HR5275 is a main-sequence star in the constellation of Virgo.
HR5275 visual magnitude is 6.24. Because of its reltive faintness, HR5275 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 HR5275:
Celestial coordinates and finder chart of HR5275
HR5275 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 HR5275 are provided in the following table:
The simplified sky map below shows the position of HR5275 in the sky:
Visibility of HR5275 from your location
Digitized Sky Survey image of HR5275
The image below is a photograph of HR5275 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 HR5275 is -0.011 arcsec per year in Right Ascension and -0.003 arcsec per year in Declination and the associated displacement for the next 10000 years is represented with the red arrow.
Distance of HR5275 from the Sun and relative movement
HR5275 is distant 204.90 light years from the Sun and it is moving towards the Sun at the speed of 23 kilometers per second.
Spectral properties of HR5275
HR5275 belongs to spectral class F4 and has a luminosity class of V corresponding to a main-sequence star.
The red dot in the diagram below shows where HR5275 is situated in the Hertzsprung–Russell diagram.