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Bearings and Lubrication

Bearings, seals and lubricants selected by flown and qualified planetary and orbital robotics programs, with the test or flight result that established each.

Three of the failures below were caused by the lubricant rather than the bearing. The Shuttle end effector snare bearings, which accelerate to about 7000 rpm in one second, failed repeatedly with a dry film until the design was changed to a wet grease [5]. The Apollo 16 Far Ultraviolet Camera azimuth ring stiffened on the Moon because it was packed with a grease normally used as a sealant, and the manual azimuth operation had never been run in a cold chamber [6]. Apollo suit seals and disconnects were relubricated with Krytox between EVAs and still clogged and leaked [7]. Lubricant selection is a qualification activity in its own right, and its test case is the duty cycle, not the bearing load.

Bearings and lubricants selected and flown

Section titled “Bearings and lubricants selected and flown”
PartManufacturerUsed bySource
71809SKFipex (wheel actuator output)[1][2]
71812SKFipex (bucket drum and arm actuator output)[1]
6706EZOipex (motor rotor)[1][2]
Cross roller bearingTHKrassor (shoulder actuator)[3]
Krytox 143AZ oilDuPontapollo-lrv[4]
Krytox oil and greaseDuPontApollo suit seals and disconnects[7]
Lubeco 905 dry filmLubecocanadarm-srms (end effector snare bearings)[5]
Braycote 3L-38 greaseBraycanadarm-srms (end effector snare bearings)[5]
Waxy low-outgassing greaseNot namedApollo 16 Far Ultraviolet Camera[6]
Pennzane 2001ANye LubricantsScreening baseline[9]
Zirconia and silicon nitride ballsNo vendor namedLunar mechanisms, candidate[8]
Spring-loaded PTFE rotary sealNo vendor namedspirit, opportunity (arm)[8]
Aeroflex rotary shaft sealAeroflexspirit, opportunity (steering)[8]
  • 71809, SKF: an angular contact ball bearing, back-to-back pair [1][2]. Ratings: Sized to fit over the harmonic drive flex cup and to react radial, axial and moment loads imparted from the terrain into the actuator [1][2]. Qualification: Survived the accelerated life test to 6,547,036 input revolutions. The failure in that test was at the motor rotor bearings, not at the output pair [1].
  • 71812, SKF: an angular contact ball bearing [1]. Ratings: Output bearings for the 160:1 excavation and arm actuators. Qualification: Covered by the same KSC campaign at 2-sigma load; results not published [1].
  • 6706, EZO: a deep groove ball bearing, wave-spring preloaded [2]. Ratings: Input bearings stacked close together, preloaded with a wave spring sized so the axial force generated by the harmonic drive wave generator could not overcome the spring [2]. Qualification: The preload calculation was wrong in practice. In the 3-sigma accelerated life test the wave generator moved axially into the flex cup regardless, and the rotor bearing springs failed, repeatedly tripping the motor current limit [1].
  • Cross roller bearing, THK. Crossed roller slewing bearing. Ratings: Carries radial, axial and moment loads in a single element between the ground side and the rotating side of the joint [3]. Qualification: Selected to remove a second bearing from the joint. The paper reports the sizing rationale and the fabrication difficulties of the 3D printed titanium housings that had to be machined coaxial to it, not a life test [3].
  • Krytox 143AZ oil, DuPont: a perfluoropolyether oil [4]. Ratings: Lubricates the 80:1 harmonic drive transmission of each wheel drive unit [4]. The motor and wave generator run sealed together in dry nitrogen at about 5.17 N/cm2 rather than in vacuum. Qualification: Flown on Apollo 15, 16 and 17 [4]. The sealed nitrogen approach was chosen over an open-to-vacuum alternate and the alternate had to be carried in parallel until the sealed unit was demonstrated under simulated lunar conditions [4].
  • Krytox oil and grease, DuPont. Perfluoropolyether oil and grease, on the extravehicular mobility unit zippers and on the helmet and glove disconnect seals. Ratings: Reapplied by the crew between EVAs [7]. Qualification: Ineffective against lunar dust. Relubrication helped but did not stop mechanisms clogging or seals leaking. Wrist bearings and rotational connectors had only a fabric cover, which was also not effective, and from Apollo 15 onward Velcro-attached dust covers were added to the front connectors [7].
  • Lubeco 905 dry film, Lubeco: a dry film lubricant [5]. Ratings: Original lubrication of the end effector throughout. In the wider arm, wet Bray grease is used in the small bearings and dry film in the other bearings, gears, ball screws and ball spline [5]. Qualification: Failed. Bearings required to accelerate to about 7000 rpm in one second failed rapidly through clogging with dry-lubricant debris [5].
  • Braycote 3L-38 grease, Bray: a perfluoropolyether grease [5]. Ratings: Replaced the dry film in the bearings that failed [5]. Qualification: No further problems to the date of the paper. The source names the same grease twice with different suffixes, 3L-38RP in the general arm description and 3L-38BP in the end effector fix, and does not reconcile them [5].
  • Waxy low-outgassing grease, type and vendor not named. Grease intended as a sealant rather than a lubricant, packed into the Far Ultraviolet Camera azimuth ring. Ratings: Packed into a 12.5 inch diameter unsealed ball bearing ring [6]. Qualification: Flight failure. Rotating the camera to each azimuth setting became progressively harder through the lunar stay. The grease stiffens appreciably below 50 F and the camera was deliberately kept in shade to protect the film [6]. No lunar dust was observed on the bearing; the cause was recorded as the wrong grease, and the manual azimuth operation had not been included in the cold chamber test program [6].
  • Pennzane 2001A, Nye Lubricants: a multiply alkylated cyclopentane, the reference lubricant against which candidate space oils are screened [9]. Ratings: Effective pressure-viscosity coefficient 11 GPa-1 at 21 C and 8.5 GPa-1 at 40 C, measured by elastohydrodynamic film thickness on the same rig as the candidates. Qualification: Used as the reference baseline in the spiral orbit tribometer campaign [9]. Candidate silahydrocarbons showed higher pressure-viscosity coefficients, 16 to 17 GPa-1 at 21 C, and a viscosity advantage extrapolated to -20 C. Results are published as curves against temperature and speed, Figs. 1, 2 and 4, not as single lifetimes [9].
  • Zirconia and silicon nitride balls, no vendor named. Ceramic rolling element bearings, a candidate for lunar surface mechanisms. Ratings: Very high hardness against dust abrasion; both run dry, which removes the lubricant from the failure set entirely in lunar vacuum [8]. Qualification: Scored highest of four dust-tolerant bearing types in a weighted trade study, with a clear gap to stainless steel and to hybrid superconducting magnetic bearings, on durability and dry running. The result is a trade score, Table 9, not a life test [8].
  • Spring-loaded PTFE rotary seal, no vendor named [8]. Spring-energized lip seal, outer diameters above about 1.5 inch, flown on the MER Instrument Deployment Device. Ratings: Flight heritage on the MER arm; tested in vacuum in the presence of lunar simulant [8]. Qualification: Effective and durable in simulant vacuum testing, and scored joint highest of three seal types in a weighted trade. Long-term stability under lunar temperature extremes and radiation remains open [8].
  • Aeroflex rotary shaft seal, Aeroflex. Dry running rotary shaft seal, on the MER wheel steering actuators. Ratings: Simple mechanism, no lubricant [8]. Qualification: Successfully limited regolith ingress in vacuum simulant testing. Requires high machining tolerances, is susceptible to misalignment on installation, and is affected by vibration; material selection for the lunar environment is unresolved [8].

