γ Equulei (gamma Equulei)
γ Equulei is a variable and multiple hypergiant star of spectral class F0 in the constellation of Equuleus.
γ Equulei visual magnitude is 4.69. Because of its moderate brightness, γ Equulei is easily visible to the naked eye from locations with dark skies, while it might be barely visible, or not visible at all, from light-polluted skies.

Celestial Coordinates
Apparent
J2000
Galactic Coordinates
Finder Chart

Magnitude, Color, Spectral Class
The red dot in the diagram below shows where γ Equulei is situated in the Hertzsprung–Russell diagram.

Star System Properties
γ Equulei is a visual double star which can be observed with binoculars or small telescopes. The table below shows key information about the γ Equulei double sysyem:
Distance, Radial Speed, Proper Motion
γ Equulei is distant 114.87 light years from the Sun and it is moving towards the Sun at the speed of 17 kilometers per second.
Alternative Designations
Visibility from Your Location
Today's γ Equulei (gamma Equulei) rise, transit and set times from Greenwich, UK are the following (all times relative to the local timezone Europe/London):