HR1035 is a variable and double supergiant star in the constellation of Camelopardalis.
HR1035 visual magnitude is 4.21. Because of its moderate brightness, HR1035 should be easily visible from locations with dark skyes, while it can be barely visible, or not visible at all, from skyes affected by light pollution.
The table below summarizes the key facts about HR1035:
Celestial coordinates and finder chart of HR1035
HR1035 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 HR1035 are provided in the following table:
The simplified sky map below shows the position of HR1035 in the sky:
Visibility of HR1035 from your location
HR1035 is circumpolar and transits at 03:26 UTC (altitude: 81.5°)
Digitized Sky Survey image of HR1035
The image below is a photograph of HR1035 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 HR1035 is -0.003 arcsec per year in Right Ascension and -0.004 arcsec per year in Declination and the associated displacement for the next 100000 years is represented with the red arrow.
Distance of HR1035 from the Sun and relative movement
HR1035 is distant 4,289.47 light years from the Sun and it is moving towards the Sun at the speed of 7 kilometers per second.
Spectral properties of HR1035
HR1035 belongs to spectral class B9 and has a luminosity class of I corresponding to a supergiant star.
The red dot in the diagram below shows where HR1035 is situated in the Hertzsprung–Russell diagram.
HR1035 star system properties
HR1035 is a visual double star which can be observed with the help of medium or large telescopes. The table below shows key information about the HR1035 double sysyem: