36 Andromedae
Star 36 Andromedae |
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AladinLite | |||||||||||||
Observation dates equinox : J2000.0 , epoch : J2000.0 |
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Constellation | Andromeda | ||||||||||||
Right ascension | 00 h 54 m 58.11 s | ||||||||||||
declination | + 23 ° 37 ′ 42 ″ | ||||||||||||
Apparent brightness | 5.46 likes | ||||||||||||
Typing | |||||||||||||
B − V color index | 1.0 | ||||||||||||
U − B color index | 0.9 | ||||||||||||
R − I index | 0.5 | ||||||||||||
Spectral class | K1 IV | ||||||||||||
Astrometry | |||||||||||||
Radial velocity | 1.5 km / s | ||||||||||||
parallax | (26.33 ± 0.65) mas | ||||||||||||
distance | (124 ± 3) ly (38.0 ± 0.9) pc |
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Visual absolute brightness M vis | approx. 2.6 mag | ||||||||||||
Proper movement | |||||||||||||
Rec. Share: | (135.43 ± 1.00) mas / a | ||||||||||||
Dec. portion: | (−48.61 ± 0.48) mas / a | ||||||||||||
Physical Properties | |||||||||||||
Other names and catalog entries |
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36 Andromedae (short 36 And ) is a star with the apparent magnitude of 5.46 mag in the constellation Andromeda . It is located between Eta and Zeta Andromedae. Its distance is about 124 light years . It is a narrow binary star system that cannot be resolved with the naked eye , the components of which, two yellow-orange sub-giants , 6.1 mag and 6.5 mag are bright. They reached their minimum distance in the periastron in 1957 when they were only 0.6 " apart; by 2040 their distance will have increased to about 1.4". They orbit each other in almost 168 years. The major semi-axis of its orbit is about 0.98 ", the eccentricity of the orbit about 0.31 and the orbit inclination about 44.6 °.
Individual evidence
- ↑ a b c d Hipparcos, the New Reduction (van Leeuwen, 2007)
- ↑ a b Hipparcos catalog (ESA 1997)
- ↑ a b c Bright Star Catalog
- ↑ John Sanford: The new cosmos star atlas . English original edition London 1989, German Stuttgart 1990, ISBN 3-440-06087-X , p. 11
- ↑ W. Matthew Muterspaugh et al. (2010): “The Phases Differential Astrometry Data Archive. II. Updated Binary Star Orbits and a Long Period Eclipsing Binary ” . The Astronomical Journal 140 (6), p. 1623-1630.