The atmosphere of our galaxy is primarily composed of hydrogen, with some helium and trace amounts of other elements. The interstellar medium (ISM) is mostly a vacuum, containing very thin plasma and varying densities, along with a dust component made of fine grains. Objects in space experience minimal friction due to this sparse environment, allowing celestial bodies to move without significant resistance. Hydrogen exists in different forms, including neutral hydrogen clouds, ionized hydrogen regions, and molecular clouds. Overall, the galaxy's composition is characterized by a vast emptiness punctuated by these scattered elements and structures.