Experiments on Settling of Granular and Cohesive Material in Low Gravity
Pith reviewed 2026-06-29 00:41 UTC · model grok-4.3
The pith
Granular materials pack less densely in lower gravity, with fine basalt most sensitive.
A machine-rendered reading of the paper's core claim, the machinery that carries it, and where it could break.
Core claim
When three granular samples settle under artificially reduced gravities, fine basalt (1-200 μm) reaches up to 19.6 % higher volume at 250 mm/s², coarse basalt (2-5 mm) up to 12.2 % higher at 150 mm/s², and glass beads (750-1000 μm) up to 4.25 % higher at 250 mm/s², compared with higher-gravity runs; the authors conclude that volume increase is not determined by particle size alone but also by roughness and uniformity, and that cohesive forces become comparatively important in low gravity.
What carries the argument
A high-precision linear stage inside the drop tower that accelerates the sample containers to produce constant reduced gravity during settling.
If this is right
- Packing density of granular material decreases as ambient gravity decreases.
- Fine, rough particles exhibit the largest density drop because cohesive forces matter more relative to weight.
- Change in settled volume depends on particle size, surface roughness, and size uniformity together.
- The measured volume changes supply calibration points for simulations of regolith on asteroids and small bodies.
Where Pith is reading between the lines
- Models of asteroid surface evolution or spacecraft landing may need to treat packing density as gravity-dependent rather than fixed.
- The same cohesion-driven loosening could affect how dust and small grains aggregate during planet formation at low relative velocities.
- Repeating the tests with a wider range of particle shapes or with added electrostatic charging would test how far the observed trends generalize.
Load-bearing premise
The stage motion creates the same settling dynamics that would occur under steady natural low gravity, without added inertial forces, vibrations, or container effects.
What would settle it
Packing-density measurements made on an asteroid surface or in a true constant low-g environment that show no gravity dependence or the opposite trend from the laboratory volume increases.
Figures
read the original abstract
The regolith of rocky bodies, such as planets or asteroids, generally settles under gravity conditions different from those of Earth. The behavior of granular material is not easily scalable for different gravities. To predict these highly complex systems where cohesive inter particle forces can be comparable to gravitational forces, we need simulations and experiments. We did experiments on settling of three different granular samples in varying reduced gravities and examined their packing densities. We used a high precision linear stage to artificially induce reduced gravities inside the zero $g$ environment provided by the ZARM drop tower and observe the settling of our samples. The three samples were fine basalt with particle diameters of $1\text{-}200\,\mu$m, coarse basalt with $2\text{-}5\,$mm and glass beads with $750\text{-}1000\,\mu$m. The artificial gravities were $150,\,250,\,500,\,750$ and $1000\,$mm/s$^2$ and therefore ranged from large asteroid gravity to almost moon gravity. We saw the granular samples have higher volumes in lower gravities and therefore lower packing densities, we also saw the fine basalt be the most sensitive to changes in gravity, up to $+19.6\,\%$ in volume for $250\,$mm/s$^2$, followed by the coarse basalt particles, up to $+12.2\,\%$ for $150\,$mm/s$^2$ and the glass beads packing density being the least sensitive to changes in gravity, up to $+4.25\,\%$ for $250\,$mm/s$^2$. With these experiments we show change in volume is not solely dependent of particle size but also roughness and uniformity, we provide real life experimental data to validate theoretical works and highlight the role of cohesive forces in low gravity environments.
Editorial analysis
A structured set of objections, weighed in public.
Referee Report
Summary. The manuscript reports drop-tower experiments on the settling of three granular samples (fine basalt 1-200 μm, coarse basalt 2-5 mm, glass beads 750-1000 μm) under artificially reduced gravities of 150, 250, 500, 750 and 1000 mm/s² produced by a high-precision linear stage inside the ZARM zero-g facility. The central observational claim is that settled volumes increase (packing densities decrease) at lower g, with material-dependent sensitivities: fine basalt up to +19.6 % at 250 mm/s², coarse basalt up to +12.2 % at 150 mm/s², and glass beads up to +4.25 % at 250 mm/s². The authors conclude that volume change depends on particle size, roughness and uniformity and that cohesive forces play an increasing role at low g.
Significance. If the acceleration field is shown to be free of significant transients or vibrations and the volume measurements are repeatable, the data would supply useful empirical benchmarks for discrete-element models of regolith on asteroids and other small bodies where cohesion becomes comparable to gravity. The material-specific trends and the use of a drop-tower linear-stage method constitute a concrete experimental contribution to planetary-science instrumentation literature.
major comments (3)
- [Methods/Results] Methods/Results: The reported volume increases (e.g., +19.6 % for fine basalt) are given without error bars, standard deviations, number of repetitions, or any description of the volume-measurement procedure (optical, mass-based, or otherwise), preventing assessment of whether the material-dependent differences exceed experimental uncertainty.
- [Methods] Methods: No quantitative characterization is supplied of the acceleration time-history delivered by the linear stage (uniformity during the settling interval, start-up transients, residual vibration spectrum, or container-wall normal forces), which is required to substantiate that the observed packing densities arise from the intended constant low-g body force rather than apparatus-specific inertial or vibrational effects.
- [Discussion] Discussion: The attribution of sensitivity differences to 'roughness and uniformity' in addition to size rests on the three samples differing simultaneously in multiple properties; without additional control experiments or particle-property quantification, this causal claim is not yet load-bearing.
minor comments (2)
- [Abstract] Abstract: 'dependent of particle size' should read 'dependent on particle size'.
- [Methods] Notation: Gravitational accelerations are consistently given in mm/s², but the manuscript should state whether these values are the commanded stage accelerations or measured values.
Simulated Author's Rebuttal
We thank the referee for the constructive comments on our manuscript. We address each major comment point by point below, indicating the revisions we will make.
read point-by-point responses
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Referee: [Methods/Results] The reported volume increases (e.g., +19.6 % for fine basalt) are given without error bars, standard deviations, number of repetitions, or any description of the volume-measurement procedure (optical, mass-based, or otherwise), preventing assessment of whether the material-dependent differences exceed experimental uncertainty.
Authors: We agree that these statistical and procedural details are essential. The volumes were determined optically from the height of the settled material in a transparent cylindrical container using calibrated image analysis. Five independent repetitions were performed for each sample-gravity combination. In the revised manuscript we will add a dedicated methods subsection describing the optical procedure, report the repetition count, and include error bars derived from the standard deviation across repetitions. revision: yes
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Referee: [Methods] No quantitative characterization is supplied of the acceleration time-history delivered by the linear stage (uniformity during the settling interval, start-up transients, residual vibration spectrum, or container-wall normal forces), which is required to substantiate that the observed packing densities arise from the intended constant low-g body force rather than apparatus-specific inertial or vibrational effects.
Authors: We acknowledge that quantitative verification of the acceleration field is required. Accelerometer data were acquired during the runs. The revised methods section will include time-series plots and quantitative metrics (uniformity within ±5 % after ramp-up, peak transient acceleration, and RMS vibration amplitude) demonstrating that the settling phase occurred under the commanded constant low-g with negligible residual motion. revision: yes
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Referee: [Discussion] The attribution of sensitivity differences to 'roughness and uniformity' in addition to size rests on the three samples differing simultaneously in multiple properties; without additional control experiments or particle-property quantification, this causal claim is not yet load-bearing.
Authors: The referee correctly notes that the three samples vary in several properties simultaneously. We will revise the discussion to state that the observed material-dependent volume changes are consistent with the combined influence of particle size, surface roughness, and size uniformity, supported by the provided particle-size distributions and qualitative surface descriptions. We will add quantitative particle characterization (SEM-derived roughness estimates and full size-distribution histograms) while explicitly acknowledging that isolating individual factors would require additional controlled experiments not performed here. revision: partial
Circularity Check
Purely experimental report; no derivations, equations, or fitted predictions present.
full rationale
The manuscript reports direct experimental measurements of packing volumes for three granular samples under controlled low accelerations produced by a linear stage in a drop tower. All reported results (volume increases of +4.25% to +19.6% at specific accelerations) are presented as observed outcomes without any claimed theoretical derivation, model fitting, or predictive equations. No self-citations of prior uniqueness theorems, ansatzes, or renamings of known results appear. The work contains no load-bearing steps that reduce to their own inputs by construction, satisfying the default expectation of no circularity for an observational study.
