Testing
Verification methods, facilities, and simulants used to qualify robotic hardware for environments that cannot be reproduced in full on Earth. Each page covers what the method reproduces, what it does not, the fidelity limits that have caused flight surprises, and the facilities where the work is done.
What ground testing has to do
Section titled “What ground testing has to do”A planetary robot is qualified on the ground against vacuum, temperature extremes, reduced gravity, radiation, abrasive and cohesive dust, and a soil whose mechanical properties are known only from a few sites. No single rig reproduces more than a subset. Combined lunar-environment testing is a design problem in its own right, because the environments constrain each other: dusty vacuum operation changes how a chamber is cleaned, pumped and accelerated [7]. The test program for a flight rover is therefore a set of partial simulations, each chosen for the failure it can expose, and the engineering question is which residual risk each leaves behind.
Families of method
Section titled “Families of method”Thermal vacuum and solar simulation. The oldest family. The measured spectral mismatch of the JPL 25-ft space simulator showed that an absorptance computed against the solar spectrum is wrong for any coating with a spectrally selective response [6]. Mars 2020 system thermal vacuum and thermal model correlation are covered on thermal vacuum testing.
Dust and abrasion. Apollo is the baseline: the catalog of dust effects on extravehicular systems traces to primary mission documents [11]. Ground work since then splits by what is measured. Three-body abrasion of common spacecraft materials against lunar simulants gives wear volumes under one controlled dry configuration [12], and abrasion of stainless steel rotating parts against Moon and Mars simulants joins simulant characterization to mechanism life [13]. Abrasion at lunar temperature extremes, which room-ambient tests do not cover, has been measured on Ti-hBN coatings [14]. Coating down-selection for dust tolerance has covered adhesion and thermal shock as well as wear [15]. The dust sealing architecture of a flight lunar rover is published with materials, compressions and labyrinth gaps [16]. Dust adhesion is the case where ambient and vacuum disagree: brushing worked in air and failed in a simulated lunar environment, which matches the Apollo outcome [10], and the requirements for the bell jar that exposed this are documented [9]. Triboelectric charging of candidate insulators has been measured on the insulator rather than the grain [43]. Details are on dust testing.
Regolith simulants. A simulant is a chosen subset of properties of a real soil. Its producer lists what it does not simulate [20]. A selection guide scores multiple lunar simulants on a common basis [17]. A simulant reformulated for operator safety rather than fidelity has published exposure measurements and a cone index gradient [18], and size-fraction-resolved geotechnical data separates flow behavior by grain size [19]. The reference values come from Apollo and Surveyor measurements [23][24], and returned Chang’e-6 farside soil is the one held measurement on real returned material that shows strongly cohesive behavior [22]. Asteroid simulants are at a proposal stage, organized by spectral class [21]. See regolith simulants.
Radiation and electrical environment. Single event testing follows a practice that originates in a heavy-ion guideline: delid the part, hold vacuum, measure flux and uniformity independently of the accelerator, and tilt the part to vary effective LET [25]. For total dose the early hardness-assurance survey found no pre-irradiation electrical screen correlating with radiation response [26]. Electromagnetic compatibility on Mars 2020 used a priority rubric to cut the source-victim pair list and measured the cost of removing shields from twisted-pair drive lines [28]. See radiation testing.
Vibration and subsystem verification. The fatigue-equivalence trade between level and duration and the tolerance bands on random vibration are laid out in a 1971 text that later standards state without justification [27]. A landing radar was tested with a simulator that generates the return per pulse from a terrain model, plus delay-line end-to-end checks [29]. Verification of reused robotic hardware, the practical problem behind heritage claims, is documented for the SPDM [33].
Mobility, sampling and field analog. Best practices for planetary roving vehicle mobility testing connect each lunar terrain vehicle requirement to a test method and a named gap [31]. The Mars 2020 sampling qualification campaign recorded cores, abrasions, seals and bits consumed [30]. A simulated search-for-life mission with automated drilling quantified operator command cycles [42]. Reduced gravity is covered on reduced gravity testing and facility envelopes on the facilities pages; a lunar test bed of basaltic cinders over coarser material is described only by a promotional web page [41].
Simulation and analog media. Underwater testing of space robotics is validated by time scaling the plan so both platforms share a disturbance robustness degree [32]. A framework of key performance indicators for multi-robot lunar mapping defines efficiency, workload and autonomy measures for field trials [34]. See simulation and digital twins.
What has been checked against flight
Section titled “What has been checked against flight”Ground qualification is checked against the flight it was predicting only rarely, and the matched cases are specific rather than general. Curiosity’s accumulated flight thermal cycles have been rainflow counted against the accelerated cycling test run on the same board design [1]. The MSL generator’s output was measured against its pre-flight prediction at three points before launch and once on the surface [2]. Mast pointing accuracy achieved on Mars was carried into the Mars 2020 requirement as an operational figure with outliers rather than as the ground expectation it replaced [3].
Other comparisons are of a different kind: a design lifetime against what flew. The Mars Exploration Rover 90 sol mission expectation was wrong for solar array dust because accumulation was slower and cleaning more frequent than predicted [36]. Spirit’s end of mission report gives whole-of-mission actuator revolution counts against tested life [35], Opportunity’s loss to a dust storm is documented with the tau and energy trend of its final sols [37], Ingenuity operated outside its design envelope through a Martian winter [38], and InSight arm activities tie commanded actions to measured outcomes with testbed force calibration [39]. Terrestrial dust-emission climatology is the contextual reference for how dust events are forced and timed [40].
Facility capability parameters have almost no counterpart of that kind. Chamber base pressure, bed density and preparation state, slope, illumination and gravity offload fidelity are published as what a rig delivers to an article standing on or inside it, and none of them is re-measured on the hardware once it is working in the place the rig stood in for. A facility envelope is therefore a capability statement and not an error bar against flight, and most stated fidelity limits are arguments from physics rather than measured discrepancies. The one lunar analog facility held with a full geotechnical, abrasivity, mineralogical and chemical characterization of the material in its beds is LUNA [8].
Two thermal vacuum cases are the exception, and both are on flight vehicles. The Mars 2020 system thermal vacuum test concluded that a cruise thruster catalyst bed heater could stay on continuously from launch, which flight contradicted, because the chamber simulated no off-Sun angle flux [4]. Perseverance’s correlated thermal model inherited the 4 percent voltage loss of the ground support equipment cabling in place of the 9 percent of the flight flex cables, which produced preheat ramp rate errors above 5 C in flight until the cable loss was corrected [5]. Both are covered on thermal vacuum testing.
What is not established
Section titled “What is not established”No held source measures the offset between a chamber or bed result and the same quantity on the surface for the same hardware, so every facility fidelity statement above rests on physics arguments. Dust adhesion results from ambient air are known to mislead [9][10], but the size of the error in vacuum is reported only for the cases tested. Heritage verification of reused hardware is documented for one program [33]. Asteroid simulants are proposed and not yet validated against returned samples [21]. Lunar farside soil properties come from one returned sample set [22]. Mission-level comparisons of qualification life against flown life exist for a few vehicles [35][36][37] and do not cover the manipulator, drill or mast classes systematically.
