A chemist turned science writer, Victoria Corless completed her Ph.D. in organic synthesis at the University of Toronto and, ever the cliché, realized lab work was not something she wanted to do for the rest of her days.
Jam packed issues filled with the latest cutting-edge research, technology and theories delivered in an entertaining and visually stunning way, aiming to educate and inspire readers of all agesHerschel’s infrared view of part of the Taurus Molecular Cloud, within which the bright, cold pre-stellar cloud L1544 can be seen at the lower left. It is surrounded by many other clouds of gas and dust of varying density.
Among all common types of molecules are those that contain the nitrile group, which is made up of triple-bonded carbon and nitrogen. These kinds of molecules are, in fact, notably abundant."The nitrile group is terribly stable," said Agúndez."Carbon and nitrogen are kept together by a triple bond, which turns out to be one of the strongest chemical bonds in nature."
To connect the newly discovered nitrile molecules to the chemistry that may have sparked life on Earth, astrochemists need to identify the interstellar reactions that produced them. Therefore, Agúndez and his colleagues searched for other molecules that might have served as starting materials for the two nitriles they detected, offering potential insights into the reaction pathways involved in their formation.
This is related to a challenge facing the field, says Agúndez — namely, that the pace of newly discovered molecules is outstripping the ability of existing models to explain how they form. For example, maleonitrile is currently not included in chemical databases.
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