ε Serpentis (epsilon Serpentis)
ε Serpentis is a main-sequence star of spectral class A2 in the constellation of Serpens.
ε Serpentis visual magnitude is 3.71. Because of its moderate brightness, ε 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
Simplified finder chart for ε Serpentis (epsilon Serpentis).
Magnitude, Color, Spectral Class
The red dot in the diagram below shows where ε Serpentis is situated in the Hertzsprung–Russell diagram.
Distance, Radial Speed, Proper Motion
ε Serpentis is distant 70.27 light years from the Sun and it is moving towards the Sun at the speed of 9 kilometers per second.
Alternative Designations
Visibility from Your Location
Today's ε Serpentis (epsilon Serpentis) rise, transit and set times from Greenwich, UK are the following (all times relative to the local timezone Europe/London):