References
- Berger, L. N. and Bell, C. (2020). Comparing Cumulative Flight Thermal Fatigue to Ground Test Results for Memory Components on the Mars Curiosity Rover
. AIAA Science and Technology Forum. Source
BibTeX
@inproceedings{berger2020comparing, title = {Comparing Cumulative Flight Thermal Fatigue to Ground Test Results for Memory Components on the Mars Curiosity Rover}, author = {Berger, Lindsey N and Bell, Charles}, booktitle = {AIAA Science and Technology Forum}, publisher = {JPL Open Repository}, year = {2020}, url = {https://dataverse.jpl.nasa.gov/dataset.xhtml?persistentId=hdl:2014/52311} } - Woerner, D., Moreno, V., Jones, L., Zimmerman, R. and Wood, E. (2012). The Mars Science Laboratory (MSL) MMRTG In-Flight : a power update
. Biennial ASCE Aerospace Division International Conference on Engineering, Science, Construction, and Operations in Challenging Environments. Source
BibTeX
@inproceedings{woerner2012mars, title = {The Mars Science Laboratory (MSL) MMRTG In-Flight : a power update}, author = {Woerner, David and Moreno, Victor and Jones, Loren and Zimmerman, Robert and Wood, Eric}, booktitle = {Biennial ASCE Aerospace Division International Conference on Engineering, Science, Construction, and Operations in Challenging Environments}, publisher = {JPL Open Repository}, year = {2012}, url = {https://dataverse.jpl.nasa.gov/dataset.xhtml?persistentId=hdl:2014/43175} } - Maurice, S., Wiens, R. C., Bernardi, P., Caïs, P., Robinson, S. H., Nelson, T., Gasnault, O., Reess, J.-M., Deleuze, M., Rull, F., Manrique, J. A., Abbaki, S., Anderson, R. B., André, Y., Angel, S., Arana, G., Battault, T., Beck, P., Benzerara, K., Bernard, S., Berthias, J.-P., Beyssac, O., Bonafous, M., Bousquet, B., Boutillier, M., Cadu, A., Castro, K., Chapron, F., Chide, B., Clark, K., Clavé, E., Clegg, S., Cloutis, E., Collin, C., Cordoba, E. C., Cousin, A., Dameury, J.-C., D'Anna, W., Daydou, Y., Debus, A., Deflores, L., Dehouck, E., Delapp, D., De Los Santos, G., Donny, C., Doressoundiram, A., Dromart, G., Dubois, B., Dufour, A., Dupieux, M., Egan, M., Ervin, J., Fabre, C., Fau, A., Fischer, W., Forni, O., Fouchet, T., Frydenvang, J., Gauffre, S., Gauthier, M., Gharakanian, V., Gilard, O., Gontijo, I., Gonzalez, R., Granena, D., Grotzinger, J., Hassen-Khodja, R., Heim, M., Hello, Y., Hervet, G., Humeau, O., Jacob, X., Jacquinod, S., Johnson, J. R., Kouach, D., Lacombe, G., Lanza, N., Lapauw, L., Laserna, J., Lasue, J., Le Deit, L., Le Mouélic, S., Le Comte, E., Lee, Q.-M., Legett, I. C., Leveille, R., Lewin, E., Leyrat, C., Lopez-Reyes, G., Lorenz, R., Lucero, B., Madariaga, J. M., Madsen, S., Madsen, M., Mangold, N., Manni, F., Mariscal, J.-F., Martinez-Frias, J., Mathieu, K., Mathon, R., McCabe, K. P., McConnochie, T., McLennan, S. M., Mekki, J., Melikechi, N., Meslin, P.-Y., Micheau, Y., Michel, Y., Michel, J. M., Mimoun, D., Misra, A., Montagnac, G., Montaron, C., Montmessin, F., Moros, J., Mousset, V., Morizet, Y., Murdoch, N., Newell, R. T., Newsom, H., Nguyen Tuong, N., Ollila, A. M., Orttner, G., Oudda, L., Pares, L., Parisot, J., Parot, Y., Pérez, R., Pheav, D., Picot, L., Pilleri, P., Pilorget, C., Pinet, P., Pont, G., Poulet, F., Quantin-Nataf, C., Quertier, B., Rambaud, D., Rapin, W., Romano, P., Roucayrol, L., Royer, C., Ruellan, M., Sandoval, B., Sautter, V., Schoppers, M. J., Schröder, S., Seran, H.-C., Sharma, S. K., Sobron, P., Sodki, M., Sournac, A., Sridhar, V., Standarovsky, D., Storms, S., Striebig, N., Tatat, M., Toplis, M., Torre-Fdez, I., Toulemont, N., Velasco, C., Veneranda, M., Venhaus, D., Virmontois, C., Viso, M., Willis, P. and Wong, K. (2021). The SuperCam Instrument Suite on the Mars 2020 Rover: Science Objectives and Mast-Unit Description
. Space Science Reviews, 47. Source
BibTeX
@article{maurice2021supercam, title = {The SuperCam Instrument Suite on the Mars 2020 Rover: Science Objectives and Mast-Unit Description}, author = {Maurice, Sylvestre and Wiens, Roger C. and Bernardi, Pernelle and Caïs, Phillippe and Robinson, Scott H. and Nelson, Tony and Gasnault, Olivier and Reess, Jean-Michel and Deleuze, Muriel and Rull, Fernando and Manrique, Jose Antonio and Abbaki, Sadok and Anderson, Ryan B. and André, Yves and Angel, S.M. and Arana, Gorka and Battault, T. and Beck, Pierre and Benzerara, Karim and Bernard, Sylvain and Berthias, J.-P. and Beyssac, Olivier and Bonafous, Marion and Bousquet, Bruno and Boutillier, M. and Cadu, A. and Castro, Kepa and Chapron, Frédéric and Chide, Baptiste and Clark, K. and Clavé, Elise and Clegg, S. and Cloutis, E. and Collin, Claude and Cordoba, Elizabeth C. and Cousin, A. and Dameury, J.-C. and D'Anna, W. and Daydou, Yves and Debus, Andre and Deflores, Lauren and Dehouck, Erwin and Delapp, Dorothea and De Los Santos, Greg and Donny, C. and Doressoundiram, Alain and Dromart, Gilles and Dubois, Bruno and Dufour, A. and Dupieux, M. and Egan, Miles and Ervin, Joan and Fabre, C. and Fau, Amaury and Fischer, Woodward and Forni, Olivier and Fouchet, Thierry and Frydenvang, Jens and Gauffre, S. and Gauthier, M. and Gharakanian, V. and Gilard, Olivier and Gontijo, Ivair and Gonzalez, R. and Granena, D. and Grotzinger, J. and Hassen-Khodja, Rafik and Heim, M. and Hello, Y. and Hervet, G. and Humeau, Olivier and Jacob, Xavier and Jacquinod, Sophie and Johnson, Jeffrey R. and Kouach, Driss and Lacombe, G. and Lanza, Nina and Lapauw, Laurent and Laserna, Javier and Lasue, J. and Le Deit, Laetitia and Le Mouélic, Stéphane and Le Comte, E. and Lee, Qiu-Mei and Legett, IV, C. and Leveille, Richard and Lewin, Eric and Leyrat, C. and Lopez-Reyes, Guillermo and Lorenz, R. and Lucero, Briana and Madariaga, Juan Manuel and Madsen, Soren and Madsen, M. and Mangold, N. and Manni, F. and Mariscal, J.-F. and Martinez-Frias, Jesus and Mathieu, K. and Mathon, R. and McCabe, Kevin P. and McConnochie, T. and McLennan, Scott M. and Mekki, J. and Melikechi, Noureddine and Meslin, Pierre-Yves and Micheau, Y. and Michel, Y. and Michel, John M. and Mimoun, David and Misra, A. and Montagnac, Gilles and Montaron, Christophe and Montmessin, Franck and Moros, J. and Mousset, V. and Morizet, Y. and Murdoch, Naomi and Newell, Raymond T. and Newsom, Horton and Nguyen Tuong, N. and Ollila, Ann M. and Orttner, G. and Oudda, L. and Pares, Laurent and Parisot, Jérôme and Parot, Yann and Pérez, René and Pheav, D. and Picot, L. and Pilleri, Paolo and Pilorget, C. and Pinet, P. and Pont, Gabriel and Poulet, F. and Quantin-Nataf, Cathy and Quertier, Benjamin and Rambaud, D. and Rapin, William and Romano, P. and Roucayrol, L. and Royer, C. and Ruellan, M. and Sandoval, B.F. and Sautter, Violaine and Schoppers, Marcel J. and Schröder, S. and Seran, H.-C. and Sharma, Shiv K. and Sobron, Pablo and Sodki, M. and Sournac, A. and Sridhar, Vishnu and Standarovsky, D. and Storms, Steven and Striebig, Nicolas and Tatat, M. and Toplis, M. and Torre-Fdez, Imanol and Toulemont, N. and Velasco, C. and Veneranda, Marco and Venhaus, Dawn and Virmontois, C. and Viso, M. and Willis, P. and Wong, K.W.}, journal = {Space Science Reviews}, volume = {217}, number = {47}, year = {2021}, doi = {10.1007/s11214-021-00807-w}, abstract = {Abstract On the NASA 2020 rover mission to Jezero crater, the remote determination of the texture, mineralogy and chemistry of rocks is essential to quickly and thoroughly characterize an area and to optimize the selection of samples for return to Earth. As part of the Perseverance payload, SuperCam is a suite of five techniques that provide critical and complementary observations via Laser-Induced Breakdown Spectroscopy (LIBS), Time-Resolved Raman and Luminescence (TRR/L), visible and near-infrared spectroscopy (VISIR), high-resolution color imaging (RMI), and acoustic recording (MIC). SuperCam operates at remote distances, primarily 2–7 m, while providing data at sub-mm to mm scales. We report on SuperCam’s science objectives in the context of the Mars 2020 mission goals and ways the different techniques can address these questions. The instrument is made up of three separate subsystems: the Mast Unit is designed and built in France; the Body Unit is provided by the United States; the calibration target holder is contributed by Spain, and the targets themselves by the entire science team. This publication focuses on the design, development, and tests of the Mast Unit; companion papers describe the other units. The goal of this work is to provide an understanding of the technical choices made, the constraints that were imposed, and ultimately the validated performance of the flight model as it leaves Earth, and it will serve as the foundation for Mars operations and future processing of the data.} } - Miller, J. R., Singh, K., Reilly, S., Novak, K. and Lyra, J. (2022). Mars 2020 System Thermal Vacuum (STV) Test Implementation and Results
. Root. Source
BibTeX
@inproceedings{miller2022mars, title = {Mars 2020 System Thermal Vacuum (STV) Test Implementation and Results}, author = {Miller, Jennifer R. and Singh, Kaustabh and Reilly, Sean and Novak, Keith and Lyra, Jackie}, journal = {Root}, publisher = {JPL Open Repository}, year = {2022}, doi = {10.48577/jpl.uhmv4z}, abstract = {No abstract available.} } - Cassler, B., Nelson, E. J. and Kempenaar, J. G. (2023). Thermal Performance of the Perseverance Rover During Mars Surface Operations
. International Conference on Environmental Systems. Source
BibTeX
@inproceedings{cassler2023thermal, title = {Thermal Performance of the Perseverance Rover During Mars Surface Operations}, author = {Cassler, Bailey and Nelson, Emma J. and Kempenaar, Jason G.}, booktitle = {International Conference on Environmental Systems}, publisher = {JPL Open Repository}, year = {2023}, doi = {10.48577/jpl.uajl0t}, abstract = {On July 30, 2020, NASA launched the Perseverance Rover as part of the Mars 2020 (M2020) mission to Mars. On February 18, 2021, the rover landed on the surface of Mars in Jezero Crater at a latitude of 18.5°N. As of the writing of this paper, the rover has completed over 700 sols of surface operations, more than one full Martian year on the surface. Landing occurred during the Martian spring (Ls=5), and the rover has since operated through the summer, fall, and winter seasons. While the rover was originally designed to support a surface mission of 1003 sols, Perseverance has been integrated as part of the planned Mars Sample Return (MSR) Campaign to bring samples back from the surface of Mars to Earth for the first time. Understanding the thermal performance of the rover will be essential to ensuring the longevity of Perseverance to perform this mission. This paper discusses the thermal performance of the rover from landing to present day, including predicted versus actual thermal performance, nominal operations, incidents and anomalies, and long-term trending data that will be used to improve energy usage for activities requiring thermal support in the future.} } - Hickey, J. R. (1965). Evaluation of the Simulated Solar Spectrum in the JPL 25-ft Space Simulator
