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A commercial rover that flies before its buyer has committed to it has to solve a problem peer-reviewed programs rarely face: proving the subsystems work at flight scale without a customer’s requirements document or a customer’s launch vehicle. FLIP, the FLEX Lunar Innovation Platform, is Astrolab’s answer. It is manifested as the primary payload on Astrobotic’s Griffin Mission One to the Nobile region of the lunar south pole, a slot that opened when NASA discontinued VIPER and converted the CLPS delivery into a large-lander demonstration carrying a comparable mass [12], [5]. FLIP is not a scaled model of anything. It carries full-sized batteries, tires, avionics, sensors and software drawn from FLEX, Astrolab’s much larger commercial rover, so that each is exercised at flight scale in the environment FLEX is meant to work in before FLEX itself exists as flight hardware [11].

The design logic follows from the mismatch between the two vehicles. FLEX is Astrolab’s large modular rover, built around a standardized payload interface with an underslung bay of up to 3 cubic meters and a removable standing crew interface so the same chassis serves suited astronauts or pure teleoperation [2]. Astrobotic’s own release once projected FLEX for a Starship landing by late 2026, a date that has since slipped [12]. NASA has separately adapted a smaller derivative, CLV-1, to its Lunar Terrain Vehicle Services program, awarding Astrolab a task order of about 219 million dollars against an IDIQ ceiling of up to 4.6 billion dollars over 13 years, with delivery anticipated by 2028 and a design mass near 950 kg [1]. FLIP sidesteps both timelines: at roughly half a tonne with a 30 kg payload allocation, it is sized to ride a medium-class commercial lander that already exists, converting a component qualification problem into a manifest problem instead of a launch vehicle problem [11], [12], [4]. NASA’s own 2025 survey of in-space servicing, assembly and manufacturing capability lists Astrolab and FLEX among the vehicles being developed for exactly this class of commercial lunar logistics [4].

ParameterValueSource
Massnearly half a metric ton[12]
Payload capacity30 kg
Wheelshyper-deformable airless tires from Venturi Space[11], [12], [3]
Battery enclosurecustom design by Venturi Space[11]
Lander compatibilitymedium-class commercial lunar landers[12]

Dimensions, drive speed, slope limit, obstacle capability, generation capacity, battery capacity, night survival, processor and communications parameters are not published. Astrolab publishes no technical documentation for this vehicle beyond its press material, and no peer-reviewed or conference publication about it has appeared.

ParameterValueSource
LanderAstrobotic Griffin[12]
Landing siteNobile region, lunar south pole
Deliveryannounced for end of 2025, subsequently stated as summer 2026[11], [12]

FLIP took the primary payload position on Griffin Mission One after the flight’s original assignment changed, when NASA canceled VIPER before delivery and Astrobotic retained the Griffin lander for a different payload manifest [12]. Astrobotic’s own record of its first lunar landing, Peregrine Mission 1, is the relevant precedent for what a Griffin-class flight actually has to survive. A single failed helium valve doomed that lander’s soft-landing attempt 92 minutes after separation, but the team still recovered 10 days 14 hours of cislunar operation and returned data from all nine payloads before a controlled re-entry, and most subsystems reached flight maturity even though the landing itself was lost [5]. Griffin Mission One is Astrobotic’s next attempt at the landing Peregrine did not complete, and it carries the consequences of that first mission’s post-flight review in its design.

Four wheels carry hyper-deformable airless tires supplied by Venturi Space, the same wheel design intended for FLEX [11]. Venturi states a duty cycle for the wheel rather than a figure specific to FLIP: four wheels carrying a two-tonne vehicle including payload, deforming to absorb ground irregularities at 15 km/h, across south-pole temperatures spanning -240 to +130 C, required to last at least 1,000 km and to resist south-pole radiation, with NASA testing and analysis of the wheel at Glenn Research Center and Johnson Space Center [3]. That duty cycle is stated for the larger FLEX vehicle; no wheel test data specific to FLIP’s roughly 500 kg mass has been released, and no speed, gradeability, obstacle height or ground-pressure result appears anywhere in Astrolab’s material [11].

