HR7272 is a multiple main-sequence star in the constellation of Lyra.
HR7272 visual magnitude is 6.74. Because of its reltive faintness, HR7272 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 HR7272:
Celestial coordinates and finder chart of HR7272
HR7272 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 HR7272 are provided in the following table:
The simplified sky map below shows the position of HR7272 in the sky:
Visibility of HR7272 from your location
Digitized Sky Survey image of HR7272
The image below is a photograph of HR7272 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 HR7272 is 0.053 arcsec per year in Right Ascension and 0.195 arcsec per year in Declination and the associated displacement for the next 1000 years is represented with the red arrow.
Distance of HR7272 from the Sun and relative movement
HR7272 is distant 159.65 light years from the Sun and it is moving towards the Sun at the speed of 41 kilometers per second.
Spectral properties of HR7272
HR7272 belongs to spectral class G1 and has a luminosity class of V corresponding to a main-sequence star.
The red dot in the diagram below shows where HR7272 is situated in the Hertzsprung–Russell diagram.
HR7272 star system properties
HR7272 is a visual double star which can be observed with the help of small or medium telescopes. The table below shows key information about the HR7272 double sysyem: