History of the Universe

History of the Universe eBook. 398 pages, 300 illustrations only £5.99

Font Smaller Font Bigger


Molecular Clouds

As the gas and dust of the disc of a galaxy is squashed by the spiral arms, the gas condenses onto stardust grains to form molecular clouds, so-called because they contain molecules, which we explain later in this story. These are so dense that light cannot pass through them. They are the dark areas we see when we look at the Milky Way. When seen through a telescope they often reflect the light of nearby stars.

Image of M16 molecular cloud by NASA, ESA, STScI, J. Hester and P. Scowen (Arizona State University)

In the Galaxy we can identify many of the molecules which life uses: methane, ammonia, water and formaldehyde have been identified. Amino acids, purines, and pyrimidines are possibly out there too, all forming on dust grains and eventually getting frozen into comets. This means that the raw materials of life are common in the Universe. Is life common too?

Get this website as an eBook only £5.99

Start Earlier Later Index Contents Timeline News Store Privacy & Cookies Non Mobile Site Font Smaller Font Bigger
History of the Universe eBook
History of the Universe eBook
Only £5.99

Written by Wyken Seagrave
Copyright © 2024 Penny Press Ltd