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Quantifying crater production and regolith overturn on the Moon with temporal imaging

Author

Listed:
  • Emerson J. Speyerer

    (Arizona State University, School of Earth and Space Exploration)

  • Reinhold Z. Povilaitis

    (Arizona State University, School of Earth and Space Exploration)

  • Mark S. Robinson

    (Arizona State University, School of Earth and Space Exploration)

  • Peter C. Thomas

    (Cornell University, Cornell Center for Astrophysics and Planetary Science)

  • Robert V. Wagner

    (Arizona State University, School of Earth and Space Exploration)

Abstract

High-resolution ‘before and after’ imaging of the Moon is used to quantify the rate of crater production and provide insights into the cratering process.

Suggested Citation

  • Emerson J. Speyerer & Reinhold Z. Povilaitis & Mark S. Robinson & Peter C. Thomas & Robert V. Wagner, 2016. "Quantifying crater production and regolith overturn on the Moon with temporal imaging," Nature, Nature, vol. 538(7624), pages 215-218, October.
    • Handle: RePEc:nat:nature:v:538:y:2016:i:7624:d:10.1038_nature19829
    DOI: 10.1038/nature19829
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    Cited by:

    1. S. Wakita & B. C. Johnson & I. Garrick-Bethell & M. R. Kelley & R. E. Maxwell & T. M. Davison, 2021. "Impactor material records the ancient lunar magnetic field in antipodal anomalies," Nature Communications, Nature, vol. 12(1), pages 1-7, December.

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