γ Serpentis (gamma Serpentis)
γ Serpentis is a variable and multiple main-sequence star of spectral class F6 in the constellation of Serpens.
γ Serpentis visual magnitude is 3.85. Because of its moderate brightness, γ Serpentis 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
Loading map...
Finder chart for γ Serpentis (gamma Serpentis).
Magnitude, Color, Spectral Class

The red dot in the diagram below shows where γ Serpentis is situated in the Hertzsprung–Russell diagram.

Star System Properties
γ Serpentis is a visual double star which can be observed only with the help of very large telescopes. The table below shows key information about the γ Serpentis double sysyem:
Distance, Radial Speed, Proper Motion
γ Serpentis is distant 36.25 light years from the Sun and it is moving far from the Sun at the speed of 7 kilometers per second.
Alternative Designations
Visibility from Your Location
Today's γ Serpentis (gamma Serpentis) rise, transit and set times from Greenwich, UK are the following (all times relative to the local timezone Europe/London):