A harmonic drive rated at 80 to 90 percent efficiency with a wet lubricant falls to as low as 50 percent unlubricated [10]. That factor of nearly two is larger than most motor sizing margins, so a dry-running mechanism is not the same mechanism with the oil left out. The IPEx Generation 1 campaign was built around this, instrumenting the actuator to separate motor, gearbox, bearing, seal and resolver losses precisely because published motor curves and gear efficiencies assume a grease, a temperature and an ambient pressure that the lunar case does not supply [2]. Measured seal drag came out at 0.03 N m maximum, under one percent of the load.

Screening a coating in air ranks it the wrong way round

Section titled “Screening a coating in air ranks it the wrong way round”

Six solid lubricating films on 440C disks were run against 6 mm 440C balls in one ball-on-disk rig at 0.49 to 3.6 N, 120 rpm, 31 to 107 mm/s and room temperature, in ultrahigh vacuum at 1e-7 Pa, in humid air at about 20 percent relative humidity, and in dry nitrogen below 1 percent [11]. Plasma-assisted CVD diamond-like carbon gives a steady-state friction coefficient of 0.07 and over a million passes to the 0.30 endurance threshold in the humid air, and 0.54 and fewer than ten passes in the vacuum. Resin-bonded MoS2 runs the other way, 0.14 and 113,570 passes in the humid air against 0.045 and over a million passes in the vacuum [11]. The two films rank in opposite order in the two environments, so a candidate coating screened in laboratory air can be the one that fails first in service.

Magnetron-sputtered MoSx against 440C in the same 1e-7 Pa vacuum has a nondimensional Holm-Archard wear coefficient of 5e-6 and a specific wear rate of 8e-7 mm3/(N.m), both independent of load across the 0.49 to 3.6 N range tested, and its endurance life falls with load as W to the power -1.4 [11]. That exponent is what an accelerated MoSx life test rests on when it raises contact pressure to buy cycles. All of it is one counterface, one temperature and unidirectional continuous sliding, which is neither a bearing nor an oscillating contact.

Four programs published a temperature, a fill fraction or a flight exposure against a named grease. The quantity that decides selection in every one of them is viscosity at the cold end, not load capacity [12][15].

