Tracking Volatile Elements in Protoplanetary Disks and on Planetary Surfaces

Tracking Volatile Elements in Protoplanetary Disks and on Planetary Surfaces

<p>The formation of planets begins with collisions of tiny, micron-sized, dust grains. These grains reside in structures known as protoplanetary disks, rotating disks consisting of gas and dust that encircle young protostars as a natural outcome of star formation. Although the processes of pla...

Full description

Bibliographic Details
Main Author: Anderson, Dana Eklund
Format: Others
Language:en
Published: 2020
Online Access:https://thesis.library.caltech.edu/11803/14/anderson_dana_2020_thesis.pdf
Anderson, Dana Eklund (2020) Tracking Volatile Elements in Protoplanetary Disks and on Planetary Surfaces. Dissertation (Ph.D.), California Institute of Technology. doi:10.7907/GZSA-DK98. http://resolver.caltech.edu/CaltechTHESIS:09282019-173537468 <http://resolver.caltech.edu/CaltechTHESIS:09282019-173537468>

Internet

https://thesis.library.caltech.edu/11803/14/anderson_dana_2020_thesis.pdf
Anderson, Dana Eklund (2020) Tracking Volatile Elements in Protoplanetary Disks and on Planetary Surfaces. Dissertation (Ph.D.), California Institute of Technology. doi:10.7907/GZSA-DK98. http://resolver.caltech.edu/CaltechTHESIS:09282019-173537468 <http://resolver.caltech.edu/CaltechTHESIS:09282019-173537468>

Similar Items