Canadian Lunar Rover
Program pages Canadian Space Agency: Canadian lunar rover mission Canadensys Aerospace: Canadian Lunar Rover
Overview
Section titled “Overview”The Canadian Lunar Rover is a solar-powered micro-rover being built by Canadensys Aerospace under contract to the Canadian Space Agency, to be delivered to the lunar south polar region on a NASA Commercial Lunar Payload Services flight [3], [4], [15]. It is the flagship of the Lunar Exploration Accelerator Program, one of three initiatives funded by the Canadian government’s February 2019 commitment of $2.05 billion alongside Canadarm3 for the Lunar Gateway and an education program, and it will be the first Canadian-led planetary exploration mission [13]. It joins a wider surge of lunar surface missions: nine landers and rovers reached the Moon between 2019 and 2024, four of them unsuccessfully [2].
Canadensys was selected as prime contractor in November 2022, the preliminary design review was completed in June 2024, and the project entered Phase C in July 2024 [13]. The science team is led from the University of Western Ontario, with instruments from Canadensys, Bubble Technology Industries and the Johns Hopkins Applied Physics Laboratory [11], [13].
The mission has three high-level objectives, in the order the team states them: demonstrate and characterize Canadian technology on the lunar surface, perform meaningful science, and increase the Canadian space sector’s readiness for later lunar missions [11], [12]. The rover is to traverse away from its landing site into intermittently and permanently shadowed areas, and the specific engineering claim made for it is that it would be the first solar-only rover to survive the lunar night [4].
Specifications
Section titled “Specifications”| Parameter | Value | Source |
|---|---|---|
| Mass | about 42 kg | [4] |
| Volume | about 0.4 m3 | [4] |
| Power | solar | [3], [4] |
| Science instruments | 6 | [13] |
| Additional cameras | 2 panoramic, 1 hazard | [13] |
| Permanently shadowed region endurance goal | up to 1 hour | [11], [12], [13] |
| Night survival goal | at least one lunar night | [4], [13] |
Wheel count, suspension, drive speed, slope limit, obstacle capability, ground pressure, generation capacity, battery capacity, processor and communications parameters are not published in any of the mission’s own abstracts. The mass has moved across those abstracts: 30 kg in the science team’s 2023 and 2024 conference papers, 35 kg in the agency’s own 2024 statement and the science team’s 2025 paper, and about 42 kg in the agency’s 2026 statement, with no explanation of the change [3], [4], [11], [12], [13].
Mission profile
Section titled “Mission profile”| Parameter | Value | Source |
|---|---|---|
| Delivery | NASA CLPS flight awarded to Firefly Aerospace | [4] |
| Launch | 2029 | |
| Destination | lunar south polar region | |
| Duration | multiple lunar days |
The delivery date has moved with the program: no earlier than late 2026 in 2023, no earlier than 2026 in the agency’s 2024 statement, and 2029 with a named provider in 2026 [4], [12], [13]. A separate and much larger Canadian vehicle, the Lunar Utility Vehicle, is on a different track: a ten-year design life, concept study contracts awarded to Canadensys, MDA Space and Mission Control in July 2025, and launch no earlier than 2033 [4].
One constraint shaped the design from the start. The landing site was to be chosen only after the mission and its instruments were selected, and high landing accuracy could not be assumed from the small commercial landers then in development, so the rover had to be designed without knowing precisely where it would be put down [11], [12]. Site selection has since narrowed to 13 candidate areas of 5 by 5 km, chosen to maximize operating time while staying close to modeled near-surface ice stability [13].
Mobility
Section titled “Mobility”Not published. None of the mission’s five abstracts states a wheel count, suspension type, drive speed, gradeability, obstacle height or ground pressure, and no terramechanics result appears. What is published about mobility is the objective: traverse away from the landing site into intermittently and permanently shadowed areas [4]. Parabolic-flight testing of wheel-soil interaction in lunar gravity, on other rover wheel designs, has measured drawbar pull to weight falling 20 percent or more and sinkage rising up to 40 percent against identically loaded 1 g tests, so a wheel design validated only on Earth is not a reliable predictor of lunar performance [5], [10].
