Rho Andromedae
Star in the constellation Andromeda
From Wikipedia, the free encyclopedia
Rho Andromedae is a star in the northern constellation of Andromeda. Its Bayer designation is Latinized from ρ Andromedae, abbreviated Rho And or ρ And, respectively. The star has an apparent visual magnitude of +5.19,[2] 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 164 light-years (50 parsecs) from the Sun.[1] It is drifting further away with a radial velocity of +10 km/s.[4]
 | |
| Observation data Epoch J2000.0 Equinox ICRS | |
|---|---|
| Constellation | Andromeda |
| Right ascension | 00h 21m 07.26896s[1] |
| Declination | +37° 58′ 06.9727″[1] |
| Apparent magnitude (V) | +5.19[2] |
| Characteristics | |
| Spectral type | F5IV-V[3] |
| U−B color index | +0.039[2] |
| B−V color index | +0.424[2] |
| Astrometry | |
| Radial velocity (Rv) | +10.4±0.6[4] km/s |
| Proper motion (μ) | RA: +57.737 mas/yr[1] Dec.: –38.838 mas/yr[1] |
| Parallax (π) | 19.9513±0.0739 mas[1] |
| Distance | 163.5 ± 0.6 ly (50.1 ± 0.2 pc) |
| Absolute magnitude (MV) | +1.73[5] |
| Details | |
| Mass | 1.812±0.024[6] M☉ |
| Radius | 3.234±0.034[6] R☉ |
| Luminosity | 18.672±0.157[6] L☉ |
| Surface gravity (log g) | 3.69±0.04[6] cgs |
| Temperature | 6,674±34[6] K |
| Metallicity [Fe/H] | –0.09±0.03[6] dex |
| Rotational velocity (v sin i) | 44[7] km/s |
| Age | 1.3[5] Gyr |
| Other designations | |
| ρ And, 27 Andromedae, BD+37 45, FK5 1009, HD 1671, HIP 1686, HR 82, SAO 53828, PPM 65222[8] | |
| Database references | |
| SIMBAD | data |
The stellar classification of this star is F5IV-V,[3] showing mixed spectral features of a main sequence and subgiant stage. It is about 1.3[5] billion years old and is spinning with a projected rotational velocity of 44 km/s.[7] The star has 1.8 times the mass of the Sun and 3.2 times the Sun's girth. The outer envelope is radiating around 18.7 times the luminosity of the Sun from its photosphere at an effective temperature of 6,674 K,[6] giving it the yellow-white hue of an F-type star.[9] X-ray emissions were detected from this star during the EXOSAT mission.[10]
Naming
In Chinese, 天廄 (Tiān Jiù), meaning Celestial Stable, refers to an asterism consisting of ρ Andromedae, θ Andromedae, σ Andromedae and seven fainter, unidentified stars. Consequently, the Chinese name for ρ Andromedae itself is 天廄二 (Tiān Jiù èr, English: the Second Star of Celestial Stable.)[11]