©All Right reserved for www.mohammedshahin.ga

Amid an enormous cloud of dust and gas, thousands of stars are forming. Many of these stars have never been seen before, but these images from the James Webb Space Telescope (JWST) are revealing them for the first time.

These pictures show the Tarantula Nebula, located about 161,000 light-years away in the Large Magellanic Cloud – a galaxy that orbits the Milky Way. The nebula is the biggest and brightest one in all the nearby galaxies, and hosts some of the hottest and most massive stars astronomers have ever seen.

The massive young stars that form a sparkling blue cluster near the centre of the above image have cleared out the gas around them with their powerful radiation and intense stellar winds, revealing pillars of relatively dense gas inside which more young stars are forming. The above image was taken with JWST’s Near-Infrared Camera (NIRCam), showing the dusty filaments that make up the web of the Tarantula Nebula.

Advertisement

But viewed in longer wavelengths by JWST’s Mid-infrared Instrument (MIRI) in the picture below, the web takes on a different countenance. These wavelengths allow us to peer deeper into the cloud than ever before, and tiny points of light indicate protostars still in the process of formation. Hydrocarbons, shown in blue and purple, skim the edges of dust clouds like ghostly veils, while the densest areas of dust obstruct JWST’s view completely, as in the lower left corner.


At the longer wavelengths of light captured by its Mid-Infrared Instrument (MIRI), Webb focuses on the area surrounding the central star cluster and unveils a very different view of the Tarantula Nebula. In this light, the young hot stars of the cluster fade in brilliance, and glowing gas and dust come forward. Abundant hydrocarbons light up the surfaces of the dust clouds, shown in blue and purple. Much of the nebula takes on a more ghostly, diffuse appearance because mid-infrared light is able to show more of what is happening deeper inside the clouds. Still-embedded protostars pop into view within their dusty cocoons, including a bright group at the very top edge of the image, left of center. Other areas appear dark, like in the lower-right corner of the image. This indicates the densest areas of dust in the nebula, that even mid-infrared wavelengths cannot penetrate. These could be the sites of future, or current, star formation.

 

The Tarantula Nebula is of particular interest to astronomers because of its frenzied rate of star formation – nowhere in our own galaxy are stars formed in such huge quantities. This makes it relatively similar to dusty galaxies from billions of years ago, when star formation in the universe was at its most intense in the universe’s so-called cosmic noon. JWST will be able to observe those galaxies, so comparing those observations with the more detailed ones of this nebula may help us understand the universe’s most active time.

Sign up to our free Launchpad newsletter for a voyage across the galaxy and beyond, every Friday