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Abstract Icy grain mantles are the main reservoir of the volatile elements that link chemical processes in dark, interstellar clouds with the formation of planets and the composition of their atmospheres. The initial ice composition is set in the cold, dense parts of molecular clouds, before the onset of star formation. With the exquisite sensitivity of the James Webb Space Telescope, this critical stage of ice evolution is now accessible for detailed study.
Authors and Affiliations Department of Earth and Planetary Sciences, Johns Hopkins University, Baltimore, Maryland, USA Z. Rustamkulov & D. K. Sing Department of Physics & Astronomy, Johns Hopkins University, Baltimore, MD, USA D. K. Sing, N. H. Allen & L. Ramos-Rosado Department of Astronomy & Astrophysics, University of California, Santa Cruz, Santa Cruz, CA, 95064, USA S. Mukherjee, A. L. Carter, N. M. Batalha, J. J. Fortney & K. Ohno Johns Hopkins APL, Laurel, MD, USA E. M. May, K. B. Stevenson & J.
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