. Jet Propulsion Laboratory, California Institute of Technology, Technical Report 32-749. Source
BibTeX
@techreport{hickey1965evaluation, title = {Evaluation of the Simulated Solar Spectrum in the {JPL} 25-ft Space Simulator}, author = {Hickey, J. R.}, number = {Technical Report 32-749}, institution = {Jet Propulsion Laboratory, California Institute of Technology}, year = {1965}, url = {https://ntrs.nasa.gov/citations/19650025700}, abstract = {Simulation of solar spectrum in space simulator} } - Hayward, E. G., Nehls, M. K., Schneider, T. A., Lynn, P., Bertone, P. F. and Vaughn, J. A. (2023). Designing the PLANET Chamber for Lunar Environment Ground Testing
. AIAA SCITECH Forum, 20220018888. Source
BibTeX
@inproceedings{hayward2023designing, title = {Designing the PLANET Chamber for Lunar Environment Ground Testing}, author = {Hayward, Erin G. and Nehls, Mary K. and Schneider, Todd A. and Lynn, Patrick and Bertone, Peter F. and Vaughn, Jason A.}, booktitle = {AIAA SCITECH Forum}, number = {20220018888}, address = {National Harbor, Maryland}, year = {2023}, doi = {10.2514/6.2023-2468}, abstract = {View Video Presentation: https://doi.org/10.2514/6.2023-2468.vid The Planetary, Lunar, and Asteroid Natural Environments Testbed (PLANET) is a new 2m x 3m high-vacuum chamber facility currently being designed and built at NASA’s Marshall Space Flight Center. When completed, it will be one of the highest-fidelity space/surface environment simulation chambers in existence. Instrumented with equipment to produce charged particle radiation, full spectrum ultraviolet, low-density plasma, and thermal extremes, PLANET can be configured to recreate the most challenging space environments. Additionally, a large regolith bed and distribution system will expose hardware to lunar regolith simulants and dust. This paper will describe the process of designing and optimizing PLANET and discuss some common considerations for performing ground-based environmental testing for lunar exploration.} } - Zemeny, A., Sardisco, L., Quinteros, S., Mikesell, T. D., Pirrie, D., Rose, L., Cowley, A. and Manick, K. (2024). The LUNA Analog Facility testbeds (ESA, EAC): contemporary characterization work of highland and mare lunar regolith simulants
. Frontiers in Space Technologies. Source
BibTeX
@article{zemeny2024luna, title = {The {LUNA} Analog Facility testbeds ({ESA}, {EAC}): contemporary characterization work of highland and mare lunar regolith simulants}, author = {Zemeny, Aliz and Sardisco, Lorenzo and Quinteros, Susana and Mikesell, T. Dylan and Pirrie, Duncan and Rose, Laura and Cowley, Aidan and Manick, Kaushik}, journal = {Frontiers in Space Technologies}, volume = {5}, pages = {1510635}, year = {2024}, doi = {10.3389/frspt.2024.1510635}, abstract = {The Luna Analog Facility, a joint ESA-DLR endeavour, consists of three components and spans an area of 1,000 m 2 , providing testbeds of simulated lunar environments. The main sections within the facility are a large area filled with lunar mare regolith simulant resembling mare regions and a smaller, individual “Dust Chamber”. The latter replicates highland conditions and contains approximately 20 tons of material, specifically simulating the fine-particle lunar regolith portion up to 250 µm. The Dust Chamber serves as a platform for testing various technologies, such as mechanical tools, robotic operations, in-situ resource utilization activities, and astronaut attire, as well as different procedures including rover and astronaut tasks. This work represents the geotechnical, geochemical and mineralogical characterization of the Lumina Sustainable Materials Ltd. 2023 batch highland simulants, from which Lunar250 is intended for use in the Luna Dust Chamber. Additionally, this work provides new results for ESA’s mare simulant, EAC-1. We provide data on particle size distribution, particle shape, abrasivity, density, water content, major and trace element geochemistry and modal mineralogy. As the simulants in the Luna Facility will be constantly overseen, this work organized by the Vulcan Facility (ESA) intends to support the monitoring of the geotechnical property variations of the simulants over time. Ultimately, we analysed several properties with different tools to emphasize how different methods and instruments affect the variability and reliability of the results.} } - Gaier, J. R. and Sechkar, E. A. (2007). Lunar Simulation in the Lunar Dust Adhesion Bell Jar
. AIAA Aerospace Sciences Meeting, NASA/TM-2007-214704. Source
BibTeX
@inproceedings{gaier2007lunar, title = {Lunar Simulation in the Lunar Dust Adhesion Bell Jar}, author = {Gaier, James R. and Sechkar, Edward A.}, booktitle = {AIAA Aerospace Sciences Meeting}, number = {NASA/TM-2007-214704}, institution = {NASA}, year = {2007}, doi = {10.2514/6.2007-963}, abstract = {The Lunar Dust Adhesion Bell Jar has been assembled at the NASA Glenn Research Center to provide a high fidelity lunar simulation facility to test the interactions of lunar dust and lunar dust simulant with candidate aerospace materials and coatings. It has a sophisticated design which enables it to treat dust in a way that will remove adsorbed gases and create a chemically reactive surface. It can simulate the vacuum, thermal, and radiation environments of the Moon, including proximate areas of illuminated heat and extremely cold shadow. It is expected to be a valuable tool in the development of dust repellant and cleaning technologies for lunar surface systems.} } - Gaier, J. R., Journey, K., Christopher, S. and Davis, S. (2011). Evaluation of Brushing as a Lunar Dust Mitigation Strategy for Thermal Control Surfaces
. International Conference on Environmental Systems, NASA/TM-2011-217231. Source
BibTeX
@inproceedings{gaier2011evaluation, title = {Evaluation of Brushing as a Lunar Dust Mitigation Strategy for Thermal Control Surfaces}, author = {Gaier, James R. and Journey, Khrissaundra and Christopher, Steven and Davis, Shanon}, booktitle = {International Conference on Environmental Systems}, number = {NASA/TM-2011-217231}, institution = {NASA}, address = {Portland, OR}, year = {2011}, url = {https://ntrs.nasa.gov/citations/20120000070}, abstract = {Evaluation of brushing to remove lunar simulant dust from thermal control surfaces is described. First, strip brushes made with nylon, PTFE, or Thunderon (Nihon Sanmo Dyeing Company Ltd.) bristles were used to remove JSC-1AF dust from AZ93 thermal control paint or aluminized FEP (AlFEP) thermal control surface under ambient laboratory conditions. Nylon and PTFE bristles removed a promising amount of dust from AZ93, and nylon and Thunderon bristles from AlFEP. But when these were tested under simulated lunar conditions in the lunar dust adhesion bell jar (LDAB), they were not effective. In a third effort, seven brushes made up of three different materials, two different geometries, and different bristle lengths and thicknesses were tested under laboratory conditions against AZ93 and AlFEP. Two of these brushes, the Zephyr fiberglass fingerprint brush and the Escoda nylon fan brush, removed over 90 percent of the dust, and so were tested in the fourth effort in the LDAB. They also performed well under these conditions recovering 80 percent or more of the original thermal performance (solar absorptance/thermal emittance) of both AZ93 and AgFEP after 20 strokes, and 90 or more percent after 200 strokes} } - Gaier, J. R. (2007). The Effects of Lunar Dust on EVA Systems During the Apollo Missions
. NASA, NASA/TM-2005-213610/REV1. Source
BibTeX
@techreport{gaier2007effects, title = {The Effects of Lunar Dust on EVA Systems During the Apollo Missions}, author = {Gaier, James R.}, number = {NASA/TM-2005-213610/REV1}, institution = {NASA}, year = {2007}, url = {https://ntrs.nasa.gov/citations/20070021819}, abstract = {Mission documents from the six Apollo missions that landed on the lunar surface have been studied in order to catalog the effects of lunar dust on Extra-Vehicular Activity (EVA) systems, primarily the Apollo surface space suit. It was found that the effects could be sorted into nine categories: vision obscuration, false instrument readings, dust coating and contamination, loss of traction, clogging of mechanisms, abrasion, thermal control problems, seal failures, and inhalation and irritation. Although simple dust mitigation measures were sufficient to mitigate some of the problems (i.e., loss of traction) it was found that these measures were ineffective to mitigate many of the more serious problems (i.e., clogging, abrasion, diminished heat rejection). The severity of the dust problems were consistently underestimated by ground tests, indicating a need to develop better simulation facilities and procedures.} } - Kobrick, R. L., Budinski, K. G., Street, K. W. J. and Klaus, D. M. (2010). Three-Body Abrasion Testing Using Lunar Dust Simulants to Evaluate Surface System Materials
. International Conference on Environmental Systems, NASA/TM-2010-216781. Source
BibTeX
