This week’s space photo shows dark clouds of dust, glowing hydrogen gas and massive stars. Most notable: a gaping hole in the center of the nebula.

N44 is an emission nebula in the Large Magellanic Cloud. In this nebula we find several young and old star groups. The nebula is a thousand light-years long and – like the Large Magellanic Cloud – is about 170,000 light-years from Earth.

What is the Large Magellanic Cloud?
The Large Magellanic Cloud is a dwarf galaxy. This galaxy is the third closest galaxy to the Milky Way. The Large Magellanic Cloud has a combined mass of about 10 billion suns. In the southern hemisphere, this galaxy is visible to the naked eye at night as a kind of faint cloud. The famous European explorer Ferdinand Magellan announced the existence of the Large Magellanic Cloud in 1519. Hence, this dwarf galaxy is named after him.

In the middle of mist a 250 light-year wide ‘hole’ can be seen† It’s a mystery why there aren’t shreds of gas and dust here. It is possible that stellar winds from the present massive stars have driven these gas clouds away, but this does not match measured wind speeds. Another possibility is that the nebula is surrounded by the expanding shells of ancient supernovae and thus created the cosmic void.

The emission nebula N44 is visible because the gas and dust present in the nebula is heated and ionized by nearby stars. In the case of ionization, an atom loses or gains an electron. Due to the heating, the gas and dust absorb energy. Then this energy is released again by emitting radiation. Many emission nebulae can also be found in our Milky Way, such as planetary nebulae (the Ring Nebula), supernova remnants (Crab Nebula) and H-11 areas

Do you want to zoom in endlessly on N44? Then download the 288 megapixel photo with a size of 153 MB.

Over the past decades, space telescopes and satellites have captured beautiful images of nebulae, galaxies, stellar nurseries and planets. Every weekend we remove one or more impressive space photos from the archive. Enjoy all the photos? View them on this page.