The isostatic state of Mead crater

Details The isostatic state of Mead crater The isostatic state of Mead crater

Nov 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994icar..112..117b&link_type=abstract

Icarus (ISSN 0019-1035), vol. 112, no. 1, p. 117-129

Computer Science

4

Cratering, Gravity Anomalies, Isostasy, Planetary Craters, Planetary Crusts, Topography, Venus (Planet), Venus Surface, Compensation, Earth (Planet), Line Of Sight, Lithosphere, Magellan Spacecraft (Nasa), Moon, Planetary Mantles, Spherical Harmonics

Scientific paper

We have analyzed high-resolution Magellan Doppler tracking data over Mead crater, using both line-of-sight and spherical harmonic methods, and have found a negative gravity anomaly of about 4-5 mgal (at spacecraft altitude, 182 km). This is consistent with no isostatic compensation of the present topography; the uncertainty in the analysis allows perhaps as much as 30% compensation at shallow depths (approximately 25 km). This is similar to observations of large craters on Earth, which are not generally compensated, but contrasts with at least some lunar basins which are inferred to have large Moho uplifts and corresponding positive Bouguer anomalies. An uncompensated load of this size requires a lithosphere with an effective elastic lithosphere thickness greater than 30 km. In order for the crust-mantle boundary not to have participated in the deformation associated with the collapse of the transient cavity during the creation of the crater, the yield strength near the top of the mantle must have been significantly higher on Earth and Venus than on the Moon at the time of basin formation. This might be due to increased strength against frictional sliding at the higher confining pressures within the larger planets. Alternatively, the thinner crusts of Earth and Venus compared to that of the Moon may result in higher creep strength of the upper mantle at shallower depths.

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