Please use this identifier to cite or link to this item:

A remote analysis of the lunar landscape

File Description SizeFormat 
Trang_David_r.pdfVersion for non-UH users. Copying/Printing is not permitted52.69 MBAdobe PDFView/Open
Trang_David_uh.pdfVersion for UH users52.66 MBAdobe PDFView/Open

Item Summary

Title: A remote analysis of the lunar landscape
Authors: Trang, David
Keywords: lunar surface
unar geomorphology
lunar volcanism
impact cratering
show 2 morenear-infrared spectroscopy
lunar remote sensing

show less
Issue Date: Dec 2014
Publisher: [Honolulu] : [University of Hawaii at Manoa], [December 2014]
Abstract: The integration of remote sensing data sets is important to producing accurate interpretations of geomorphological features on the lunar surface. Studies of the surface can reveal the geological history of the Moon and Earth, provide key observations to the early Solar System, assist in refining surface process models, and find important resources for future exploration. The dissertation goals are to advance current remote sensing tools and techniques and use new global data sets and products from Kaguya and the Lunar Reconnaissance Orbiter missions to better understand impact craters and volcanic features. We improved remote sensing tools by characterizing the optical properties of olivine and pyroxene and producing a technique that uses crater degradation state to determine the crater age. We used these tools along with the new data sets and derived products to understand the changes in crater morphology with time, determine the origin of concentric craters, and classify localized pyroclastic deposits based upon physical and compositional properties. From these projects, we successfully modeled the optical properties of olivine and pyroxene by using the Modified Gaussian Model. Also, we calibrated the degree of freshness scale to absolute model ages. In studying lunar geomorphology, we deduced that igneous intrusions underneath small craters (<15 km in diameter) are likely to produce concentric craters. Finally, we found a relationship between surface rock abundance, glass proportion and maximum deposit thickness of localized pyroclastic deposits, which we used to categorize these deposits into four groups.
Description: Ph.D. University of Hawaii at Manoa 2014.
Includes bibliographical references.
Rights: All UHM dissertations and theses are protected by copyright. They may be viewed from this source for any purpose, but reproduction or distribution in any format is prohibited without written permission from the copyright owner.
Appears in Collections:Ph.D. - Geology and Geophysics

Items in ScholarSpace are protected by copyright, with all rights reserved, unless otherwise indicated.