HR1675 is a giant star in the constellation of Camelopardalis.
HR1675 visual magnitude is 6.17. Because of its reltive faintness, HR1675 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 HR1675:
Celestial coordinates and finder chart of HR1675
HR1675 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 HR1675 are provided in the following table:
The simplified sky map below shows the position of HR1675 in the sky:
Visibility of HR1675 from your location
HR1675 is circumpolar and transits at 00:38 UTC (altitude: 79.6°)
Digitized Sky Survey image of HR1675
The image below is a photograph of HR1675 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 HR1675 is 0.011 arcsec per year in Right Ascension and 0.006 arcsec per year in Declination and the associated displacement for the next 10000 years is represented with the red arrow.
Distance of HR1675 from the Sun and relative movement
HR1675 is distant 477.31 light years from the Sun and it is moving towards the Sun at the speed of 4 kilometers per second.
Spectral properties of HR1675
HR1675 belongs to spectral class A2 and has a luminosity class of III corresponding to a giant star.
The red dot in the diagram below shows where HR1675 is situated in the Hertzsprung–Russell diagram.