A Cosmic Tarantula, Caught by NASA’s Webb

Take a moment to stare into thousands of never-before-seen young stars in the Tarantula Nebula. The James Webb Space Telescope reveals details of the structure and composition of the nebula, as well as dozens of background galaxies.

Stellar nursery 30 Doradus gets its nickname of the Tarantula Nebula from its long, dusty filaments. Located in the Large Magellanic Cloud galaxy, it’s the largest and brightest star-forming region near our own galaxy, plus home to the hottest, most massive stars known.

The center of this image, taken by Webb’s Near-Infrared Camera instrument (NIRCam), has been hollowed out by the radiation from young, massive stars (seen in sparkling pale blue). Only the densest surrounding areas of the nebula resist erosion, forming the pillars that appear to point back towards the cluster of stars in the center. The pillars are home to still-forming stars, which will eventually leave their dusty cocoons and help shape the nebula.

Why is this nebula interesting to astronomers? Unlike in our Milky Way, the Tarantula Nebula is producing new stars at a furious rate. Though close to us, it is similar to the gigantic star-forming regions from when the universe was only a few billion years old, and star formation was at its peak — a period known as “cosmic noon.” Since the Tarantula is close to us, it is easy to study in detail to help us learn more about the universe’s past.

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