Meet a star / Andromeda

Alpheratz

Alpheratz is a blue-white star, far hotter than the Sun, in the constellation Andromeda.

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

How far

97 light years

The light you see from Alpheratz tonight set off about 97 years ago. Everything we know about it is that much out of date.

How bright

110 Suns

It gives out 110 times as much visible light as the Sun. It is one of the hundred brightest stars in the night sky. It is easy to see by eye on a clear night.

Astronomers put its brightness in our sky at magnitude 2.07. Smaller numbers are brighter, and the faintest stars the eye can see are about 6.

How hot

About 11,000 K

That is the temperature of its surface, worked out from its spectral type, B9p, with a standard table of how hot stars of each type are. It is a guide and not a measurement, and could be out by a tenth or so. For stars as hot as this, colour is a poor thermometer, because most of their light is ultraviolet, so the type is the better guide. 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.

AlpheratzThe Sun

In your sky now

Working it out…

Its names

Its own name
Alpheratz
By constellation (Bayer)
Alpha Andromedae
Hipparcos catalogue
HIP 677
Henry Draper catalogue
HD 358
Spectral type
B9p

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 read from the spectral type with the table of Pecaut and Mamajek (2013), and the words are written for this site.

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