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YAOKI

YAOKI in a manufacturer publicity image on regolith simulant. The vehicle is two large wheels on a single common axle either side of a dumbbell-shaped carbon fiber body; each wheel rim carries slotted circumferential grousers, and the camera aperture is centred on the body face between two LEDs, so the same optical assembly works whichever way up the rover comes to rest Dymon Co., Ltd.

A rover that rides down to the surface inside a CLPS lander’s payload bay has to survive an uncontrolled drop, has no ground crew to right it if it lands wrong, and gets one lander’s worth of power and radio range to work with. Most of the small lunar rovers flown since 2019 answer that problem by keeping mass and part count to a minimum and by making the vehicle indifferent to which way up it ends up [8]. YAOKI is Dymon Co., Ltd.’s answer: a 498 g two-wheeled rover, 15 x 15 x 10 cm, built around a single axle with one wheel at each end of a central body [12], [10], rated to withstand 100 G and designed to keep working after impact and after coming to rest either way up. It flew on the Intuitive Machines IM-2 Nova-C lander, launched 26 February 2025 [1], and was not deployed because the lander came to rest on its side [2].

The single-axle, two-wheel layout with no suspension and no steering actuators is one of two architectures this generation of micro-rovers converged on for the same constraint. JAXA’s SORA-Q, flown on Hakuto-R M1 and again as LEV-2 on SLIM, instead folds a ball into two eccentric hemispherical wheels with a tail stabilizer, trading YAOKI’s axle symmetry for a transformable housing that also serves as the stowed launch configuration [3]. Both designs put the entire mobility and impact-survival problem into passive mechanical geometry rather than into control software, because there is no ground link fast enough to recover a teleoperated vehicle that tips over. A JPL survey of the same period places small CLPS-class rovers like YAOKI within a broader field of extreme-terrain and planetary mobility work [4], and a 2024 review of the surge in lunar landers and rovers from 2019 onward counts nine such missions launched and four failed by that point, the base rate against which IM-2’s outcome sits [8].

The vehicle was originally manifested on Astrobotic’s Peregrine lander under an agreement announced on 14 October 2019, for a 2021 flight [11]. Peregrine Mission One launched instead on 8 January 2024 without YAOKI aboard, and was lost in cislunar space after a valve failure ruptured its oxidizer tank about 92 minutes after separation [6]; Dymon’s rover had by then moved to IM-2. Dymon states eight years of development with the base technology completed in 2018 and more than 100 tests passed. The name is from a Japanese proverb about getting up again however many times one falls, and the self-righting design is the literal expression of it [12].

No peer-reviewed or conference publication on YAOKI was located. Vehicle numbers below come from Dymon and from Mitsubishi Chemical Group, which supplied the exterior materials [12], [10]. The NASA conference paper cited [1] covers the IM-2 flight, not the rover.

ParameterValueSource
Mass498 gmanufacturer [12], [10]
Dimensions15 x 15 x 10 cmmanufacturer [10]
Wheels2, on one common axlemanufacturer [11]
Impact tolerance100 Gmanufacturer [12], [10]
Body materialCFRP with cyanate ester resin matrixsupplier [10]
Wheel materialpolyamide-imide
Camera lens treatmentanti-soiling coating
Self-rightingyes, operates either way upmanufacturer [12], [10]

Drive speed, slope limit, obstacle capability, power source, battery capacity, radio band, data rate, processor and thermal limits are not published. For comparison, a compiled record of every vehicle that has actually driven on the Moon puts the operating limit for wheeled lunar mobility at a ground contact pressure below about 7 to 10 kPa and a slope capability around 25 degrees [9]; nothing in the public YAOKI material states where its two-wheel, no-suspension geometry sits against either figure.

These describe IM-2, not the rover.

