Abstract
Observations have shown that most small bodies of diameters larger than 300 m are covered by regolith materials, i.e. an active layer of loose unconsolidated rocks and dust, which has been shaped by various space weathering effects. Thus, a detailed look at the grains’ dynamics is apparently important and necessary for the understanding of above processes. The ejecta from a meteorite impact may experience different evolutional histories and end up with different fates. Differing from around planets, the orbital motion and surface motion around a small body are not clearly demarcated, because: first, the gravity from a small body is usually weak, and the minimum launch speed could be easily reached each by a natural grain on the surface; second, small bodies have no atmosphere, i.e., once an object lifts from the surface, it is counted as orbital motion. This chapter presents our method to model the migration of individual grain on asteroid’s surface. In Sect. 6.2, a global valid method for gravitational filed calculation is developed; Sect. 6.3 proposes an event-driven model to implement full simulation of an individual particle moving over the surface of an asteroid; Sect. 6.4 includes basic tests as verification to the model proposed; Sect. 6.5 demonstrates a possible application of our method, to explore the surface mechanical environment of a specified asteroid 1620 Geographos, and to find out the connections between the local geological features and the dynamical behaviours of the test particle.
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References
Clark BE, Hapke B, Pieters C (2002) Asteroid space weathering and regolith evolution. In: William F et al (eds) Asteroids III, Univ. Arizona Press, Tucson, AZ, pp 603–612
Werner RA, Scheeres DJ (1997) Exterior gravitation of a polyhedron derived and compared with harmonic and mascon gravitation representations of asteroid 4769 Castalia. Celest Mech Dyn Astron. 65:313–344
Petrović S (1996) Determination of the potential of homogeneous polyhedral bodies using line integrals. J. Geodesy 71:44–52
Tsoulis D, Petrović S (2001) On the singularities of the gravity field of a homogeneous polyhedral body. Geophysics 66:535–539
Shirman LA, Séquin CH (1987) Local surface interpolation with Bézier patches. Comput Aided Geom Des 4:279–295
Hudson RS, Ostro SJ (1999) Physical model of Asteroid 1620 Geographos from radar and optical data. Icarus 140:369–378
Pudasaini SP, Hutter K (2007) Avalanche dynamics: dynamics of rapid flows of dense granular avalanches. Springer, Heidelberg
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Yu, Y. (2016). Natural Motion Near the Surface of Small Bodies. In: Orbital Dynamics in the Gravitational Field of Small Bodies. Springer Theses. Springer, Berlin, Heidelberg. https://doi.org/10.1007/978-3-662-52693-4_6
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DOI: https://doi.org/10.1007/978-3-662-52693-4_6
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