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Evolution of Volatiles from Europa's Interior into its Ocean

Melwani Daswani M & Vance SD

Melwani Daswani M & Vance SD () Goldschmidt Abstracts, 1777

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01c: Plenary Hall, Thursday 25th June 05:54 - 05:57

Mohit Melwani Daswani View all 2 abstracts at Goldschmidt2020
Steven D. Vance

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.

Submitted by My Riebe on Sunday 21st June 07:53
CIs and CMs have both experienced aqueous alteration which formed a lot of the water bearing minerals. When did this happen in your model? It is commonly assumed that aqueous alteration happened on the parent body. Would this be a first generation parent body that then formed Europa?


Submitted by Aki Takigawa on Wednesday 24th June 12:58
How will the results change if the initial objects are more ice and volatile-rich bodies like comets?


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