Power and energy
Section titled “Power and energy”Solar only [3], [4]. No generation figure, battery capacity or duty cycle is published. The absence matters, because both distinguishing capabilities claimed for the vehicle are energy problems: operating for up to an hour inside a permanently shadowed region, where there is no sunlight, and surviving a lunar night on solar power alone [4], [11], [12], [13]. A solar-only rover operating near the pole has a Canadian precedent in method rather than hardware: Carnegie Mellon’s Hyperion demonstrated sun-synchronous route planning, timing travel to keep a fixed array facing the Sun, in two 24-hour circuits at Devon Island in the Canadian High Arctic [14].
Thermal
Section titled “Thermal”No temperature limits, heater strategy or radiator design is published. Night survival and the permanently shadowed region excursion are stated as goals rather than as analyzed or tested capability [4], [13]. The environment they would have to survive is documented independently of the mission: Apollo 15 measured diurnal extremes of 374 K to 92 K [7], and NASA’s cross-program design specification sets equatorial design extremes of 391 K at local noon against 96 K before sunrise, with permanently shadowed regions colder still [9].
Compute and avionics
Section titled “Compute and avionics”Not published. A Teledyne UDOS007 micro-dosimeter hybrid microcircuit records total ionizing dose in silicon through the mission, but that is a science instrument rather than a statement about the avionics it sits beside [13].
Autonomy
Section titled “Autonomy”The stereo camera pair generates three-dimensional information used for navigation, and the hazard camera is described as being used primarily for navigation as well as for target identification [13]. No onboard autonomous navigation, hazard detection or fault response is described in any of the published material. Vision-based lunar navigation of this kind is typically developed and tested in dedicated indoor analogue yards before flight, using graded sand and gravel rather than true regolith simulant to keep the test area large and the optics realistic [8]; no such facility or test campaign is named for this rover.
Communications
Section titled “Communications”Not published.
Payload and instruments
Section titled “Payload and instruments”| Instrument | Provider | Function | Source |
|---|---|---|---|
| StereoCam | Canadensys | navigation ranging and three-band color science | [3], [13] |
| Multispectral Imager | Canadensys | regolith and rock mineralogy within about 1 m of the front of the rover | [13] |
| NISA-1000 | Canadensys | single infrared band for water ice and mafic mineral detection | [13] |
| LHANS | Bubble Technology Industries | hydrogen as a proxy for water ice, plus Ti, Fe, Ca, P, K, Th, U by gamma ray | [11], [12], [13] |
| Radiation Micro-Dosimeter | Teledyne sensor, BTI and Canadensys integration | total ionizing dose in silicon along the traverse | [3], [13] |
| LAFORGE | Johns Hopkins APL, furnished by NASA | multispectral thermal infrared imaging radiometer | [13] |
The camera geometry is given in design detail in the science team’s most recent status report. The stereo pair sits near the top of the rover with a 40 cm horizontal separation, each camera covering 144 degrees horizontally by 104 degrees vertically and pitched 20 degrees below horizontal; the multispectral imager looks forward and down at 45 degrees, covering 35 by 26 degrees and reaching about a meter ahead, illuminated by six LED pairs from 365 to 950 nm; NISA-1000 covers 26 by 20 degrees pitched 14 degrees down; the two panoramic cameras cover 186 by 186 degrees each; and the hazard camera is mounted low, forward, at 45 degrees below horizontal [13]. The 2024 paper gives a stereo separation of about 30 cm and fields of roughly 140 by 100 degrees, and the change is not noted [12].
LAFORGE is the instrument the rover carries for another agency under a CSA-NASA agreement. It is specified for accuracy at the low end of the lunar temperature range, better than 5 K at 40 K and 2 K at 65 K, which is the range that matters inside a permanently shadowed region [13].
