Modelling the outcomes of high-velocity impacts between small solar system bodies (Q1311623)
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scientific article; zbMATH DE number 486916
| Language | Label | Description | Also known as |
|---|---|---|---|
| English | Modelling the outcomes of high-velocity impacts between small solar system bodies |
scientific article; zbMATH DE number 486916 |
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Modelling the outcomes of high-velocity impacts between small solar system bodies (English)
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2 February 1995
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An algorithm for numerical modelling of distribution of small bodies of the solar system after their catastrophic impacts is considered. The calculations are carried out using experimental parameters of asteroids fragments for selected stable velocities and masses. In particular, the influence of the gravitational reaccumulation of small bodies is investigated by some examples. The algorithm can be used in theoretical and experimental investigations. The paper contains 46 references.
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experimental parameters
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asteroids
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gravitational reaccumulation
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0.87527895
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0.8595974
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0.83784276
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0.8299532
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0.82483613
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