HR7249 is a variable main-sequence star in the constellation of Sagittarius.
HR7249 visual magnitude is 5.54. Because of its reltive faintness, HR7249 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 HR7249:
Celestial coordinates and finder chart of HR7249
HR7249 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 HR7249 are provided in the following table:
The simplified sky map below shows the position of HR7249 in the sky:
Visibility of HR7249 from your location
Digitized Sky Survey image of HR7249
The image below is a photograph of HR7249 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 HR7249 is 0.006 arcsec per year in Right Ascension and 0.008 arcsec per year in Declination and the associated displacement for the next 100000 years is represented with the red arrow.
Distance of HR7249 from the Sun and relative movement
HR7249 is distant 1,530.52 light years from the Sun and it is moving towards the Sun at the speed of 20 kilometers per second.
Spectral properties of HR7249
HR7249 belongs to spectral class B2 and has a luminosity class of V corresponding to a main-sequence star.
The red dot in the diagram below shows where HR7249 is situated in the Hertzsprung–Russell diagram.