The instrument complement is not the one the mission started with. The 2023 paper lists a FROST suite including a Lyman-alpha instrument and a close-up imager, which were replaced during Phase B [11], [12].
Modes of operation
Section titled “Modes of operation”Not published as a set. The operations described are traverse with imaging, hydrogen and elemental mapping along the traverse, thermal imaging during the first lunar day, and excursions into shadowed areas of up to an hour [11], [12], [13].
Ground operations
Section titled “Ground operations”Not published.
Technologies developed
Section titled “Technologies developed”The mission’s first objective is technology demonstration rather than science, and the capability it is built to demonstrate is night survival on solar power alone in a 42 kg vehicle, together with a short excursion into a permanently shadowed region [4], [11], [12], [13]. Both remain claims: no supporting analysis, thermal model or test result has been published. The Canadian analogue-testing tradition this mission draws on predates it by nearly a decade: Devon Island in the Canadian High Arctic has served as a Mars/Moon analogue site for rover navigation datasets and ground-ice prospecting field tests with a stereo camera and ground-penetrating radar, work that shares several authors with this mission’s science team [1], [6].
What has been published is an instrument set designed around a common camera platform. Four of the six science instruments and all three engineering cameras are built from the same Nano-Compatible Immersive Situational Awareness imager, differentiated by optics, filters and illumination rather than by detector: a stereo pair for ranging and color, a panchromatic unit with six LED pairs for multispectral work, a long-pass infrared unit for water ice, and wide-field units for panorama and hazard detection [13].
References
Section titled “References”References
- Barfoot, T. D., Furgale, P. T., Osinski, G. R., Ghafoor, N. and Williams, K. K. (2010). Field testing of robotic technologies to support ground ice prospecting in martian polygonal terrain
. Planetary and Space Science, 4. Source
BibTeX
@article{barfoot2010field, title = {Field testing of robotic technologies to support ground ice prospecting in martian polygonal terrain}, author = {Barfoot, Timothy D. and Furgale, Paul T. and Osinski, Gordon R. and Ghafoor, Nadeem and Williams, Kevin K.}, journal = {Planetary and Space Science}, volume = {58}, number = {4}, pages = {671--681}, publisher = {Elsevier BV}, year = {2010}, doi = {10.1016/j.pss.2009.09.021} } - Chien, S. A., Visentin, G. and Basich, C. (2024). Exploring Beyond Earth using Space Robotics: Update
. Science Robotics. Source
BibTeX
@article{chien2024exploring, title = {Exploring Beyond Earth using Space Robotics: Update}, author = {Chien, Steve A. and Visentin, Gianfranco and Basich, Connor}, journal = {Science Robotics}, publisher = {JPL Open Repository}, year = {2024}, doi = {10.48577/jpl.2ezlhn}, abstract = {Robotic spacecraft enable exploration of our solar system, beyond our human presence. While spacecraft have explored every planet in the solar system, the frontiers of space robotics are at the cutting edge of landers, rovers, and now atmospheric explorers where robotic spacecraft must interact intimately with their environment to explore beyond the reach of flyby and orbital remote sensing.In 2017, we surveyed space robotics - telling the rich history of robotic explorers to the Moon, Mars, and beyond. In this article, we describe the tremendous growth in space robotics missions in the period 2017-2024 with many new entities participating in missions to the surface of the Moon, Mars, and beyond. We also describe the recent development of aerial missions to planets and moons as exemplified by the Ingenuity helicopter on Mars, the Dragonfly mission to Titan, and the planned Sample Recovery Helicopter to Mars. As with the 2017 survey, we seek to provide a big picture of developments and directions in space robotics. Additionally, we focus on sub orbital robotics - landers, rovers, and aerial vehicles, with associated challenges in sensing, manipulation, and mobility.} } - Morisset, C. E., Bergeron, M., Haltigin, T., Hill, P., Lamarche, T., Lange, C., Moroso, F., Picard, M. and Saint-Jacques, D. (2024). Canada's Rover Development for Lunar Surface Exploration
