Eta Orionis
Eta Orionis is a blue-white star, far hotter than the Sun, in the constellation Orion. It is in the long, steady part of its life, making helium from hydrogen in its core, as the Sun is.
How far
980 light years
The light you see from Eta Orionis tonight set off about 980 years ago. Everything we know about it is that much out of date.
Distances this great are hard to measure, and this one could be out by a fifth or more.
How bright
3,600 Suns
It gives out 3,600 times as much visible light as the Sun. It is easy to see by eye on a clear night.
Astronomers put its brightness in our sky at magnitude 3.35. Smaller numbers are brighter, and the faintest stars the eye can see are about 6.
How hot
Hotter than 14,000 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 OrionisThe 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 Orionis
- Hipparcos catalogue
- HIP 25281
- Henry Draper catalogue
- HD 35411
- Spectral type
- B1V + B2
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.