The Tarantula Nebula is a large H II region in the Large Magellanic Cloud (LMC), forming its south-east corner.
James Webb Space Telescope's NIRCam view of the Tarantula Nebula
Hubble's high resolution view of the star-forming region of Tarantula Nebula and the R136 super star cluster at its center
Detail of RMC 136a, cluster NGC 2070
An H II region or HII region is a region of interstellar atomic hydrogen that is ionized. It is typically in a molecular cloud of partially ionized gas in which star formation has recently taken place, with a size ranging from one to hundreds of light years, and density from a few to about a million particles per cubic centimetre. The Orion Nebula, now known to be an H II region, was observed in 1610 by Nicolas-Claude Fabri de Peiresc by telescope, the first such object discovered.
NGC 604, a giant H II region in the Triangulum Galaxy
Dark star-forming regions within the Eagle Nebula commonly referred to as the Pillars of Creation
Orion Nebula
A small portion of the Tarantula Nebula, a giant H II region in the Large Magellanic Cloud