41 Comae Berenices
41 Comae Berenices is a giant star in the constellation of Coma Berenices.
41 Comae Berenices visual magnitude is 4.8. Because of its moderate brightness, 41 Comae Berenices should be easily visible from locations with dark skyes, while it can be barely visible, or not visible at all, from skyes affected by light pollution.
The table below summarizes the key facts about 41 Comae Berenices:
Celestial coordinates and finder chart of 41 Comae Berenices
41 Comae Berenices is situated north of the celestial equator, as such, it is more easily visible from the northern hemisphere. Celestial coordinates for the J2000 equinox as well as galactic coordinates of 41 Comae Berenices are provided in the following table:
The simplified sky map below shows the position of 41 Comae Berenices in the sky:
Visibility of 41 Comae Berenices from your location
Location: Greenwich, United Kingdom [change]
Latitude: 51° 28’ 47” N
Longitude: 0° 00’ 00” E
Today's 41 Comae Berenices rise, transit and set times from Greenwich, United Kingdom [change] are the following (all times relative to the local timezone Europe/London):
Digitized Sky Survey image of 41 Comae Berenices
The image below is a photograph of 41 Comae Berenices 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 41 Comae Berenices is 0.031 arcsec per year in Right Ascension and -0.07 arcsec per year in Declination and the associated displacement for the next 10000 years is represented with the red arrow.
Distance of 41 Comae Berenices from the Sun and relative movement
41 Comae Berenices is distant 303.26 light years from the Sun and it is moving towards the Sun at the speed of 16 kilometers per second.
Spectral properties of 41 Comae Berenices
41 Comae Berenices belongs to spectral class K5 and has a luminosity class of III corresponding to a giant star.
The red dot in the diagram below shows where 41 Comae Berenices is situated in the Hertzsprung–Russell diagram.