HR1485

HR1485 is a double sub-giant star in the constellation of Mensa.

HR1485 visual magnitude is 6.76. Because of its reltive faintness, HR1485 should be visible only from locations with dark skies, while it is not visible at all from skies affected by light pollution.

The proper motion of HR1485 is -0.018 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.

Key facts about HR1485

Celestial coordinates and finder chart of HR1485

HR1485 is situated close to the southern celestial pole and, as such, it is easilty visible for most part of the year from the southern hemisphere. Celestial coordinates for the J2000 equinox as well as galactic coordinates of HR1485 are provided in the following table:

The simplified sky map below shows the position of HR1485 in the sky:

Visibility of HR1485 from your location

HR1485 is currently not visible from Greenwich, United Kingdom edit_location_alt

Distance of HR1485 from the Sun and relative movement

HR1485 is distant 324.38 light years from the Sun and it is moving towards the Sun at the speed of 5 kilometers per second.

Spectral properties of HR1485

HR1485 belongs to spectral class A7 and has a luminosity class of IV corresponding to a sub-giant star.

The red dot in the diagram below shows where HR1485 is situated in the Hertzsprung–Russell diagram.

HR1485 star system properties

HR1485 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 HR1485 double sysyem:

Alternative designations of HR1485