PartManufacturerUsed bySource
Braycote 600EF greaseBrayperseverance (maxon bearings)[12]
Braycote 601EF greaseBrayRejected for sliding contacts[12]
Braycote lubricant, MSL actuatorsBraycuriosity (31 actuators)[13]
Bray 602 greaseBrayMars rover gearbox study[14]
Braycote 601 greaseCastrolLDEF drive shafts[15]
Apiezon H thermal greaseApiezonLDEF heat pipe[15]
PentasilahydrocarbonNot namedScreening candidate[9]
Krytox 143AB oilDuPontScreening baseline[9]
  • Braycote 600EF grease, Bray, in the Mars 2020 maxon flat motor bearings [12]. Ratings: filled to 15 to 20 percent of free volume, measured by mass and documented per bearing [12]. Qualification: the fill fraction was set from ExoMars gearbox lifetime failures rather than from a new test. The same grease in the Perseverance coring drill percussion mechanism had to be cut to about 3 percent of free volume for a -70 C cold start [18], which is recorded on Gearing and Actuators.
  • Braycote 601EF grease, Bray [12]. Ratings: considered for the same gearbox. Qualification: found fundamentally unsuitable for sliding surfaces, so the gearbox planet sliding contacts were converted to rolling contact on needle bearings [12]. The lubricant decision changed the bearing architecture rather than the other way round.
  • Braycote lubricant, MSL actuators, Bray. Ratings: the lubricant viscosity sets the minimum allowable temperature for the actuator [13]. Qualification: all 31 MSL actuators were qualified by soak at -70 C, and 15 C of margin was added to give a -55 C minimum operational allowable flight temperature for the input stage against -70 C for the output stage [13].
  • Bray 602 grease, Bray, in a planetary gearbox for a Mars rover actuator study [14]. Ratings: measured on three of the five stages of the primary gearbox with a torque watch. Qualification: input torque is nearly linear from ambient down to -75 C and then rises tenfold between -75 and -95 C [14]. The knee, not the ambient value, is the number an actuator is sized against.
  • Braycote 601 grease, Castrol, on Long Duration Exposure Facility trailing edge drive shafts for 69 months [15]. Ratings: PTFE-filled perfluoropolyether, exposed to ultraviolet with no atomic oxygen [15]. Qualification: base oil viscosity came back lower than the control, interpreted as ultraviolet chain scission of the polyether. Infrared showed no new carbonyl, so no oxidation, but new peaks between 1100 and 1400 wavenumbers suggest degradation of the PTFE filler, and two new differential scanning calorimetry endotherms appeared at about 106 C and 211 C, the second unexplained [15]. The grease had darkened to black and the cause was not identified.
  • Apiezon H thermal grease, Apiezon, on a heat pipe flown on the same facility, shielded from atomic oxygen and ultraviolet. Ratings: tested after flight against a control under NASA SP-13-0022A [15]. Qualification: total mass loss 2.32 percent flight against 0.97 percent control, with volatile condensable material similar at 0.66 against 0.58 percent [15]. The authors attribute the difference to moisture picked up between retrieval and test, and reproduced it by humidity conditioning a control to 1.38 percent.
  • Pentasilahydrocarbon, vendor not named, a candidate space oil of a structure similar to MJD991029. Ratings: pressure-viscosity coefficient 17 plus or minus 0.3 GPa-1 at 21 C and 13.5 plus or minus 1 at 40 C, estimated from elastohydrodynamic film thickness [9]. Qualification: 1000 hours in an MPB 1219 angular contact bearing with 440C balls and races, 20 mg of free oil, 600 rpm, 75 C, 20 lb axial load at 1e-5 Pa, ending with no degradation and ample free oil remaining [9]. Single specimens, all fluids unformulated.
  • Krytox 143AB oil, DuPont [9]. Ratings: run as a comparison in the same 1000 hour vacuum bearing test. Qualification: the bearing ran dry and the oil degraded, while Pennzane 2001A was comparable to the silahydrocarbon [9]. The Krytox family flew on the Apollo Lunar Roving Vehicle transmission in a sealed nitrogen atmosphere rather than in vacuum, and that seal is what this test removes.

Cold welding measured as an adhesion force

Section titled “Cold welding measured as an adhesion force”

Metal-to-metal contact under vacuum was measured on a pin-on-disc rig below 5e-8 mbar, with the static load stepped to the full Hertzian elastic limit, an impact energy forty times the yield energy, specimens ground to below 0.1 micrometer Ra, and ten seconds closed and ten open per cycle [16]. Aluminum alloy AA7075 against itself gave the highest uncoated adhesion of the set, 1775 mN under impact, above titanium and against the common assumption that titanium is the dangerous contact material. Titanium alloy IMI834 against AISI 440C stainless gave 9500 mN under fretting at only 4 N of applied load, against 960 mN under impact at 29 N and below 100 mN in static contact after 25000 cycles at the same 29 N [16]. Fretting at a quarter of the load produced ten times the adhesion of impact, so a static contact test does not bound a joint that vibrates.

DuPont Vespel SP3, a polyimide filled with 15 mass percent molybdenum disulphide, against the same stainless gave 5 mN under impact and 58 mN under fretting, because no metal-to-metal bond can form [16]. The same family fared as well in flight: Vespel SP-21, a graphite-filled polyimide, was exposed for 69 months on the Long Duration Exposure Facility and its friction coefficient after retrieval was unchanged from unflown controls, about 0.15 after run-in over 10000 cycles [15]. That friction number was measured on a ground tribometer in laboratory air, so what the flight establishes is that the exposure did not change it. A tungsten disulphide dry film on the same facility’s grapple shafts came back with the bulk lubricant intact and no discernible difference between ram and trailing surfaces, but no surface analysis was performed and its tribological properties were never measured after flight [15].