. Annual Meeting of the Lunar Exploration Analysis Group, 5021. Source
BibTeX
@inproceedings{csa2024canada, title = {Canada's Rover Development for Lunar Surface Exploration}, author = {Morisset, C. E. and Bergeron, M. and Haltigin, Timothy and Hill, P. and Lamarche, T. and Lange, Caroline and Moroso, F. and Picard, M. and Saint-Jacques, D.}, booktitle = {Annual Meeting of the Lunar Exploration Analysis Group}, number = {5021}, year = {2024}, url = {https://www.hou.usra.edu/meetings/leag2024/pdf/5021.pdf} } - Morisset, C.-E., Haltigin, T., Hill, P., Picard, M., Lamarche, T., Hamilton, D., Moroso, F., Sevigny, J., Podwalski, K. and Saint-Jacques, D. (2026). Updates on Canada's Rover Development for the Lunar South Pole
. Ices in the Solar System, 4019. Source
BibTeX
@inproceedings{csa2026updates, title = {Updates on Canada's Rover Development for the Lunar South Pole}, author = {Morisset, C.-E. and Haltigin, Timothy and Hill, P. and Picard, M. and Lamarche, T. and Hamilton, D. and Moroso, F. and Sevigny, J. and Podwalski, K. and Saint-Jacques, D.}, booktitle = {Ices in the Solar System}, number = {4019}, year = {2026}, url = {https://www.hou.usra.edu/meetings/ices2026/pdf/4019.pdf} } - Daca, A. (2023). Predicting Planetary Rover Mobility in Reduced Gravity Using 1-g Experiments
. Unpublished. Source
BibTeX
@phdthesis{daca2023predicting, title = {Predicting Planetary Rover Mobility in Reduced Gravity Using 1-g Experiments}, author = {Daca, Adriana}, journal = {Unpublished}, school = {Concordia University}, address = {Montreal, Quebec, Canada}, type = {PhD thesis}, month = {February}, year = {2023}, doi = {10.13140/rg.2.2.12718.28485}, abstract = {Traversing granular regolith, especially in reduced gravity environments, remains a potential challenge for wheeled rovers. Mitigating hazards for planetary rovers requires testing in representative environments, but direct Earth-based testing fails to account for the effect of reduced gravity on the soil itself. Here, experimental apparatus and techniques for reduced-gravity flight testing are used to systematically evaluate three existing Earth-based testing methods and develop guidelines for their use and interpretation: (i) reduced-weight testing, (ii) matching soil testing instrument response through soil simulant design, and (iii) granular scaling laws (GSL). \nExperimentation campaigns flying reduced-gravity parabolas, with soil and wheel both in lunar-g, have shown reductions in net traction of 20% or more and increases in sinkage of up to 40% compared to Earth-based testing methods (i) and (ii). Scaled-wheel testing, according to GSL (method iii) has shown better agreement with reduced-g tests (less than 10% error) and also tends to err on the side of conservative predictions. \nLimitations of GSL are investigated including a recently proposed cohesion constraint (that the wheel radius ratio must be the inverse of the gravity ratio) and the effects of wheel size and aspect ratio on GSL’s accuracy. It was found that the cohesion constraint can most likely be ignored for mildly cohesive soils such as lunar regolith. Limits on wheel sizes and aspect ratio variation are also proposed. \nThe application of GSL to planetary rover testing is demonstrated through two studies undertaken in collaboration with NASA’s Jet Propulsion Laboratory. One study compares wheel designs for a skid-steer lunar rover in single-wheel tests scaled by GSL, demonstrating that diagonal grousers improve turning performance without requiring larger wheels. The second study involves application of GSL to the design of two reconfigurable test platforms for evaluating steep-terrain mobility performance. \nAnother aspect of rover mobility testing—normal force control in single-wheel testbeds—is also investigated. An improved method for single-wheel testing, using a 4-bar mechanism, essentially eliminates normal force oscillations from frictional vertical sliders. \nFinally, guidelines for conducting and interpreting 1-g mobility tests for lunar rovers are presented, and potential avenues for future research are outlined.