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Plume-surface interactions: a review of experimental work

Plume-surface interactions: a review of experimental work
Plume-surface interactions: a review of experimental work
During the final metres of the powered descent of Apollo 11, astronauts Neil Armstrong and Buzz Aldrin lost sight of the lunar surface. As the retro-rockets fired towards the lunar dust – or regolith – to decelerate the spacecraft, soil erosion occurred and the blowing dust led to severe visual obstruction. After a successful landing, the presence of dust continued to impact the mission with adverse effects including respiratory problems and difficulty in performing tasks due to clogging of mechanisms, amongst others. As these effects were observed in subsequent missions, the “dust problem” was identified as one of the main challenges of extra-terrestrial surface exploration. In this work, the focus is placed on dust dispersal, which arises from the interaction between a rocket exhaust flow – or plume – and the planetary surface. Termed plume-surface interactions (PSI), this field of study encompasses the complex phenomena caused by the erosion and lofting of regolith particles. These particles, which are ejected at high-speeds, can lead to damage to the spacecraft hardware or a reduction in functionality. Moreover, plumes redirected back towards the landers can induce destabilising loads prior to touch-down, risking the safety of the landing. To achieve a sustained presence on the Moon, as planned by NASA’s Artemis programme, it is essential that PSI are well understood and mitigating measures are put in place, particularly if spacecraft are to land in the vicinity of lunar habitats. Although experimental work began in the 1960s and mission PSI were first recorded in 1969, a fundamental understanding of this phenomena has not yet been achieved. In this paper, a compendium of experimental PSI is presented, identifying the main challenges associated with the design of tests, stating important lessons learnt and the shortcomings of available experimental data and findings. Lastly, recommendations for future experimental work are presented.
0094-5765
892-912
Jimenez Cuesta, Claudia
3244c22a-8bbf-4c24-9d39-d0bd341c2e51
Davis, Jack
4f15584d-66ee-4d86-b6ff-194afd7b38eb
Worrall, Kevin
93a21d52-c9b5-4097-94ad-225ab03b6503
Cammarano, Andrea
c0c85f55-3dfc-4b97-9b79-e2554406a12b
Zare-Behtash, Hossein
74be9b97-cb09-49c6-9f75-7ec58c0dd16c
Jimenez Cuesta, Claudia
3244c22a-8bbf-4c24-9d39-d0bd341c2e51
Davis, Jack
4f15584d-66ee-4d86-b6ff-194afd7b38eb
Worrall, Kevin
93a21d52-c9b5-4097-94ad-225ab03b6503
Cammarano, Andrea
c0c85f55-3dfc-4b97-9b79-e2554406a12b
Zare-Behtash, Hossein
74be9b97-cb09-49c6-9f75-7ec58c0dd16c

Jimenez Cuesta, Claudia, Davis, Jack, Worrall, Kevin, Cammarano, Andrea and Zare-Behtash, Hossein (2024) Plume-surface interactions: a review of experimental work. Acta Astronautica, 226 (Pt. 1), 892-912. (doi:10.1016/j.actaastro.2024.09.021).

Record type: Review

Abstract

During the final metres of the powered descent of Apollo 11, astronauts Neil Armstrong and Buzz Aldrin lost sight of the lunar surface. As the retro-rockets fired towards the lunar dust – or regolith – to decelerate the spacecraft, soil erosion occurred and the blowing dust led to severe visual obstruction. After a successful landing, the presence of dust continued to impact the mission with adverse effects including respiratory problems and difficulty in performing tasks due to clogging of mechanisms, amongst others. As these effects were observed in subsequent missions, the “dust problem” was identified as one of the main challenges of extra-terrestrial surface exploration. In this work, the focus is placed on dust dispersal, which arises from the interaction between a rocket exhaust flow – or plume – and the planetary surface. Termed plume-surface interactions (PSI), this field of study encompasses the complex phenomena caused by the erosion and lofting of regolith particles. These particles, which are ejected at high-speeds, can lead to damage to the spacecraft hardware or a reduction in functionality. Moreover, plumes redirected back towards the landers can induce destabilising loads prior to touch-down, risking the safety of the landing. To achieve a sustained presence on the Moon, as planned by NASA’s Artemis programme, it is essential that PSI are well understood and mitigating measures are put in place, particularly if spacecraft are to land in the vicinity of lunar habitats. Although experimental work began in the 1960s and mission PSI were first recorded in 1969, a fundamental understanding of this phenomena has not yet been achieved. In this paper, a compendium of experimental PSI is presented, identifying the main challenges associated with the design of tests, stating important lessons learnt and the shortcomings of available experimental data and findings. Lastly, recommendations for future experimental work are presented.

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Accepted/In Press date: 7 September 2024
e-pub ahead of print date: 2 October 2024
Published date: 19 November 2024

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Local EPrints ID: 502554
URI: http://eprints.soton.ac.uk/id/eprint/502554
ISSN: 0094-5765
PURE UUID: e8fb3d7a-7ffa-42ec-937b-33770ce08bd3
ORCID for Andrea Cammarano: ORCID iD orcid.org/0000-0002-8222-8150
ORCID for Hossein Zare-Behtash: ORCID iD orcid.org/0000-0002-4769-4076

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Date deposited: 01 Jul 2025 16:30
Last modified: 22 Aug 2025 02:43

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Contributors

Author: Claudia Jimenez Cuesta
Author: Jack Davis
Author: Kevin Worrall
Author: Andrea Cammarano ORCID iD
Author: Hossein Zare-Behtash ORCID iD

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