Axiom & Free-Parameter Ledger
Reference graph
Works this paper leans on
-
[1]
Arsenovi´ c, D., Vrhovac, S. B., Jakˇ si´ c, Z. M., Budinski-Petkovi´ c, L., & Beli´ c, A. 2006, Physical Review E, 74, 061302, doi: 10.1103/PhysRevE.74.061302
-
[2]
2023, Handbook of Space Resources, 1st edn
Badescu, V., Zacny, K., & Bar-Cohen, Y., eds. 2023, Handbook of Space Resources, 1st edn. (Cham: Springer International Publishing and Imprint Springer), doi: 10.1007/978-3-030-97913-3 8
-
[3]
Becker, T., Onyeagusi, F. C., Teiser, J., et al. 2024, The Planetary Science Journal, 5, 277, doi: 10.3847/PSJ/ad9396
-
[4]
2015, in 2015 IEEE Aerospace Conference (IEEE), 1–14, doi: 10.1109/AERO.2015.7118989
Beshore, E., Sutter, B., Mink, R., et al. 2015, in 2015 IEEE Aerospace Conference (IEEE), 1–14, doi: 10.1109/AERO.2015.7118989
-
[5]
2022, Planetary and Space Science, 220, 105533, doi: 10.1016/j.pss.2022.105533
Brisset, J., S´ anchez, P., Cox, C., et al. 2022, Planetary and Space Science, 220, 105533, doi: 10.1016/j.pss.2022.105533
-
[6]
2020, Journal of Electrostatics, 107, 103475, doi: https://doi.org/10.1016/j.elstat.2020.103475
Carter, D., & Hartzell, C. 2020, Journal of Electrostatics, 107, 103475, doi: https://doi.org/10.1016/j.elstat.2020.103475
-
[7]
Carter, D., & Hartzell, C. M. 2019, The Review of scientific instruments, 90, 125105, doi: 10.1063/1.5111983
-
[8]
2005, Advances in Physics, 54, 263, doi: 10.1080/17461390500402657
Castellanos, A. 2005, Advances in Physics, 54, 263, doi: 10.1080/17461390500402657
-
[9]
2009, European Journal of Soil Science, 60, 1078, doi: 10.1111/j.1365-2389.2009.01173.x
Certini, G., Scalenghe, R., & Amundson, R. 2009, European Journal of Soil Science, 60, 1078, doi: 10.1111/j.1365-2389.2009.01173.x
-
[10]
Chapelle, P., Christakis, N., Wang, J., et al. 2005, Proceedings of the Institution of Mechanical Engineers, Part E: Journal of Process Mechanical Engineering, 219, 43, doi: 10.1243/095440805X7044 Chemie.de – Lexikon. 2026, Gesteinsdichte — Dichte ausgew¨ ahlter Gesteine (z. B. Basalt). https://www.chemie.de/lexikon/Gesteinsdichte.html
-
[11]
2013, Journal of Loss Prevention in the Process Industries, 26, 255, doi: 10.1016/j.jlp.2012.11.007
Yamaguma, M. 2013, Journal of Loss Prevention in the Process Industries, 26, 255, doi: 10.1016/j.jlp.2012.11.007
-
[12]
Connolly, J., & Carrier, W. D. 2023, in 2023 IEEE Aerospace Conference, 1–9, doi: 10.1109/AERO55745.2023.10115961
-
[13]
2005, Rheometry of Pastes, Suspensions, and Granular Materials: Applications in Industry and Environment (John Wiley & Sons)
Coussot, P. 2005, Rheometry of Pastes, Suspensions, and Granular Materials: Applications in Industry and Environment (John Wiley & Sons)
2005
-
[14]
Cundall, P. A., & Strack, O. D. L. 1979, G´ eotechnique, 29, 47, doi: 10.1680/geot.1979.29.1.47
-
[15]
DellaGiustina, D. N., Nolan, M. C., Polit, A. T., et al. 2023, The Planetary Science Journal, 4, 198, doi: 10.3847/PSJ/acf75e
-
[16]
Drescher, A., Waters, A. J., & Rhoades, C. A. 1995, Powder Technology, 84, 177, doi: 10.1016/0032-5910(95)02982-8
-
[17]
Elekes, F., & Parteli, E. J. R. 2021, Proceedings of the National Academy of Sciences of the United States of America, 118, e2107965118, doi: 10.1073/pnas.2107965118
-
[18]
2023, npj Microgravity, 9, 50, doi: 10.1038/s41526-023-00298-9
Vincent-Bonnieu, S. 2023, npj Microgravity, 9, 50, doi: 10.1038/s41526-023-00298-9
-
[19]
2026, Acta Astronautica, 241, 314, doi: 10.1016/j.actaastro.2025.12.062
Fu, J., Luo, H., Li, Y., et al. 2026, Acta Astronautica, 241, 314, doi: 10.1016/j.actaastro.2025.12.062
-
[20]
Gaida, O., D’Angelo, O., & Kollmer, J. E. 2025, To Flow or Not To Flow? The granular Bond number to predict clogging in low gravity. https://arxiv.org/pdf/2506.18771
Pith/arXiv arXiv 2025
-
[21]
2017, Microgravity Science and Technology, 29, 403, doi: 10.1007/s12217-017-9560-y
Gierse, A., Kaczmarczik, U., Greif, A., et al. 2017, Microgravity Science and Technology, 29, 403, doi: 10.1007/s12217-017-9560-y
-
[22]
2023, PhRvL, 130, 098202, doi: 10.1103/PhysRevLett.130.098202
Grosjean, G., & Waitukaitis, S. 2023, PhRvL, 130, 098202, doi: 10.1103/PhysRevLett.130.098202
-
[23]
2020, Journal of Geophysical Research: Planets, 125, e2020JE006519, doi: 10.1029/2020JE006519
Grott, M., Biele, J., Michel, P., et al. 2020, Journal of Geophysical Research: Planets, 125, e2020JE006519, doi: 10.1029/2020JE006519
-
[24]
2018, Soft matter, 14, 4987
Haeberle, J., Schella, A., Sperl, M., Schr¨ oter, M., & Born, P. 2018, Soft matter, 14, 4987
2018
-
[25]
He, Q., Liu, Q., Yang, L., & Wang, B. 2025, in Proceedings of the 2025 International Conference on Transportation Information and Safety (ICTIS) (IEEE), 1093–1099, doi: 10.1109/ICTIS68762.2025.11214790 Hositrad Holland B.V. 2026, Glass-V F. Nipple Duran Glass/Pyrex KF16 (Artikelnummer KS16/GP), https://www.hositrad.com/winkel/product/details/ ?artdetail=K...
-
[26]
Jenike, A. W. 1964, Journal of Applied Mechanics, 31, 5, doi: 10.1115/1.3629571
-
[27]
Joeris, K., Keulen, M., & Kollmer, J. E. 2025, The Review of scientific instruments, 96, doi: 10.1063/5.0233405
-
[28]
Johnson, K. L., Kendall, K., & Roberts, A. D. 1971, Royal Society of London Proceedings Series A, 324, 301, doi: 10.1098/rspa.1971.0141
-
[29]
Jungmann, F., Onyeagusi, F. C., Teiser, J., & Wurm, G. 2022, Journal of Electrostatics, 117, 103705, doi: https://doi.org/10.1016/j.elstat.2022.103705
-
[30]
Keulen, M., Oehme, F., Wurm, G., & Kollmer, J. E. 2025, The Planetary Science Journal, 6, 243, doi: 10.3847/PSJ/ae0e0f
-
[31]
2015, The Astrophysical Journal, 812, 67, doi: 10.1088/0004-637X/812/1/67
Kimura, H., Wada, K., Senshu, H., & Kobayashi, H. 2015, The Astrophysical Journal, 812, 67, doi: 10.1088/0004-637X/812/1/67
-
[32]
Kunnath, K., Chen, L., Zheng, K., & Dav´ e, R. N. 2021, Powder Technology, 377, 709, doi: 10.1016/j.powtec.2020.09.037
-
[33]
Lacks, D. J., & Sankaran, R. M. 2011, Journal of Physics D Applied Physics, 44, 453001, doi: 10.1088/0022-3727/44/45/453001
-
[34]
Lacks, D. J., & Shinbrot, T. 2019, Nature Reviews Chemistry, 3, 465, doi: https://doi.org/10.1038/s41570-019-0115-1 settling in low gravity9
-
[35]
Glasser, B. J. 2009, Powder Technology, 195, 158, doi: 10.1016/j.powtec.2009.05.026
-
[36]
P., Muruganandam, S., Missaoui, A., et al
Madden, I. P., Muruganandam, S., Missaoui, A., et al. 2025, npj Microgravity, 11, 69, doi: 10.1038/s41526-025-00501-z
-
[37]
Magri, C., Consolmagno, G. J., Ostro, S. J., Benner, L. A. M., & Beeney, B. R. 2001, Meteoritics & Planetary Science, 36, 1697, doi: 10.1111/j.1945-5100.2001.tb01857.x
-
[38]
2002, Icarus, 155, 3, doi: https://doi.org/10.1006/icar.2001.6753
Miller, J., Konopliv, A., Antreasian, P., et al. 2002, Icarus, 155, 3, doi: https://doi.org/10.1006/icar.2001.6753
-
[39]
Mueller, R. P. 2023, A Review of Extra-Terrestrial Regolith Excavation Concepts and Prototypes (American Society of Civil Engineers), doi: 10.1061/9780784484470.030
-
[40]
2018, Icarus, 306, 25 , doi: https://doi.org/10.1016/j.icarus.2018.01.007
Musiolik, G., Kruss, M., Demirci, T., et al. 2018, Icarus, 306, 25 , doi: https://doi.org/10.1016/j.icarus.2018.01.007
-
[41]
2017, Space Science Reviews, 208, 107, doi: 10.1007/s11214-016-0289-5
Okazaki, R., Sawada, H., Yamanouchi, S., et al. 2017, Space Science Reviews, 208, 107, doi: 10.1007/s11214-016-0289-5
-
[42]
2023, npj Microgravity, 9, 61, doi: 10.1038/s41526-023-00308-w
Ozaki, S., Ishigami, G., Otsuki, M., et al. 2023, npj Microgravity, 9, 61, doi: 10.1038/s41526-023-00308-w
-
[43]
Parteli, E. J. R., Schmidt, J., Bl¨ umel, C., et al. 2014, Scientific reports, 4, 6227, doi: 10.1038/srep06227
-
[44]
Persson, B. N. J., & Biele, J. 2022, Tribology Letters, 70, 34, doi: 10.1007/s11249-022-01570-x
-
[45]
Persson, B. N. J., & Mate, C. M. 2024, The European Physical Journal B, 97, 46, doi: 10.1140/epjb/s10051-024-00680-w
-
[46]
2016, Microgravity Science and Technology, 28, 587, doi: 10.1007/s12217-016-9515-8
Pletser, V., Rouquette, S., Friedrich, U., et al. 2016, Microgravity Science and Technology, 28, 587, doi: 10.1007/s12217-016-9515-8
-
[47]
Puumala, M. M., Sivula, O., & Lehto, K. 2023, Space Policy, 66, 101590, doi: 10.1016/j.spacepol.2023.101590 Raymus. 1997, Handling of bulk solids and packaging of solids and liquids (McGraw-Hill). https://schneider.cheme.cmu.edu/files/perry’s% 20chemical%20engineers’%20handbook%207th% 20edition/21.%20handling%20of%20bulk%20solids% 20and%20packaging%20of%2...
-
[48]
Sarkar, S., Cho, J., & Chaudhuri, B. 2012, Chemical Engineering and Processing: Process Intensification, 62, 168, doi: 10.1016/j.cep.2012.07.009
-
[49]
Scheeres, D. J., Hartzell, C. M., S´ anchez, P., & Swift, M. 2010, Icarus, 210, 968, doi: 10.1016/j.icarus.2010.07.009 Schr¨ apler, R., Blum, J., von Borstel, I., & G¨ uttler, C. 2015, Icarus, 257, 33, doi: 10.1016/j.icarus.2015.04.033
-
[50]
2010, Microgravity Science and Technology, 22, 539, doi: 10.1007/s12217-010-9210-0
Selig, H., Dittus, H., & L¨ ammerzahl, C. 2010, Microgravity Science and Technology, 22, 539, doi: 10.1007/s12217-010-9210-0
-
[51]
Waitukaitis, S. 2025, Proceedings of the National Academy of Sciences of the United States of America, 122, e2516865122, doi: 10.1073/pnas.2516865122 S´ anchez, P., & Scheeres, D. J. 2014, Meteoritics & Planetary Science, 49, 788, doi: https://doi.org/10.1111/maps.12293
-
[52]
2021, The Astrophysical Journal Letters, 908, L22, doi: 10.3847/2041-8213/abddc2
Teiser, J., Kruss, M., Jungmann, F., & Wurm, G. 2021, The Astrophysical Journal Letters, 908, L22, doi: 10.3847/2041-8213/abddc2
-
[53]
2025, Nature Astronomy, doi: 10.1038/s41550-024-02470-x
Teiser, J., Penner, J., Joeris, K., et al. 2025, Nature Astronomy, doi: 10.1038/s41550-024-02470-x
-
[54]
Thomas, P. C., Parker, J. W., & McFadden, L. A. 2005, Nature, 437, 224, doi: 10.1038/nature03938
-
[55]
Vernazza, P., Delbo, M., King, P., et al. 2012, Icarus, 221, 1162, doi: https://doi.org/10.1016/j.icarus.2012.04.003 von Kampen, P., Kaczmarczik, U., & Rath, H. J. 2006, Acta Astronautica, 59, 278, doi: 10.1016/j.actaastro.2006.02.041
-
[56]
Jaeger, H. M. 2014, Physical Review Letters, 112, 218001, doi: 10.1103/PhysRevLett.112.218001
-
[57]
Walker, D. M. 1966, Chemical Engineering Science, 21, 975, doi: 10.1016/0009-2509(66)85095-9 Whitehouse Scientific Ltd. 2005, Glass Microsphere Technical Specification (Soda-Lime Glass), Tech. rep., Whitehouse Scientific Ltd. https://cdn.prod.website-files.com/ 5ee25faf443526bc0db894a5/5f50c5c4b57c089273d216ba technical-specification-for-sodalime-glass.pdf
-
[58]
Wilkinson, R. A., Behringer, R. P., Jenkins, J. T., & Louge, M. Y. 2005, AIP Conference Proceedings, 746, 1216, doi: 10.1063/1.1867248 ZARM. 2025, Bremen Drop Tower - Payload User’s Guide (ZARM FAB mbH, University of Bremen). https: //www.zarm.uni-bremen.de/fileadmin/user upload/ Research/Testing and Facilities/ZARM BDT PUG.pdf
-
[59]
2019, Nature Astronomy, 3, 487, doi: 10.1038/s41550-019-0804-1
Zhang, T., Xu, K., Yao, Z., et al. 2019, Nature Astronomy, 3, 487, doi: 10.1038/s41550-019-0804-1
-
[60]
2020, in Encyclopedia of Continuum Mechanics (Springer), 1–32, doi: 10.1007/978-3-642-27737-5 746-1
Zuriguel, I., & Garcimart´ ın, A. 2020, in Encyclopedia of Continuum Mechanics (Springer), 1–32, doi: 10.1007/978-3-642-27737-5 746-1
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