The gap between a stated duty cycle and a demonstrated one is the ordinary condition of lunar wheel-soil work, not a defect specific to Astrolab. The only published reduced-gravity wheel-soil dataset in this class comes from parabolic-flight tests of a different wheel, an ExoMars-style prototype driven through Martian simulant under 20 to 30 seconds of lunar and Martian gravity at a time, with wheel load held constant against the ground-test baseline so gravity’s effect on the soil could be isolated: drawbar pull fell 20 percent on average in lunar gravity and maximum sinkage rose 38 percent, both statistically significant [6]. No test of this kind has been run against a hyper-deformable airless tire of the type Venturi has built, so the wheel’s on-Moon performance is, at present, an engineering claim rather than a measured or simulated one.

Dust sealing of the wheel actuators is named as one of the things the mission is there to test, which places it among the open questions rather than among the solved ones [11].

Solar generation with batteries supplied by Venturi Space in a custom enclosure of Venturi’s design, at the same physical size as those intended for FLEX [11]. Generation capacity, battery capacity, night survival and duty cycle are not published for FLIP itself. Astrolab’s press material claims lunar-night survival for the battery enclosure with no energy, insulation or temperature figures attached [11].

Protective coatings for the solar array and the radiator are among the technologies the mission is to test, and performance in south-polar temperatures is named as an objective [11]. No temperature limits, heater strategy or radiator area is published.

The stakes of that test are set by a mechanism the Apollo program already documented [7] across all six landings: dust degradation of thermal control is nonlinear, eleven percent areal dust coverage is enough to double solar absorptance, the Lunar Roving Vehicle’s own batteries exceeded their operating temperature limits on Apollo 16 and 17 from exactly this mechanism, and ground testing consistently underestimated the problem, since brushing that cleared dust reliably in a chamber did not clear it on the Moon. FLIP’s coating and dust-sealing tests address the same failure mode on hardware that has not yet flown.

Described only as critical avionics systems carried at full size [12]. No processor, memory or radiation tolerance approach is published.

Not published.

Not published.

The rover carries a 30 kg payload allocation, part of which Astrolab states will go toward investigations into mitigating the risk lunar dust poses to vehicles, structures and spacecraft systems: protective-coating tests on the solar array and radiator, measurement of dust accumulation rate on surfaces, and new dust-sealing strategies for the wheel actuators [12]. No instrument has been named. No measurement technique, coating identification or success criterion has been published for any of the three, a gap consistent with the layered, largely untested state of lunar dust mitigation technology generally [8].

A published taxonomy of lunar dust mitigation technologies groups countermeasures into four layers, avoiding dust generation, preventing it sticking or entering, removing it, and tolerating it, and argues that layering several 90-percent-effective measures beats relying on one 99-percent one [8]. FLIP’s planned tests span at least two of those layers, prevention by coating and toleration by sealing, but nothing about which specific mitigation approach within either layer was chosen has been disclosed.

Not published.

Not published.

The program’s contribution is the pathfinder itself: a deliberately intermediate vehicle whose purpose is to fly the flight-sized subsystems of a larger rover on a lander that already exists, rather than waiting for the launch vehicle the larger rover needs [11]. The subsystems being proven that way are the batteries and their enclosure, the hyper-deformable airless tires, the avionics, the sensors and the software, the protective coatings on the solar array and radiator, and the dust sealing of the wheel actuators.

VIPER is the closest available comparison for what that qualification work actually involves on a lunar rover of similar class, even though VIPER never flew. Its systems integration record documents a 40 km wheel endurance test to failure over lunar simulant and rocks, slip characterization at a dedicated terrain facility, sink-tank testing in glass beads to develop entrapment-escape gaits for soft polar shadowed-region soil, and two rover-egress campaigns with Astrobotic that changed the Griffin rampway design after finding rover-lander interferences no CAD model had caught [9]. None of that class of ground test result has been published for FLIP. Software cost alone was a material factor in VIPER’s schedule, estimated with a dedicated life-cycle cost model built from historical module-sizing analogies and parametric cross-checks, an effort scale VIPER’s cancellation did not remove from the class of vehicle FLIP belongs to [10].

