Meet a star / Canes Venatici

Cor Caroli B

Cor Caroli B is a yellow-white star, a little hotter than the Sun, in the constellation Canes Venatici. It is in the long, steady part of its life, making helium from hydrogen in its core, as the Sun is.

A drawing in the star's own colour, worked out from its measured colour index. It is not a photograph.

How far

120 light years

The light you see from Cor Caroli B tonight set off about 120 years ago. Everything we know about it is that much out of date.

How bright

6.8 Suns

It gives out 6.8 times as much visible light as the Sun. It can just be seen by eye from a really dark place.

Astronomers put its brightness in our sky at magnitude 5.61. Smaller numbers are brighter, and the faintest stars the eye can see are about 6.

How hot

About 7,200 K

That is the temperature of its surface, worked out from its colour, so it is a guide and not a measurement. It could be out by a few hundred degrees. The Sun's is 5,772 K. Hotter stars are bluer and cooler stars are redder, the same way a poker in a fire goes from red to white.

Cor Caroli BThe Sun

In your sky now

Working it out…

Its names

Its own name
Cor Caroli B
By constellation (Bayer)
Alpha-1 Canum Venaticorum
Hipparcos catalogue
HIP 63121
Henry Draper catalogue
HD 112412
Spectral type
F0V

Where this comes from

Distance, brightness, colour and spectral type are from the HYG star database, version 4.4, by David Nash, shared under a Creative Commons Attribution-ShareAlike 4.0 licence. Its distances are those measured by the Hipparcos satellite. The temperature is worked out here from the colour with the formula of Ballesteros (2012), and the words are written for this site.

To read more: Colour and brightness, How stars live and die, Measuring distance.