Molecular Cloud

A molecular cloud, sometimes called a stellar nursery, is a type of interstellar cloud, the density and size of which permit absorption nebulae, the formation of molecules, and the formation of H II regions. This is in contrast to other areas of the interstellar medium that contain predominantly ionized gas. Molecular hydrogen is difficult to detect by infrared and radio observations, so the molecule most often used to determine the presence of H₂ is carbon monoxide. The ratio between CO luminosity and H₂ mass is thought to be constant, although there are reasons to doubt this assumption in observations of some other galaxies. Within molecular clouds are regions with higher density, where much dust and many gas cores reside, called clumps. These clumps are the beginning of star formation if gravitational forces are sufficient to cause the dust and gas to collapse.

Read more in the app

James Webb pierces the cold heart of the Chameleon molecular cloud to map out the complex chemicals that could form life around new stars.

James Webb Space Telescope uncovers building blocks of life in icy molecular cloud

Webb Peers Into Frozen Heart of Molecular Cloud – Unveils Dark Side of Pre-Stellar Ice Chemistry