Lunar Seismic Tomography and the Early Earth
Author:
Affiliation:
1. Graduate School of Science, Tohoku University
2. Earth-Life Science Institute, Tokyo Institute of Technology
3. Department of General System Studies, The University of Tokyo
Publisher
Tokyo Geographical Society
Subject
Earth-Surface Processes,Geology,Geophysics,Geography, Planning and Development,Global and Planetary Change
Link
https://www.jstage.jst.go.jp/article/jgeography/127/5/127_127.619/_pdf
Reference53 articles.
1. Arai, T., Takeda, H., Yamaguchi, A. and Ohtake, M. (2008): A new model of lunar crust: Asymmetry in crustal composition and evolution. Earth, Planets and Space, 60, 433-444.
2. Arai, T., Hawke, B., Giguere, T., Misawa, K., Miyamoto, M. and Kojima, H. (2010): Antarctic lunar meteorites Yamato-793169, Asuka-881757, MIL 05035, and MET 01210 (YAMM): Launch pairing and possible cryptomare origin. Geochimica et Cosmochimica Acta, 74, 2231-2248.
3. Chenet, H., Lognonne, P., Wieczorek, M. and Mizutani, H. (2006): Lateral variations of lunar crustal thickness from the Apollo seismic data set. Earth and Planetary Science Letters, 243, 1-14.
4. Dohm, J.M. and Maruyama, S. (2015): Habitable trinity. Geoscience Frontiers, 6, 95-101.
5. Frohlich, C. and Nakamura, Y. (2009): The physical mechanisms of deep moonquakes and intermediate-depth earthquakes: How similar and how different?. Physics of the Earth and Planetary Interiors, 173, 365-374.
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