Huge bubbles of ionised hydrogen gas mark the home of a colourful stellar nursery in the Large Magellanic Cloud, a satellite galaxy on the Milky Way’s doorstep at a relatively close 160,000 light years. A region in the LMC known as LHA 120-N 180B, made up of a gargantuan bubble of ionised hydrogen surrounded by a quartet of smaller bubbles, is home to a massive young star with 12 times the mass of the Sun that is emitting a tightly collimated jet stretching across 33 light years (see second image below).
Known as Herbig-Haro 1177, it is the first such jet observed in visible light in another galaxy, thanks in large part to the relatively small amount of dust in the LMC. Such jets are usually associated with accretion discs and have been observed extending from both low- and high-mass stars. This image was captured by the Multi Unit Spectroscopic Explorer instrument – MUSE – on the European Southern Observatory’s Very Large Telescope.