Dust in a sliding contact roughens the softer face

Section titled “Dust in a sliding contact roughens the softer face”

Titanium alloy coupons were run against aluminum 6061 and PTFE discs for three minutes at 1.3 rpm and 8.6e-5 torr, with and without about 142 g/m2 of LHS-1D lunar simulant [17]. Against aluminum the coupon surface roughness came out at 0.014 plus or minus 0.002 micrometers with dust and 0.008 plus or minus 0.001 without, from an as-polished control of 0.005. Against PTFE the pairing gave 0.012 plus or minus 0.003 with dust and 0.006 plus or minus 0.001 without, the dust-free case being statistically indistinguishable from the as-polished surface [17]. Both dusted increases are significant at p below 0.05, over three profilometry regions of 1 mm each, in a three minute test that is not a life test.

References

  1. Schuler, J. M., Smith, J. D., Nick, A. J., Buckles, B. C., Dyas, J. E., Ortega, V. V., Cloud, J. M., Dokos, A. G., Zhang, E. L., Wang, J. J., Baron, M. A., Muller, T. J., Clark, C. J. and Howe, M. W. (2024). ISRU Pilot Excavator (IPEx) Technology Readiness Level 5 Design Overview . AIAA AVIATION Forum and ASCEND, 20240008162. Source
    BibTeX
    @inproceedings{schuler2024isru,
      title = {ISRU Pilot Excavator (IPEx) Technology Readiness Level 5 Design Overview},
      author = {Schuler, Jason M. and Smith, Jonathan D. and Nick, Andrew J. and Buckles, Bradley C. and Dyas, Jeffrey E. and Ortega, Victoria V. and Cloud, Joseph M. and Dokos, Adam G. and Zhang, Elizabeth L. and Wang, Jerry J. and Baron, Michael A. and Muller, Thomas J. and Clark, Casey J. and Howe, Musashi W.},
      booktitle = {AIAA AVIATION Forum and ASCEND},
      number = {20240008162},
      institution = {NASA},
      year = {2024},
      doi = {10.2514/6.2024-4890},
      abstract = {This paper details the mechanical and mechatronic design of the Technology Readiness Level (TRL)-5 In-Situ Resource Utilization (ISRU) Pilot Excavator (IPEx). IPEx is a robotic excavator designed for a technology demonstration of regolith mining in the lunar south pole region. The novel design uses pairs of counter-acting excavation tools called bucket drums, that dig at the same time in opposing directions to reduce the reaction force needed, thereby enabling mining with a small, low-mass, robotic system. IPEx builds on the prior work of the Regolith Advanced Surface Systems Operations Robot (RASSOR), which is the TRL-4 implementation of this concept. The TRL-5 IPEx subsystems that are discussed in this paper include: Regolith Delivery Subsystem (RDS), Mobility Subsystem (MS), Cameras and Dust Mitigation Subsystem (CDMS), and Thermal Control Subsystem (TCS). Each subsystem is described in detail with rationale for design selections. Dust tolerance is a key feature for IPEx, and this paper details a thermal control system with an actuated radiator cover and phase change material as well as camera modules with removable electrodynamic dust shields (EDS). Additional components such as actuators, wheels, and bucket drums are discussed in detail. Due to their complexity, the avionics and software subsystems will be discussed in a separate publication.}
    }
  2. Clark, C. J., Smith, J. D., Nick, A. J., Ortega, V. V., Schuler, J. M., Dyas, J. E. and Lahl, J. (2025). Design and Testing of TRL5 IPEx Actuators . IEEE Aerospace Conference, 20250000003. Source
    BibTeX
    @inproceedings{clark2025design,
      title = {Design and Testing of TRL5 IPEx Actuators},
      author = {Clark, Casey J. and Smith, Jonathan Drew and Nick, Andrew J. and Ortega, Victoria V. and Schuler, Jason M. and Dyas, Jeffrey E. and Lahl, John},
      booktitle = {IEEE Aerospace Conference},
      number = {20250000003},
      institution = {NASA},
      address = {Big Sky, MT},
      year = {2025},
      url = {https://ntrs.nasa.gov/citations/20250000003},
      abstract = {NASA is advancing In-Situ Resource Utilization (ISRU) by focusing on missions aimed at establishing sustainable infrastructure on the Moon and Mars. On the Moon, regolith serves as the most abundant resource. To support ISRU objectives, a 30-kg-class robot called ISRU Pilot Excavator (IPEx) is being developed to excavate 10,000 kg of lunar regolith during a future technology demonstration mission. IPEx uses novel excavation tools, called bucket drums, which are hollow cylinders with scoops staggered around the outside. Regolith is collected with the scoops and flows into the drum where it is captured by an internal baffle system. The excavator can then transport the regolith in the drum and reverse the direction of the drum rotation to dispense the regolith out. IPEx uses two sets of bucket drums that dig simultaneously in opposing directions and results in counteracting excavation forces. This combination of bucket drum excavation tools and counteracting excavation forces enables low mass robotic excavators to effectively dig in reduced gravity environments. This is a significant departure from terrestrial excavators that rely on high mass to produce tractive forces to counteract the forces of excavation.
    