ParameterValueSource
LanderIntuitive Machines Nova-C, IM-2[1]
Launch26 February 2025
Planned surface durationup to two weeks of lunar daylight
Landing6 March 2025, Mons Mouton, 250 m from target[2]
Outcomelander on its side, rover not deployed
Mission end7 March 2025

Athena landed on its side inside a crater at Mons Mouton, about 250 m from the intended site [2]. Intuitive Machines did not expect the lander to recharge, given the sun direction, the solar panel orientation and the crater temperatures, and declared the mission concluded on 7 March 2025. NASA’s PRIME-1 suite accelerated several payload milestones before the batteries depleted. Its centerpiece, the TRIDENT rotary-percussive drill built by Honeybee Robotics for this same lander, did not penetrate the surface in that orientation [5]; YAOKI, riding the same lander, was not deployed either. The two payloads failed for the same reason, an attitude the lander was never meant to operate in, not for any fault of their own.

The earlier Peregrine assignment did not fly with YAOKI aboard; the rover moved to IM-2 [11].

Two wheels on a single axle [12], described by the manufacturer as the smallest effective rover wheels produced [11]. The architecture has no suspension and no steering actuators; with two ground contacts and a body suspended between them, attitude about the axle is unconstrained, which is why the vehicle is designed to operate inverted. Dymon states it can be thrown into a cave and continue working [10], which is the same requirement as the 100 G impact rating.

Wheels are polyamide-imide, chosen for cold and heat resistance, wear resistance and impact strength, specifically so the wheels survive being dropped onto the lunar surface from a deployer [10]. No drawbar pull, slip or slope data has been published.

The body is carbon fiber reinforced plastic in a cyanate ester resin matrix, chosen for low permittivity and temperature resistance [10]. It replaced an aluminum design, and the substitution gave about 30 percent lower mass, a five times better safety factor, and about 4 million yen lower lunar transport cost per unit. The deployer that releases the rover from the lander uses the same cyanate ester CFRP. Mass is the cost driver for a vehicle of this class, and the material substitution is quantified against lunar transport cost rather than against structural performance alone.

No solar array, battery capacity or night survival capability is published.

Not published as a subsystem [12]. The only thermal information is at material level: the cyanate ester CFRP body is selected for temperature resistance and the polyamide-imide wheels for cold and heat resistance [10].

None claimed in the manufacturer material [12], [11]. The vehicle is operated through the lander. A contemporary micro-rover, MoonRanger, was built for the opposite case, a mission with no real-time link to Earth at all, and its designers found that dead reckoning alone on a lunar analog drifted about 5 percent of distance traveled over an unsupervized traverse [7]. YAOKI’s short-range, lander-relay teleoperation avoids that problem by never asking the rover to navigate further than the lander can see, which is one reason a two-wheel vehicle with no onboard perception is a workable design for this mission class even though it would not be for a multi-kilometer trek.

Through the lander, which on IM-2 also hosted a 4G/LTE network for other payloads [1]. YAOKI’s own band, data rate and range are not published [12].

A camera is the payload. Its lens carries an anti-soiling coating developed against lunar regolith, whose jagged particle shape and electrostatic behavior make it adhere to optics [10]. The photograph above shows the camera aperture flanked by two lamps on the body face. Sensor format, resolution and field of view are not published.

Deployment is from a dedicated deployer on the lander, from which the rover is dropped to the surface [10].

The transferable results are material substitutions with quantified outcomes: a cyanate ester CFRP body replacing aluminum at about 30 percent lower mass and five times the safety factor, polyamide-imide wheels qualified against drop impact, and an anti-soiling lens coating developed specifically against regolith adhesion [10]. The single-axle, two-wheel, operates-either-way-up architecture is the second result, and it has not been demonstrated on the lunar surface because the vehicle was never deployed [2].

Drive speed, slope limit, obstacle capability, power source, battery capacity, radio band, data rate, processor and thermal design margins have not been published by Dymon or by any third party, and no peer-reviewed or conference paper on the rover itself was located; every number above traces to manufacturer and supplier marketing material [12], [10]. Because YAOKI was never deployed on the lunar surface, none of its mobility, thermal or communications claims have flight validation, and the vehicle’s actual performance against the ground contact pressure and slope limits established for prior lunar rovers [9] remains unmeasured.

