HR967 is a multiple main-sequence star in the constellation of Camelopardalis.
HR967 visual magnitude is 6.36. Because of its reltive faintness, HR967 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 HR967:
HR967 is above the horizon from Greenwich, United Kingdom .
Celestial coordinates and finder chart of HR967
HR967 is situated close to the northern celestial pole and, as such, it is visible for most part of the year from the northern hemisphere. Celestial coordinates for the J2000 equinox as well as galactic coordinates of HR967 are provided in the following table:
The simplified sky map below shows the position of HR967 in the sky:
Visibility of HR967 from your location
Location: Greenwich, United Kingdom
Latitude: 51° 28’ 47” N
Longitude: 0° 00’ 00” E
HR967 is circumpolar and transits at 09:59 UTC (altitude: 75.8°)
Digitized Sky Survey image of HR967
The image below is a photograph of HR967 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 HR967 is -0.01 arcsec per year in Right Ascension and 0.01 arcsec per year in Declination and the associated displacement for the next 10000 years is represented with the red arrow.
Distance of HR967 from the Sun and relative movement
HR967 is distant 595.98 light years from the Sun and it is moving towards the Sun at the speed of 6 kilometers per second.
Spectral properties of HR967
HR967 belongs to spectral class A3 and has a luminosity class of V corresponding to a main-sequence star.
The red dot in the diagram below shows where HR967 is situated in the Hertzsprung–Russell diagram.
HR967 star system properties
HR967 is a visual double star which can be observed only with the help of very large telescopes. The table below shows key information about the HR967 double sysyem: