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Updated: Jul 17, 2026

Investigation of Early Plasma Evolution Induced by Ultrashort Laser Pulses
11:20

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Published on: July 2, 2012

ニオビウム-ジルコニウムクロノメトリーと太陽系初期開発

Maria Schönbächler1, Mark Rehkämper, Alex N Halliday

  • 1Institute of Isotope Geology and Mineral Resources, ETH Zürich, 8092 Zürich, Switzerland. maria@erdw.ethz.ch

Science (New York, N.Y.)
|March 2, 2002
PubMed
まとめ

ニオビウム-92 (92Nb) 崩壊は,初期の太陽系プロセスについての洞察を提供します. 新しい研究は,初期太陽系92Nb/93Nb比が低い (<3 x 10(-5) であることを示し,以前の高い推定値に異議を唱え,惑星の微分化モデルに影響を与えた.

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