2026-04-23 ミシガン大学
A new study of the interstellar comet 3I/ATLAS led by the University of Michigan shows that its water has a remarkably high content of deuterium. This form of hydrogen is comparatively less abundant in our solar system, enabling researchers to glean new insights about other planetary processes at work in our galaxy. Image credit: Hans Anderson, Michigan News
＜関連情報＞
- https://news.umich.edu/the-interstellar-comet-3i-atlas-was-born-somewhere-much-different-from-our-solar-system/
- https://www.nature.com/articles/s41550-026-02850-5
3I/ATLASにおける水のD/H比は、別の惑星系における形成条件の探査に役立つ Water D/H in 3I/ATLAS as a probe of formation conditions in another planetary system
Luis E. Salazar Manzano,Teresa Paneque-Carreño,Martin A. Cordiner,Edwin A. Bergin,Hsing Wen Lin (林省文),Dariusz C. Lis,David W. Gerdes,Jennifer B. Bergner,Nicolas Biver,Dominique Bockelée-Morvan,Dennis Bodewits,Steven B. Charnley,Jacques Crovisier,Davide Farnocchia,Viviana V. Guzmán,Stefanie N. Milam,John W. Noonan,Anthony J. Remijan,Nathan X. Roth & John J. Tobin
Nature Astronomy Published:23 April 2026
DOI:https://doi.org/10.1038/s41550-026-02850-5
Abstract
Water reservoirs in the Solar System exhibit a deuterium enrichment that links back to the physical environment at the time of stellar birth. Gas-phase and ice-grain deuterium enrichments occur through chemical processes that operate at low temperatures (<30 K) pointing towards an origin in the prestellar molecular cloud or in the outer parts of the protoplanetary disk. However, not all stars are born in environments similar to our Sun, nor do their subsequent evolutionary histories follow the same path. These environmental differences can be traced by the water deuterium-to-hydrogen (D/H) ratio. Here we use ALMA observations of the interstellar comet 3I/ATLAS to constrain the water D/H ratio in extrasolar cometary material. With a water D/H value of[D/H]H2O＞6.6×10-3, 3I/ATLAS shows a deuterium enrichment exceeding Earth’s ocean value by more than a factor of about 40 and typical Solar System cometary values by more than a factor of about 30. The elevated deuterium enrichment points to water that formed under colder, less irradiated conditions and from less thermally processed material, consistent with an origin in a planetary system that formed under different physical and chemical conditions than our own.
