Meet a star / Aquarius

Eta Aquarii

Eta Aquarii is a blue-white star, far hotter than the Sun, in the constellation Aquarius. It is a subgiant: a star just beginning to leave the long, steady part of its life.

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

How far

170 light years

The light you see from Eta Aquarii tonight set off about 170 years ago. Everything we know about it is that much out of date.

How bright

56 Suns

It gives out 56 times as much visible light as the Sun. It can be seen by eye away from bright lights.

Astronomers put its brightness in our sky at magnitude 4.04. Smaller numbers are brighter, and the faintest stars the eye can see are about 6.

How hot

Hotter than 11,000 K

That is the temperature of its surface, worked out from its colour, so it is a guide and not a measurement. For stars as blue as this one, colour is a poor thermometer: most of their light is ultraviolet, which the eye and this sum do not see, and the true figure can be far higher. 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.

Eta AquariiThe Sun

In your sky now

Working it out…

Its names

It has no name of its own. Its name by constellation is a Greek letter and the constellation it is in, a way of naming begun by Johann Bayer in 1603.

By constellation (Bayer)
Eta Aquarii
Hipparcos catalogue
HIP 111497
Henry Draper catalogue
HD 213998
Spectral type
B9IV-Vn

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.