HD 201298

Star in the constellation Equuleus From Wikipedia, the free encyclopedia

HD 201298 (HR 8090) is a solitary star located in the northern constellation Equuleus, just next to 3 Equulei. It has an apparent magnitude of 6.14,[1] making it barely visible to the naked eye under ideal conditions. The star is situated at a distance of 1,140 light years[2] but is drifting away with a heliocentric radial velocity of 20 km/s.[6]

Right ascension21h 08m 28.1388s[2]
Declination+06° 59′ 21.695″[2]
Quick facts Observation data Epoch J2000 Equinox J2000, Constellation ...
HD 201298
Location of HD 201298 (circled)
Observation data
Epoch J2000      Equinox J2000
Constellation Equuleus[1]
Right ascension 21h 08m 28.1388s[2]
Declination +06° 59′ 21.695″[2]
Apparent magnitude (V) 6.14[1]
Characteristics
Evolutionary stage red giant branch?[3]
Spectral type M0 III[4]
U−B color index +1.97[5]
B−V color index +1.66[5]
Astrometry
Radial velocity (Rv)20 ± 2[6] km/s
Proper motion (μ) RA: âˆ’10.643 mas/yr[2]
Dec.: +2.479 mas/yr[2]
Parallax (π)2.8646±0.0533 mas[2]
Distance1,140 ± 20 ly
(349 ± 6 pc)
Absolute magnitude (MV)−0.39[7]
Details
Mass1.83[8] M☉
Radius117[8] R☉
Luminosity1,648[9] L☉
Surface gravity (log g)0.413[10] cgs
Temperature3,732[9] K
Rotational velocity (v sin i)4.5 ± 1[11] km/s
Other designations
12 G. Equueli, AG+06°2888, BD+06°4754, FK5 3692, GC 29548, HD 201298, HIP 104357, HR 8090, SAO 126566[12][13]
Database references
SIMBADdata
Close

HD 201298 has a stellar classification of M0 III, indicating that it is ageing M-type star[4] that is probably on the red giant branch.[3] As a result, it has expanded to 117 times the Sun's girth.[8] At present it has 1.83 times the mass of the Sun[8] and shines with a luminosity of 1,648 L☉ from its enlarged photosphere at an effective temperature of 3,732 K,[9] which gives it an orange glow. HD 201298 spins leisurely with a projected rotational velocity of 4.5±1 km/s,[11] slightly faster than most giants.

References

Related Articles

Wikiwand AI