HR: 1340h
AN: P23A-0224    [Abstracts]
TI: Deep Moonquakes: Remaining Problems
AU: * Nakamura, Y
EM: yosio@utig.ig.utexas.edu
AF: Institute for Geophysics, University of Texas at Austin, 4412 Spicewood Springs Road, Bldg. 600, Austin, TX 78759-8500 United States
AB: We have recently reexamined more than 9000 previously unidentified seismic events catalogued during the Apollo landing missions and positively identified for the first time about 30 deep moonquake nests on the far side of the Moon. Although only a few of them are currently locatable, the relative arrival times among stations for the rest and presence or absence of seismic signals at particular stations suggest that either (a) the region within about $40\deg$ of the antipode is aseismic or (b) the deep interior of the Moon severely attenuates or deflects seismic waves. Aside from the obvious question of how to distinguish between such hypothetical models, this effort raised several more general questions concerning the use of deep moonquake signals to infer the structure and dynamics of the deep interior of the Moon. Among more important ones are: (1) How reliable are the seismic arrival picks from which to compute the seismic velocity variations in the Moon? (2) How do the possible lateral variations in seismic velocity affect the computed radial variation in seismic velocity at depth? (3) Can we tell more about the distribution and mechanism of deep moonquakes from the newly expanded database of identified deep moonquakes? Questions (1) and (2) are especially important because the inferred deep internal structure of the Moon depends critically on their answers. answering these questions may demand additional data collected on future lunar missions, but some may be resolved with further examination of the existing data.
DE: 5430 Interiors (8147)
DE: 5475 Tectonics (8149)
DE: 6250 Moon (1221)
SC: Planetary Sciences [P]
MN: 2004 AGU Fall Meeting