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dc.contributor.authorShober, Patrick M.
dc.contributor.supervisorPhil Blanden_US
dc.contributor.supervisorGretchen Benedixen_US
dc.contributor.supervisorEllie Sansomen_US

Since people started studying meteorites, scientists have attempted to better understand the parent bodies they originated from. Although, this is difficult because, unlike a terrestrial rock, you do not have access to the outcrop. The Near-Earth Object (NEO) population is the source of all meteorites found on Earth. Using the orbital data collected from the Desert Fireball Network, my work clarified the connections between meteorites and their source NEOs. I primarily did this analysis by employing rigorous numerical modeling techniques to constrain the dynamical and physical properties of asteroidal debris.

dc.publisherCurtin Universityen_US
dc.titleMeteoroid Orbital Analysis: Connecting Meteorites and Asteroidsen_US
curtin.departmentSchool of Earth and Planetary Sciencesen_US
curtin.accessStatusOpen accessen_US
curtin.facultyScience and Engineeringen_US
curtin.contributor.orcidShober, Patrick M. [0000-0003-4766-2098]en_US

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