    IPEx is made up of several custom actuators that all need to be verified for their intended application. This paper focuses on the initial design, testing and modifications of three actuators: the mobility actuator, the shoulder actuator, and the excavation actuator.
    
    Each actuator was tested under four separate test profiles: ambient motor characterization, hot and cold motor characterization, accelerated life test (ALT), and concept of operations (ConOps) test. The motor characterization tests enabled derivation of torque equations for each actuator to estimate output torque without implementing sensors. The accelerated life tests were successful for each actuator and verified the motors’ ability to survive the mission. For the ConOps test, only the bucket drum actuator performed a complete ConOps without the need to restart the test. Overall, the first series of testing resulted in various failure modes and minor design alterations for each actuator. The test results, failure modes, and design alterations are highlighted within this paper. This paper focuses on discussing the mobility, excavation, and shoulder actuator design, testing principles, and results that qualified it as a TRL 5 system.}
    }
  3. Mueller, R. P., Smith, J. D., Schuler, J. M., Nick, A. J., Gelino, N. J., Leucht, K. W., Townsend, I. I. and Dokos, A. G. (2016). Design of an Excavation Robot: Regolith Advanced Surface Systems Operations Robot (RASSOR) 2.0 . Earth and Space, 20210011366. Source
    BibTeX
    @inproceedings{mueller2016design,
      title = {Design of an Excavation Robot: Regolith Advanced Surface Systems Operations Robot (RASSOR) 2.0},
      author = {Mueller, Robert P. and Smith, Jonathan D. and Schuler, Jason M. and Nick, Andrew J. and Gelino, Nathan J. and Leucht, Kurt W. and Townsend, Ivan I. and Dokos, Adam G.},
      booktitle = {Earth and Space},
      number = {20210011366},
      pages = {163-174},
      institution = {NASA},
      year = {2016},
      doi = {10.1061/9780784479971.018},
      abstract = {To continue on a sustainable and flexible path, NASA needs to address the challenge of collecting and moving large amounts of regolith at the destination. Acquiring the water resources on Mars will require mining significant quantities of regolith, and this is not possible with the state-of-the-art low mass excavation systems. Low gravity environments (Mars = 3/8G) and launch mass restrictions limit the traction and the resulting reaction force of the vehicle, making current terrestrial techniques impractical. This project addressed this challenge by developing a completely new technology that can mine large quantities of regolith on Mars. Recent measurements by the “Curiosity” rover on Mars have found that the regolith contains ~2% water by weight globally, ~4% in Jezero Crater (Human Architecture Team’s reference landing site), and much more at the poles. RASSOR 2.0 is a planetary excavator, which has a mass of 66 kg, with a 0.38 kg vehicle mass per kilogram, per hour of excavation rate and power usage of 4 W per kg of regolith excavation rate. A single RASSOR 2.0 can excavate a minimum of 2.7 metric tons of regolith per day. This is accomplished by using counteracting excavation forces on two opposing digging implements called bucket drums and an autonomous mining control system. This work has addressed several major research areas outlined in the NASA Technology Area (TA) 04 Robotics and Autonomous Systems and TA 07 Human Destination Systems roadmaps. This project started at Technology Readiness Level (TRL) 4 as a low fidelity “proof of concept” prototype which has successfully demonstrated basic regolith simulant excavation functionality in a lab-scale gravity off load test. The foundational technology described here was awarded US patent number: US 9027265 for a “Zero horizontal reaction force excavator” on May 12, 2015.}
    }
  4. Jones, C. S. J. and Nola, F. J. (1971). Mobility systems activity for lunar rovers at MSFC . NASA, NASA-TM-. Source
    BibTeX
    @techreport{jones1971mobility,
      title = {Mobility systems activity for lunar rovers at MSFC},
      author = {Jones, C. S., Jr. and Nola, F. J.},
      number = {NASA-TM-},
      institution = {NASA},
      year = {1971},
      url = {https://ntrs.nasa.gov/citations/19720004516},
      abstract = {The Apollo Lunar Roving Vehicle (LRV) mobility system is described. Special emphasis is given to the redundancy aspects and to the selection of the drive motors. A summary chart of the performance on the lunar surface during the Apollo 15 flight is included. An appendix gives details on some development work on high efficiency drive systems and compares these systems to the selected system.}
    }
  5. Daniell, R. G. and Sachdev, S. S. (1982). The Design and Development of an End Effector for the Shuttle Remote Manipulator System . Aerospace Mechanisms Symposium, 19820015473. Source
    BibTeX
    @inproceedings{daniell1982design,
      title = {The Design and Development of an End Effector for the Shuttle Remote Manipulator System},
      author = {Daniell, R. G. and Sachdev, S. S.},
      booktitle = {Aerospace Mechanisms Symposium},
      number = {19820015473},
      institution = {NASA},
      year = {1982},
      url = {https://ntrs.nasa.gov/citations/19820015473},
