42 Camelopardalis
42 Camelopardalis is a sub-giant star in the constellation of Camelopardalis.
42 Camelopardalis visual magnitude is 5.14. Because of its reltive faintness, 42 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 42 Camelopardalis:
Celestial coordinates and finder chart of 42 Camelopardalis
42 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 42 Camelopardalis are provided in the following table:
The simplified sky map below shows the position of 42 Camelopardalis in the sky:

Visibility of 42 Camelopardalis from your location
Location: Greenwich, United Kingdom
Latitude: 51° 28’ 47” N
Longitude: 0° 00’ 00” E
Timezone: Europe/London
42 Camelopardalis is circumpolar and transits at 14:27 UTC (altitude: 73.9°)
Digitized Sky Survey image of 42 Camelopardalis
The image below is a photograph of 42 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 42 Camelopardalis is 0.002 arcsec per year in Right Ascension and 0.002 arcsec per year in Declination and the associated displacement for the next 100000 years is represented with the red arrow.

Distance of 42 Camelopardalis from the Sun and relative movement
42 Camelopardalis is distant 867.02 light years from the Sun and it is moving far from the Sun at the speed of 5 kilometers per second.
Spectral properties of 42 Camelopardalis
42 Camelopardalis belongs to spectral class B4 and has a luminosity class of IV corresponding to a sub-giant star.
The red dot in the diagram below shows where 42 Camelopardalis is situated in the HertzsprungāRussell diagram.
