Beta Gruis

Beta Gruis (β Gruis, abbreviated Beta Gru, β Gru), formally named Tiaki /tiˈɑːki/, is the second brightest star in the southern constellation of Grus. It was once considered the rear star in the tail of the constellation of the (Southern) Fish, Piscis Austrinus: it, with Alpha, Delta, Theta, Iota, and Lambda Gruis, belonged to Piscis Austrinus in medieval Arabic astronomy.

Beta Gruis
Location of β Gruis (circled)
Observation data
Epoch J2000      Equinox J2000
Constellation Grus
Right ascension 22h 42m 40.05027s
Declination 46° 53 04.4752
Apparent magnitude (V) 2.146 (2.0 - 2.3)
Characteristics
Evolutionary stage AGB
Spectral type M5 III
U−B color index +1.757
B−V color index +1.620
Variable type SRb
Astrometry
Radial velocity (Rv)+1.6 km/s
Proper motion (μ) RA: +135.16 mas/yr
Dec.: 4.38 mas/yr
Parallax (π)18.43 ± 0.42 mas
Distance177 ± 4 ly
(54 ± 1 pc)
Absolute magnitude (MV)−1.61±0.052
Details
Mass2.4 M
Radius138 R
Luminosity2,500 L
Surface gravity (log g)0.4 cgs
Temperature3,480 K
Metallicity [Fe/H]0.0 dex
Other designations
Tiaki, Beta Gru, CD47 14308, FK5 856, HR 8636, HD 214952, HIP 112122, SAO 231258.
Database references
SIMBADdata
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