
science & techESA/Hubble
The Tarantula Nebula is one of the most intense star factories nearby
The Large Magellanic Cloud is a companion galaxy of the Milky Way, about 160,000 light-years away. It contains the Tarantula Nebula, one of the largest and most intense star-forming regions known in our galactic neighbourhood. Its spidery gas filaments gave the region its name. Nearby, stacked bubbles form the Honeycomb Nebula, carved out by winds and radiation from young stars. The fierce activity makes it a close-up laboratory for how massive stars form.
Dense clouds of gas collapse under their own gravity when they become cold enough, forming new stars. Massive young stars emit strong ultraviolet radiation and stellar winds, which heat and push the surrounding gas. That pressure carves out the bubbles and filaments, and can trigger further star formation at their edges.
The Tarantula is close enough to study star birth in detail, which is hard in the distant galaxies where most stars formed. It shows how a single region can hold many generations of stars, each shaped by the ones before it.
Star-forming regions dominated by massive stars often produce bubbles and shells, and the Orion Nebula in the Milky Way shows similar sculpting by radiation. The Tarantula shows the same process on a far larger scale.
If the Tarantula Nebula were as close to Earth as the Orion Nebula, it would be bright enough to cast shadows.
ESA/Hubble · CC BY 4.0
Image: ESA/Hubble & NASA Acknowledgements: Judy Schmidt ( Geckzilla )
