HR1650 is a variable and double hypergiant star in the constellation of Camelopardalis.
HR1650 visual magnitude is 6.37. Because of its reltive faintness, HR1650 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 HR1650:
Celestial coordinates and finder chart of HR1650
HR1650 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 HR1650 are provided in the following table:
The simplified sky map below shows the position of HR1650 in the sky:
Visibility of HR1650 from your location
HR1650 is circumpolar and transits at 00:47 UTC (altitude: 65.0°)
Digitized Sky Survey image of HR1650
The image below is a photograph of HR1650 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 HR1650 is -0.007 arcsec per year in Right Ascension and -0.008 arcsec per year in Declination and the associated displacement for the next 100000 years is represented with the red arrow.
Distance of HR1650 from the Sun and relative movement
HR1650 is distant 420.65 light years from the Sun and it is moving far from the Sun at the speed of 7 kilometers per second.
Spectral properties of HR1650
HR1650 belongs to spectral class A0 and has a luminosity class of V corresponding to a hypergiant star.
The red dot in the diagram below shows where HR1650 is situated in the Hertzsprung–Russell diagram.
HR1650 star system properties
HR1650 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 HR1650 double sysyem: