Seismic effects of the Caloris basin impact, Mercury

Thesis (S.M.)--Massachusetts Institute of Technology, Dept. of Earth, Atmospheric, and Planetary Sciences, 2011.

Bibliographic Details
Main Author: Lü, Jiangning
Other Authors: Maria T. Zuber.
Format: Thesis
Language:eng
Published: Massachusetts Institute of Technology 2012
Subjects:
Online Access:http://hdl.handle.net/1721.1/69472
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author Lü, Jiangning
author2 Maria T. Zuber.
author_facet Maria T. Zuber.
Lü, Jiangning
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description Thesis (S.M.)--Massachusetts Institute of Technology, Dept. of Earth, Atmospheric, and Planetary Sciences, 2011.
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spelling mit-1721.1/694722019-04-12T15:28:43Z Seismic effects of the Caloris basin impact, Mercury Lü, Jiangning Maria T. Zuber. Massachusetts Institute of Technology. Dept. of Earth, Atmospheric, and Planetary Sciences. Massachusetts Institute of Technology. Dept. of Earth, Atmospheric, and Planetary Sciences. Earth, Atmospheric, and Planetary Sciences. Thesis (S.M.)--Massachusetts Institute of Technology, Dept. of Earth, Atmospheric, and Planetary Sciences, 2011. Cataloged from PDF version of thesis. Page 46 blank. Includes bibliographical references (p. 41-45). Striking geological features on Mercury's surface have been linked to tectonic disruption associated with the Caloris impact and have the potential to provide information on the interior structure of Mercury. The unusual disrupted terrain located directly at the antipode of the 1500-km-diameter Caloris basin could have plausibly formed as a consequence of focused seismic waves generated by the massive impact event. In this paper, we revisit the antipodal seismic focusing effects of the Caloris impact by developing physically consistent structure models for Mercury and parameterized seismic source models for the Caloris impact. If the focused seismic body waves caused the disrupted terrain, then the amplitudes of the waves and the areal extent of surface disruptions could be used for estimating the seismic energy imparted by the impact. In this study, we show that effects of direct body waves are small relative to those of the focused guided waves. Two types of guided waves are generated by the Caloris impact. One is the conventional Rayleigh wave generated by the impact. The second is the mantle guided waves trapped between the core and the free surface. Mantle guided waves, not mentioned in previous studies, may have played an important role in the creation of the disrupted terrain. We find that the early core state has only moderate effects on the antipodal response to the Caloris impact. The fact that the zone of predicted disruption for both fluid and solid core cases is smaller than the observed region of chaotic terrain suggests either that the antipodal response to the Caloris impact may have been modulated by the shallow structure of Mercury, or that the energy imparted by the impact was larger than those used in this study. by Jiangning Lü. S.M. 2012-02-29T17:57:52Z 2012-02-29T17:57:52Z 2011 2011 Thesis http://hdl.handle.net/1721.1/69472 775585855 eng M.I.T. 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. See provided URL for inquiries about permission. http://dspace.mit.edu/handle/1721.1/7582 46 p. application/pdf Massachusetts Institute of Technology
spellingShingle Earth, Atmospheric, and Planetary Sciences.
Lü, Jiangning
Seismic effects of the Caloris basin impact, Mercury
title Seismic effects of the Caloris basin impact, Mercury
title_full Seismic effects of the Caloris basin impact, Mercury
title_fullStr Seismic effects of the Caloris basin impact, Mercury
title_full_unstemmed Seismic effects of the Caloris basin impact, Mercury
title_short Seismic effects of the Caloris basin impact, Mercury
title_sort seismic effects of the caloris basin impact mercury
topic Earth, Atmospheric, and Planetary Sciences.
url http://hdl.handle.net/1721.1/69472
work_keys_str_mv AT lujiangning seismiceffectsofthecalorisbasinimpactmercury