      abstract = {The design requirements, the design, and qualification and development test problems encountered on the Remote Manipulator End Effector are described. The constraints and interfaces with the arm, the Orbiter, and the payload are identified. The design solution to meet the requirements is a unique device that provides a soft-docking feature termed capture and a hard-docking feature termed rigidization.}
    }
  6. (1972). Apollo 16 Mission Report . NASA, NASA-TM-. Source
    BibTeX
    @techreport{anon1972apollo,
      title = {Apollo 16 Mission Report},
      number = {NASA-TM-},
      institution = {NASA},
      year = {1972},
      url = {https://ntrs.nasa.gov/citations/19720026127},
      abstract = {Information is provided on the operational and engineering aspects of the Apollo 16 mission. Customary units of measurement are used in those sections of the report pertaining to spacecraft systems and trajectories. The International System of Units is used in sections pertaining to science activities.}
    }
  7. Gaier, J. R. (2005). The Effects of Lunar Dust on EVA Systems During the Apollo Missions . NASA Glenn Research Center, NASA/TM-2005-213610, 20050160460. Source
    BibTeX
    @techreport{gaier2005effects,
      title = {The Effects of Lunar Dust on EVA Systems During the Apollo Missions},
      author = {Gaier, James R.},
      number = {NASA/TM-2005-213610, 20050160460},
      institution = {NASA Glenn Research Center},
      year = {2005},
      url = {https://ntrs.nasa.gov/citations/20050160460},
      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.}
    }
  8. Cannon, K. M., Dreyer, C. B., Sowers, G. F., Schmit, J., Nguyen, T., Sanny, K. and Schertz, J. (2022). Working with lunar surface materials: Review and analysis of dust mitigation and regolith conveyance technologies . Acta Astronautica. Source
    BibTeX
    @article{cannon2022working,
      title = {Working with lunar surface materials: Review and analysis of dust mitigation and regolith conveyance technologies},
      author = {Cannon, Kevin M. and Dreyer, Christopher B. and Sowers, George F. and Schmit, John and Nguyen, Thao and Sanny, Keoni and Schertz, Joshua},
      journal = {Acta Astronautica},
      volume = {196},
      pages = {259--274},
      year = {2022},
      doi = {10.1016/j.actaastro.2022.04.037},
      abstract = {The Moon's dusty surface environment threatens any equipment that operates there, especially for long-duration infrastructure needed for a sustained lunar presence. This is doubly true for systems that convey regolith, which by agitating the soil are certain to generate dust. Here, we provide a comprehensive review of technologies that have been proposed to convey regolith on the lunar surface, and to mitigate against dust hazards that are generated by such transport systems. We define functional taxonomies for both regolith conveyance and dust mitigation, then carry out quantitative trade studies in several categories for each. Examples include passive and active dust mitigation, and horizontal and near vertical conveyance. Conveyance technologies that scored particularly high include wheeled haulers, conveyor belts, and auger/hopper transfer points. High scoring dust mitigation technologies include the lotus leaf passive coating, Electrodynamic Dust Shield, and boots or bellow made of fiberglass fabric. We also explore novel or unconventional concepts and describe how dust mitigation and regolith conveyance can be combined using a systems approach with multiple technologies layered together. The results from the trade studies and the subsequent recommendations constitute a practical guide that can be used for designing and developing systems that must perform efficiently and reliably to carry out useful tasks on the Moon or Mars, such as resource extraction, construction, and additive manufacturing.}
    }
  9. Jones, W. R. J., Jansen, M. J., Gschwender, L. J., Snyder, C. E. J., Sharma, S. K., Predmore, R. E. and Dube, M. J. (2001). The Tribological Properties of Several Silahydrocarbons for Use in Space Mechanisms . Journal of Synthetic Lubrication, NASA/TM-2001-211196. Source
    BibTeX
    @article{jones2001tribological,
      title = {The Tribological Properties of Several Silahydrocarbons for Use in Space Mechanisms},
      author = {Jones, W. R., Jr. and Jansen, M. J. and Gschwender, L. J. and Snyder, C. E., Jr. and Sharma, Shiv K. and Predmore, R. E. and Dube, Michael J.},
      journal = {Journal of Synthetic Lubrication},
      volume = {20},
      number = {NASA/TM-2001-211196},
      pages = {303-315},
      institution = {NASA},
      address = {Liege},
      year = {2001},
      doi = {10.1002/jsl.3000200404},
      abstract = {Abstract Silahydrocarbons are members of a relatively new class of liquid lubricants with great potential for use in space mechanisms. They are unimolecular species consisting of silicon, carbon, and hydrogen. They possess unique wear, viscosity, and volatility properties while retaining the ability to solubilise conventional additives. The tribological properties of several members of this class, including tri‐, tetra‐, and penta‐compounds, are presented. These properties include viscosity‐temperature, viscosity—pressure, vapour pressure, lubricant life, traction, and reciprocating and four‐ball wear rates. Lubricant lifetimes were determined using a vacuum ball bearing simulator, the spiral orbit tribometer. Wear was measured using a Cameron Plint reciprocating tribometer and wear rates with a vacuum four‐ball tribometer. Conventional viscometry was used for viscosity—temperature measurements and a Knudsen cell for vapour pressure. Thermogravimetric analysis was also used for volatility measurements. Pressure—viscosity coefficients (α—values) were estimated from elastohydrodynamic lubrication film thickness measurements. These properties are compared to those of existing state‐of‐the‐art space lubricants.}
