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Abstract Details

Magmatic Degassing of Trace Elements in Martian Meteorites

Yang S, Humayun M, Irving T, Righter K, Peslier A, Zanda B & Hewins R

Yang S, Humayun M, Irving T, Righter K, Peslier A, Zanda B & Hewins R (2020) Goldschmidt Abstracts, 2020 3001

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01c: Room 1, View in program

Shuying Yang View all 2 abstracts at Goldschmidt2020
Munir Humayan View all 2 abstracts at Goldschmidt2020
Tony Irving
Kevin Righter
Anne Peslier View all 2 abstracts at Goldschmidt2020
Brigitte Zanda
Roger Hewins

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
Do you know why there is only an effect in Ge? Looking at the enrichment factor plot for terrestrial volcanoes it seems like Ge has an average enrichment factor.

Submitted by Patricia Clay on
For the bulk meteorite measurements, do you have to worry about loss /modification of more mobile elements due to residence time on Earth's surface?

Submitted by Tomohiro Usui on
As bulk-rock Mg# of cumulate rocks (nakhlites & chassignites) would not represent melt compositions, I think it seems to be a bit difficult to use Mg# as an indicator of magmatic fractionation of nakhlites & chassignites.

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