Abstract Details
(2020) Mn-Cr Chronological Constraints on the Thermal Evolution of IIAB Iron Meteorite Parent Body
Anand A, Pape J, Wille M, Mezger K & Hofmann B
https://doi.org/10.46427/gold2020.57
The author has requested that this abstract is not discussed on social media.
The author has not provided any additional details.
01a: Room 1, Monday 22nd June 22:36 - 22:39
Aryavart Anand
View abstracts at 3 conferences in series
Jonas Pape View abstracts at 3 conferences in series
Martin Wille View all 3 abstracts at Goldschmidt2020
Klaus Mezger View all 3 abstracts at Goldschmidt2020
Beda Hofmann
Jonas Pape View abstracts at 3 conferences in series
Martin Wille View all 3 abstracts at Goldschmidt2020
Klaus Mezger View all 3 abstracts at Goldschmidt2020
Beda Hofmann
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 Ke Zhu on Tuesday 16th June 20:40
Hi Dr. Anand, thanks for this great presentation. It is a good idea to use Mn-Cr model age to date iron meteorites. My question is how did you define the solar system initial of e53Cr and the canoncial value of 53Mn/55Mn. Furthermore, what is the e54Cr data of the iron meteorites and the uncertainty of your data. Thanks.
Dear Mr. Ke, Thank you for taking interest in our work. The model ages are calculated relative to the CAI formation age assuming solar system initial e53Cr, chondritic 55Mn/52Cr and a canonical 53Mn/55Mn reported in Trinquier et al., 2008. The external precision (2SE) on 53Cr/52Cr is around 0.04e.
Hi Dr. Anand, thanks for this great presentation. It is a good idea to use Mn-Cr model age to date iron meteorites. My question is how did you define the solar system initial of e53Cr and the canoncial value of 53Mn/55Mn. Furthermore, what is the e54Cr data of the iron meteorites and the uncertainty of your data. Thanks.
Dear Mr. Ke, Thank you for taking interest in our work. The model ages are calculated relative to the CAI formation age assuming solar system initial e53Cr, chondritic 55Mn/52Cr and a canonical 53Mn/55Mn reported in Trinquier et al., 2008. The external precision (2SE) on 53Cr/52Cr is around 0.04e.
Sign in to ask a question.