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R Reticuli

Variable star in the constellation Reticulum From Wikipedia, the free encyclopedia

R Reticuli, also listed under the duplicate variable star designation S Reticuli,[3] is a Mira variable star in the southern constellation Reticulum. It is an aging red giant star on the asymptotic giant branch[4] with a stellar classification that varies between M4e to M7.5e,[5] being hottest near maximum visual magnitude.[10] The brightness of the star varies between apparent visual magnitudes 6.35 and 14.2[3] with an average period of 281.08±0.58 d.[11] The mean maximum magnitude is 7.57 and the mean minimum magnitude 13.80.[11]

Right ascension04h 33m 32.83070s[2]
Declination−63° 01 44.9951[2]
Apparentmagnitude(V)6.35 – 14.2[3]
Quick facts Constellation, Right ascension ...
R Reticuli

The visual band light curve of R Reticui, from AAVSO data[1]
Observation data
Epoch J2000      Equinox ICRS
Constellation Reticulum
Right ascension 04h 33m 32.83070s[2]
Declination −63° 01 44.9951[2]
Apparent magnitude (V) 6.35 – 14.2[3]
Characteristics
Evolutionary stage AGB[4]
Spectral type M4e - M7.5e[5]
B−V color index 1.099±0.045[6]
Variable type Mira[5]
Astrometry
Radial velocity (Rv)26.0±4.6[6] km/s
Proper motion (μ) RA: +12.111[2] mas/yr
Dec.: +16.384[2] mas/yr
Parallax (π)1.3622±0.0492 mas[2]
Distance2,390 ± 90 ly
(730 ± 30 pc)
Details
Mass0.88+0.04
−0
[7] M
Radius249+21
−34
[8] R
Luminosity7,571±1,671[8] L
Surface gravity (log g)−0.445[7] cgs
Temperature3,410+264
−131
[8] K
Metallicity [Fe/H]0.55[7] dex
Other designations
R Ret, S Ret, HD 29383, HIP 21252, SAO 249053[9]
Database references
SIMBADdata
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