14 Camelopardalis is a main-sequence star in the constellation of Camelopardalis.
14 Camelopardalis visual magnitude is 6.5. Because of its reltive faintness, 14 Camelopardalis 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 14 Camelopardalis:
Celestial coordinates and finder chart of 14 Camelopardalis
14 Camelopardalis 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 14 Camelopardalis are provided in the following table:
The simplified sky map below shows the position of 14 Camelopardalis in the sky:
Visibility of 14 Camelopardalis from your location
14 Camelopardalis is circumpolar and transits at 00:23 UTC (altitude: 78.8°)
Digitized Sky Survey image of 14 Camelopardalis
The image below is a photograph of 14 Camelopardalis 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 14 Camelopardalis is -0.036 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 14 Camelopardalis from the Sun and relative movement
14 Camelopardalis is distant 268.09 light years from the Sun and it is moving towards the Sun at the speed of 4 kilometers per second.
Spectral properties of 14 Camelopardalis
14 Camelopardalis belongs to spectral class A7 and has a luminosity class of V corresponding to a main-sequence star.
The red dot in the diagram below shows where 14 Camelopardalis is situated in the Hertzsprung–Russell diagram.