3 Andromedae

3 Andromedae, abbreviated 3 And, is a single star in the northern constellation of Andromeda. 3 Andromedae is the Flamsteed designation. It is visible to the naked eye with an apparent visual magnitude of 4.64. The distance to this star, as determined from an annual parallax shift of 18 mas, is 181 light years. It is moving closer to the Earth with a heliocentric radial velocity of 35 km/s, and has a relatively large proper motion, traversing the celestial sphere at 0.236″·yr−1.

3 Andromedae
3 Andromedae (circled) in a close northerly run-of-stars asterism 5, 7, 8, 11 being close by, south-westward.
Observation data
Epoch J2000      Equinox J2000
Constellation Andromeda
Right ascension 23h 04m 10.98185s
Declination +50° 03 07.5297
Apparent magnitude (V) 4.64
Characteristics
Evolutionary stage giant
Spectral type K0 IIIb
B−V color index 1.058±0.003
Astrometry
Radial velocity (Rv)−34.7±0.3 km/s
Proper motion (μ) RA: 166.374 mas/yr
Dec.: 167.463 mas/yr
Parallax (π)17.9785 ± 0.1522 mas
Distance181 ± 2 ly
(55.6 ± 0.5 pc)
Absolute magnitude (MV)0.97
Details
Mass1.71 M
Radius10 R
Luminosity49 L
Surface gravity (log g)2.61±0.11 cgs
Temperature4,668±45 K
Metallicity [Fe/H]−0.08 dex
Rotational velocity (v sin i)1.0 km/s
Age2.27 Gyr
Other designations
3 And, BD+49° 4028, HD 218031, HIP 113919, HR 8780, SAO 52649, PPM 41448, LTT 16772
Database references
SIMBADdata

This is an evolved giant star with a stellar classification of K0 IIIb, where the 'b' suffix indicated a lower luminosity giant. It is a red clump star, which means it is generating energy through helium fusion at its core. This star has an estimated 1.7 times the mass of the Sun (M), and, at the age of 2.3 billion years, has expanded to 10 times the Sun's radius (R). It is radiating 49 times the Sun's luminosity from its enlarged photosphere at an effective temperature of 4,668 K.

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