This multiwavelength image of the Tarantula Nebula, one of the brightest and largest regions of star formation to Earth, shows X-rays from Chandra that reveal gas that has been blown away in winds from the surfaces of young, massive stars and heated to millions of degrees by shock waves, like sonic booms from supersonic jets. The infrared data from Webb shows thousands of young stars, plus swaths of cool dust that will provide the ingredients to one day form new stars and planets. Hubble optical data uncovers hydrogen gas that is warmer than seen with Webb, as well as some individual stars through the nebula.
X-ray: NASA/CXC/Ohio State Univ./J. Rodriguez et al; Infrared: NASA/ESA/CSA/STScI; Optical: NASA/ESA/STScI; Image Processing: NASA/CXC/SAO/P. Edmonds

Data from NASA’s Chandra X-ray Observatory, NASA’s James Webb Space Telescope, and NASA’s Hubble Space Telescope combine to reveal a vibrant view of 30 Doradus, or the Tarantula Nebula, in this Aug. 11, 2026, image. Located in the Large Magellanic Cloud, a small neighbor galaxy to the Milky Way about 160,000 light-years from Earth, the Tarantula has thousands of young stars embedded in a vibrant honeycomb-like structure of gas and dust.

By studying the data from Chandra, Hubble, and Webb, combined with data from the agency’s retired Spitzer Space Telescope, astronomers determined that the Tarantula may be losing energy from several sources, including hot gas escaping from the nebula.

Learn more about this image.

Image credit: X-ray: NASA/CXC/Ohio State Univ./J. Rodriguez et al; Infrared: NASA/ESA/CSA/STScI; Optical: NASA/ESA/STScI; Image Processing: NASA/CXC/SAO/P. Edmonds

Source: www.nasa.gov

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