HR: 15:25h
AN: P43C-07 [Abstracts]
TI: Lunar Tidal Deformation and the Internal Structure of the Moon
AU: * Sohl, F
EM: Frank.Sohl@dlr.de
AF: DLR Institute of Planetary Research, Rutherfordstr. 2, Berlin, 12489, Germany
AU: Hussmann, H
EM: Hauke.Hussmann@dlr.de
AF: DLR Institute of Planetary Research, Rutherfordstr. 2, Berlin, 12489, Germany
AU: Grott, M
EM: Matthias.Grott@dlr.de
AF: DLR Institute of Planetary Research, Rutherfordstr. 2, Berlin, 12489, Germany
AU: Knapmeyer, M
EM: Martin.Knapmeyer@dlr.de
AF: DLR Institute of Planetary Research, Rutherfordstr. 2, Berlin, 12489, Germany
AU: Oberst, J
EM: Juergen.Oberst@dlr.de
AF: DLR Institute of Planetary Research, Rutherfordstr. 2, Berlin, 12489, Germany
AB:
Monitoring tidally-induced deformations of the Moon from orbiting and landed spacecraft would provide important
clues on the constitution of the lunar interior, thereby augmenting the Apollo seismic data record. A major
advantage is that the tidal forcing function for a synchronously rotating satellite like the Moon is accurately known
and precise tidal potential catalogues can be produced. A higher temporal resolution and precision than with
space techniques alone can be achieved by additionally emplacing one or several landers on the lunar surface.
However, tidal measurements may be significantly impeded by instrumental drift, instrument coupling to the
surface, and local sources of noise. We will present relations between key tidal parameters that can be retrieved
from an instrument suite monitoring tidally-induced changes of local gravity, tilt, latitude and strain at the surface
and the constitution of the deep interior of the Moon. A most promising approach would involve time-varying
gravitational field observations from an orbiting spacecraft combined with long-term monitoring of tidally-induced
gravity changes at the lunar surface.
DE: 5417 Gravitational fields (1221)
DE: 5430 Interiors (8147)
DE: 5460 Physical properties of materials
DE: 6250 Moon (1221)
DE: 6297 Instruments and techniques
SC: Planetary Sciences [P]
MN: 2007 Fall Meeting