@inproceedings{kobrick2010three, title = {Three-Body Abrasion Testing Using Lunar Dust Simulants to Evaluate Surface System Materials}, author = {Kobrick, Ryan L. and Budinski, Kenneth G. and Street, Kenneth W., Jr. and Klaus, David M.}, booktitle = {International Conference on Environmental Systems}, number = {NASA/TM-2010-216781}, institution = {NASA}, year = {2010}, doi = {10.2514/6.2010-6077}, abstract = {Numerous unexpected operational issues relating to the abrasive nature of lunar dust, such as scratched visors and spacesuit pressure seal leaks, were encountered during the Apollo missions. To avoid reoccurrence of these unexpected detrimental equipment problems on future missions to the Moon, a series of two- and three-body abrasion tests were developed and conducted in order to begin rigorously characterizing the effect of lunar dust abrasiveness on candidate surface system materials. Two-body scratch tests were initially performed to examine fundamental interactions of a single particle on a flat surface. These simple and robust tests were used to establish standardized measurement techniques for quantifying controlled volumetric wear. Subsequent efforts described in the paper involved three-body abrasion testing designed to be more representative of actual lunar interactions. For these tests, a new tribotester was developed to expose samples to a variety of industrial abrasives and lunar simulants. The work discussed in this paper describes the three-body hardware setup consisting of a rotating rubber wheel that applies a load on a specimen as a loose abrasive is fed into the system. The test methodology is based on ASTM International (ASTM) B611, except it does not mix water with the abrasive. All tests were run under identical conditions. Abraded material specimens included poly(methyl methacrylate) (PMMA), hardened 1045 steel, 6061-T6 aluminum (Al) and 1018 steel. Abrasives included lunar mare simulant JSC-1A-F (nominal size distribution), sieved JSC-1A-F (μm particle diameter), lunar highland simulant NU-LHT-2M, alumina (average diameter of 50 μm used per ASTM G76), and silica (50/70 mesh used per ASTM G65). The measured mass loss from each specimen was converted using standard densities to determine total wear volume in cm3. Abrasion was dominated by the alumina and the simulants were only similar to the silica (i.e., sand) on the softer materials of aluminum and PMMA. The nominal JSC-1A-F consistently showed more abrasion wear than the sieved version of the simulant. The lunar dust displayed abrasivity to all of the test materials, which are likely to be used in lunar landing equipment. Based on this test experience and pilot results obtained, recommendations are made for systematic abrasion testing of candidate materials intended for use in lunar exploration systems and in other environments with similar dust challenges.} } - Kalácska, G., Barkó, G., Shegawu, H., Kalácska, Á., Zsidai, L., Keresztes, R. and Károly, Z. (2024). The Abrasive Effect of Moon and Mars Regolith Simulants on Stainless Steel Rotating Shaft and Polytetrafluoroethylene Sealing Material Pairs
. Materials, 17. Source
BibTeX
@article{kalacska2024abrasive, title = {The Abrasive Effect of Moon and Mars Regolith Simulants on Stainless Steel Rotating Shaft and Polytetrafluoroethylene Sealing Material Pairs}, author = {Kalácska, Gábor and Barkó, György and Shegawu, Hailemariam and Kalácska, Ádám and Zsidai, László and Keresztes, Róbert and Károly, Zoltán}, journal = {Materials}, volume = {17}, number = {17}, pages = {4240}, publisher = {MDPI AG}, year = {2024}, doi = {10.3390/ma17174240}, abstract = {For space missions to either the Moon or Mars, protecting mechanical moving parts from the abrasive effects of prevailing surface dust is crucial. This paper compares the abrasive effects of two lunar and two Martian simulant regoliths using special pin-on-disc tests on a stainless steel/polytetrafluoroethylene (PTFE) sealing material pair. Due to the regolith particles entering the contact zone, a three-body abrasion mechanism took place. We found that friction coefficients stabilised between 0.2 and 0.4 for all simulants. Wear curves, surface roughness measurements, and microscopic images all suggest a significantly lower abrasion effect of the Martian regoliths than that of the lunar ones. It applies not only to steel surfaces but also to the PTFE pins. The dominant abrasive micro-mechanism of the disc surface is micro-ploughing in the case of all tests, while the transformation of the counterface is mixed. The surface of pin material is plastically transformed through micro-ploughing, while the material is removed through micro-cutting due to the slide over hard soil particles.} } - Sukumaran, A. K., Rengifo, S., Aguiar, B., Mohammed, S. M., Scott, W., Renfro, M., Chu, S.-H., Park, C. and Agarwal, A. (2026). Erosion Behavior of Ti-hBN Multifunctional Coatings in A Custom-Made Planetary Test Rig at Extreme Lunar Temperatures
. Tribology International. Source
BibTeX
@article{sukumaran2026erosion, title = {Erosion Behavior of Ti-hBN Multifunctional Coatings in A Custom-Made Planetary Test Rig at Extreme Lunar Temperatures}, author = {Sukumaran, Abhijith Kunneparambil and Rengifo, Sara and Aguiar, Brandon and Mohammed, Sohail M.A.K. and Scott, William and Renfro, Michael and Chu, Sang-Hyon and Park, Cheol and Agarwal, Arvind}, journal = {Tribology International}, volume = {202}, pages = {110339}, publisher = {Elsevier BV}, year = {2026}, doi = {10.1016/j.triboint.2024.110339}, abstract = {Spacecraft landings and takeoffs on the lunar surface, along with extreme temperature variations between day and night (-196 to 150° C), cause high-velocity dust impacts and erosion, resulting in the premature failure of structures. Ti/2 vol% hBN coatings were deposited using atmospheric (APS) and vacuum plasma spray (VPS) using cryo-milled powder feedstock to protect the structural components. The erosion performance of coatings at extreme lunar temperature regimes (-150 to 150° C) was evaluated in a custom-made planetary erosion test rig (PETR) at low (50 mph) and high impact velocities (250 mph). The mass loss of VPS coatings was reduced by 50% compared to the APS coatings and 40% compared to the Ti6Al4V substrate. The cryogenic temperature induces brittleness in the material, rendering it susceptible to extreme conditions of material loss. The particle impact-deformation behavior was captured using a high-speed camera to study the erosion mechanism. This analysis revealed chipping in substrates and brittle APS coatings, while particles rebounding and embedding were observed in VPS coatings. Energy calculations, aided by particle trajectory tracking from the high-speed camera, have conclusively shown that VPS coatings absorb 5–10% more energy than APS coatings during erosion tests. A modified erosion index was developed incorporating the fracture toughness and temperatures. New erosion models for brittle and ductile target materials are proposed for developing erosion-resistant material systems.} } - Wiesner, V. L., Wohl, C. J., King, G. C., Gordon, K. L., Das, L. and Hernandez, J. J. (2023). Protective Coatings for Lunar Dust Tolerance
. NASA, NASA/TM-20230003195. Source
BibTeX
@techreport{wiesner2023protective, title = {Protective Coatings for Lunar Dust Tolerance}, author = {Wiesner, Valerie L. and Wohl, Christopher J. and King, Glen C. and Gordon, Keith L. and Das, Lopamudra and Hernandez, Jonathan J.}, number = {NASA/TM-20230003195}, institution = {NASA}, year = {2023}, url = {https://ntrs.nasa.gov/citations/20230003195}, abstract = {Materials capable of withstanding the harsh lunar environment are critically needed to support long duration, sustainable missions on the Moon’s surface. Lunar dust significantly threatens the durability and reusability of components and vehicles due to possessing a fine, jagged morphology and highly abrasive nature. These characteristics result in the particles eroding, adhering and/or embedding onto component surfaces and into device confined geometries (e.g., gear housing, interlocking systems, etc.) potentially leading to premature failure. The aim of this study is to identify and characterize wear-resistant commercial-off-the-shelf (COTS) materials, including advanced ceramics, for use as protective coatings to minimize abrasion and adhesion caused by lunar dust. Preliminary testing that mimics various aspects of lunar dust degradation, such as abrasive wear and adhesion, suggests that COTS ceramic coatings can improve lunar dust tolerance and protect underlying metallic substrates.} } - McBryan, E., Francis, P. and Sobey, A. (2025). Dust Mitigation for the VIPER Mobility System
. International Conference on Environmental Systems, 20250005201. Source
BibTeX
@inproceedings{mcbryan2025dust, title = {Dust Mitigation for the VIPER Mobility System}, author = {McBryan, Emily and Francis, Parker and Sobey, Alexander}, booktitle = {International Conference on Environmental Systems}, number = {20250005201}, institution = {NASA}, year = {2025}, doi = {10.32865/2346/108814}, abstract = {NASA’s Volatiles Investigating Polar Exploration Rover (VIPER) is built to prospect, provide ground truth measurements, and build regional maps of the volatiles at the lunar South Pole that were previously detected by Lunar Reconnaissance Orbiter (LRO), Lunar Crater Observation and Sensing Satellite (LCROSS), and Chandrayaan-1. The rover’s mobility system, responsible for navigating the moon’s partially defined terrain, is the part of VIPER that is most exposed to the lunar surface environment. To ensure it can survive the thermal extremes and lunar regolith, the VIPER project utilized resources across NASA centers to create and evaluate a multi-functional environmental protection strategy. The project’s approach combined thermal insulation with dust protection in a flexible barrier across dynamic actuated joints to serve as the first defense between the hardware and the environment. Additionally, the VIPER project integrated a selection of seals (labyrinth, Nomex felt, and spring-energized PTFE) with individual mechanisms to further mitigate dust infiltration and abrasion risk to the bearings, motors, and sensors. In stages, the project performed extensive testing through a matrix of simulated environmental parameters to evaluate performance margins from the component level to the integrated mobility system. This paper addresses the project’s lessons learned, with an emphasis on systems integration and how this work can affect future long-duration lunar surface systems, such as crewed unpressurized rovers and in-situ resource utilization robotics.} } - Slabic, A., Gruener, J. E., Kovtun, R. N., Rickman, D. L., Sibille, L., Oravec, H. A., Edmunson, J. and Keprta, S. (2024). Lunar Regolith Simulant User's Guide, Revision A
. NASA, NASA/TM-20240011783. Source
BibTeX
