β Equulei (beta Equulei)
β Equulei is a multiple main-sequence star of spectral class A3 in the constellation of Equuleus.
β Equulei visual magnitude is 5.16. Because of its faintness, β Equulei is visible to the naked eye only from locations with very dark skies, while it is not visible at all from skies affected by light pollution.

Celestial Coordinates
Apparent
J2000
Galactic Coordinates
Finder Chart

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

Star System Properties
β Equulei 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 β Equulei double sysyem:
Distance, Radial Speed, Proper Motion
β Equulei is distant 359.82 light years from the Sun and it is moving towards the Sun at the speed of 11 kilometers per second.
Alternative Designations
Visibility from Your Location
Today's β Equulei (beta Equulei) rise, transit and set times from Greenwich, UK are the following (all times relative to the local timezone Europe/London):