The global effects of impact-induced seismic activity on fractured asteroid surface morphology

James E. Richardson, H. Jay Melosh, Richard J. Greenberg, David P. O'Brien

Research output: Contribution to journalArticle

118 Citations (Scopus)

Abstract

Impact-induced seismic vibrations have long been suspected of being an important surface modification process on small satellites and asteroids. In this study, we use a series of linked seismic and geomorphic models to investigate the process in detail. We begin by developing a basic theory for the propagation of seismic energy in a highly fractured asteroid, and we use this theory to model the global vibrations experienced on the surface of an asteroid following an impact. These synthetic seismograms are then applied to a model of regolith resting on a slope, and the resulting downslope motion is computed for a full range of impactor sizes. Next, this computed downslope regolith flow is used in a morphological model of impact crater degradation and erasure, showing how topographic erosion accumulates as a function of time and the number of impacts. Finally, these results are applied in a stochastic cratering model for the surface of an Eros-like body (same volume and surface area as the asteroid), with craters formed by impacts and then erased by the effects of superposing craters, ejecta coverage, and seismic shakedown. This simulation shows good agreement with the observed 433 Eros cratering record at a Main Belt exposure age of 400 ± 200 Myr, including the observed paucity of small craters. The lowered equilibrium numbers (loss rate = production rate) for craters less than ∼100 m in diameter is a direct result of seismic erasure, which requires less than a meter of mobilized regolith to reproduce the NEAR observations. This study also points to an upper limit on asteroid size for experiencing global, surface-modifying, seismic effects from individual impacts of about 70-100 km (depending upon asteroid seismic properties). Larger asteroids will experience only localized (regional) seismic effects from individual impacts.

Original languageEnglish (US)
Pages (from-to)325-349
Number of pages25
JournalIcarus
Volume179
Issue number2
DOIs
StatePublished - Dec 15 2005

Fingerprint

asteroids
asteroid
craters
crater
regolith
cratering
vibration
seismic energy
seismic property
impactors
synthetic seismogram
seismograms
ejecta
seismic activity
effect
erosion
surface area
degradation
slopes
propagation

Keywords

  • Asteroids, composition
  • Asteroids, eros
  • Impact processes
  • Regoliths
  • Surfaces, asteroids

ASJC Scopus subject areas

  • Space and Planetary Science
  • Astronomy and Astrophysics

Cite this

The global effects of impact-induced seismic activity on fractured asteroid surface morphology. / Richardson, James E.; Melosh, H. Jay; Greenberg, Richard J.; O'Brien, David P.

In: Icarus, Vol. 179, No. 2, 15.12.2005, p. 325-349.

Research output: Contribution to journalArticle

Richardson, James E. ; Melosh, H. Jay ; Greenberg, Richard J. ; O'Brien, David P. / The global effects of impact-induced seismic activity on fractured asteroid surface morphology. In: Icarus. 2005 ; Vol. 179, No. 2. pp. 325-349.
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