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Astronomers Detect Rare Fully Deuterated Methanol in Space

Astronomers detected fully deuterated methanol orbiting the infant protostar IRAS 4A2, marking the first time the heavy organic molecule has been identified in space.

A molecule of alcohol long studied exclusively inside terrestrial laboratories has been confirmed in the interstellar medium, offering astronomers a direct chemical record of the raw materials available when planetary systems begin to form.

The finding centers on fully deuterated methanol, designated with the chemical formula CD₃OD. In this heavy variant, every hydrogen atom in an ordinary methanol molecule is replaced by deuterium, a stable isotope of hydrogen carrying an extra neutron.

The COMPASS Large Program Survey of Eleven Protostars

An international scientific collaboration made the discovery using the Atacama Large Millimeter/submillimeter Array, a system of 66 dishes situated at an elevation of 5,000 meters (16,404 feet) in northern Chile’s Atacama Desert, where the arid, thin atmosphere provides near-transparency to submillimeter and millimeter wavelengths. The observations formed part of the COMPASS program—which represents a deliberate departure from how astrochemistry has historically been done. The program examined eleven Sun-like young stars across different environments and evolutionary stages, all observed with the same instrument and the same spectral coverage. Researchers now face the compelling query of how these chemical building blocks might shape planetary environments and possibly drive the genesis of life.

The survey aims to map how chemical complexity evolves during the earliest stages of stellar birth. Through the project’s consistent use of identical instrument configurations and spectral ranges across various targets, researchers can systematically evaluate protostars of differing ages and surroundings to shed light on how molecular intricacy grows during star formation.

The analysis revealed that infant protostars are surrounded by a surprisingly complex organic starting kit, including organic molecules such as methanol, the simplest alcohol in the universe. Methanol was first discovered around young stars in 2017, but the current research pointed out that the presence of methanol molecules may be more widespread among low-mass protostars than previously thought.

Unlocking the Thermal History of Molecular Clouds

The discovery of CD₃OD carries profound implications for how astronomers read stellar histories. Functioning as a molecular relic, deuterium fractionation involves the concentration of deuterium within specific compounds to levels drastically higher than its standard cosmic frequency of roughly 15 atoms per million hydrogen atoms. Acting as a chemical archive, it details the temperature conditions of molecular cloud material during the earliest and chilliest stages of stellar genesis, well before any protostar formed.

This isotopic enrichment preserves a record of the thermal conditions when temperatures in a pre-stellar core drop, where the normal ratio between deuterium and hydrogen in the surrounding gas shifts dramatically upward. That grain-surface pathway is also how deuterium gets locked into the molecule.

Detailed spectroscopic data required to hunt for CD₃OD only emerged in a 2023 study outlining the molecule’s rotational properties, which determined that while discovery by ALMA was “within reach,” it had not yet been accomplished. COMPASS achieved it.

Detection of Heavy Methanol Around Young Stars

Comprehensive technical descriptions are provided in the COMPASS overview paper, explaining that finding CD₃OD depended on combining an accurate spectroscopic blueprint for precise targeting with the high sensitivity needed to pick out its weak signals amidst the background interference of numerous other chemical species in the identical gas cloud.

We are just beginning to tap into the richness of this dataset, and with further analyses, we will uncover completely new relationships regarding the chemical evolution taking place during the process of planet formation, as quoted from the announcement featuring Ágnes Kóspál.