14 Pegasi is a main-sequence star in the constellation of Pegasus.
14 Pegasi visual magnitude is 5.04. Because of its reltive faintness, 14 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 14 Pegasi:
Celestial coordinates and finder chart of 14 Pegasi
14 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 14 Pegasi are provided in the following table:
The simplified sky map below shows the position of 14 Pegasi in the sky:
Visibility of 14 Pegasi from your location
Digitized Sky Survey image of 14 Pegasi
The image below is a photograph of 14 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 14 Pegasi is 0.019 arcsec per year in Right Ascension and -0.027 arcsec per year in Declination and the associated displacement for the next 10000 years is represented with the red arrow.
Distance of 14 Pegasi from the Sun and relative movement
14 Pegasi is distant 302.41 light years from the Sun and it is moving towards the Sun at the speed of 23 kilometers per second.
Spectral properties of 14 Pegasi
14 Pegasi belongs to spectral class A1 and has a luminosity class of V corresponding to a main-sequence star.
The red dot in the diagram below shows where 14 Pegasi is situated in the Hertzsprung–Russell diagram.