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.
Astronomers have discovered a second interstellar cloud near the center of the Milky Way that is extraordinarily rich in complex molecules, including several molecules associated with prebiotic chemistry. The newly studied ...
The universe has been having fewer and fewer stellar "babies." Over the past 4.5 billion years, the rate of star birth has crashed to less than half of what it once was. But here's the twist: the most essential "fuel" for ...
Astronomy
Sep 1, 2026
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A team of researchers led by the University of Hawaiʻi at Mānoa Department of Chemistry has uncovered a faster way large carbon-based molecules may form in space, helping solve a long-standing mystery about how some of the ...
Astrobiology
Aug 27, 2026
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You may have heard the phrase "we are made of star-stuff." This statement by the astronomer Carl Sagan refers to the fact that elements heavier than hydrogen and helium were forged in the centers of the first stars. But how ...
Astronomy
Aug 16, 2026
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We've been covering the journey of the Habitable Worlds Observatory for some time now. Over the past few years, it's gone from a proposal to a relatively fleshed-out plan for how and what the next Great Observatory should ...
Astronomy
Jul 27, 2026
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Sub-Neptunes are the most common type of planet in our galaxy. Bigger than Earth but smaller than Neptune, these worlds remain deeply mysterious because scientists still do not know what they are made of. What astronomers ...
Astronomy
Jul 10, 2026
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Stars like our sun are formed from the collapse of stellar objects called prestellar cores, cold and dense concentrations of gas and dust held together by gravity. While many questions remain about the exact mechanisms of ...
Astronomy
Jul 10, 2026
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The space between stars may seem like a barren desert, but over the past few decades scientists have been finding all sorts of interesting chemicals in it. From the precursors to proteins to the building blocks of cell membranes, ...
Astronomy
Jun 10, 2026
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Billions of years ago, a young spiral galaxy began to grow in a crowded part of the universe. It pulled in gas and small companion galaxies, slowly building up the bright central region and sweeping spiral arms we see today.
Astronomy
May 14, 2026
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You're a long-necked Titanosaur grazing the plains and chomping away on tree leaves about 100 million years ago in the Early Cretaceous in what would eventually become a future Starbucks location. You look up at the night ...
Planetary Sciences
May 11, 2026
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