Continents sliding away from a central explosion does appear to produce the shapes and features of most of Earth's crust in a simple, straightforward way. Once it is clear that an event happened, the discussion about whether it is possible or not is over, and the question turns to "how?". How did the landmasses slide?
For perspective, note that while several thousand miles is a long way for us humans, most of the continents slid only 12-16% of the distance around the world at the equator. Australia went farthest: 23% of Earth's circumference.
People are too small to experiment with huge continents, so any explanation must be speculation. However, there is an interesting possibility.
An odd phenomenon has been identified on Earth and other members of the solar system. Large landslides don't just fall to the base of the mountain the way small ones do; they often go great distances, some up to 30 times the distance they fell.
Dr. H. J. Melosh has proposed that long-runnout landslides, earthquake slip, and the making of complex craters reveal a characteristic of the crust. Put simply, it temporarily acts like a fluid when enough stress is applied.
known on a small scale as a Bingham Fluid, Melosh suggests that
fluidization at the base of large landslides reduces friction
to near zero. He calls it acoustic fluidization.
In a paper computer-modelling long-runnout landslides, Melosh and two others wrote: "For rock masses with volumes exceeding 109 m3, these landslides regularly run out more than 10 times longer than the height they fall from."
"Many mechanisms have been proposed to explain this apparent reduction of friction: riding atop a cushion of trapped air; lubrication by water; a basal frictional melt layer; frictionally warmed ice; frictional velocity-weakening; a basal layer of colliding grains (dispersive grain flow); and acoustic fluidization."
"Our results are very similar to the predictions of the acoustic fluidization hypothesis, where the flow is effectively fluidized by local variations in the contact forces between the grains. Acoustic fluidization is similar to the pore pressure fluctuations observed in debris flows, but without an interstitial fluid. The acoustic fluidization wavelength is determined by the size of the rock fragments in the slide."
"Friction is reduced even during the earliest stages of the slide. Although the slides have similar maximum velocities, larger slides initially accelerate faster than the smaller slides, implying a smaller effective coefficient of friction even at the onset of sliding."
"We note that channelized slides do not exhibit
systematically longer runout distances than unconfined slides, suggesting that
spreading perpendicular to the main slide path is not of fundamental importance
to the runout."
Corresponding to the falling side of a mountain that powers a landslide, the explosive power released by the giant meteorite on impact would have set the landmasses in motion with the force of billions of megatons of TNT, generating acoustic energy. The continental crust's mass would confine the acoustic energy to the base of the crust.
Shi Jian-chun, Ma Yue-hua, Bao Gang. 2009. The Formation Model of Multi-ring Basins Based on the Theory of Impact Tsunami. Chinese Astronomy and Astrophysics, Vol. 33, pp. 287-292.
There is an important
feature of long-runnout landslides that have stopped moving:
"Ridges formed at the front and rear of the debris support
the hypothesis that the leading edges of the slide initially ground
to a halt and the rest of the material piled up behind it."
The Shock Dynamics scenario
With all the action at the surface, it follows that features in the oceanic crust are fairly shallow. They include these:
Mid-ocean ridges and transform faults, where surface melting results from the removal of the weight of continental crust (pressure relief melting).
Trenches (green line) along the leading edges of landmasses result from the rapid application of the weight of continental crust. Towards the end of a continent's run, friction compresses the leading edge, raising mountains.
A crustal wave (red line) from the low angle impact was launched in the direction of travel of the meteorite, and "froze" in the end to form an inclined trench.