@techreport{slabic2024lunar, title = {Lunar Regolith Simulant User's Guide, Revision A}, author = {Slabic, Ane and Gruener, John E. and Kovtun, Rostislav N. and Rickman, Douglas L. and Sibille, Laurent and Oravec, Heather A. and Edmunson, Jennifer and Keprta, Sean}, number = {NASA/TM-20240011783}, institution = {NASA}, year = {2024}, url = {https://ntrs.nasa.gov/citations/20240011783}, abstract = {This guide is titled Lunar Regolith Simulant User's Guide, Rev A, and two points need to be made about the title. First, is the use of the term "regolith". During the Apollo Program, the term "soil" was used for taking a sample of the loose material on the surface, and then cataloging that sample in the lunar curation database as a "soil sample". By the 1980s, the term "regolith" gained favor by lunar scientists. In the Lunar Sourcebook (Heiken et al., 1991), regolith is defined as "a general term for the layer or mantle of fragmental and unconsolidated rock material, whether residual or transported and of highly varied character, that nearly everywhere forms the surface of the land and overlies or covers bedrock". Regolith is a terrestrial term that seems to go back to 1897, according to a recent paper by Huggett (2023). Huggett summed up his paper by writing, "soil and regolith are one in the same". "Regolith" will mostly be used throughout this guide, as it tends to separate in one's mind the unique nature of the Moon's surface when compared to the inherent bias humans have in their mind when they hear and use the word "soil". When referring to Apollo samples, "soil" is used for historical context and in some places the simple term "lunar simulant" is also used. Secondly, Rev A is used in the title because NASA released its first Lunar Regolith Simulant User's Guide in 2010, near the end of NASA's Constellation Program (Schrader et al., 2010). This guide follows in the pattern of that first guide and will be updated on a periodic basis as new simulants are created, characterized and used, and as new information emerges about the Moon's regolith due to new lunar exploration missions, both robotic and human.} } - Gerdts, S., Moreland, S. and Marteau, E. (2025). GRC-3b-DST, a Geotechnical Simulant for Cohesive Mars and Moon Mobility and Excavation Testing With Reduced Respirable Silica
. NASA, NASA/TM-20250006761. Source
BibTeX
@techreport{gerdts2025grc, title = {GRC-3b-DST, a Geotechnical Simulant for Cohesive Mars and Moon Mobility and Excavation Testing With Reduced Respirable Silica}, author = {Gerdts, Stephen and Moreland, Scott and Marteau, Eloise}, number = {NASA/TM-20250006761}, institution = {NASA}, year = {2025}, doi = {10.64631/puln8817}, abstract = {This study presents the development and evaluation of a modified version of the GRC-3b lunar soil simulant designed to address both geotechnical performance and operator safety in terrestrial mobility and excavation testing. While GRC-3b is widely used due to its cost-effectiveness and similarity to extraterrestrial regolith, its fine silica content poses significant health risks during handling. To mitigate this, a dust-suppressing additive was introduced, producing GRC-3b-DST. The modified simulant maintained the original particle size distribution and classification as a well-graded silty sand but exhibited increased cohesion and a lower minimum density, enhancing its ability to replicate compacted regolith conditions. Laboratory testing, including modified Proctor compaction, simple shear tests, and cone penetrometer correlations, confirmed that the geotechnical properties of GRC-3b-DST are consistent and predictable, making it suitable for high-fidelity terrain simulations. Safety testing using OSHA-compliant air sampling showed respirable silica concentrations remained well below permissible exposure limits during soil preparation, indicating a significant reduction in airborne hazards. These findings suggest that GRC-3b-DST offers a safer, more versatile alternative for use in large-scale test environments where repeatable geomechanical properties and minimized health risks are essential.} } - Windisch, L., Linke, S., Jütte, M., Baasch, J., Kwade, A., Stoll, E. and Schilde, C. (2022). Geotechnical and Shear Behavior of Novel Lunar Regolith Simulants TUBS-M, TUBS-T, and TUBS-I
. Materials, 23. Source
BibTeX
@article{windisch2022geotechnical, title = {Geotechnical and Shear Behavior of Novel Lunar Regolith Simulants {TUBS-M}, {TUBS-T}, and {TUBS-I}}, author = {Windisch, Lisa and Linke, Stefan and Jütte, Magnus and Baasch, Julian and Kwade, Arno and Stoll, Enrico and Schilde, Carsten}, journal = {Materials}, volume = {15}, number = {23}, pages = {8561}, year = {2022}, doi = {10.3390/ma15238561}, abstract = {The return to the Moon is an important short-term goal of NASA and other international space agencies. To minimize mission risks, technologies, such as rovers or regolith processing systems, must be developed and tested on Earth using lunar regolith simulants that closely resemble the properties of real lunar soil. So far, no singular lunar simulant can cover the multitude of use cases that lunar regolith involves, and most available materials are poorly characterized. To overcome this major gap, a unique modular system for flexible adaptable novel lunar regolith simulants was developed and chemically characterized in earlier works. To supplement this, the present study provides comprehensive investigations regarding geotechnical properties of the three base regolith simulant systems: TUBS-M, TUBS-T, and TUBS-I. To evaluate the engineering and flow properties of these heterogeneous materials under various conditions, shear tests, particle size analyses, scanning electron microscope observations, and density investigations were conducted. It was shown that small grains <25 µm (lunar dust) are highly compressive and cohesive even at low external stress. They are particularly important as a large amount of fine dust is present in lunar regolith and simulants (x50 = 76.7 to 96.0 µm). Further, ring shear and densification tests revealed correlations with damage mechanisms caused by local stress peaks for grains in the mm range. In addition, an explanation for the occurrence of considerable differences in the literature-based data for particle sizes was established by comparing various measurement procedures. The present study shows detailed geotechnical investigations of novel lunar regolith simulants, which can be used for the development of equipment for future lunar exploration missions and in situ resource utilization under realistic conditions. The results also provide evidence about possible correlations and causes of known soil-induced mission risks that so far have mostly been described phenomenologically.} } - Exolith Lab. (2018). What Is Simulated?. sciences.ucf.edu/class/wp-content/uploads/sites/23/2018/10/WhatIsSimu...
BibTeX
@misc{exolith2018what, title = {What Is Simulated?}, author = {{Exolith Lab}}, organization = {Center for Lunar and Asteroid Surface Science, University of Central Florida}, year = {2018}, url = {https://sciences.ucf.edu/class/wp-content/uploads/sites/23/2018/10/WhatIsSimulated.pdf} } - Metzger, P. T., Britt, D. T., Covey, S. D. and Lewis, J. S. (2023). Results of the 2015 Workshop on Asteroid Simulants. arxiv.org/pdf/2306.03068
BibTeX
@misc{metzger2023results, title = {Results of the 2015 Workshop on Asteroid Simulants}, author = {Metzger, Philip T. and Britt, D. T. and Covey, S. D. and Lewis, John S.}, year = {2023}, url = {https://arxiv.org/pdf/2306.03068} } - Qi, S., Li, L., Hou, X., Qiao, S., Ma, X., Lu, X., Cong, J., Hao, R., Zhang, C., Li, J., Elsworth, D., Yang, W., Li, X.-H. and Wu, F.-Y. (2025). Strongly Cohesive Lunar Soil Identified at the Chang'e-6 Landing Site
. Nature Astronomy. Source
BibTeX
@article{qi2025strongly, title = {Strongly Cohesive Lunar Soil Identified at the Chang'e-6 Landing Site}, author = {Qi, Shengwen and Li, Lihui and Hou, Xiaokun and Qiao, Sijia and Ma, Xiandong and Lu, Xiao and Cong, Jianing and Hao, Ruipeng and Zhang, Chi and Li, Jinhua and Elsworth, Derek and Yang, Wei and Li, Xian-Hua and Wu, Fu-Yuan}, journal = {Nature Astronomy}, volume = {10}, pages = {214-223}, year = {2025}, doi = {10.1038/s41550-025-02715-3}, abstract = {Abstract The physical properties of lunar soil are critical to understanding its evolution. However, the extent of the diversity among the global lunar soils remains unclear owing to limited sampling sites. Here we present a systematic investigation of the angle of repose (AOR), particle morphology and size distribution of soil obtained at the Chang’e-6 (CE-6) landing site, the first sample from the lunar farside. The CE-6 sample has a maximum static AOR of 52.9°, which is substantially higher than those of the Chang’e-5 and Apollo soil simulants. In addition, a substantially larger dynamic AOR of 70.4° is exhibited by the CE-6 sample compared with the CE-5 soil simulant, indicating a stronger cohesive property. This strong cohesive property can be attributed to the high plagioclase abundance and potentially strong space weathering at the sampling, especially impact reworking, which resulted in a fine particle size ( D 60 = 48.4 μm) of the CE-6 sample with a high portion of the intermediate fraction (that is, 11–125 μm) and a more complex morphology with a small mean sphericity ( S mean = 0.58). These characteristics enhance the cohesiveness by strengthening electrostatic and van der Waals forces. This finding discloses key factors controlling the AOR and provides a fresh genesis perspective for understanding the physical properties of lunar soil, with implications for lunar evolution and future lunar resource utilization.} } - Heiken, G. H., Vaniman, D. T. and French, B. M. (1991). Lunar Sourcebook: A User's Guide to the Moon
. Endeavour. Source
BibTeX
@book{heiken1991lunar, title = {Lunar Sourcebook: A User's Guide to the Moon}, author = {Heiken, Grant H. and Vaniman, David T. and French, Bevan M.}, journal = {Endeavour}, volume = {16}, pages = {96}, publisher = {Cambridge University Press}, year = {1991}, doi = {10.1016/0160-9327(92)90014-g} } - Surveyor Scientific Evaluation Advisory Team. (1968). Surveyor Project Final Report, Part 2: Science Results
. Jet Propulsion Laboratory, NASA-CR-101584. Source
BibTeX
@techreport{surveyor1968surveyorb, title = {Surveyor Project Final Report, Part 2: Science Results}, author = {{Surveyor Scientific Evaluation Advisory Team}}, number = {NASA-CR-101584}, institution = {Jet Propulsion Laboratory}, year = {1968}, url = {https://ntrs.nasa.gov/citations/19690019967} } - Nichols, D. K., Price, W. E. and Malone, C. (1984). A Guideline for Heavy Ion Radiation Testing for Single Event Upset (SEU)
