Cryogenic Cometary Sample Return
Andrew J. Westphal, Larry R. Nittler, Rhonda Stroud, Michael E., Zolensky, Nancy L. Chabot, Neil Dello Russo, Jamie E. Elsila, Scott A., Sandford, Daniel P. Glavin, Michael E. Evans, Joseph A. Nuth, Jessica, Sunshine, Ronald J. Vervack Jr, Harold A. Weaver

TL;DR
A cryogenic cometary sample return mission would provide unprecedented insights into primitive solar system materials, especially ices and gases, revealing their mineralogical and chemical relationships at extremely low temperatures.
Contribution
This paper advocates for a cryogenic cometary sample return mission, emphasizing technological advancements and scientific importance, which were previously unfeasible due to technological immaturity.
Findings
Cryogenic samples can reveal primitive solar system materials.
Technological advances now enable feasible cryogenic sample return missions.
Such samples will enhance understanding of early solar nebula chemistry.
Abstract
Comets likely formed in the outer regions of the protosolar nebula where they incorporated and preserved primitive presolar materials, volatiles resident in the outer disk, and more refractory materials from throughout the disk. The return of a sample of volatiles (i.e., ices and entrained gases), along with other components of a cometary nucleus, will yield numerous major scientific opportunities. We are unaccustomed to thinking of ices through a mineralogical/petrological lens, but at cryogenic temperatures, ices can be regarded as mineral components of rocky material like any other. This is truly Terra Incognita, as a sample from a natural cryogenic (10s of K) environment is unprecedented in any setting; currently, we can only make educated guesses about the nature of these materials on a microscopic scale. Such samples will provide an unparalleled look at the primordial gases and…
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Taxonomy
TopicsAstro and Planetary Science · Spacecraft and Cryogenic Technologies · Molecular Spectroscopy and Structure
