ι Pegasi (iota Pegasi)
ι Pegasi is a variable and double main-sequence star of spectral class F5 in the constellation of Pegasus.
ι Pegasi visual magnitude is 3.76. Because of its moderate brightness, ι Pegasi 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
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Finder chart for ι Pegasi (iota Pegasi).
Magnitude, Color, Spectral Class
The red dot in the diagram below shows where ι Pegasi is situated in the Hertzsprung–Russell diagram.
Star System Properties
ι Pegasi 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 ι Pegasi double sysyem:
Distance, Radial Speed, Proper Motion
ι Pegasi is distant 38.33 light years from the Sun and it is moving towards the Sun at the speed of 4 kilometers per second.
Alternative Designations
Visibility from Your Location
Today's ι Pegasi (iota Pegasi) rise, transit and set times from Greenwich, UK are the following (all times relative to the local timezone Europe/London):