H3+: Interstellar Chemistry Molecule
This is a news story, published by MSN, that relates primarily to Michigan State University news.
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H₂ moleculeBrighter Side News
•Science
Science
Scientists discover new sources of the molecule that built the universe
85% Informative
Trihydrogen cation, H, is a key player in the formation of new molecules and the cooling of interstellar gas clouds.
A new study from Michigan State University has uncovered fresh insights into these pathways, particularly in compounds known as methyl halogens and pseudohalogens.
The findings could reshape the understanding of H formation and impact on astrochemistry.
The study’s findings were achieved through a combination of ultrafast laser spectroscopy and high-level quantum chemistry simulations.
Even a small increase in H abundance due to these mechanisms could have significant implications.
Star formation models, which rely on accurate chemical composition data, may need revision to account for newly discovered reactions.
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