ASTROCHEMISTRY

Stars and stellar systems in our Galaxy form within dense (~100000 H2 molecules per cc) and cold (~10 K) fragments of interstellar molecular clouds, called pre-stellar cores. Important chemical.



Stars and stellar systems in our Galaxy form within dense (~100000 H2 molecules per cc) and cold (~10 K) fragments of interstellar molecular clouds, called pre-stellar cores. Important chemical.



Our solar system formed 4.5 billion years ago in an extremely chaotic environment and has evolved significantly over that time. What we see today is an organized inner solar system with four.

[jessialak]

Thank you miss, 😔 l have a project work, so this is very helpfull to me