    }
  10. Chun, W. and Brunson, P. (1987). Actuators for a Space Manipulator . NASA, 19890000730. Source
    BibTeX
    @techreport{chun1987actuators,
      title = {Actuators for a Space Manipulator},
      author = {Chun, W. and Brunson, P.},
      number = {19890000730},
      institution = {NASA},
      year = {1987},
      url = {https://ntrs.nasa.gov/citations/19890000730},
      abstract = {The robotic manipulator can be decomposed into distinct subsytems. One particular area of interest of mechanical subsystems is electromechanical actuators (or drives). A drive is defined as a motor with an appropriate transmission. An overview is given of existing, as well as state-of-the-art drive systems. The scope is limited to space applications. A design philosophy and adequate requirements are the initial steps in designing a space-qualified actuator. The focus is on the d-c motor in conjunction with several types of transmissions (harmonic, tendon, traction, and gear systems). The various transmissions will be evaluated and key performance parameters will be addressed in detail. Included in the assessment is a shuttle RMS joint and a MSFC drive of the Prototype Manipulator Arm. Compound joints are also investigated. Space imposes a set of requirements for designing a high-performance drive assembly. Its inaccessibility and cryogenic conditions warrant special considerations. Some guidelines concerning these conditions are present. The goal is to gain a better understanding in designing a space actuator.}
    }
  11. Miyoshi, K. (2000). Solid Lubrication Fundamentals and Applications, Chapter 6: Friction and Wear Properties of Selected Solid Lubricating Films . NASA Glenn Research Center, NASA/TM-2000-107249, Chapter 6. Source
    BibTeX
    @techreport{miyoshi2000solid,
      title = {Solid Lubrication Fundamentals and Applications, Chapter 6: Friction and Wear Properties of Selected Solid Lubricating Films},
      author = {Miyoshi, Kazuhisa},
      number = {NASA/TM-2000-107249, Chapter 6},
      institution = {NASA Glenn Research Center},
      year = {2000},
      url = {https://ntrs.nasa.gov/citations/20010017158},
      abstract = {This chapter focuses attention on the friction and wear properties of selected solid lubricating films to aid users in choosing the best lubricant, deposition conditions, and operational variables. For simplicity, discussion of the tribological properties of concern is separated into two parts. The first part of the chapter discusses the different solid lubricating films selected for study including commercially developed solid film lubricants: (1) bonded molybdenum disulfide (MoS2), (2) magnetron-sputtered MoS2, (3) ion-plated silver, (4) ion-plated lead, (5) magnetron-sputtered diamondlike carbon (MS DLC), and (6) plasma-assisted, chemical-vapor-deposited diamondlike carbon (PACVD DEC) films. Marked differences in the friction and wear properties of the different films resulted from the different environmental conditions (ultrahigh vacuum, humid air, and dry nitrogen) and the solid film lubricant materials. The second part of the chapter discusses the physical and chemical characteristics, friction behavior, and endurance life of the magnetron-sputtered MoS2 films. The role of interface species and the effects of applied load, film thickness, oxygen pressure, environment, and temperature on the friction and wear properties are considered.}
    }
  12. Loschiavo, M., Phillips, R., Mikhaylov, R. and Braunschweig, L. (2020). Mars 2020 Maxon Commercial Motor Development from COTS to Flight Qualified Motors, Gearbox, and Detent Brake: Issues Overcome and Lessons Learned . Aerospace Mechanisms Symposium. Source
    BibTeX
    @inproceedings{loschiavo2020mars,
      title = {Mars 2020 Maxon Commercial Motor Development from COTS to Flight Qualified Motors, Gearbox, and Detent Brake: Issues Overcome and Lessons Learned},
      author = {Loschiavo, Michael and Phillips, Robin and Mikhaylov, Rebecca and Braunschweig, Lynn},
      booktitle = {Aerospace Mechanisms Symposium},
      publisher = {JPL Open Repository},
      year = {2020},
      url = {https://dataverse.jpl.nasa.gov/dataset.xhtml?persistentId=hdl:2014/52357}
    }
  13. Novak, K. S., Liu, Y., Lee, C.-J. and Hendricks, S. (2010). Mars Science Laboratory rover actuator thermal design . International Conference on Environmental Systems. Source
    BibTeX
    @inproceedings{novak2010mars,
      title = {Mars Science Laboratory rover actuator thermal design},
      author = {Novak, Keith S. and Liu, Yuanming and Lee, Chern-Jiin and Hendricks, Steven},
      booktitle = {International Conference on Environmental Systems},
      publisher = {American Institute of Aeronautics and Astronautics},
      year = {2010},
      doi = {10.2514/6.2010-6196},
