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Updated: May 12, 2026

Methods for Measuring the Orientation and Rotation Rate of 3D-printed Particles in Turbulence
12:34

Methods for Measuring the Orientation and Rotation Rate of 3D-printed Particles in Turbulence

Published on: June 24, 2016

小惑星"862アポロ"の自転の加速は,放射線トルクによるものです

Mikko Kaasalainen1, Josef Durech, Brian D Warner

  • 1Department of Mathematics and Statistics, Rolf Nevanlinna Institute, PO Box 68, FI-00014 University of Helsinki, Finland. mikko.kaasalainen@helsinki.fi

Nature
|March 9, 2007
PubMed
まとめ

小惑星から反射する太陽光によって引き起こされるヤルコフスキー・オキーフ・ラデヴスキー・パダック (YORP) 効果は,小惑星1862アポロの自転速度の変化を直接観測した. この発見は,YORP効果が小惑星の動力学に大きな影響を与えていることを確認しています.

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