Jeff Nettles, Ph.D.Candidate

Department of Earth & Planetary Sci.
Planetary Geosciences Institute
118 EPS Building
University of Tennessee
Knoxville, TN 37996-1410

Voice : (865) 974-0466
E-mail : jnettle1@utk.edu


Ph. D. Research Area

TITLE : Petrology of Chondrule Precursors and Accretion of Particles in Ordinary Chondrites

My PhD research deals with two processes that were at work in the nebula that formed our solar system: the formation of chondrules, and aerodynamic sorting of nebular particles, such as metal grains. My studies of both these processes should give us some new clues about the way in which the solar system formed.

Chondrules are small, generally-round "balls" that are the dominant constituent of chondrite meteorites. While the formation of chondrules is still largely unknown, we do know that heating of the material in the nebula was involved. Something else we know is that chondrules were not quite the first materials to have formed in our solar system. We know this because chondrules can be found to contain "relict grains" - little bits of crystals whose composition and/or texture don't fit with the other crystals in the chondrule that are "left-overs" from the chondrule-forming process. So, if we know that there were materials that existed before chondrules, what were they? That's what I'm trying to answer with my research. It turns out that the materials that became chondrules were heated to varying degrees - some completely melted, some experienced quite a bit of partial melting, and others experienced only slight partial melting. Since the ones that were only slightly melted look most like the chondrule precursors, I'm studying them to develop an inventory of materials that were the precursors to chondrules. That's the first part of my research.

The second part of my research has to do with sorting of nebular particles in the nebula. It's been shown that the distribution of sizes of chondrules in one meteorite differs from the distribution of chondrule sizes in another meteorite, and this is one of the observations that have led to the idea that there was some sort of sorting mechanism in the nebula. Previous work has shown that the sorting is probably occurring aerodynamically rather than by mass, so my goal is to see how much the shape of a nebular particle (primarily metal grains and chondrules) affected its sorting. To do this, I'm employing X-ray tomography (more commonly known as "cat-scans?), though at much higher resolution that the scans that hospitals use. This way we can get highly-detailed, 3D measurements of the meteorites without having to destroy them. And again, this should give us some exciting new details about the way our solar system formed.


Publications



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