. Jet Propulsion Laboratory, California Institute of Technology, JPL Publication 84-22. Source
BibTeX
@techreport{nichols1984guideline, title = {A Guideline for Heavy Ion Radiation Testing for Single Event Upset (SEU)}, author = {Nichols, Donald K. and Price, William E. and Malone, Carl}, number = {JPL Publication 84-22}, institution = {Jet Propulsion Laboratory, California Institute of Technology}, year = {1984}, url = {https://ntrs.nasa.gov/citations/19840020507}, abstract = {A guideline for heavy ion radiation testing for single event upset was prepared to assist new experimenters in preparing and directing tests. How to estimate parts vulnerability and select an irradiation facility is described. A broad brush description of JPL equipment is given, certain necessary pre-test procedures are outlined and the roles and testing guidelines for on-site test personnel are indicated. Detailed descriptions of equipment needed to interface with JPL test crew and equipment are not provided, nor does it meet the more generalized and broader requirements of a MIL-STD document. A detailed equipment description is available upon request, and a MIL-STD document is in the early stages of preparation.} } - Pease, R. L. and Young, P. A. (1980). Total Dose Hardness Assurance. Volume I: Identification of Techniques
. BDM Corporation, Albuquerque, New Mexico, AFWL-TR-79-53, Vol. I; BDM/TAC-78-764-TR-R1; AD-A085012. Source
BibTeX
@techreport{pease1980total, title = {Total Dose Hardness Assurance. Volume I: Identification of Techniques}, author = {Pease, R. L. and Young, P. A.}, number = {AFWL-TR-79-53, Vol. I; BDM/TAC-78-764-TR-R1; AD-A085012}, institution = {BDM Corporation, Albuquerque, New Mexico}, month = {2}, year = {1980}, url = {https://apps.dtic.mil/sti/citations/ADA085012} } - Curtis, A. J., Tinling, N. G. and Abstein, J. H. T. (1971). Selection and Performance of Vibration Tests
. The Shock and Vibration Information Center, U.S. Department of Defense, SVM-8. Source
BibTeX
@techreport{curtis1971selection, title = {Selection and Performance of Vibration Tests}, author = {Curtis, Allen J. and Tinling, Nickolas G. and Abstein, Jr., Henry T.}, number = {SVM-8}, institution = {The Shock and Vibration Information Center, U.S. Department of Defense}, year = {1971}, doi = {10.21236/ad0737830}, abstract = {;Contents: Introduction; Selection of appropriate test method; Simulation characteristics of test methods; Vibration equipment requirements; Test performance and control; Acquisition and processing of test data.} } - Gonzales, E. C. and Huang, N. (2020). Electromagnetic Compatibility Test and Analysis Campaign of NASA's Mars 2020 Rover Final Submission
. EMC/SIPI. Source
BibTeX
@inproceedings{gonzales2020electromagnetic, title = {Electromagnetic Compatibility Test and Analysis Campaign of NASA's Mars 2020 Rover Final Submission}, author = {Gonzales, Edward C and Huang, Nelson}, booktitle = {EMC/SIPI}, publisher = {JPL Open Repository}, year = {2020}, url = {https://dataverse.jpl.nasa.gov/dataset.xhtml?persistentId=hdl:2014/52292} } - Chapin, E., Grando, M. B., Hamilton, G. A., Pak, K. S., Pollard, B. D., Shaffer, S. J. and Wu, C. (2013). Methods for testing the Mars Science Laboratory’s Landing Radar
. IEEE Radar Conference. Source
BibTeX
@inproceedings{chapin2013methods, title = {Methods for testing the Mars Science Laboratory’s Landing Radar}, author = {Chapin, Elaine and Grando, Maurio B. and Hamilton, Gary A. and Pak, Kyung S. and Pollard, Brian D. and Shaffer, Scott J. and Wu, Chialin}, booktitle = {IEEE Radar Conference}, volume = {aas 12 91}, pages = {1-4}, year = {2013}, doi = {10.1109/radar.2013.6586044}, abstract = {The Mars Science Laboratory's rover named Curiosity successfully landed on Mars on August 6, 2012. One component of the Mars Science Laboratory (MSL) Entry, Descent, and Landing (EDL) system was the Terminal Descent Sensor (TDS) landing radar. In this paper we describe laboratory testing of this radar performed before launch.} } - Megivern, J., Duffy, E., Lashore, M., Colwell, I., Wehage, K. and Gori, M. (2021). Simulating Mars: Enabling Testing of the Perseverance Rover Sampling and Caching Subsystem on Earth
. IEEE Aerospace Conference. Source
BibTeX
@inproceedings{megivern2021simulating, title = {Simulating Mars: Enabling Testing of the Perseverance Rover Sampling and Caching Subsystem on Earth}, author = {Megivern, Jeffrey and Duffy, Elizabeth and Lashore, Michael and Colwell, Ian and Wehage, Kristopher and Gori, Marcello}, booktitle = {IEEE Aerospace Conference}, pages = {1-15}, year = {2021}, doi = {10.1109/aero53065.2022.9843666}, abstract = {The development of the Sampling and Caching Subsystem (SCS) on the JPL Perseverance Rover lies at the intersection of testing, robotics, and geology. The SCS team established three primary system test campaigns and venues to aid in the development of SCS through verification and validation testing – Qualification Model Dirty Testing (QMDT) to provide a venue for testing in a Martian environment, Vehicle System Testbed (VSTB) for testing while integrated with the mobility subsystem on Martian-like terrain, and the Flight Software Testbed (FSWTB) for conducting tests using the flight motor controllers and software system on a hexapod which had the ability to simulate rover tilt. Each venue contributed a vital piece to the SCS building blocks. However, the QMDT venue operating within a simulated Martian environment provided a sui generis opportunity to fine tune the entire sampling and caching process while building the team's knowledge base about rock drillability, system life, and target selection. On Earth, because Martian rocks are not readily available, the development team utilized geoanalogs to the rocks and regolith on Mars. With rock simulant drillability characteristics like density and compressibility defined, these geoanalog rocks are ready to be drilled into as on the Martian surface. A key aspect of interacting with Martian rocks is drilling target identification and selection. The Perseverance robotic system uses on-board cameras, instrumentation, and software to collect enough information to identify potential scientific targets. With the targets identified, SCS can place the Corer and abrade the surface or collect a sample. For a ground test activity like QMDT, the test team did not have all of the camera and instrumentation systems that the rover does, so the team developed ground test equivalents to process a rock, build a target map, and define the target. The team constructed a Rock Scanning Station to build a 3D point cloud of the rock which was then processed and evaluated in a Target Downselect Tool. Key outputs from the Target Downselect Tool can be uploaded directly to the robotic software system to simulate and build the robotic sequences used in tests. With these insights and programmatic definition of targets, the QMDT test team was able to make the same decisions that the Perseverance surface operations team does. In addition, valuable lessons learned from developing the target selection ground tools and using them in QMDT were implemented into the tools used for surface operations.} } - Creager, C., Breckenridge, J., Johnson, K., Oravec, H., Moreland, S., Sobey, A. and McBryan, E. (2025). Best Practices for the Testing of Planetary Roving Vehicle Mobility Systems and Tires
. NASA, 20250003470. Source
BibTeX
@techreport{creager2025best, title = {Best Practices for the Testing of Planetary Roving Vehicle Mobility Systems and Tires}, author = {Creager, Colin and Breckenridge, John and Johnson, Kyle and Oravec, Heather and Moreland, Scott and Sobey, Alexander and McBryan, Emily}, number = {20250003470}, institution = {NASA}, year = {2025}, url = {https://ntrs.nasa.gov/citations/20250003470}, abstract = {NASA has an extensive history of conducting mobility testing on planetary tires, rovers, and mobility subsystems. This paper contains a summary of the best practices and lessons learned from past test approaches, as well as from relevant test methodologies external to NASA, with a focus on tires and mobility systems. It is intended to be a resource for future planetary rover developments. This document, which will be released in two phases, serves two objectives: 1) compile the existing knowledge of mobility related testing within NASA; and 2) identify major gaps in mobility related test needs and suggest potential paths forward. This first release of the document (early 2025) captures information based on the authors’ existing knowledge and an abbreviated literature review. A more thorough version will be released in late 2025 and will include more information on test methods external to NASA, as well as additional lessons learned through further investigations. The Lunar Terrain Vehicle (LTV) is used as case study to help identify major test needs; however, this document is intended to be applicable to a wide range of potential missions. Though no current mobility standards exist for the testing of planetary tires and mobility subsystems, future motive is to utilize the information from this whitepaper to guide the development of NASA mobility test standards.} } - Verhagen, J., Krantz, E., Sidrane, C., Dörner, D., De Carli, N., Roque, P., Mao, H., Tibert, G., Stenius, I., Fuglesang, C., Dimarogonas, D. and Tumova, J. (2026). Validation of Space Robotics in Underwater Environments via Disturbance Robustness Equivalency
. IEEE International Conference on Robotics and Automation. Source
BibTeX
@inproceedings{verhagen2026validation, title = {Validation of Space Robotics in Underwater Environments via Disturbance Robustness Equivalency}, author = {Verhagen, Joris and Krantz, Elias and Sidrane, Chelsea and Dörner, David and De Carli, Nicola and Roque, Pedro and Mao, Huina and Tibert, Gunnar and Stenius, Ivan and Fuglesang, Christer and Dimarogonas, Dimos and Tumova, Jana}, booktitle = {IEEE International Conference on Robotics and Automation}, pages = {5327-5334}, year = {2026}, doi = {10.1109/icra57385.2026.11697381} } - Bassett, D. A. and Abramovici, A. (1999). Special Purpose Dexterous Manipulator (SPDM) Requirements Verification
. International Symposium on Artificial Intelligence, Robotics and Automation in Space. Source
BibTeX