References

  1. Edwards, B., Wagner, R. S., Zemba, M., Klein, T. E., Maestro, L. and Dow, J. (2025). Envisioned Lunar Surface Communications Using 3GPP Cellular and Wi-Fi Technologies . International Conference on Space Operations. Source
    BibTeX
    @inproceedings{edwards2025envisioned,
      title = {Envisioned Lunar Surface Communications Using 3GPP Cellular and Wi-Fi Technologies},
      author = {Edwards, Bernard and Wagner, Raymond S. and Zemba, Michael and Klein, Thierry E. and Maestro, Luis and Dow, John},
      booktitle = {International Conference on Space Operations},
      year = {2025},
      url = {https://ntrs.nasa.gov/citations/20250001947},
      abstract = {Under NASA’s Artemis Program, NASA plans to collaborate with commercial and international partners to establish a long-term human and robotic presence on the Moon. Critical lunar infrastructure includes having a robust surface wireless communications and navigation network to be developed over time by many organizations, public and private. NASA’s Space Technology Mission Directorate (STMD) has envisioned a lunar surface future that includes the use of 3rd Generation Partnership Project (3GPP) cellular and 802.11 Wi-Fi technologies. NASA and Nokia Bell Labs are studying and validating the benefits and trade-offs of using 3GPP 4G and 5G technologies originally developed for use here on Earth, and how 3GPP technologies and 802.11 Wi-Fi technologies can be integrated to provide a robust and resilient end-to-end network architecture and solution design. Furthermore, as the 3GPP organization defines future 6G capabilities, NASA wants to understand how that could enhance lunar science and exploration missions and commercial endeavours to provide even more advanced, scalable and high-performance connectivity solutions. The vision is to provide human and robotic missions on the Moon with similar communications and navigation capabilities to what mobile users have on Earth, while adapting these technologies into space-hardened solutions that withstand the environmental and operational challenges of the lunar surface. STMD’s Tipping Point program seeks industry-developed space technologies that can both foster commercial space capabilities and benefit future NASA missions. Via Tipping Point, Nokia Bell Labs will demonstrate the use of 4G / LTE on the lunar surface on the Intuitive Machines IM-2 mission. This will be followed with a technology demonstration with astronauts on the Artemis III lunar landing. This paper provides an overview of NASA’s current and planned future work on using 3GPP and 802.11 Wi-Fi on the Moon.}
    }
  2. (2026). Spaceflight Now: Intuitive Machines' IM-2 Moon mission ends with lander on its side. spaceflightnow.com/2025/03/07/intuitive-machines-im-2-mission-ends-wi...
    BibTeX
    @misc{spaceflightnowintuitive,
      title = {Spaceflight Now: Intuitive Machines' IM-2 Moon mission ends with lander on its side},
      organization = {spaceflightnow.com},
      year = {2026},
      url = {https://spaceflightnow.com/2025/03/07/intuitive-machines-im-2-mission-ends-with-lander-on-its-side-on-the-moon/}
    }
  3. Hirano, D., Inazawa, M., Sutoh, M., Sawada, H., Kawai, Y., Nagata, M., Sakoda, G., Yoneda, Y. and Watanabe, K. (2024). Transformable Nano Rover for Space Exploration . IEEE Robotics and Automation Letters, 4. Source
    BibTeX
    @article{hirano2024transformable,
      title = {Transformable Nano Rover for Space Exploration},
      author = {Hirano, Daichi and Inazawa, Mariko and Sutoh, Masataku and Sawada, Hirotaka and Kawai, Yuta and Nagata, Masaharu and Sakoda, Gen and Yoneda, Yousuke and Watanabe, Kimitaka},
      journal = {IEEE Robotics and Automation Letters},
      volume = {9},
      number = {4},
      pages = {3139--3146},
      year = {2024},
      doi = {10.1109/lra.2024.3363529},
