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Variable Oort Cloud Flux due to the Galactic Tide

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Collisional Processes in the Solar System

Part of the book series: Astrophysics and Space Science Library ((ASSL,volume 261))

Abstract

We review the subject of the time dependence of the component of Oort cloud comet flux due to the adiabatic Galactic tide, including the possibility of detecting such a signal in the terrestrial cratering record.

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Matese, J.J., Innanen, K.A., Valtonen, M.J. (2001). Variable Oort Cloud Flux due to the Galactic Tide. In: Marov, M.Y., Rickman, H. (eds) Collisional Processes in the Solar System. Astrophysics and Space Science Library, vol 261. Springer, Dordrecht. https://doi.org/10.1007/978-94-010-0712-2_5

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  • DOI: https://doi.org/10.1007/978-94-010-0712-2_5

  • Publisher Name: Springer, Dordrecht

  • Print ISBN: 978-94-010-3832-4

  • Online ISBN: 978-94-010-0712-2

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