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Recent Advancements and Motivations of Simulated Pluto Experiments
Authors:Caitlin J Ahrens  William M Grundy  Kathleen E Mandt  Paul D Cooper  Orkan M Umurhan  Vincent F Chevrier
Institution:1.Arkansas Center for Space and Planetary Sciences,University of Arkansas,Fayetteville,USA;2.Lowell Observatory,Northern Arizona University,Flagstaff,USA;3.Space Science and Engineering Division,Southwest Research Institute,San Antonio,USA;4.Department of Chemistry and Biochemistry,George Mason University,Fairfax,USA;5.NASA Ames Research Center,Moffett Field,USA
Abstract:This review of Pluto laboratory research presents some of the recent advancements and motivations in our understanding enabled by experimental simulations, the need for experiments to facilitate models, and predictions for future laboratory work. The spacecraft New Horizons at Pluto has given a large amount of scientific data already rising to preliminary results, spanning from the geology to the atmosphere. Different ice mixtures have now been detected, with the main components being nitrogen, methane, and carbon monoxide. Varying geology and atmospheric hazes, however, gives us several questions that need to be addressed to further our understanding. Our review summarizes the complexity of Pluto, the motivations and importance of laboratory simulations critical to understanding the low temperature and pressure environments of icy bodies such as Pluto, and the variability of instrumentation, challenges for research, and how simulations and modeling are complimentary.
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