      abstract = {This letter introduces a novel nano rover designed to transform its shape for efficient movement on lunar surfaces. The rover, resembling a compact ball, has a diameter of roughly 80 mm and a mass around 250 g. Its transformational mechanism allows for compactness during planetary transportation, with enhanced mobility achieved through the use of extendable wheels, a tail stabilizer, and cameras. To traverse soft terrains efficiently, the rover utilizes an eccentric wheel mechanism, offering two distinct movement modes based on wheel synchronization. This mechanism provides a locomotion velocity of 20 mm/s or more on a flat surface. Moreover, it features onboard image processing to detect spacecraft shielded by Multi-Layer Insulation (MLI) films, facilitating autonomous control and selective image transmission. This rover has been deployed in a real space mission, having been mounted on a lunar lander. This letter presents the design specifics of this transformable rover and results from field tests simulating lunar conditions. These tests affirmed the efficacy of the proposed motion mechanism and onboard image processing.}
    }
  4. Nesnas, I. (2023). Robotics and Autonomy for Space Applications . Root. doi.org/10.48577/jpl.oikho7
    BibTeX
    @misc{nesnas2023robotics,
      title = {Robotics and Autonomy for Space Applications},
      author = {Nesnas, Issa},
      journal = {Root},
      year = {2023},
      doi = {10.48577/jpl.oikho7},
      abstract = {No abstract available.}
    }
  5. Zacny, K., Chu, P., Vendiola, V., Paulsen, G., Creekmore, J., Goldman, J., Kleinhenz, J., Smith, J. and Colaprete, A. (2025). TRIDENT Ice Mining Drill for Lunar Volatile Prospecting for PRIME-1 and VIPER Missions . The Planetary Science Journal, 12. Source
    BibTeX
    @article{zacny2025trident,
      title = {{TRIDENT} Ice Mining Drill for Lunar Volatile Prospecting for {PRIME-1} and {VIPER} Missions},
      author = {Zacny, Kris and Chu, Philip and Vendiola, Vincent and Paulsen, Gale and Creekmore, Justin and Goldman, Jason and Kleinhenz, Julie and Smith, James and Colaprete, Anthony},
      journal = {The Planetary Science Journal},
      volume = {6},
      number = {12},
      pages = {297},
      year = {2025},
      doi = {10.3847/psj/ae0b51},
      abstract = {Abstract The Regolith and Ice Drill for Exploration of New Terrains (TRIDENT) is a 1 m class drill developed for capturing regolith and ice during the Volatiles Investigating Polar Exploration Rover (VIPER) and the Polar Resources Ice Mining Experiment (PRIME-1) lander missions to the south pole of the Moon. The drill employs decoupled rotation and percussion mechanisms to allow for three modes: rotation, percussion, and rotation–percussion, depending on operational goals and the material strength. TRIDENT can be operated in such a way that it can characterize subsurface material and deliver cuttings to the surface for characterization by other instruments. TRIDENT includes a drill-bit-integrated temperature sensor and an auger-integrated heater with a colocated temperature sensor 35 cm above the bit for thermal conductivity measurement. The heater can also be used in cases of ice adherence (freezing in) and to enhance the sublimation of ice from the cuttings pile. TRIDENT collects and delivers subsurface regolith onto the surface using a “bite” sampling approach: cuttings are captured in the auger flutes, the auger is retracted after drilling a 10 cm bite, and then 10 cm worth of cuttings are deposited onto the surface, forming a cuttings cone. This regolith cone is then analyzed by instruments Mass Spectrometer Observing Lunar Operations (MSOLO) and NIRVSS on the VIPER and MSOLO on the PRIME-1 missions. The drilling activity creates a seismic signal that can be detected on any associated