HR7297 is a main-sequence star in the constellation of Telescopium.
HR7297 visual magnitude is 6.38. Because of its reltive faintness, HR7297 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 HR7297:
Celestial coordinates and finder chart of HR7297
HR7297 is situated south of the celestial equator, as such, it is more easily visible from the southern emisphere. Celestial coordinates for the J2000 equinox as well as galactic coordinates of HR7297 are provided in the following table:
The simplified sky map below shows the position of HR7297 in the sky:
Visibility of HR7297 from your location
HR7297 is currently not visible from Greenwich, United Kingdom [change]
Digitized Sky Survey image of HR7297
The image below is a photograph of HR7297 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 HR7297 is -0.013 arcsec per year in Right Ascension and -0.065 arcsec per year in Declination and the associated displacement for the next 10000 years is represented with the red arrow.
Distance of HR7297 from the Sun and relative movement
HR7297 is distant 148.59 light years from the Sun and it is moving towards the Sun at the speed of 24 kilometers per second.
Spectral properties of HR7297
HR7297 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 HR7297 is situated in the Hertzsprung–Russell diagram.