Published February 15, 2024 | Version Published
Journal Article Open

Dimensionless argument: a narrow grain size range near 2 mm plays a special role in river sediment transport and morphodynamics

  • 1. ROR icon University of Illinois Urbana-Champaign
  • 2. ROR icon Tsinghua University
  • 3. ROR icon California Institute of Technology
  • 4. ROR icon Durham University
  • 5. ROR icon Simon Fraser University

Abstract

The grain size 2 mm is the conventional border between sand and gravel. This size is used extensively, and generally without much physical justification, to discriminate between such features as sedimentary deposit type (clast-supported versus matrix-supported), river type (gravel bed versus sand bed), and sediment transport relation (gravel versus sand). Here we inquire as to whether this 2 mm boundary is simply a social construct upon which the research community has decided to agree or whether there is some underlying physics. We use dimensionless arguments to show the following for typical conditions on Earth, i.e., natural clasts (e.g., granitic or limestone) in 20 C water. As grain size ranges from 1 to 5 mm (a narrow band including 2 mm), sediment suspension becomes vanishingly small at normal flood conditions in alluvial rivers. We refer to this range as pea gravel. We further show that bedload movement of a clast in the pea gravel range with, for example, a size of 4 mm moving over a bed of 0.4 mm particles has an enhanced relative mobility compared to a clast with a size of 40 mm moving over a bed of the same 4 mm particles. With this in mind, we use 2 mm here as shorthand for the narrow pea gravel range of 1–5 mm over which transport behavior is distinct from both coarser and finer material. The use of viscosity allows the delineation of a generalized dimensionless bed grain size discriminator between “sand-like” and “gravel-like” rivers. The discriminator is applicable to sediment transport on Titan (ice clasts in flowing methane/ethane liquid at reduced gravity) and Mars (mafic clasts in flowing water at reduced gravity), as well as Earth.

Copyright and License

© Author(s) 2024. This work is distributed under the Creative Commons Attribution 4.0 License.

Published by Copernicus Publications on behalf of the European Geosciences Union.

Acknowledgement

Michael Church provided valuable comments, which have been incorporated into the text. The authors acknowledge helpful reviews from Enrica Viparelli and an anonymous reviewer.

Funding

The participation of Gary Parker has been supported in part by the W. H. Johnson chair of the Department of Earth Science and Environmental Change, University of Illinois, Urbana-Champaign, USA. The participation of Chenge An has been supported by the National Natural Science Foundation of China (grant no. 52009063) and the Young Elite Scientists Sponsorship Program of CAST (grant no. 2021QNRC001).

Additional Information

This paper was edited by Jens Turowski and reviewed by Enrica Viparelli and one anonymous referee.

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Additional details

Related works

Is new version of
Discussion Paper: 10.5194/egusphere-2023-1705 (DOI)

Funding

University of Illinois Urbana-Champaign
Department of Earth Science and Environmental Change -
National Natural Science Foundation of China
52009063
China Association for Science and Technology
2021QNRC001

Dates

Accepted
2023-11-14

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Caltech groups
Division of Geological and Planetary Sciences (GPS)
Publication Status
Published