      abstract = {NASA will launch a 900 kg rover, part of the Mars Science Laboratory (MSL) mission, to Mars in October of 2011. The MSL rover is scheduled to land on Mars in August of 2012. The rover employs 31, electric-motor driven actuators to perform a variety of engineering and science functions including: mobility, camera pointing, telecommunications antenna steering, soil and rock sample acquisition and sample processing. This paper describes the MSL rover actuator thermal design. The actuators have stainless steel housings and planetary gearboxes that are lubricated with a wet lubricant. The lubricant viscosity increases with decreasing temperature. Warm-up heaters are required to bring the actuators up to temperature (above -55 C) prior to use in the cold wintertime environment of Mars (when ambient atmosphere temperatures are as cold as -113 C). Analytical thermal models of all 31 MSL actuators have been developed. The actuators have been analyzed and warm-up heaters have been designed to improve actuator performance in cold environments. Thermal hardware for the actuators has been specified, procured and installed. This paper presents actuator thermal analysis predicts, and describes the actuator thermal hardware and its operation. In addition, warm-up heater testing and thermal model correlation efforts for the Remote Sensing Mast (RSM) elevation actuator are discussed.}
    }
  14. Gillis-Smith, G. R. (1996). Mars Pathfinder Lander Deployment Mechanisms . JPL Open Repository. Source
    BibTeX
    @inproceedings{gillissmith1996mars,
      title = {Mars Pathfinder Lander Deployment Mechanisms},
      author = {Gillis-Smith, Greg R.},
      publisher = {JPL Open Repository},
      year = {1996},
      url = {https://dataverse.jpl.nasa.gov/dataset.xhtml?persistentId=hdl:2014/24167}
    }
  15. Dursch, H. W., Spear, W. S., Miller, E. A., Bohnhoff-Hlavacek, G. L. and Edelman, J. (1992). Analysis of systems hardware flown on LDEF. Results of the systems special investigation group . Legacy CDMS, 19920022433. Source
    BibTeX
    @techreport{dursch1992analysis,
      title = {Analysis of systems hardware flown on LDEF. Results of the systems special investigation group},
      author = {Dursch, Harry W. and Spear, W. Steve and Miller, Emmett A. and Bohnhoff-Hlavacek, Gail L. and Edelman, Joel},
      number = {19920022433},
      institution = {Legacy CDMS},
      year = {1992},
      url = {https://ntrs.nasa.gov/citations/19920022433},
      abstract = {The Long Duration Exposure Facility (LDEF) was retrieved after spending 69 months in low Earth orbit (LEO). LDEF carried a remarkable variety of mechanical, electrical, thermal, and optical systems, subsystems, and components. The Systems Special Investigation Group (Systems SIG) was formed to investigate the effects of the long duration exposure to LEO on systems related hardware and to coordinate and collate all systems analysis of LDEF hardware. Discussed here is the status of the LDEF Systems SIG investigation through the end of 1991.}
    }
  16. Merstallinger, A., Semerad, E. and Dunn, B. D. (2003). Influence of Coatings and Alloying on Cold Welding due to Impact and Fretting . European Space Mechanisms and Tribology Symposium. Source
    BibTeX
    @inproceedings{merstallinger2003cold,
      title = {Influence of Coatings and Alloying on Cold Welding due to Impact and Fretting},
      author = {Merstallinger, A. and Semerad, E. and Dunn, B. D.},
      booktitle = {European Space Mechanisms and Tribology Symposium},
      year = {2003},
      url = {https://www.esmats.eu/esmatspapers/pastpapers/pdfs/2003/merstallinger.pdf}
    }
  17. Wiesner, V. L., King, G. C., Domack, C. S., Widener, B. M., Gordon, K. L. and Wohl, C. J. (2024). Testbed for Lunar Extreme Environment Wear Tolerant Applications . Aerospace Mechanisms Symposium. Source
    BibTeX
    @inproceedings{wiesner2024testbed,
      title = {Testbed for Lunar Extreme Environment Wear Tolerant Applications},
      author = {Wiesner, Valerie L. and King, Glen C. and Domack, Christopher S. and Widener, Brandon M. and Gordon, Keith L. and Wohl, Christopher J.},
      booktitle = {Aerospace Mechanisms Symposium},
      address = {Hampton, Virginia},
      year = {2024},
      url = {https://ntrs.nasa.gov/citations/20240003704},
      abstract = {The abrasive dust from lunar regolith poses significant long-term durability and performance challenges to materials, vehicles, mechanisms and structures that will be used for the next generation of lunar exploration. The development of advanced materials, coatings and device technologies that can withstand these abrasive particles and extreme environmental conditions is critical. However, the lack of standardized and accessible methods for evaluating such materials and devices in a facsimile of the harsh lunar environment hinders progress in dust-tolerant technologies. To address this challenge, NASA Langley Research Center is creating an extreme environment testbed. This reconfigurable testbed will allow rapid, repeatable wear testing of material and candidate mechanisms under vacuum conditions, facilitating the development of critical materials technologies for lunar exploration. Preliminary results from exposing an actuating mechanism similar to a pin joint to lunar regolith simulant under high vacuum are reported.}
    }
  18. Chrystal, K. (2020). Percussion Mechanism for the Mars2020 Coring Drill . Aerospace Mechanisms Symposium. Source
    BibTeX
    @inproceedings{chrystal2020percussion,
      title = {Percussion Mechanism for the Mars2020 Coring Drill},
      author = {Chrystal, Kyle},
      booktitle = {Aerospace Mechanisms Symposium},
      publisher = {JPL Open Repository},
      year = {2020},
      url = {https://dataverse.jpl.nasa.gov/dataset.xhtml?persistentId=hdl:2014/52361}
    }