33 Pegasi is a multiple main-sequence star in the constellation of Pegasus.
33 Pegasi visual magnitude is 6.04. Because of its reltive faintness, 33 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 33 Pegasi:
Celestial coordinates and finder chart of 33 Pegasi
33 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 33 Pegasi are provided in the following table:
The simplified sky map below shows the position of 33 Pegasi in the sky:
Visibility of 33 Pegasi from your location
Digitized Sky Survey image of 33 Pegasi
The image below is a photograph of 33 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 33 Pegasi is 0.337 arcsec per year in Right Ascension and -0.015 arcsec per year in Declination and the associated displacement for the next 1000 years is represented with the red arrow.
Distance of 33 Pegasi from the Sun and relative movement
33 Pegasi is distant 110.51 light years from the Sun and it is moving towards the Sun at the speed of 23 kilometers per second.
Spectral properties of 33 Pegasi
33 Pegasi belongs to spectral class F7 and has a luminosity class of V corresponding to a main-sequence star.
The red dot in the diagram below shows where 33 Pegasi is situated in the Hertzsprung–Russell diagram.
33 Pegasi star system properties
33 Pegasi is a visual double star which can be observed with binoculars or small telescopes. The table below shows key information about the 33 Pegasi double sysyem: