Preprints
https://doi.org/10.5194/esurf-2023-11
https://doi.org/10.5194/esurf-2023-11
19 Oct 2023
 | 19 Oct 2023
Status: this preprint was under review for the journal ESurf. A revision for further review has not been submitted.

Computational Sedimentation Modelling Calibration: a tool to measure the settling velocity at different gravity conditions

Nikolaus Josef Kuhn and Federica Trudu

Abstract. Research in zero or reduced gravity is essential to prepare and support planetary sciences and space exploration. In this study, an instrument specifically designed to measure the settling velocity of sediment particles under normal, hyper-, and reduced gravity conditions is presented. Once operational, it will be used to examine the quality of analogue terrestrial sedimentation environments for planetary research, especially for Mars. The lower gravity on Mars potentially reduces drag on particles settling in water, which in turn may affect the texture of sedimentary rocks forming in a given body of water moving down-slope. To assess the potential impact, an instrument was designed to simulate sediment settling at gravities different from Earth during parabolic flights. The trajectories of particles settling in water were recorded during the ascending part of a parabola (about 1.8 g), under reduced gravity conditions (Martian and lunar) and on Earth. The data were used to compute the terminal settling velocity of isolated and small groups of particles and compared to the results calculated using a semi theoretical formula derived in 2004 by Ferguson and Church (Ferguson & Church, 2004). The experimental data confirm the expected trend, i.e., that the values predicted using models calibrated with data collected at terrestrial gravity underestimate settling velocity on Mars. The results also demonstrate that the instrument is operational, providing a Martian gravity analogue for sedimentation studies on Earth.

Publisher's note: Copernicus Publications remains neutral with regard to jurisdictional claims made in the text, published maps, institutional affiliations, or any other geographical representation in this preprint. The responsibility to include appropriate place names lies with the authors.
Nikolaus Josef Kuhn and Federica Trudu

Status: closed (peer review stopped)

Comment types: AC – author | RC – referee | CC – community | EC – editor | CEC – chief editor | : Report abuse
  • RC1: 'Comment on esurf-2023-11', Anonymous Referee #1, 08 Nov 2023
    • AC1: 'Reply on RC1', Federica Trudu, 19 Jan 2024
  • RC2: 'Comment on esurf-2023-11', Anonymous Referee #2, 01 Dec 2023
    • AC2: 'Reply on RC2', Federica Trudu, 19 Jan 2024

Status: closed (peer review stopped)

Comment types: AC – author | RC – referee | CC – community | EC – editor | CEC – chief editor | : Report abuse
  • RC1: 'Comment on esurf-2023-11', Anonymous Referee #1, 08 Nov 2023
    • AC1: 'Reply on RC1', Federica Trudu, 19 Jan 2024
  • RC2: 'Comment on esurf-2023-11', Anonymous Referee #2, 01 Dec 2023
    • AC2: 'Reply on RC2', Federica Trudu, 19 Jan 2024
Nikolaus Josef Kuhn and Federica Trudu
Nikolaus Josef Kuhn and Federica Trudu

Viewed

Total article views: 531 (including HTML, PDF, and XML)
HTML PDF XML Total Supplement BibTeX EndNote
380 103 48 531 49 25 31
  • HTML: 380
  • PDF: 103
  • XML: 48
  • Total: 531
  • Supplement: 49
  • BibTeX: 25
  • EndNote: 31
Views and downloads (calculated since 19 Oct 2023)
Cumulative views and downloads (calculated since 19 Oct 2023)

Viewed (geographical distribution)

Total article views: 502 (including HTML, PDF, and XML) Thereof 502 with geography defined and 0 with unknown origin.
Country # Views %
  • 1
1
 
 
 
 
Latest update: 17 Dec 2024
Download
Short summary
In many ways, the surface of the planet Mars is similar to that of Earth. However, Mars' lower gravity has an effect on the sedimentation and transport of sedimentary material and the texture of sedimentary rocks. Using specific experimental equipment to measure settling velocity aboard a parabolic flight, it was possible to observe how sediments settled at Martian gravity. These experiments serve as analogues for surface processes on Mars.