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Numerical Solutions for the Orbital Motion of the Solar System over the Past 100 Myr: Limits and New Results* - MaRDI portal

Numerical Solutions for the Orbital Motion of the Solar System over the Past 100 Myr: Limits and New Results*

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Publication:5982433

DOI10.3847/1538-3881/AA8CCEWikidataQ69163196 ScholiaQ69163196MaRDI QIDQ5982433

Richard E. Zeebe

Publication date: 20 October 2017

Published in: The Astronomical Journal (Search for Journal in Brave)






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