Gamma Reticuli

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Gamma Reticuli
Diagram showing star positions and boundaries of the Reticulum constellation and its surroundings
Cercle rouge 100%.svg

Location of γ Reticuli (circled)
Observation data
Epoch J2000.0      Equinox J2000.0
Constellation Reticulum
Right ascension 04h 00m 53.81s
Declination −62° 09′ 33.7″
Apparent magnitude (V) +4.48
Distance 490 ly
(150 pc)
Spectral type M4III
Other designations
γ Reticuli, γ Ret, Gamma Ret, CPD−62  312, GC 4855, HD 25705, HIP 18744, HR 1264, PPM 353858, SAO 248925

Gamma Reticuli (Gamma Ret, γ Reticuli, γ Ret) is a red M-type giant with an apparent magnitude of +4.48. It is approximately 490 light years from Earth.

Gamma Reticuli is moving through the Galaxy at a speed of 24.8 km/s relative to the Sun. Its projected Galactic orbit carries it between 24,100 and 39,200 light years from the center of the Galaxy.[1]

References