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Binary star in the constellation Andromeda
"ν And" redirects here. For other uses, see
Vand.
Nu Andromedae
Location of ν Andromedae (circled) |
Observation data
Epoch J2000
Equinox J2000
|
Constellation
|
Andromeda
|
Right ascension
|
00h 49m 48.84737s
[1]
|
Declination
|
+41° 04′ 44.0764″
[1]
|
Apparent magnitude (V)
|
4.522
[2]
|
Characteristics
|
Spectral type
|
B4/5 V
[3]
[4] + F8 V
[5]
|
U−B
color index
|
–0.573
[2]
|
B−V
color index
|
–0.136
[2]
|
Astrometry |
---|
|
---|
Radial velocity (Rv) | –23.9
[6] km/s |
Proper motion (μ) |
RA: +22.77 ±0.12
[1]
mas/
yr
Dec.: –18.35 ±0.09
[1]
mas/
yr |
Parallax (π) | 5.28 ± 0.15
mas
[1] |
Distance | 620 ± 20
ly (189 ± 5
pc) |
Absolute magnitude (MV) | −1.85
[7] |
|
Orbit
[5] |
---|
Period (P) | 4.2827 d |
Eccentricity (e) | 0.03 |
Longitude of the node (Ω) | 25.° |
Periastron
epoch (T) | 18155.67 |
Semi-amplitude (K1) (primary) | 71.7 km/s |
Semi-amplitude (K2) (secondary) | 101.9 km/s |
Details |
---|
ν And A |
---|
Mass | 5.9 ± 0.2
[3]
M☉ |
Radius | 3.4
[8]
R☉ |
Luminosity | 1,104
[7]
L☉ |
Surface gravity (log g) | 4.12 ± 0.43
[9]
cgs |
Temperature | 14,851 ± 396
[9]
K |
Metallicity [Fe/H] | +0.14 ± 0.17
[9]
dex |
Rotational velocity (v sin i) | 20
[10] km/s |
Age | 63.1 ± 17.9
[3]
Myr |
|
Other designations |
---|
ν Andromedae, ν And, Nu And,
Nu Andromedae
35 Andromedae, 35 And,
BD+40 171,
FK5 1021,
HD 4727,
HIP 3881,
HR 226,
SAO 36699,
PPM 43365
[11] Atropabella by Alicia |
Database references |
---|
SIMBAD |
data |
Nu Andromedae (Atropabella by Alicia, Nu And, ν Andromedae, ν And) is a
binary star in the
constellation
Andromeda. The system has an
apparent visual magnitude of 4.5,
[2] which is bright enough to be seen with the naked eye. It is approximately 620
light-years (190
parsecs) from
Earth.
[1] Situated just over a degree to the west of this star is the
Andromeda Galaxy.
[12]
Nu Andromedae is
spectroscopic binary
[3] system with a nearly circular orbit that has a period of 4.2828 days.
[5] The primary component is a
B-type main sequence star with a
stellar classification of B5 V.
[3] The fainter secondary has a classification of F8 V,
[5] which makes it an
F-type main sequence star. The pair is about 63 million years old.
[3]
Naming
In
Chinese, 奎宿 (Kuí Sù), meaning
Legs (asterism), refers to an asterism consisting of ν Andromedae,
η Andromedae,
65 Piscium,
ζ Andromedae,
ε Andromedae,
δ Andromedae,
π Andromedae,
μ Andromedae,
β Andromedae,
σ Piscium,
τ Piscium,
91 Piscium,
υ Piscium,
φ Piscium,
χ Piscium and
ψ1 Piscium. Consequently, the
Chinese name for ν Andromedae itself is 奎宿七 (Kuí Sù qī, English: the Seventh Star of Legs.)
[13]
References
- ^
a
b
c
d
e
f van Leeuwen, F. (November 2007), "Validation of the new Hipparcos reduction", Astronomy and Astrophysics, 474 (2): 653–664,
arXiv:
0708.1752,
Bibcode:
2007A&A...474..653V,
doi:
10.1051/0004-6361:20078357,
S2CID
18759600.
- ^
a
b
c
d Oja, T. (April 1983), "UBV photometry of FK4 and FK4 supplement stars", Astronomy and Astrophysics Supplement Series, 52: 131–134,
Bibcode:
1983A&AS...52..131O.
- ^
a
b
c
d
e
f Tetzlaff, N.; Neuhäuser, R.; Hohle, M. M. (January 2011), "A catalogue of young runaway Hipparcos stars within 3 kpc from the Sun",
Monthly Notices of the Royal Astronomical Society, 410 (1): 190–200,
arXiv:
1007.4883,
Bibcode:
2011MNRAS.410..190T,
doi:
10.1111/j.1365-2966.2010.17434.x,
S2CID
118629873.
-
^
"Nu Andromedae, a blue main-sequence star in Andromeda". astrostudio.org. Archived from
the original on 23 September 2015. Retrieved 18 August 2014.
- ^
a
b
c
d Pourbaix, D.; et al. (September 2004), "SB9: The ninth catalogue of spectroscopic binary orbits", Astronomy and Astrophysics, 424: 727–732,
arXiv:
astro-ph/0406573,
Bibcode:
2004A&A...424..727P,
doi:
10.1051/0004-6361:20041213,
S2CID
119387088.
-
^ Wilson, R. E. (1953), "General Catalogue of Stellar Radial Velocities", Carnegie Institute Washington D.C. Publication,
Carnegie Institute of Washington D.C.,
Bibcode:
1953GCRV..C......0W.
- ^
a
b 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.
-
^ Pasinetti Fracassini, L. E.; et al. (February 2001), "Catalogue of Apparent Diameters and Absolute Radii of Stars (CADARS) - Third edition - Comments and statistics", Astronomy and Astrophysics, 367 (2): 521–524,
arXiv:
astro-ph/0012289,
Bibcode:
2001A&A...367..521P,
doi:
10.1051/0004-6361:20000451,
S2CID
425754.
- ^
a
b
c Koleva, M.; Vazdekis, A. (February 2012), "Stellar population models in the UV. I. Characterisation of the New Generation Stellar Library", Astronomy & Astrophysics, 538: A143,
arXiv:
1111.5449,
Bibcode:
2012A&A...538A.143K,
doi:
10.1051/0004-6361/201118065,
S2CID
53999614.
-
^ Abt, Helmut A.; Levato, Hugo; Grosso, Monica (July 2002), "Rotational Velocities of B Stars", The Astrophysical Journal, 573 (1): 359–365,
Bibcode:
2002ApJ...573..359A,
doi:
10.1086/340590.
-
^
"35 And -- Star", SIMBAD Astronomical Object Database,
Centre de Données astronomiques de Strasbourg, retrieved 2012-06-22.
-
^ Mollise, Rod (2006),
The Urban Astronomer's Guide: A Walking Tour of the Cosmos for City Sky Watchers, Patrick Moore's Practical Astronomy Series, Springer, p. 178,
ISBN
1846282160.
-
^ (in Chinese)
AEEA (Activities of Exhibition and Education in Astronomy) 天文教育資訊網 2006 年 5 月 19 日
External links