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.
An international team of astronomers using the Atacama Large Millimeter/submillimeter Array (ALMA), of which the U.S. National Science Foundation National Radio Astronomy Observatory is a partner (NSF NRAO), has combined ...
Astronomy
2 hours ago
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More and more details about 3I/ATLAS are filtering through the scientific process as time goes on. Our third known interstellar visitor attracted the attention of some of the world's most powerful observatories when it was ...
Planetary Sciences
Sep 22, 2026
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Before there was Earth, there was chemistry. In the unimaginable cold, dark clouds where stars and planets are born, carbon molecules assemble into more complex forms—starting a chemical journey that could eventually deliver ...
Astrobiology
Sep 14, 2026
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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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