Page 2: Research news on Interstellar molecules

Interstellar molecules as a research area focuses on the detection, identification, and characterization of molecules in the interstellar medium (ISM), and on understanding their formation pathways, destruction processes, and astrochemical evolution. It integrates radio, millimeter, infrared, and UV spectroscopy with theoretical chemistry and reaction-kinetics modeling to constrain physical conditions in molecular clouds, diffuse clouds, and circumstellar envelopes. Research addresses gas-phase and grain-surface chemistry, isotopic fractionation, and the role of UV radiation, cosmic rays, and shocks in driving molecular complexity. This field informs models of star and planet formation, the chemical enrichment of galaxies, and the potential prebiotic inventory delivered to nascent planetary systems.

Chemists help solve mystery of missing space sulfur

For decades, astrochemists have been looking for sulfur atoms in space and finding surprisingly little of the element that is a key ingredient to life. A new study could point to where it has been hiding.

Tracking molecules in the interstellar medium

Stars don't form out of nothing, but tracking the gas and dust that do eventually form stars is hard. They float around the galaxy at almost absolute zero, emitting essentially no light, and generally making life difficult ...

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