Nothing about FLIP’s own vehicle has been demonstrated yet, and nothing about it has been published in a form that carries a measurement.

Every quantitative figure specific to FLIP comes from the manufacturer or its landing services partner, not from a reviewed publication, and no peer-reviewed or conference paper about the vehicle has appeared [11], [12]. Dimensions, drive speed, slope and obstacle limits, generation and battery capacity, night survival, and communications parameters are absent entirely. The wheel duty cycle cited above describes the larger FLEX vehicle, not the roughly 500 kg FLIP, and no source states whether the same tire design meets the same duty cycle at FLIP’s lower mass [3]. Delivery date has already slipped once, from an announced end of 2025 to a subsequently stated summer 2026, and no source reconciles that slip with Griffin Mission One’s own schedule [11], [12]. Nothing in the corpus describes a ground test campaign for FLIP comparable to VIPER’s wheel endurance, slip characterization or egress testing, so whether FLIP has undergone equivalent verification, or is flying without it, cannot currently be established [9].

References

  1. (2026). Astrolab: NASA Selects Astrolab to Provide Lunar Rover for Artemis. astrolab.space/2026/05/26/nasa-selects-astrolab-to-provide-lunar-rove...
    BibTeX
    @misc{astrolabnasa,
      title = {Astrolab: NASA Selects Astrolab to Provide Lunar Rover for Artemis},
      organization = {astrolab.space},
      year = {2026},
      url = {https://www.astrolab.space/2026/05/26/nasa-selects-astrolab-to-provide-lunar-rover-for-artemis-astronauts-return-to-the-moon/}
    }
  2. (2026). Astrolab: FLEX Rover. astrolab.space/flex-rover
    BibTeX
    @misc{astrolabflex,
      title = {Astrolab: FLEX Rover},
      organization = {astrolab.space},
      year = {2026},
      url = {https://www.astrolab.space/flex-rover/}
    }
  3. (2026). Venturi Space: World premiere, Venturi's hyper-deformable lunar wheel. venturi.space/en/article/world-premiere-venturi-hyper-deformable-luna...
    BibTeX
    @misc{venturispaceworld,
      title = {Venturi Space: World premiere, Venturi's hyper-deformable lunar wheel},
      organization = {venturi.space},
      year = {2026},
      url = {https://venturi.space/en/article/world-premiere-venturi-hyper-deformable-lunar-wheel/}
    }
  4. Mulvaney, J., Arney, D., Williams, C., Morel, J., Stockdale, C., Whitlock, C. and Balaji, V. (2025). In-Space Servicing, Assembly, and Manufacturing (ISAM) State of Play, 2025 Edition . NASA, 20250008988. Source
    BibTeX
    @techreport{nasa2025space,
      title = {In-Space Servicing, Assembly, and Manufacturing (ISAM) State of Play, 2025 Edition},
      author = {Mulvaney, John and Arney, Dale and Williams, Christina and Morel, Jose and Stockdale, Christopher and Whitlock, Christopher and Balaji, Vishruth},
      number = {20250008988},
      institution = {NASA},
      year = {2025},
      url = {https://ntrs.nasa.gov/citations/20250008988},
      abstract = {The future of spaceflight will yield increasingly more ambitious missions to support civil, national security, 
    and commercial space sectors. Achieving some of these missions will not be feasible by launching an 
    integrated, fully functioning system on a single launch vehicle. Future science and human exploration 
    missions will require payloads that are larger than any foreseeable launch vehicle fairing, national security 
    missions will require persistent assets that are mobile and resilient, and commercial space missions will 
    require cost-effective ways to update to the latest technology on orbit.
    
