description 30 Doradus Overview
30 Doradus, commonly called the Tarantula Nebula, is a vast ionized-hydrogen region in the Large Magellanic Cloud, a satellite galaxy of the Milky Way. It contains the dense central cluster R136, whose massive young stars supply much of the radiation that illuminates the surrounding gas. The nebula is an important nearby laboratory for studying massive-star formation, stellar winds, and starburst conditions.
insights Ranking position
30 Doradus ranks #5 of 668 in the Nebula ranking, behind Eagle Nebula, ahead of Tarantula Nebula.
help 30 Doradus FAQ
Is 30 Doradus inside the Milky Way?
No, 30 Doradus lies in the Large Magellanic Cloud, a satellite galaxy of the Milky Way. It is roughly 160,000 light-years from Earth and is also known as the Tarantula Nebula.
What is forming stars at the center of the Tarantula Nebula?
Its central region contains the young cluster R136, whose massive stars flood surrounding hydrogen with ultraviolet radiation. R136 includes some of the most massive and luminous stars known.
Can the Tarantula Nebula be seen without a telescope?
From sufficiently dark Southern Hemisphere locations, the broader 30 Doradus region can be detected within the Large Magellanic Cloud. Binoculars or a telescope reveal it much more clearly, while observatories such as Hubble and Webb show its dense clusters and sculpted gas.
Was Supernova 1987A part of 30 Doradus?
Supernova 1987A occurred in the Large Magellanic Cloud near the Tarantula Nebula region, although not in its central R136 cluster. It became the closest supernova observed since the invention of the telescope and was visible from Earth in 1987.
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