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Astrochemistry by MIT
This educational note coming out of MIT is a resource that gives an in-depth overview on astrochemistry, focusing primarily on the topic of spectral lines and their significance in understanding cosmic entities. The topics included are as follows: Radio Telescope Mechanics Emission/Absorption of Spectral Lines Detection of Stars Detection of Planets Detection of Galaxies. This paper will try to help students acquire more significant knowledge in space science: the processes of chemistry and the principles upon which astronomy observations are based.
Author(s): MIT
NA Pages 
Sulfur Ice Astrochemistry A Review of Laboratory Studies
The review by Duncan V. Mifsud and other authors points at the role which sulfur plays in the special world of astrochemistry as an element of paramount importance to biological systems and planetary geology. A pdf of laboratory studies involving sulfur-bearing molecules include spectroscopy and results from experiments on thermal and photochemical processing. Charged particle bombardment and radiolysis of sulfur ice analogues are discussed for a better understanding of the behavior of sulfur in extraterrestrial environments. The current document concludes with proposed further research directions and continues to highlight the importance of sulfur in astrochemical processes.
Author(s): Duncan V. Mifsud, Zuzana Kanuchova, Péter Herczku, Sergio Ioppolo
38 Pages
Astrochemistry The Cradle of Life
Professor Nigel Mason discusses in his paper the chemical origins of life, covering the synthesis of nucleobases and DNA. Included in this also are the historical experiments, such as Urey-Miller, and examines the chemistry of prebiotic types in conditions similar to those prevailing on early Earth. This note covers important results with regard to the question of life on Mars: investigations about meteorites from Mars and ozone formation and depletion. It is an interesting overview of astrochemical processes that could well have led to the origin of life on Earth and elsewhere in the universe, founded on a blend of experimental data and theoretical insights.
Author(s): Professor Nigel Mason
99 Pages