable type SRd[5]
Astrometry
Radial velocity (Rv) -56.00[6] km/s
Proper motion (μ) RA: -2.74[1] mas/yr
Dec.: -2.66[1] mas/yr
Parallax (π) 0.81 ± 0.36[1] mas
Distance 3,500[7] pc
Absolute magnitude (MV) -9.4[7]
Details
Radius 1,535[7][8] R
Luminosity 550,000[7] L
Temperature 4,015[8] K
Other designations
HD 212466, HIP 110504, SAO 34387, BD+55°2737, AAVSO 2219+55A
Database references
SIMBAD data

RW Cephei is an orange hypergiant star in the constellation Cepheus. One of the largest stars known, RW Cephei is estimated at 1,535 solar radii, which is larger than the orbit of Jupiter.

RW Cephei is also a semi-regular variable star of type SRd, meaning that it is a slowly varying yellow giant or supergiant. Its surface is subject to pulsations in temperature and luminosity. Over the past 50 to 70 years it has varied from classes G8 to M0 with no discernible pattern.[9] Despite its variable spectral type, it has been listed as a spectral standard star for type "K2 0-Ia".[3]

The distance to RW Cephei has been estimated on the basis of its spectroscopic luminosity and is assumed to be a member of the Cepheus OB1 association at 3,500 parsecs. This is several times further than the distance implied by the Hipparcos parallax, although the apparent diameter of the star is larger than the measured parallax and variable.[9][2]

The temperature intermediate between the red supergiants and yellow hypergiants, and itself varying considerably, has led to it being variously considered as a red hypergiant or [10] or yellow hypergiant.[11]

References

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See also

<<< 7. VV Cephei A 9. KY Cygni/VY Canis Majoris >>>