inertial measurement unit that is turned on during the activity, which enables seismic science. TRIDENT represents two decades of technology development for planetary applications and could be deployed on any future missions to other solar system bodies. TRIDENT on the PRIME-1 mission has been successfully deployed in horizontal orientation (this orientation was due to the lander being in an off nominal landing orientation). All actuators, sensors, and heaters worked as designed. Even though the drill did not penetrate regolith, it was covered in regolith that fell onto the drill during the landing operation. VIPER is scheduled to launch to the Moon at the end of 2027 on Blue Origin’s Mk1 lander.}
    }
  6. Astrobotic Technology. (2024). Peregrine Mission 1 Post-Mission Report . Astrobotic Technology. Source
    BibTeX
    @techreport{astrobotic2024peregrine,
      title = {Peregrine Mission 1 Post-Mission Report},
      author = {{Astrobotic Technology}},
      institution = {Astrobotic Technology},
      month = {August},
      year = {2024},
      url = {https://www.astrobotic.com/wp-content/uploads/2024/08/PM1_Post-Mission-Report_2024-1.pdf}
    }
  7. Kumar, V., Sai, S. S., Vijayarangan, S., Wettergreen, D., Jones, H., Callaghan, P., Jamal, H. and Whittaker, W. L. (2020). Formulation of Micro-Rover Autonomy Software for Lunar Exploration . International Symposium on Artificial Intelligence, Robotics and Automation in Space (i-SAIRAS). Source
    BibTeX
    @inproceedings{kumar2020formulation,
      title = {Formulation of Micro-Rover Autonomy Software for Lunar Exploration},
      author = {Kumar, Varsha and Sai, Shyam S. and Vijayarangan, Srinivas and Wettergreen, David and Jones, Heather and Callaghan, Patrick and Jamal, Haidar and Whittaker, William L.},
      booktitle = {International Symposium on Artificial Intelligence, Robotics and Automation in Space (i-SAIRAS)},
      year = {2020},
      url = {https://www.hou.usra.edu/meetings/isairas2020fullpapers/pdf/5068.pdf}
    }
  8. 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.}
    }
  9. Kring, D. A. (2006). Lunar Mobility Review . Lunar and Planetary Institute, Lunar Exploration Initiative. Source
    BibTeX
    @techreport{kring2006lunar,
      title = {Lunar Mobility Review},
      author = {Kring, David A.},
      institution = {Lunar and Planetary Institute, Lunar Exploration Initiative},
      year = {2006},
      url = {https://www.lpi.usra.edu/science/kring/lunar_exploration/briefings/lunar_mobility_review.pdf}
    }
  10. (2021). Dymon: YAOKI Project. dymon.co.jp/en/yaoki
    BibTeX
    @misc{dymonyaoki,
      title = {Dymon: YAOKI Project},
      organization = {dymon.co.jp},
      year = {2021},
      url = {https://dymon.co.jp/en/yaoki/}
    }
  11. (2026). Mitsubishi Chemical Group: The lunar rover YAOKI's exterior, crafted almost entirely by the Group. mcgc.com/english/kaiteki_solution_center/oursolution/10.html
    BibTeX
    @misc{mitsubishichemicalgrouplunar,
      title = {Mitsubishi Chemical Group: The lunar rover YAOKI's exterior, crafted almost entirely by the Group},
      organization = {mcgc.com},
      year = {2026},
      url = {https://www.mcgc.com/english/kaiteki_solution_center/oursolution/10.html}
    }
  12. (2019). Astrobotic and Dymon Announce Agreement to Bring the First Japanese Lunar Rover to the Moon. astrobotic.com/astrobotic-and-dymon-announce-agreement-to-bring-the-f...
    BibTeX
    @misc{astroboticanddymonannounceagreementtobringthefirstjapaneselunarrovertothemoonyaoki,
      title = {Astrobotic and Dymon Announce Agreement to Bring the First Japanese Lunar Rover to the Moon},
      organization = {astrobotic.com},
      year = {2019},
      url = {https://www.astrobotic.com/astrobotic-and-dymon-announce-agreement-to-bring-the-first-japanese-lunar-rover-to-the-moon/}
    }