@inproceedings{bassett1999special, title = {Special Purpose Dexterous Manipulator (SPDM) Requirements Verification}, author = {Bassett, D. A. and Abramovici, A.}, booktitle = {International Symposium on Artificial Intelligence, Robotics and Automation in Space}, address = {ESTEC, Noordwijk}, year = {1999}, url = {http://robotics.estec.esa.int/i-SAIRAS/isairas1999/s02-02.pdf} } - Richter, J., Oberacker, D., Ligeza, G., Bickel, V., Arm, P., Talbot, W., Besselmann, M. G., Kehl, F., Schnell, T., Kolvenbach, H., Dillmann, R., Roennau, A. and Hutter, M. (2026). A Practical Framework of Key Performance Indicators for Multi-Robot Lunar and Planetary Field Tests
. arXiv. Source
BibTeX
@article{richter2026practical, title = {A Practical Framework of Key Performance Indicators for Multi-Robot Lunar and Planetary Field Tests}, author = {Richter, Julia and Oberacker, David and Ligeza, Gabriela and Bickel, Valentin and Arm, Philip and Talbot, William and Besselmann, Marvin Große and Kehl, Florian and Schnell, Tristan and Kolvenbach, Hendrik and Dillmann, Rüdiger and Roennau, Arne and Hutter, Marco}, journal = {arXiv}, year = {2026}, doi = {10.48550/arxiv.2601.20529}, abstract = {Robotic prospecting for critical resources on the Moon, such as ilmenite, rare earth elements, and water ice, requires robust exploration methods given the diverse terrain and harsh environmental conditions. Although numerous analog field trials address these goals, comparing their results remains challenging because of differences in robot platforms and experimental setups. These missions typically assess performance using selected, scenario-specific engineering metrics that fail to establish a clear link between field performance and science-driven objectives. In this paper, we address this gap by deriving a structured framework of KPI from three realistic multi-robot lunar scenarios reflecting scientific objectives and operational constraints. Our framework emphasizes scenario-dependent priorities in efficiency, robustness, and precision, and is explicitly designed for practical applicability in field deployments. We validated the framework in a multi-robot field test and found it practical and easy to apply for efficiency- and robustness-related KPI, whereas precision-oriented KPI require reliable ground-truth data that is not always feasible to obtain in outdoor analog environments. Overall, we propose this framework as a common evaluation standard enabling consistent, goal-oriented comparison of multi-robot field trials and supporting systematic development of robotic systems for future planetary exploration.} } - Callas, J. L. (2015). Mars Exploration Rover Spirit End of Mission Report
. Jet Propulsion Laboratory, California Institute of Technology, JPL D-91176. Source
BibTeX
@techreport{callas2015spirit, title = {Mars Exploration Rover Spirit End of Mission Report}, author = {Callas, John L.}, number = {JPL D-91176}, institution = {Jet Propulsion Laboratory, California Institute of Technology}, year = {2015}, url = {https://ntrs.nasa.gov/citations/20160001767}, abstract = {The Mars Exploration Rover (MER) Spirit landed in Gusev crater on Mars on January 4, 2004, for a prime mission designed to last three months (90 sols). After more than six years operating on the surface of Mars, the last communication received from Spirit occurred on Sol 2210 (March 22, 2010). Following the loss of signal, the Mars Exploration Rover Project radiated over 1400 commands to Mars in an attempt to elicit a response from the rover. Attempts were made utilizing Deep Space Network X-Band and UHF relay via both Mars Odyssey and the Mars Reconnaissance Orbiter. Search and recovery efforts concluded on July 13, 2011. It is the MER project's assessment that Spirit succumbed to the extreme environmental conditions experienced during its fourth winter on Mars. Focusing on the time period from the end of the third Martian winter through the fourth winter and end of recovery activities, this report describes possible explanations for the loss of the vehicle and the extent of recovery efforts that were performed. It offers lessons learned and provides an overall mission summary.} } - Herman, J. A., Wood, E. G. and Chin, K. B. (2021). Power Operations of the Mars Exploration Rovers
. AIAA Propulsion and Energy Forum. Source
BibTeX
@inproceedings{herman2021power, title = {Power Operations of the Mars Exploration Rovers}, author = {Herman, Jennifer A. and Wood, Eric G. and Chin, Keith B.}, booktitle = {AIAA Propulsion and Energy Forum}, publisher = {American Institute of Aeronautics and Astronautics}, year = {2021}, doi = {10.2514/6.2021-3255}, abstract = {View Video Presentation: https://doi.org/10.2514/6.2021-3255.vid The rovers of the National Aeronautics and Space Administration’s (NASA) Mars Exploration Rovers (MER) project, Spirit (MER-A) and Opportunity (MER-B), safely landed on the surface of Mars three weeks apart during January 2004. Spirit and Opportunity were built and operated by the Jet Propulsion Laboratory (JPL), which is managed by the California Institute of Technology (Caltech) for NASA. Spirit landed at Gusev Crater, 14.8 degrees south of the equator, and operated continuously on the surface of Mars from January 4, 2004 until last contact from Spirit on March 22, 2010. Opportunity landed at Meridiani Planum, a location 2.5 degrees south of the Martian equator. Opportunity operated continuously on the Martian surface from January 25, 2004 until the last received transmission from Opportunity on June 10, 2018. The goal of the MER project was to determine if Mars ever had a habitable environment, in particular, if it ever had water. During their missions, both Spirit and Opportunity found evidence that liquid water once flowed on the surface of Mars. Both Spirit and Opportunity used a 1.33 m2 triple-junction solar array as their power sources. Based on observations of the original Mars rover, the Sojourner rover of the Mars Pathfinder mission that landed on Mars on July 4, 1997, the expectation was that the Martian dust would rapidly accumulate on the solar arrays of Spirit and Opportunity, and that the rovers would not have enough energy to continue operations after 90 Martian days (sols). Instead, due in part to lower dust accumulation rates than expected and numerous dust cleaning events, the Spirit and Opportunity rovers continued to operate on the Martian surface for over 2000 sols (MER-A) and 5000 sols (MER-B), respectively. During this time, the rovers experienced multiple Martian winters and several dust storms. Any spacecraft on the Martian surface is vulnerable to dust, especially solar-powered spacecraft. The Spirit and Opportunity rovers were operational on the Martian surface for much longer than expected due in part to aeolian removal of dust from their solar arrays. The first few dust removal events were a pleasant surprise to the MER operations teams; however, over time a pattern began to arise. In over three Mars Years on the surface, the Power operations team tracked the solar array Dust Factor at Gusev Crater (location of MER-A) and observed that there were several significant dust removal and deposition events in Mars Year (MY) 27, even in the absence of a large dust storm. In MY 28 at Gusev Crater, the large atmospheric opacity (Tau) increase lagged significant dust removal events. Overall at Gusev Crater, there was a pattern of steady dust accumulation on the solar arrays, with a small number of significant dust cleaning events. At Meridiani Planum, where Opportunity rover operated for over seven Mars Years (late MY 26 to mid MY 34), a clear and consistent pattern of dust movement emerged. Meridiani Planum had a predictable, seasonally dependent pattern of gradual and continuous dust accumulation and removal. In summary, this paper explains the reasons for the development of the solar array Dust Factor and how it was used in mission operations. In particular, this paper describes the MMPAT software package, how it models array energy, including the important assumptions, model inputs and sources of error. And finally, this paper will show how the calculated solar array Dust Factor was used at Gusev Crater and Meridiani Planum to predict dust accumulation rates and weather patterns, and the importance of this generated data set for current and future solar- powered missions to Mars, such as the InSight lander and the planned Mars Sample Return rover.} } - Staab, M. S., Herman, J. A., Reich, K., Sridhar, V. and Nelson, R. W. (2020). MER Opportunity dust-storm recovery operations and implications for future Mars surface missions
. IEEE Aerospace Conference. Source
BibTeX
@inproceedings{staab2020mer, title = {MER Opportunity dust-storm recovery operations and implications for future Mars surface missions}, author = {Staab, Michael S. and Herman, Jennifer A. and Reich, Kevin and Sridhar, Vishnu and Nelson, Robert W.}, booktitle = {IEEE Aerospace Conference}, pages = {1-20}, publisher = {IEEE}, year = {2020}, doi = {10.1109/aero47225.2020.9172528}, abstract = {In June 2018, NASA's Mars Exploration Rover Opportunity became engulfed in the most intense global dust storm observed in its 14-year mission and in Mars' recorded history. Sapped of life-giving solar energy, Opportunity fell silent to ground operators on June 11, in what would be its final call home. Over the course of the next eight months, the MER team employed numerous recovery efforts and radiated over one thousand commands to wake the silent rover. Although unsuccessful, MER's dust-storm recovery team changed the paradigm of dust-storm operations from Opportunity's survival of a previous global dust storm in 2007. In this paper, the authors offer a glimpse into MER's recovery efforts and lessons learned from Opportunity dust-storm operations for future solar-powered Mars surface missions. First, the authors discuss the indicators of the approaching dust storm and the actions the team employed to reduce Opportunity's power consumption and preserve available battery charge prior to loss of contact. Second, the authors discuss the team's recovery efforts until Opportunity's declared End-of-Mission, the steps the team took to re-establish contact with Opportunity, the assumptions made during each step of the recovery process, and the commanding actions employed. Finally, the authors discuss the operational impacts of global dust storms on the safe and successful operation of solar-powered spacecraft on the Martian surface, and offer design recommendations for future solar-powered missions from the lessons learned during Opportunity's 14-year mission and experience through two global dust storms.} } - Anderson, J. L., Karras, J. T., Cacan, M., Kubiak, G., Pyrzak, G., Dor, H. and Pipenberg, B. (2023). Ingenuity, One Year of Flying on Mars
