37 Pegasi is a double main-sequence star in the constellation of Pegasus.
37 Pegasi visual magnitude is 5.48. Because of its reltive faintness, 37 Pegasi should be visible only from locations with dark skyes, while it is not visible at all from skyes affected by light pollution.
The table below summarizes the key facts about 37 Pegasi:
Celestial coordinates and finder chart of 37 Pegasi
37 Pegasi is situated close to the celestial equator, as such, it is at least partly visible from both hemispheres in certain times of the year. Celestial coordinates for the J2000 equinox as well as galactic coordinates of 37 Pegasi are provided in the following table:
The simplified sky map below shows the position of 37 Pegasi in the sky:
Visibility of 37 Pegasi from your location
Digitized Sky Survey image of 37 Pegasi
The image below is a photograph of 37 Pegasi from the Digitized Sky Survey 2 (DSS2 - see the credits section) taken in the red channel. The area of sky represented in the image is 0.5x0.5 degrees (30x30 arcmins). The proper motion of 37 Pegasi is -0.023 arcsec per year in Right Ascension and -0.144 arcsec per year in Declination and the associated displacement for the next 1000 years is represented with the red arrow.
Distance of 37 Pegasi from the Sun and relative movement
37 Pegasi is distant 172.21 light years from the Sun and it is moving far from the Sun at the speed of 1 kilometers per second.
Spectral properties of 37 Pegasi
37 Pegasi belongs to spectral class F2 and has a luminosity class of V corresponding to a main-sequence star.
The red dot in the diagram below shows where 37 Pegasi is situated in the Hertzsprung–Russell diagram.
37 Pegasi star system properties
37 Pegasi is a visual double star which can be observed with the help of large telescopes. The table below shows key information about the 37 Pegasi double sysyem: