HR2346 is a main-sequence star in the constellation of Camelopardalis.
HR2346 visual magnitude is 6.54. Because of its reltive faintness, HR2346 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 HR2346:
Celestial coordinates and finder chart of HR2346
HR2346 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 HR2346 are provided in the following table:
The simplified sky map below shows the position of HR2346 in the sky:
Visibility of HR2346 from your location
HR2346 is circumpolar and transits at 02:09 UTC (altitude: 61.9°)
Digitized Sky Survey image of HR2346
The image below is a photograph of HR2346 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 HR2346 is 0.001 arcsec per year in Right Ascension and 0.017 arcsec per year in Declination and the associated displacement for the next 10000 years is represented with the red arrow.
Distance of HR2346 from the Sun and relative movement
HR2346 is distant 373.42 light years from the Sun and it is moving towards the Sun at the speed of 7 kilometers per second.
Spectral properties of HR2346
HR2346 belongs to spectral class A1 and has a luminosity class of V corresponding to a main-sequence star.
The red dot in the diagram below shows where HR2346 is situated in the Hertzsprung–Russell diagram.