Asset Publisher

The hot, gaseous components of the Milky Way's halo – artist's impression

The hot, gaseous components of the Milky Way's halo – artist's impression


Date: 16 January 2020
Satellite: XMM-Newton
Copyright: ESA

This artist's impression shows the Milky Way (the small galaxy depicted at the centre of the frame) and its halo (the extended gaseous region).

A halo is a vast region of gas, stars and invisible dark matter surrounding a galaxy. It is a key component of a galaxy, connecting it to wider intergalactic space, and is thus thought to play an important role in galactic evolution.

A study using ESA's XMM-Newton X-ray space observatory now shows that the Milky Way's halo contains not one but three different components of hot gas, with the hottest of these being a factor of ten hotter than previously thought. This is the first time multiple gas components structured in this way have been discovered in not only the Milky Way, but in any galaxy.

The study also found that the halo has a different chemical makeup than predicted – it contains less iron than expected, indicating that the halo has been enriched by massive dying stars, and also less oxygen, likely due to this element being taken up by dusty particles in the halo.

This image illustrates the halo in three different shades – emerald, yellow and green. These all mix together throughout the halo, and each represents gas of a different temperature.

Last Update: 16 January 2020
13-Aug-2020 12:20 UT

ShortUrl Portlet

Shortcut URL

https://sci.esa.int/s/wRLE5j8

Related Images

Related Videos

Related Publications

Related Links

Documentation