This article has been reviewed according to Science X's editorial process and policies. Editors have highlighted the following attributes while ensuring the content's credibility:


trusted source


Image: Hubble's new view of the Tarantula Nebula

Image: Hubble’s new view of the Tarantula Nebula
Credit: ESA/Hubble & NASA, C. Murray, E. Sabbi; Acknowledgment: Y. -H. Chu

A snapshot of the Tarantula Nebula (also known as 30 Doradus) is featured in this image from the NASA/ESA Hubble Space Telescope. The Tarantula Nebula is a large star-forming region of ionized hydrogen gas that lies 161,000 light-years from Earth in the Large Magellanic Cloud, and its turbulent clouds of gas and dust appear to swirl between the region's bright, newly formed stars.

The Tarantula Nebula is a familiar site for Hubble. It is the brightest star-forming region in our galactic neighborhood and home to the hottest, most known. This makes it a perfect natural laboratory in which to test out theories of star formation and evolution, and Hubble has a rich variety of images of this region. The NASA/ESA/CSA James Webb Space Telescope also recently delved into this region, revealing thousands of never-before-seen young stars.

This new image combines data from two different observing proposals. The first was designed to explore the properties of the dust grains that exist in the void between stars that make up the dark clouds winding through this image. This proposal, which astronomers named Scylla, reveals how interacts with starlight in a variety of environments. It complements another Hubble program called Ulysses, which characterizes the stars. This image also incorporates data from an observing program studying star formation in conditions similar to the , as well as cataloging the stars of the Tarantula Nebula for future science with Webb.

Provided by NASA

Citation: Image: Hubble's new view of the Tarantula Nebula (2023, February 6) retrieved 20 June 2024 from
This document is subject to copyright. Apart from any fair dealing for the purpose of private study or research, no part may be reproduced without the written permission. The content is provided for information purposes only.

Explore further

Hubble views bright variable star V 372 Orionis and a smaller companion star


Feedback to editors