(2020) A Sketch for a Photolytic History of Organic Molecules in the Solar System
Orthous-Daunay F-R, Piani L, Flandinet L, Thissen R, Wolters C, Vuitton V, Poch O, Moynier F, Sugawara I, Naraoka H & Tachibana S
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01c: Plenary Hall, Thursday 25th June 05:30 - 05:33
Listed below are questions that have been submitted by the community that the author will try and cover in their presentation. To submit a question, ensure you are signed in to the website. Authors or session conveners approve questions before they are displayed here.
The temperature of moon and Ryugu in the day time reached higher than room T. Are another reactions expected at higher T? Do depolymerization rates just increase at higher T?
The sapphire substrate may simulate the silicate minerals in CC. Could other minerals such as small metal grains in meteorites enhance/modify the reaction network as a catalyst?
Would other processes such as heating also lead to loss of the same small compounds? If so, would that result in a different fingerprint that can be distinguished from the UV one?
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