Rho Andromedae

Rho Andromedae, Latinized from ρ Andromedae, is the Bayer designation for a star in the northern constellation of Andromeda. It has an apparent visual magnitude of +5.19, which, according to the Bortle Dark-Sky Scale, is bright enough to be seen with the naked eye from dark suburban skies. Based upon parallax measurements, this star is at a distance of approximately 162 light-years (50 parsecs) from the Sun. It is drifting further away with a radial velocity of +10 km/s.

Rho Andromedae
Location of ρ Andromedae (circled)
Observation data
Epoch J2000.0      Equinox J2000.0
Constellation Andromeda
Right ascension 00h 21m 07.26896s
Declination +37° 58 06.9727
Apparent magnitude (V) +5.19
Characteristics
Spectral type F5IV-V
U−B color index +0.039
B−V color index +0.424
Astrometry
Radial velocity (Rv)+10.4±0.6 km/s
Proper motion (μ) RA: +57.599 mas/yr
Dec.: –38.378 mas/yr
Parallax (π)20.1874 ± 0.1179 mas
Distance161.6 ± 0.9 ly
(49.5 ± 0.3 pc)
Absolute magnitude (MV)+1.73
Details
Radius3.37+0.07
−0.03
 R
Luminosity17.93±0.13 L
Surface gravity (log g)3.84 cgs
Temperature6,471+25
−66
 K
Metallicity [Fe/H]–0.09 dex
Rotational velocity (v sin i)44 km/s
Age1.3 Gyr
Other designations
ρ And, 27 Andromedae, BD+37 45, FK5 1009, HD 1671, HIP 1686, HR 82, SAO 53828, PPM 65222
Database references
SIMBADdata

The stellar classification of this star is F5IV-V, showing mixed spectral features of a main sequence and subgiant stage. It is about 1.3 billion years old with 3.4 times the girth of the Sun and is spinning with a projected rotational velocity of 44 km/s. The outer envelope is radiating around 18 times the luminosity of the Sun from its photosphere at an effective temperature of 6,471 K, giving it the yellow-white hue of an F-type star. X-ray emissions were detected from this star during the EXOSAT mission.

This article is issued from Wikipedia. The text is licensed under Creative Commons - Attribution - Sharealike. Additional terms may apply for the media files.