Molecular Clouds

Molecular clouds are large, dense, and cold regions of the interstellar medium composed primarily of molecular hydrogen (H2) and other molecules such as carbon monoxide (CO), helium (He), and ammonia (NH3). These clouds are the birthplace of stars and planets, as the dense regions within them can collapse under their own gravity to form protostars. Molecular clouds are also important for the study of astrochemistry, as they contain a wide variety of molecules that can be used to study the chemical processes that occur in space. They are typically found in the spiral arms of galaxies, and can range in size from a few to hundreds of light years across.

Your Previous Searches

Random Picks

Neil Armstrong: Neil Armstrong was an American astronaut and aeronautical engineer who became the first person to walk on the Moon. He was the commander of the Apollo 11 mission, which successfully landed on the Moon on July 20, 1969. Armstrong's contribut ... Read More >>
Ionic Conductivity: Ionic conductivity is the ability of a material to conduct electric current through the movement of ions. In the context of space and astronautical engineering, ionic conductivity is an important property for materials used in batteries, fu ... Read More >>
Assembly Buildings: Assembly Buildings refer to the structures designed and built for the purpose of assembling, integrating, and testing spacecraft and their components. These buildings are equipped with specialized tools, equipment, and facilities to support ... Read More >>

Molecular Clouds

Your Previous Searches

Random Picks

Top News

Bestselling author explains the science of happiness: "You can do the work"...

November's full moon, known as the Beaver Moon, is the last supermoon of 2024. H...

You can't put a price on the sense of awe particle physics inspires...

If you want to stretch your gift game into days this holiday, check out these ad...

November brings a bonanza of meteor showers...