} } - Furgale, P., Carle, P., Enright, J. and Barfoot, T. D. (2012). The Devon Island rover navigation dataset
. The International Journal of Robotics Research, 6. Source
BibTeX
@article{furgale2012devon, title = {The Devon Island rover navigation dataset}, author = {Furgale, Paul and Carle, Pat and Enright, John and Barfoot, Timothy D.}, journal = {The International Journal of Robotics Research}, volume = {31}, number = {6}, pages = {707-713}, publisher = {SAGE Publications}, year = {2012}, doi = {10.1177/0278364911433135}, abstract = {In this paper we present a rover navigation dataset collected at a Mars/Moon analogue site on Devon Island, in the Canadian High Arctic. The dataset is split into two parts. The first part contains rover traverse data: stereo imagery, Sun vectors, inclinometer data, and ground-truth position information from a differential global positioning system (DGPS) collected over a 10-km traverse. The second part contains long-range localization data: 3D laser range scans, image panoramas, digital elevation models, and GPS data useful for global position estimation. All images are available in common formats and other data is presented in human-readable text files. To facilitate use of the data, Matlab parsing scripts are included.} } - 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} } - Ludivig, P., Calzada-Diaz, A., Olivares Mendez, M. A., Voos, H. and Lamamy, J. (2020). Building a Piece of the Moon: Construction of Two Indoor Lunar Analogue Environments
. International Astronautical Congress, IAC-20-A3.2B.3. Source
BibTeX
@inproceedings{ludivig2020building, title = {Building a Piece of the {Moon}: Construction of Two Indoor Lunar Analogue Environments}, author = {Ludivig, Philippe and Calzada-Diaz, Abigail and Olivares Mendez, Miguel Angel and Voos, Holger and Lamamy, Julien}, booktitle = {International Astronautical Congress}, number = {IAC-20-A3.2B.3}, organization = {International Astronautical Federation}, year = {2020}, url = {https://orbilu.uni.lu/handle/10993/45539} } - NASA. (2020). Cross-Program Design Specification for Natural Environments (DSNE), Revision G
. NASA Marshall Space Flight Center. Source
BibTeX
@techreport{nasa2020cross, title = {Cross-Program Design Specification for Natural Environments (DSNE), Revision G}, author = {{NASA}}, institution = {NASA Marshall Space Flight Center}, year = {2020}, url = {https://ntrs.nasa.gov/citations/20200000867}, abstract = {The DSNE completes environment-related specifications for architecture, system-level, and lower-tier documents by specifying the ranges of environmental conditions that must be accounted for by NASA ESD Programs. To assure clarity and consistency, and to prevent requirements documents from becoming cluttered with extensive amounts of technical material, natural environment specifications have been compiled into this document. The intent is to keep a unified specification for natural environments that each Program calls out for appropriate application.} } - Niksirat, P., Daca, A. and Skonieczny, K. (2020). The effects of reduced-gravity on planetary rover mobility
. IEEE Transactions on Nuclear Science, 7. Source
BibTeX
