Award Date
5-15-2026
Degree Type
Thesis
Degree Name
Master of Science (MS)
Department
Physics and Astronomy
First Committee Member
Jason Steffen
Second Committee Member
Zhaohuan Zhu
Third Committee Member
Stephen Lepp
Fourth Committee Member
Pamela Burnley
Number of Pages
47
Abstract
Chondrites, a type of primitive asteroid, are thought to have formed from dust and gas early in the life of our Solar System. These chondrites have remained unchanged since their formation, avoiding being melted or differentiated like other rocky bodies have. Due to this unique characteristic, chondrites can give us useful insight into how asteroids, planetesimals, and even the terrestrial planets formed. In order to study chondrites and their formation, I used code developed by Li et al. (2020), which utilizes thermodynamic code GRAINS (Petaev 2009), to see what conditions the chondrites may have originated from. GRAINS uses a variety of chemical elements, along with hundreds of gaseous and condensed phases, in order to calculate the chemical equilibrium of a system. I varied multiple parameters of the Solar System’s protoplanetary disk from the values found in Li et al. (2020) in order to find which set of conditions yield simulated results closest to the known chemical composition of various chondrite families. The results from this disk code suggest that the carbonaceous and ordinary chondrites have narrow formation channels, located around 2-4 AU from the sun across most of the simulation length. This result is true across almost all of the best-fitting models. The enstatite chondrites do not seem to have one specific formation location, but have well-fitting regions that start between 3-5 AU and continue outwards in the disk.
Controlled Subject
asteroid; Chondrites (Meteorites); Chondrites (Meteorites)--Analysis
Disciplines
Astrophysics and Astronomy | Physical Sciences and Mathematics | The Sun and the Solar System
File Format
File Size
11900 KB
Degree Grantor
University of Nevada, Las Vegas
Language
English
Repository Citation
Perron, Isabelle M., "The Origins of Chondrite Families" (2026). UNLV Theses, Dissertations, Professional Papers, and Capstones. 5603.
https://oasis.library.unlv.edu/thesesdissertations/5603
Rights
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