Star in the constellation Andromeda
Not to be confused with Andromeda III .
3 Andromedae
3 Andromedae (circled) in a close northerly run-of-stars asterism – 5, 7, 8, 11 being close by, south-westward.
Observation dataEpoch J2000 Equinox J2000
Constellation
Andromeda
Right ascension
23 04 10.98269
Declination
+50° 03′ 07.5255″
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 )−34.87±0.12 km/s Proper motion (μ) RA: 165.837 mas /yr Dec.: 167.716 mas /yr Parallax (π)17.2629 ± 0.0918 mas Distance 189 ± 1 ly (57.9 ± 0.3 pc ) Absolute magnitude (MV )0.97
Details Mass 1.71 M ☉ Radius 10 R ☉ Luminosity 49 L ☉ Surface gravity (log g )2.61±0.11 cgs Temperature 4,668±45 K Metallicity −0.08 dex Rotational velocity (v sin i )1.0 km/s Age 2.27 Gyr
Other designations 3 And , BD +49° 4028, HD 218031, HIP 113919, HR 8780, SAO 52649, PPM 41448, LTT 16772
Database references SIMBAD data
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 17.3 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.
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.
References
^ Vallenari, A.; et al. (Gaia collaboration) (2023). "Gaia Data Release 3. Summary of the content and survey properties" . Astronomy and Astrophysics . 674 : A1. arXiv :2208.00211 . Bibcode :2023A&A...674A...1G . doi :10.1051/0004-6361/202243940 . S2CID 244398875 .
Gaia DR3 record for this source at VizieR .
^ Anderson, E.; Francis, Ch. (2012), "XHIP: An extended hipparcos compilation", Astronomy Letters , 38 (5): 331, arXiv :1108.4971 , Bibcode :2012AstL...38..331A , doi :10.1134/S1063773712050015 , S2CID 119257644 .
^ Tautvaišienė, G.; et al. (December 2010), "C, N and O abundances in red clump stars of the Milky Way", Monthly Notices of the Royal Astronomical Society , 409 (3): 1213–1219, arXiv :1007.4064 , Bibcode :2010MNRAS.409.1213T , doi :10.1111/j.1365-2966.2010.17381.x , S2CID 119182458 .
^ Keenan, Philip C.; McNeil, Raymond C. (1989), "The Perkins catalog of revised MK types for the cooler stars", Astrophysical Journal Supplement Series , 71 : 245, Bibcode :1989ApJS...71..245K , doi :10.1086/191373 .
^ Luck, R. Earle (2015), "Abundances in the Local Region. I. G and K Giants", Astronomical Journal , 150 (3), 88, arXiv :1507.01466 , Bibcode :2015AJ....150...88L , doi :10.1088/0004-6256/150/3/88 , S2CID 118505114 .
^ Massarotti, Alessandro; et al. (January 2008), "Rotational and Radial Velocities for a Sample of 761 HIPPARCOS Giants and the Role of Binarity", The Astronomical Journal , 135 (1): 209–231, Bibcode :2008AJ....135..209M , doi :10.1088/0004-6256/135/1/209 .
Feuillet, Diane K.; et al. (2016), "Determining Ages of APOGEE Giants with Known Distances", The Astrophysical Journal , 817 (1): 40, arXiv :1511.04088 , Bibcode :2016ApJ...817...40F , doi :10.3847/0004-637X/817/1/40 , S2CID 118675933 .
De Medeiros, J. R.; et al. (November 2000), "Rotation and lithium in single giant stars", Astronomy and Astrophysics , 363 : 239–243, arXiv :astro-ph/0010273 , Bibcode :2000A&A...363..239D .
"3 And" . SIMBAD . Centre de données astronomiques de Strasbourg . Retrieved September 12, 2018.
Eggleton, P. P.; Tokovinin, A. A. (September 2008), "A catalogue of multiplicity among bright stellar systems", Monthly Notices of the Royal Astronomical Society , 389 (2): 869–879, arXiv :0806.2878 , Bibcode :2008MNRAS.389..869E , doi :10.1111/j.1365-2966.2008.13596.x , S2CID 14878976 .
Gontcharov, G. A. (2006), "Pulkovo Compilation of Radial Velocities for 35 495 Hipparcos stars in a common system", Astronomy Letters , 32 (11): 759–771, arXiv :1606.08053 , Bibcode :2006AstL...32..759G , doi :10.1134/S1063773706110065 , S2CID 119231169 .
Lépine, Sébastien; Shara, Michael M. (March 2005), "A Catalog of Northern Stars with Annual Proper Motions Larger than 0.15" (LSPM-NORTH Catalog)", The Astronomical Journal , 129 (3): 1483–1522, arXiv :astro-ph/0412070 , Bibcode :2005AJ....129.1483L , doi :10.1086/427854 , S2CID 2603568 .
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