. IEEE Aerospace Conference. Source
BibTeX
@inproceedings{anderson2023ingenuity, title = {Ingenuity, One Year of Flying on Mars}, author = {Anderson, Joshua L. and Karras, Jaakko T. and Cacan, Martin and Kubiak, Gerik and Pyrzak, Guy and Dor, Harel and Pipenberg, Benjamin}, booktitle = {IEEE Aerospace Conference}, publisher = {JPL Open Repository}, year = {2023}, doi = {10.1109/aero55745.2023.10115837} } - Golombek, M., Hudson, T., Bailey, P., Balabanska, N., Marteau, E., Charalambous, C., Baker, M., Lemmon, M., White, B. R., Lorenz, R. D., Spohn, T., Maki, J., Kallemeyn, P., Garvin, J. B., Newman, C., Hurst, K., Murdoch, N., Williams, N., Banerdt, W. B., Lognonné, P., Delage, P., Lapeyre, R., Gaudin, E., Yana, C., Verdier, N., Panning, M. P., Trebi-Ollennu, A., Ali, K., Mittelholz, A., Johnson, C. S., Langlais, B., Warner, N., Grant, J., Daubar, I. J., Ansan, V., Vrettos, C., Spiga, A., Banfield, D., Gomez, A. R., Mishra, P., Dotson, R., Krause, C., Sainton, G. and Gabsi, T. (2023). Results from InSight Robotic Arm Activities
. Space Science Reviews. Source
BibTeX
@article{golombek2023results, title = {Results from InSight Robotic Arm Activities}, author = {Golombek, M. and Hudson, T. and Bailey, Philip and Balabanska, Nadya and Marteau, E. and Charalambous, C. and Baker, Michael and Lemmon, M. and White, Bruce R. and Lorenz, Ralph D. and Spohn, Tilman and Maki, J. and Kallemeyn, P. and Garvin, James B. and Newman, C. and Hurst, Kenneth and Murdoch, Naomi and Williams, N. and Banerdt, W. Bruce and Lognonné, P. and Delage, P. and Lapeyre, R. and Gaudin, E. and Yana, Charles and Verdier, N. and Panning, Mark P. and Trebi-Ollennu, Ashitey and Ali, K. and Mittelholz, A. and Johnson, Christopher S. and Langlais, B. and Warner, N. and Grant, J. and Daubar, Ingrid J. and Ansan, Veronique and Vrettos, Christos and Spiga, Aymeric and Banfield, Don and Gomez, Annabel R. and Mishra, Pranay and Dotson, Ryan and Krause, Christian and Sainton, G. and Gabsi, T.}, journal = {Space Science Reviews}, publisher = {JPL Open Repository}, year = {2023}, doi = {10.48577/jpl.87kgn1} } - Schepanski, K., Tegen, I., Todd, M. C., Heinold, B., Bönisch, G., Laurent, B. and Macke, A. (2009). Meteorological processes forcing Saharan dust emission inferred from MSG-SEVIRI observations of subdaily dust source activation and numerical models
. IEEE Robotics and Automation Letters, D10. Source
BibTeX
@article{schepanski2009meteorological, title = {Meteorological processes forcing Saharan dust emission inferred from MSG-SEVIRI observations of subdaily dust source activation and numerical models}, author = {Schepanski, K. and Tegen, I. and Todd, M. C. and Heinold, B. and Bönisch, G. and Laurent, B. and Macke, A.}, journal = {IEEE Robotics and Automation Letters}, volume = {114}, number = {D10}, publisher = {American Geophysical Union (AGU)}, year = {2009}, doi = {10.1029/2008jd010325}, abstract = {Fifteen‐minute Meteosat Second Generation (MSG) Spinning Enhanced Visible and Infrared Imager (SEVIRI) infrared dust index images are used to identify dust source areas. The observations of dust source activation (DSA) are compiled in a 1° × 1° map for the Sahara and Sahel, including temporal information at 3‐hourly resolution. Here we use this data set to identify the most active dust source areas and the time of day when dust source activation occurs most frequently. In the Sahara desert 65% of DSA (March 2006 to February 2008) occurs during 0600–0900 UTC, pointing toward an important role of the breakdown of the nocturnal low‐level jet (LLJ) for dust mobilization. Other meteorological mechanisms may lead to dust mobilization including density currents initiated by deep convective systems which mobilize dust fronts (haboobs) occurring preferentially in the afternoon hours and cyclonic activities. The role of the nocturnal LLJ for dust mobilization in the Sahara is corroborated by regional model studies and analysis of meteorological station data.} } - Rusch, E. and Ramirez, M. (2019). Lunar Test Bed a Playground for Emerging Space Technology. minesnewsroom.com/news/lunar-test-bed-playground-emerging-space-techn...
BibTeX
@misc{rusch2019lunar, title = {Lunar Test Bed a Playground for Emerging Space Technology}, author = {Rusch, Emilie and Ramirez, Mark}, organization = {Colorado School of Mines Newsroom}, year = {2019}, url = {https://www.minesnewsroom.com/news/lunar-test-bed-playground-emerging-space-technology} } - Stoker, C. R., Glass, B. J., Stucky, T. R., Dave, A. I., Kobayashi, L. T., Quinn, R. C., Moreno-Paz, M., Sánchez-García, L., Mora, M. F., Kehl, F., Parro, V., Willis, P. A., Davila, A., Noe Dobrea, E., Rask, J. C. and Ricardo, D. (2023). A Mission Simulating the Search for Life on Mars with Automated Drilling, Sample Handling, and Life Detection Instruments Performed in the Hyperarid Core of the Atacama Desert, Chile
. Astrobiology. Source
BibTeX
@inproceedings{stoker2023mission, title = {A Mission Simulating the Search for Life on Mars with Automated Drilling, Sample Handling, and Life Detection Instruments Performed in the Hyperarid Core of the Atacama Desert, Chile}, author = {Stoker, Carol R. and Glass, Brian J. and Stucky, Thomas R. and Dave, Arwen I. and Kobayashi, Linda T. and Quinn, Richard C. and Moreno-Paz, Mercedes and Sánchez-García, Laura and Mora, Maria F. and Kehl, Florian and Parro, Víctor and Willis, Peter A. and Davila, Alfonso and Noe Dobrea, Eldar and Rask, Jon C. and Ricardo, Daniel}, booktitle = {Astrobiology}, publisher = {JPL Open Repository}, year = {2023}, doi = {10.48577/jpl.tx9qwo}, abstract = {We report on a field demonstration of a rover-based drilling mission to search for biomolecular evidence of life in the arid core of the Atacama Desert, Chile. The KREX2 rover carried the Honeybee Robotics one meter depth TRIDENT (The Regolith and Ice Drill for Exploration of New Terrains) drill and a robotic arm with scoop that delivered subsurface fines to three flight prototype instruments: 1) The Signs of Life Detector (SOLID), a protein and biomolecule analyzer based on Fluorescence Sandwich Microarray Immunoassay; 2) the Planetary In-Situ Capillary Electrophoresis System (PISCES), an amino acid analyzer based on Subcritical Water Extraction coupled to microchip electrophoresis analysis; and 3) a Wet Chemistry Laboratory cell to measure soluble ions using Ion Selective Electrodes and Chronopotentiometry. A California-based science team selected and directed drilling and sampling of three sites separated by hundreds of meters that included a light-toned basin area showing evidence of aqueous activity surrounded by rocky desert pavement. Biosignatures were detected in basin samples collected at depths ranging from 20 to 80 cm but were not detected in the surrounding area. Subsurface stratigraphy of the units drilled was interpreted from drill sensor data as fine-scale layers of sand/clay sediments interspersed with layers of harder material in the basins and a uniform subsurface composed of course-to-fine sand in the surroundings. The mission timeline and number of commands sent to accomplish each activity were tracked. The deepest sample collected (80 cm) required 55 commands including drilling and delivery to three instruments. Elapsed time required for drilling and sample handling was less than three hours to collect sample from 72 cm depth including time devoted to recovery from a jammed drill. The experiment demonstrated drilling, sample transfer technologies and instruments that accomplished successful detection of biomolecular evidence of life in one of the most biologically sparse environments on Earth.} } - Mantovani, J. G. (2001). A Study of the Electrostatic Interaction Between Insulators and Martian/Lunar Soil Simulants
. NASA Kennedy Space Center, 20020050541. Source
BibTeX
@techreport{mantovani2001study, title = {A Study of the Electrostatic Interaction Between Insulators and Martian/Lunar Soil Simulants}, author = {Mantovani, James G.}, number = {20020050541}, institution = {NASA Kennedy Space Center}, year = {2001}, url = {https://ntrs.nasa.gov/citations/20020050541}, abstract = {Using our previous experience with the Mars Environmental Compatibility Assessment (MECA) electrometer, we have designed a new type of aerodynamic electrometer. The goal of the research was to measure the buildup of electrostatic surface charge on a stationary cylindrical insulator after windborne granular particles have collided with the insulator surface in a simulated dust storm. The experiments are performed inside a vacuum chamber. This allows the atmospheric composition and pressure to be controlled in order to simulate the atmospheric conditions near the equator on the Martian surface. An impeller fan was used to propel the dust particles at a cylindrically shaped insulator under low vacuum conditions. We tested the new electrometer in a 10 mbar CO2 atmosphere by exposing two types of cylindrical insulators, Teflon (1.9 cm diameter) and Fiberglass (2.5 cm diameter), to a variety of windborne granular particulate materials. The granular materials tested were JSC Mars-1 simulant, which is a mixture of coarse and fine (<5microns diameter) particle sizes, and some of the major mineral constituents of the Martian soil. The minerals included Ottawa sand (SiO2), iron oxide (Fe2O3), aluminum oxide (Al2O3) and magnesium oxide (MgO). We also constructed a MECA-like electrometer that contained an insulator capped planar electrode for measuring the amount of electrostatic charge produced by rubbing an insulator surface over Martian and lunar soil simulants. The results of this study indicate that it is possible to detect triboelectric charging of insulator surfaces by windborne Martian soil simulant, and by individual mineral constituents of the soil simulant. We have also found that Teflon and Fiberglass insulator surfaces respond in different ways by developing opposite polarity surface charge, which decays at different rates after the particle impacts cease.} }