Tarantula Nebula
The Tarantula Nebula (also known as NGC 2070 or 30 Doradus) is the largest and most active star-forming region in the Local Group, located in the Large Magellanic Cloud about 160,000–170,000 light‑years away. Spanning roughly 600 light‑years, it hosts massive young star clusters like R136, contains some of the most massive stars known (up to ~200 M☉), and is shaped by intense radiation, stellar winds, and supernovae.
Source: science.nasa.gov
APODs including "Tarantula Nebula"
The Large Magellanic Cloud Galaxy
02/10/2024
It is the largest satellite galaxy of our home Milky Way Galaxy. If you live in the south, the Large Magellanic Cloud (LMC) is quite noticeable, spanning about 10 degrees across the night sky, which is 20 times larger than the full moon towards the southern constellation of the dolphinfish (Dorado). Being only about 160,000 light years away, many details of the LMC's structure can be seen, such as its central bar and its single spiral arm. The LMC harbors numerous stellar nurseries where new stars are being born, which appear in pink in the featured image. It is home to the Tarantula Nebula, the currently most active star forming region in the entire Local Group, a small collection of nearby galaxies dominated by the massive Andromeda and Milky Way galaxies. Studies of the LMC and the Small Magellanic Cloud (SMC) by Henrietta Swan Leavitt led to the discovery of the period-luminosity relationship of Cepheid variable stars that are used to measure distances across the nearby universe. Survey: Color Blindness and Astronomical Images