Tarantula Nebula - Wikipedia The Tarantula Nebula (also known as 30 Doradus) is a large H II region in the Large Magellanic Cloud (LMC), forming its south-east corner (from Earth's perspective)
A Cosmic Tarantula, Caught by NASA’s Webb - NASA Once upon a space-time, a cosmic creation story unfolded: Thousands of never-before-seen young stars spotted in a stellar nursery called 30 Doradus, captured by NASA’s James Webb Space Telescope
NASA SVS | 30 Doradus: A Massive Star-Forming Region 30 Doradus (the Tarantula Nebula) is a very bright and active star-forming region outside of the Milky Way galaxy, at 160,000 light-years away “30 Dor” is home to the central star cluster NGC 2070, including the most active region, R136, which appears in the central-right area of the image
Caldwell 103 - Science@NASA 30 Doradus is the brightest star-forming region in our galactic neighbourhood and home to the most massive stars ever seen The nebula resides 170 000 light-years away in the Large Magellanic Cloud, a small, satellite galaxy of our Milky Way
Webb Captures A Cosmic Tarantula | ESA Webb Thousands of never-before-seen young stars are spotted in a stellar nursery called 30 Doradus, captured by the NASA ESA CSA James Webb Space Telescope Nicknamed the Tarantula Nebula for the appearance of its dusty filaments in previous telescope images, the nebula has long been a favourite for astronomers studying star formation
Tarantula Nebula (30 Doradus) - Constellation Guide The Tarantula Nebula (30 Doradus) is a vast star-forming region located approximately 160,000 light-years away in the constellation Dorado It is part of the Large Magellanic Cloud (LMC), the brightest satellite galaxy of the Milky Way
Hubble’s New View of the Tarantula Nebula - NASA Science 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