@article{niksirat2020effects, title = {The effects of reduced-gravity on planetary rover mobility}, author = {Niksirat, Parna and Daca, Adriana and Skonieczny, Krzysztof}, journal = {IEEE Transactions on Nuclear Science}, volume = {39}, number = {7}, pages = {797-811}, publisher = {SAGE Publications}, year = {2020}, doi = {10.1177/0278364920913945}, abstract = {One of the major challenges faced by planetary exploration rovers today is the negotiation of difficult terrain, such as fine granular regolith commonly found on the Moon and Mars. Current testing methods on Earth fail to account for the effect of reduced gravity on the soil itself. This work characterizes the effects of reduced gravity on wheel–soil interactions between an ExoMars rover wheel prototype and a martian soil simulant aboard parabolic flights producing effective martian and lunar gravitational accelerations. These experiments are the first to collect wheel–soil interaction imagery and force/torque sensor data alongside wheel sinkage data. Results from reduced-gravity flights are compared with on-ground experiments with all parameters equal, including wheel load, such that the only difference between the experiments is the effect of gravity on the soil itself. In lunar gravity, a statistically significant average reduction in traction of 20% is observed compared with 1 g, and in martian gravity an average traction reduction of 5–10% is observed. Subsurface soil imaging shows that soil mobilization increases as gravity decreases, suggesting a deterioration in soil strength, which could be the cause of the reduction in traction. Statistically significant increases in wheel sinkage in both martian and lunar gravity provide additional evidence for decreased soil strength. All of these observations (decreased traction, increased soil mobilization, and increased sinkage) hinder a rover’s ability to drive, and should be considered when interpreting results from reduced-load mobility tests conducted on Earth.} } - Osinski, G. R., Edmundson, P., Hackett, J., Newman, J., Visscher, P., Cloutis, E. A., Lemelin, M., Morisset, C.-E., Picard, M., Greenhagen, B. T., Cahill, J. T. S., MacEwan, S. J. and Smith, M. B. (2023). The Canadian Lunar Rover Mission (LRM): A Micro-Rover Mission to the South Pole of the Moon
. Lunar and Planetary Science Conference, 2487. Source
BibTeX
@inproceedings{osinski2023canadian, title = {The Canadian Lunar Rover Mission (LRM): A Micro-Rover Mission to the South Pole of the Moon}, author = {Osinski, G. R. and Edmundson, P. and Hackett, J. and Newman, J. and Visscher, P. and Cloutis, Edward A. and Lemelin, Myriam and Morisset, C.-E. and Picard, M. and Greenhagen, Benjamin T. and Cahill, Joshua T. S. and MacEwan, S. J. and Smith, M. B.}, booktitle = {Lunar and Planetary Science Conference}, number = {2487}, year = {2023}, url = {https://www.hou.usra.edu/meetings/lpsc2023/pdf/2487.pdf} } - Osinski, G. R., Edmundson, P., Cloutis, E. A., Lemelin, M., Morisset, C.-E., Picard, M., Lamarche, T., Greenhagen, B. T., Smith, M. B., Harrison, T., Hackett, J., Newman, J., Cahill, J. T. S., Colaprete, T., Cunje, A., Daly, M., Flemming, R., Hardgrove, C., Herd, C. D. K., Neish, C. D., Preston, L., Siegler, M., Sirek, A., Tornabene, L. L. and Williams, D. (2024). The Canadian Lunar Rover: An Update
. Lunar and Planetary Science Conference, 1728. Source
BibTeX
@inproceedings{osinski2024canadian, title = {The Canadian Lunar Rover: An Update}, author = {Osinski, G. R. and Edmundson, P. and Cloutis, Edward A. and Lemelin, Myriam and Morisset, C.-E. and Picard, M. and Lamarche, T. and Greenhagen, Benjamin T. and Smith, M. B. and Harrison, T. and Hackett, J. and Newman, J. and Cahill, Joshua T. S. and Colaprete, Tony and Cunje, A. and Daly, M. and Flemming, R. and Hardgrove, Craig and Herd, Chris D. K. and Neish, Catherine D. and Preston, L. and Siegler, M. and Sirek, A. and Tornabene, L. L. and Williams, D.}, booktitle = {Lunar and Planetary Science Conference}, number = {1728}, year = {2024}, url = {https://www.hou.usra.edu/meetings/lpsc2024/pdf/1728.pdf} } - Osinski, G. R., Cloutis, E. A., Lemelin, M., Edmundson, P., Morisset, C.-E., Picard, M., Lamarche, T., Greenhagen, B. T., Smith, M. B., Tornabene, L. L., Cahill, J. T. S., Colaprete, T., Cunje, A., Daly, M., Donaldson Hanna, K., Elder, C. M., Flemming, R., Hackett, J., Hardgrove, C., Herd, C. D. K., Lees, D., Lim, D., MacEwan, S. J., Mirmalek, Z., Neish, C. D., Newman, J., Preston, L., Siegler, M., Sirek, A. and Williams, D. (2025). The Canadian Lunar Rover Mission to the South Polar Region of the Moon: A Status Report
