HR7200 is a variable sub-giant star in the constellation of Sagitta.
HR7200 visual magnitude is 6.69. Because of its reltive faintness, HR7200 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 HR7200:
Celestial coordinates and finder chart of HR7200
HR7200 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 HR7200 are provided in the following table:
The simplified sky map below shows the position of HR7200 in the sky:
Visibility of HR7200 from your location
Digitized Sky Survey image of HR7200
The image below is a photograph of HR7200 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 HR7200 is 0.007 arcsec per year in Right Ascension and 0.017 arcsec per year in Declination and the associated displacement for the next 10000 years is represented with the red arrow.
Distance of HR7200 from the Sun and relative movement
HR7200 is distant 1,516.28 light years from the Sun and it is moving towards the Sun at the speed of 10 kilometers per second.
Spectral properties of HR7200
HR7200 belongs to spectral class B2 and has a luminosity class of IV corresponding to a sub-giant star.
The red dot in the diagram below shows where HR7200 is situated in the Hertzsprung–Russell diagram.