51 Andromedae

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Star
51 Andromedae
AladinLite
Observation
dates equinoxJ2000.0 , epoch : J2000.0
Constellation Andromeda
Right ascension 01 h 37 m 59.56 s
declination + 48 ° 37 ′ 41.6 ″
Apparent brightness 3.57 likes
Typing
B − V color index +1.28 
U − B color index +1.45 
R − I index +0.65 
Spectral class K3 III
Astrometry
Radial velocity (+16.15 ± 0.19) km / s
parallax (18.76 ± 0.74)  mas
distance (174 ± 7)  ly
(53 ± 2)  pc  
Proper movement 
Rec. Share: (+61.95 ± 0.17)  mas / a
Dec. portion: (−112.15 ± 0.17)  mas / a
Physical Properties
Other names
and catalog entries
Bayer name υ Persei
Flamsteed name 51 Andromedae
Bonn survey BD + 47 ° 467
Bright Star Catalog HR 464 [1]
Henry Draper Catalog HD 9927 [2]
Hipparcos catalog HIP 7607 [3]
SAO catalog SAO 37375 [4]
Tycho catalog TYC 3282-2271-1 [5]Template: Infobox star / maintenance / specification of the TYC catalog
Other names FK5  52

51 Andromedae (proper name: Nembus , former name Ypsilon Persei ) is a bright K-type giant in the constellation Andromeda and is around 174  light years from Earth .

The star is already mentioned by Ptolemy in the Almagest and placed in the constellation Andromeda. In Johann Bayer's Uranometria from 1603, the star appears as υ Persei in the constellation of Perseus . The International Astronomical Union moved the celestial body back into the constellation Andromeda and John Flamsteed's designation 51 Andromedae prevailed. Both Johann Bayer and Johann Elert Bode use the name of the star as a nembus .

literature

Individual evidence

  1. a b c d Hipparcos catalog
  2. a b c SIMBAD database
  3. a b c Bright Star Catalog
  4. Famaey et al .: Local kinematics of K and M giants from CORAVEL / Hipparcos / Tycho-2 data. Revisiting the concept of superclusters. ; in: Astronomy and Astrophysics , Vol. 430, 2005, pp. 165ff. bibcode : 2005A & A ... 430..165F
  5. Morton Wagman: Lost Stars. P. 240, McDonald and Woodward, Blacksburg, Virginia 2003 ISBN 0-939923-78-5