HR 244

Star in the constellation Cassiopeia From Wikipedia, the free encyclopedia

HR 244 is a single[8] star in the constellation Cassiopeia. It has a yellow-white hue and is visible to the naked eye with an apparent visual magnitude of 4.80.[3] Based upon parallax measurements, it is located at a distance of 62 light years from the Sun, and is drifting further away with a radial velocity of +20.7 km/s;[2] around 546,000 years ago it passed within 38 light-years of the Sun.[5] The star has a relatively high proper motion, traversing the celestial sphere at the rate of 0.183 arcseconds per annum.[9]

Quick facts Observation data Epoch J2000 Equinox J2000, Constellation ...
HR 244
Location of HR 244 (circled in red)
Observation data
Epoch J2000      Equinox J2000
Constellation Cassiopeia[1]
Right ascension 00h 53m 04.19644s[2]
Declination +61° 07 26.2993[2]
Apparent magnitude (V) 4.80[3]
Characteristics
Evolutionary stage subgiant[2]
Spectral type F9V[4]
B−V color index 0.540±0.008[5]
Astrometry
Radial velocity (Rv)+20.68±0.12[2] km/s
Proper motion (μ) RA: –68.298[2] mas/yr
Dec.: +169.435[2] mas/yr
Parallax (π)52.9017±0.1037 mas[2]
Distance61.7 ± 0.1 ly
(18.90 ± 0.04 pc)
Absolute magnitude (MV)3.44[5]
Details
Mass1.194[6] M
Radius1.77[2] R
Luminosity3.7[2] L
Surface gravity (log g)0.53[3] cgs
Temperature5,986[2] K
Metallicity [Fe/H]0.04[6] dex
Rotational velocity (v sin i)8.1[3] km/s
Age5.3[6] Gyr
Other designations
BD+60°124, GJ 41, HD 5015, HIP 4151, HR 244, SAO 11444, WDS J00531+6107A[7]
Database references
SIMBADdata
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This object is an F-type star with a stellar classification of F9V.[4] Despite the spectral class, evolutionary models show it to have left the main sequence and is now a subgiant.[2] It is 5.3[6] billion years old and is spinning with a projected rotational velocity of 8 km/s.[3] The star has 1.2[6] times the mass of the Sun and 1.8[2] times the Sun's radius. It is radiating 3.7 times the luminosity of the Sun from its photosphere at an effective temperature of 5,986 K.[2]

References

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