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Updated: Apr 12, 2026

Laboratory Drop Towers for the Experimental Simulation of Dust-aggregate Collisions in the Early Solar System
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土星から発生する高速度な塵の流れが,土星から発生する高速度な塵の流れです

Sascha Kempf1, Ralf Srama, Mihaly Horányi

  • 1MPI für Kernphysik, Saupfercheckweg 1, 69117 Heidelberg, Germany. Sascha.Kempf@mpi-hd.mpg.de

Nature
|January 22, 2005
PubMed
まとめ

土星の環からの高速な塵粒子は,カッシーニ宇宙船によって検出されました. これらの粒子は土星の磁気圏によって活性化され,太陽風の流れと相互作用します.

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