Errors in minimum plate velocity determined from paleomagnetic data

Abstract

In prior studies paleomagnetic data have been used to determine ancient minimum velocities of the continents. The greatest minimum velocities, ∼50 km/m.y., exceed the present‐day absolute velocities of the major continents. This result is important because the observation that present‐day oceanic plates move faster than present‐day continental plates can be treated as a major constraint on plate dynamics. However, these prior studies are limited because they ignore known errors in the paleomagnetic data. In this paper we present a technique for incorporating these errors and using them to estimate 95% confidence limits on the minimum velocities. This new technique was applied to Pennsylvanian to Cretaceous paleomagnetic data from North America and to the ancient geometry of Laurasia. When errors are considered, minimum velocities are 10 to 50 km/m.y. lower than when errors are ignored. Additional uncertainties owing to a hypothesized clockwise rotation of the Colorado Plateau, a source of many of the data, are considered and found to alter the minimum velocities only negligibly. Allowing for uncertainties in the pole positions, uncertainties in ages, and the uncertainty due to possible rotation of the Colorado plateau, we estimate that Laurasia moved at least 48 km/m.y. from Early Jurassic to Early Cretaceous time, and at least 43 km/m.y. from Pennsylvanian through Late Triassic time. There is only a 5% risk that the true minimum velocities are lower than these lower bounds. These velocities are less than the peak velocities over short intervals found in prior analyses, but exceed the average velocities previously found for Triassic and Jurassic time. These newly estimated velocities are still much higher than the present velocities of the continents and, as in the prior studies, imply that the slow motion characteristic of major continents at present is not a fundamental attribute of plate motions.

Cenozoic global plate motions

“…1711 1.9164 2.2647 -0.2642 0.2240 -0.0606 ?h 0.0093 0.0078 0.0022 0.0008 0.0016 -0 1968 2.0183 2.0865 -0.3996 0.0751 -0 Contrary to our earlier working hypothesis, the Cenozoic Era might not be long enough for an independent plate geometry to evolve. Analyses of paleomagnetic data for much earlier epochs, such as the Jurassic and Triassic, show that continents moved much faster than they do at present, whereas the same analyses applied to Cenozoic paleomagnetic data suggest slow motion of continents [Gordon et al, 1979;Ullrich and Van der Voo, 1981;Bryan and Gordon, 1986]. This suggests that examination of ancient plate motions is useful, but one must look much further into the past than was previously thought.…”