MISIP 2017: "Basalt from Vesta: Major and Trace Element Heterogeneity Preserved on the Surface of the Asteroid"


Misasa International Students Intership Program 2017 Participants

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Tanya Kizovski

Canada

University of Toronto

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Sam Edwards

Canada

University of Toronto

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Chad Dodge

United States of America

California State University

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Susana Maria Hoyos Muñoz

Colombia

EAFIT (Escuela de Administración y Finanzas y Tecnologías) University

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Hsin-Yu Chen

Taiwan

National Cheng-Kung University

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Katarzyna Liszewska

Poland

University of Warsaw


Project Summary: Abstract

The 2017 MISIP internship program focused on analyzing three eucrite meteorites (Juvinas, Camel Donga, and Millbillillie) believed to be from the asteroid 4-Vesta. This study was completed in order to analyze and compare these three meteorites in order to determine how they originally formed, and gain a better understanding of the igneous and post-igneous processes on their parent body. The eucrites examined in this study are compositionally similar to terrestrial basalts and are believed to have originally crystallized at or near surface on 4-Vesta.

The eucrites were examined by completing detailed petrographic analysis, measuring major and trace element concentrations, and determining isotopic ratios for age and source determination. Major element, trace element, and isotope ratios indicate that these three meteorites are from the same parent body and underwent similar processes after formation. Evidence of mixing and multiple reheating events can be linked to multiple and frequent impacts soon after Vesta’s formation. This indicates that impact processes played a major role in early planetary formation. The presence of silica may be indicative of hydrothermal processes on Vesta (or in transit to Earth), which has implications for the timing and distribution of water in the solar system.


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