HR3379 is a giant star in the constellation of Camelopardalis.
HR3379 visual magnitude is 6.15. Because of its reltive faintness, HR3379 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 HR3379:
Celestial coordinates and finder chart of HR3379
HR3379 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 HR3379 are provided in the following table:
The simplified sky map below shows the position of HR3379 in the sky:
Visibility of HR3379 from your location
HR3379 is circumpolar and transits at 03:29 UTC (altitude: 67.9°)
Digitized Sky Survey image of HR3379
The image below is a photograph of HR3379 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 HR3379 is -0.015 arcsec per year in Right Ascension and -0.099 arcsec per year in Declination and the associated displacement for the next 1000 years is represented with the red arrow.
Distance of HR3379 from the Sun and relative movement
HR3379 is distant 355.12 light years from the Sun and it is moving far from the Sun at the speed of 16 kilometers per second.
Spectral properties of HR3379
HR3379 belongs to spectral class G7 and has a luminosity class of III corresponding to a giant star.
The red dot in the diagram below shows where HR3379 is situated in the Hertzsprung–Russell diagram.