Some seismic effects on small bodies of the solar system

Astronomy and Astrophysics – Astronomy

Scientific paper

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Hypervelocity Impact, Meteorite Collisions, Meteorite Craters, Phobos, Seismic Waves, Elastic Waves, Propagation Velocity, Seismic Energy, Solar System, Standing Waves

Scientific paper

This letter demonstrates that both parallel grooves and a deficiency of small craters, such as have been observed on Phobos, can develop from internal oscillations in a solid satellite that are induced by a collision with a suitable meteoroid. A limit is placed on the period of the induced vibrations, and it is shown that a system of standing waves with a period of 0.2 sec could have generated an organized system of furrows with a characteristic spacing of about 200 m on Phobos. The energy carried by these waves is estimated to have been approximately 5 x 10 to the 18th erg for a regolith density of 2 g/cu cm. It is concluded that the impact of a meteoroid generating a crater about 4 km in diameter could also simultaneously produce a regular system of grooves and denude craters of small diameter.

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