For information on how to participate in the teletalks, please check the SOFIA Tele-Talk page.
For information on how to participate in the teletalks, please check the SOFIA Tele-Talk page.
For information on how to participate in the teletalks, please check the SOFIA Tele-Talk page.
For information on how to participate in the teletalks, please check the SOFIA Tele-Talk page.
For information on how to participate in the teletalks, please check the SOFIA Tele-Talk page.
Understanding the chemical pathways to the formation of molecules in various astrophysical settings is at the heart of astrochemical research. In particular, the icy mantles formed on interstellar dust grains and their processing by galactic cosmic rays or high-energy ultraviolet photons are thought to be the origin of many observed molecules, including those that are prebiotic. As interstellar regions evolve into stellar and planetary systems, these molecules may be seeded to planets and moons and contribute to important (geo)chemical processes and the possible emergence of life.
For information on how to participate in the teletalks, please check the SOFIA Tele-Talk page.
For information on how to participate in the Tele-Talks, please check the SOFIA Tele-Talk page.
For information on how to participate in the teletalks, please check the SOFIA Tele-Talk page.
For information on how to participate in the teletalks, please check the SOFIA Tele-Talk page.