32 Pegasi is a multiple giant star in the constellation of Pegasus.
32 Pegasi visual magnitude is 4.81. Because of its moderate brightness, 32 Pegasi should be easily visible from locations with dark skyes, while it can be barely visible, or not visible at all, from skyes affected by light pollution.
The table below summarizes the key facts about 32 Pegasi:
Celestial coordinates and finder chart of 32 Pegasi
32 Pegasi is situated north of the celestial equator, as such, it is more easily visible from the northern hemisphere. Celestial coordinates for the J2000 equinox as well as galactic coordinates of 32 Pegasi are provided in the following table:
The simplified sky map below shows the position of 32 Pegasi in the sky:
Visibility of 32 Pegasi from your location
Digitized Sky Survey image of 32 Pegasi
The image below is a photograph of 32 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 32 Pegasi is 0.018 arcsec per year in Right Ascension and 0.002 arcsec per year in Declination and the associated displacement for the next 10000 years is represented with the red arrow.
Distance of 32 Pegasi from the Sun and relative movement
32 Pegasi is distant 607.08 light years from the Sun and it is moving far from the Sun at the speed of 8 kilometers per second.
Spectral properties of 32 Pegasi
32 Pegasi belongs to spectral class B9 and has a luminosity class of III corresponding to a giant star.
The red dot in the diagram below shows where 32 Pegasi is situated in the Hertzsprung–Russell diagram.
32 Pegasi star system properties
32 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 32 Pegasi double sysyem: