LEADER 01459nam 2200433 450 001 9910480641903321 005 20180628190722.0 035 $a(CKB)3710000001444382 035 $a(MiAaPQ)EBC4983483 035 $a(DLC) 2017045995 035 $a(EXLCZ)993710000001444382 100 $a20170831h20172017 uy| 0 101 0 $aeng 135 $aurcnu|||||||| 181 $2rdacontent 182 $2rdamedia 183 $2rdacarrier 200 00$aMoving bodies in interaction-- interacting bodies in motion $eintercorporeality, interkinesthesia, and enaction in sports /$fedited by Christian Meyer, Ulrich v. 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The code accurately solves the elastic dynamic equations and describes the effects of fracture and friction, which makes it possible to investigate the shapes of impact outcomes produced by asteroid collisions and subsequent gravitational accumulation of fragments. The author parallelizes the code with high parallelization efficiency; accordingly, it can be used to conduct high-resolution simulations with the aid of supercomputers and clarify the shapes of small remnants produced through the catastrophic destruction of asteroids. The author demonstrates that flat asteroids can only be produced by impacts involving objects with similar mass and low velocity, which suggests that the flat asteroids in our solar system were created in the planet formation era and have kept their shapes until today. The author also shows that asteroid collisions under certain conditions can produce the extremely elongated shape of an interstellar minor body, 1I/?Oumuamua. 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