35 Pegasi is a multiple hypergiant star in the constellation of Pegasus.
35 Pegasi visual magnitude is 4.79. Because of its moderate brightness, 35 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 35 Pegasi:
Celestial coordinates and finder chart of 35 Pegasi
35 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 35 Pegasi are provided in the following table:
The simplified sky map below shows the position of 35 Pegasi in the sky:
Visibility of 35 Pegasi from your location
Digitized Sky Survey image of 35 Pegasi
The image below is a photograph of 35 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 35 Pegasi is 0.081 arcsec per year in Right Ascension and -0.308 arcsec per year in Declination and the associated displacement for the next 1000 years is represented with the red arrow.
Distance of 35 Pegasi from the Sun and relative movement
35 Pegasi is distant 159.88 light years from the Sun and it is moving far from the Sun at the speed of 54 kilometers per second.
Spectral properties of 35 Pegasi
35 Pegasi belongs to spectral class K0 and has a luminosity class of III corresponding to a hypergiant star.
The red dot in the diagram below shows where 35 Pegasi is situated in the Hertzsprung–Russell diagram.
35 Pegasi star system properties
35 Pegasi is a visual double star which can be observed with the help of small or medium telescopes. The table below shows key information about the 35 Pegasi double sysyem: