HR2350 is a main-sequence star in the constellation of Camelopardalis.
HR2350 visual magnitude is 6.65. Because of its reltive faintness, HR2350 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 HR2350:
Celestial coordinates and finder chart of HR2350
HR2350 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 HR2350 are provided in the following table:
The simplified sky map below shows the position of HR2350 in the sky:
Visibility of HR2350 from your location
HR2350 is circumpolar and transits at 01:26 UTC (altitude: 59.4°)
Digitized Sky Survey image of HR2350
The image below is a photograph of HR2350 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 HR2350 is 0.01 arcsec per year in Right Ascension and -0.052 arcsec per year in Declination and the associated displacement for the next 10000 years is represented with the red arrow.
Distance of HR2350 from the Sun and relative movement
HR2350 is distant 225.14 light years from the Sun and it is moving far from the Sun at the speed of 6 kilometers per second.
Spectral properties of HR2350
HR2350 belongs to spectral class A5 and has a luminosity class of V corresponding to a main-sequence star.
The red dot in the diagram below shows where HR2350 is situated in the Hertzsprung–Russell diagram.