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Abstract
Grooved and hilly terrains occur at the antipode of major basins on the Moon (Imbrium, Orientale) and Mercury (Caloris). Such terrains may represent extensive landslides and surface disruption produced by impact-generatedP-waves and antipodal convergence of surface waves. Order-of-magnitude calculations for an Imbrium-size impact (1034 erg) on the Moon indicateP-wave-induced surface displacements of 10 m at the basin antipode that would arrive prior to secondary ejecta. Comparable surface waves would arrive subsequent to secondary ejecta impacts beyond 103 km and would increase in magnitude as they converge at the antipode. Other seismically induced surface features include: subdued, furrowed crater walls produced by landslides and concomitant secondary impacts; emplacement and leveling of light plains units owing to seismically induced ‘fluidization’ of slide material; knobby, pitted terrain around old basins from enhancement of seismic waves in ancient ejecta blankets; and perhaps the production and enhancement of deep-seated fractures that led to the concentration of farside lunar maria in the Apollo-Ingenii region.
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References
Baldwin, R. B.: 1963,The Measure of the Moon, 488 pp., Univ. of Chicago Press, Chicago.
Bullen, K. E.: 1963,An Introduction to the Theory of Seismology, 381 pp., Cambridge University Press, Cambridge.
Eggleton, R. E. and Marshall, C. H.: 1962,Astrogeol. Studies Semiann. Prog. Rept., February 1961-August 1961, pt. A, 132–137, U.S. Geol. Survey open-file report.
Gault, D. E.: 1974, in R. Greeley and P. Schultz (eds.),A Primer in Lunar Geology, 137–176, NASA TM-62, 359.
Gault, D. E. and Heitowit, E. D.: 1963,Proc. Sixth Hypervelocity Impact Symposium,2, 419.
Gault, D. E. and Wedekind, J. A.: 1969,J. Geophys. Res.74, 6780.
Gault, D. E., Quaide, W. L., and Oberbeck, V. R.: 1968, in B. M. French and N. M. Short (eds.)Shock Metamorphism of Natural Materials, 87–99, Mono Book Corp., Baltimore.
Gault, D. E., Shoemaker, E. M., and Moore, H. J.: 1963,Spray Ejected from the Lunar Surface by Meteoroid Impact, NASA TN D-1767, Ames Research Center.
Howard, K. A., Wilhelms, D. E., and Scott, D. H.: 1974,Rev. Geophys. Space Phys.74, 309.Stratigraphy, preprint.
Johnson, S. W., Smith, J. A., Franklin, E. G., Moraski, L. K., and Teal, D. J.: 1969,J. Geophys. Res.74, 4838.
Latham, G. V., McDonald, W. G., and Moore, H. J.: 1970a,Science168, 242.
Latham, G., Ewing, M., Dorman, J., Press, F., Toksőz, N., Sutton, G., Meissner, R., Duennebier, F., Nakamura, Y., Kovach, R., and Yates, M.: 1970b,Science170, 620.
Latham, G. V., Ewing, M., Press, F., Sutton, G., Dorman, J., Nakamura, Y., Toksőz, N., Lammlein, D., and Duennebier, F.: 1972, inApollo 16 Preliminary Science Report, 9:1-9:29, NASA SP-315.
McGarr, A., Latham, G. V., and Gault, D. E.: 1969,J. Geophys. Res.74, 5981.
Moore, H. J., Hodges, C. A., and Scott, D. H.: 1974, inProc. Fourth Lunar Sci. Conf., Geochim. Cosmochim. Acta, (in press).
Murray, B. C., Belton, M. J. S., Danielson, G. E., Davies, M. E., Gault, D. E., Hapke, B.,O'Leary, B., Strom, R. G., Suomi, V., and Trask, N.: 1974,Science185, 169.
Pollack, J. B., Veverka, J., Noland, M., Sagan, C., Hartmann, W. K., Duxbury, T. C., Born, G. H., Milton, D. J., and Smith, B. A.: 1972,Icarus17, 394.
Rinehart, J. S.: 1960,Quart. Colorado Sch. Mines55, No. 4, 155 pp., Goldon.
Rinehart, J. S.: 1968, in B. M. French and N. M. Short (eds.),Shock Metamorphism of Natural Materials, 31–42, Mono Book Corp., Baltimore.
Schultz, P. H.: 1972,A Preliminary Morphologic Study of the Lunar Surface, 967 pp., Ph.D. Thesis, University of Texas at Austin.
Schultz, P. H.: 1974,Moon Morphology, University of Texas Press, Austin, (in press).
Stöffler, D., Gault, D. E., Wedekind, J., and Polkowski, G.: 1974,J. Geophys. Res., (in press).
Stuart-Alexander, D. E. and Howard, K. E.: 1970,Icarus12, 440–456.
Titley, S. R.: 1966, ‘Seismic Energy as an Agent of Morphologic Modification on the Moon’, inAstrogeol. Studies Ann. Prog. Rept. July 1, 1965-July 1, 1966, pt. A, 87–103,U.S. Geol. Survey open-file report.
Titley, S. R. and Eggleton, R. E.: 1964, ‘Description of an Extensive Hummocky Deposit Around the Humorum Basin’, inAstrogeol. Studies Ann. Prog. Rept., July 1963-July, 1964, pt. A, 85–89,U.S. Geol. Survey open-file report.
Trask, N. J. and Titley, S. R.: 1966, ‘Geologic Map of the Pitatus Region of the Moon’,U.S. Geol. Survey Misc. Geol. Inv. Map I-485.
Wilhelms, D. E. and McCauley, J. F.: 1971, ‘Geologic Map of the Near Side of the Moon’,U.S. Geol. Survey Misc. Geol. Inv. Map I-703.
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Space Science Division, NASA Ames Research Center, Moffett Field, Calif., USA
Peter H. Schultz & Donald E. Gault
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Schultz, P.H., Gault, D.E. Seismic effects from major basin formations on the moon and mercury.The Moon12, 159–177 (1975). https://doi.org/10.1007/BF00577875
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