. Lunar and Planetary Science Conference, 2221. Source
BibTeX
@inproceedings{osinski2025canadian, title = {The Canadian Lunar Rover Mission to the South Polar Region of the Moon: A Status Report}, author = {Osinski, G. R. and Cloutis, Edward A. and Lemelin, Myriam and Edmundson, P. and Morisset, C.-E. and Picard, M. and Lamarche, T. and Greenhagen, Benjamin T. and Smith, M. B. and Tornabene, L. L. and Cahill, Joshua T. S. and Colaprete, Tony and Cunje, A. and Daly, M. and Donaldson Hanna, K. and Elder, Catherine M. and Flemming, R. and Hackett, J. and Hardgrove, Craig and Herd, Chris D. K. and Lees, David and Lim, D. and MacEwan, S. J. and Mirmalek, Zara and Neish, Catherine D. and Newman, J. and Preston, L. and Siegler, M. and Sirek, A. and Williams, D.}, booktitle = {Lunar and Planetary Science Conference}, number = {2221}, year = {2025}, url = {https://www.hou.usra.edu/meetings/lpsc2025/pdf/2221.pdf} } - Wettergreen, D., Tompkins, P., Urmson, C., Wagner, M. and Whittaker, W. (2005). Sun-Synchronous Robotic Exploration: Technical Description and Field Experimentation
. The International Journal of Robotics Research, 1. Source
BibTeX
@article{wettergreen2005sunsynchronous, title = {Sun-Synchronous Robotic Exploration: Technical Description and Field Experimentation}, author = {Wettergreen, David and Tompkins, Paul and Urmson, Chris and Wagner, Michael and Whittaker, William}, journal = {The International Journal of Robotics Research}, volume = {24}, number = {1}, pages = {3--30}, year = {2005}, doi = {10.1177/0278364904046632}, abstract = {Sun-synchronous robotic exploration is accomplished by reasoning about sunlight: where the Sun is in the sky, where and when shadows will fall, and how much power can be obtained through various courses of action. We conducted experiments in the Canadian high arctic using a solar-powered rover to prove the concept of Sun-synchronous exploration. Using knowledge of orbital mechanics, local terrain, and locomotion power, the rover Hyperion planned Sun-synchronous routes to visit designated sites while obtaining the necessary solar power for continuous operation. Hyperion executed its plan, beginning and ending each 24-h period with batteries fully charged, after traveling two circuits of more than 6 km in barren, Mars-like terrain. The objective of the Sun-Synchronous Navigation project (http://www.frc.ri.cmu.edu/sunsync) was to create hardware and software technologies needed to realize Sun-synchronous exploration and to validate these technologies in field experimentation. In the process, we learned important technical lessons regarding rover mechanism, motion control, planning algorithms, and system architecture. In this paper we describe the concept of Sun-synchronous exploration. We overview the design of the robot Hyperion and the software system that enables it to operate in synchrony with the Sun. We then discuss results and lessons from analysis of our field experiments. This paper describes rover and planetary exploration research at Carnegie Mellon during 2000-2002.} } - (2025). Canadian Space Agency: Canadian lunar rover mission. asc-csa.gc.ca/eng/astronomy/moon-exploration/lunar-rover-mission.asp
BibTeX
@misc{canadianspaceagencycanadian, title = {Canadian Space Agency: Canadian lunar rover mission}, organization = {asc-csa.gc.ca}, year = {2025}, url = {https://www.asc-csa.gc.ca/eng/astronomy/moon-exploration/lunar-rover-mission.asp} }
Further reading
- (2026). Canadensys Aerospace: Canadian Lunar Rover. canadensys.com/canadensys-aerospace-awarded-csa-lunar-rover-contract