    In-space Servicing, Assembly, and Manufacturing (ISAM) can vastly expand the performance, availability, 
    and lifetime of space systems compared to the traditional paradigm of launching an asset with no intent 
    to ever interact with it again. ISAM capabilities foster an ecosystem that changes the space operations 
    paradigm, creating the foundation for sustainable exploration and serving as a multiplier for other 
    capabilities like space logistics, power generation, and reusability.
    
    Previous achievements in ISAM have enabled ambitious human and robotic space missions. The 
    assembly, operation, and maintenance of NASA’s International Space Station (ISS); servicing missions to
    the Hubble Space Telescope (HST); and Northrop Grumman’s Mission Extension Vehicle (MEV) 
    demonstrate the dramatic operational missions that can be achieved using ISAM capabilities. Many 
    current and upcoming flight demonstrations are advancing areas that will enable the next generation of 
    civil, national security, and commercial space missions.
    
    This document describes the current state of ISAM missions, activities, and technologiesto the best ability 
    of the authors. Compiling and organizing the available ISAM capabilities will help mission designers 
    incorporate ISAM technologies into their concepts, create the starting point for technology development 
    plans and roadmaps, and provide technologists a survey of the field they are developing. This document 
    divides the ISAM capabilities into 11 functional capability areas that describe the functions or activities 
    that can be performed in space using ISAM.}
    }
  5. 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}
    }
  6. 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.}
    }
  7. Gaier, J. R. (2007). The Effects of Lunar Dust on EVA Systems During the Apollo Missions . NASA, NASA/TM-2005-213610/REV1. Source
    BibTeX
    @techreport{gaier2007effects,
      title = {The Effects of Lunar Dust on EVA Systems During the Apollo Missions},
      author = {Gaier, James R.},
      number = {NASA/TM-2005-213610/REV1},
      institution = {NASA},
      year = {2007},
      url = {https://ntrs.nasa.gov/citations/20070021819},
      abstract = {Mission documents from the six Apollo missions that landed on the lunar surface have been studied in order to catalog the effects of lunar dust on Extra-Vehicular Activity (EVA) systems, primarily the Apollo surface space suit. It was found that the effects could be sorted into nine categories: vision obscuration, false instrument readings, dust coating and contamination, loss of traction, clogging of mechanisms, abrasion, thermal control problems, seal failures, and inhalation and irritation. Although simple dust mitigation measures were sufficient to mitigate some of the problems (i.e., loss of traction) it was found that these measures were ineffective to mitigate many of the more serious problems (i.e., clogging, abrasion, diminished heat rejection). The severity of the dust problems were consistently underestimated by ground tests, indicating a need to develop better simulation facilities and procedures.}
    }
  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. Andrews, D. (2023). VIPER: Systems Integration Status . International Astronautical Congress, 20230001799. Source
    BibTeX
    @inproceedings{andrews2023viper,
      title = {VIPER: Systems Integration Status},
      author = {Andrews, Daniel},
      booktitle = {International Astronautical Congress},
      number = {20230001799},
      institution = {NASA},
      address = {Baku},
      year = {2023},
      url = {https://ntrs.nasa.gov/citations/20230001799},
      abstract = {NASA’s Artemis Program plans to return humans to the Moon for an extended stay. To do so will require substantial resources to sustain that continued human presence, including continuous supplies delivered from the Earth. Given the expense and complexity of resource deliveries from Earth, if some resources were indigenously available, substantial logistical savings could be available by “living off the land”, wherever possible. 
    
    The LCROSS[1] , LRO and other missions have confirmed the presence of resources such as water-ice and other volatiles in lunar polar regions, so the next step is to understand the scientific nature and physical distribution of those candidate resources. Those local volatiles could be processed into propellants and human life-supporting needs, reducing risk of maintaining a permanent human presence on the Moon. 
    
    The Volatiles Investigating Polar Exploration Resource (VIPER) is a surface mobility scientific platform, designed to spend ~100 days mapping and surveying four different Ice Stability Regions to understand the scientific nature and distribution of water and other volatiles. VIPER will also provide scientific mineralogical context of the lunar regolith, such as the presence of silicon and light metals in lunar regolith, providing a composite picture of resource availability and sustainment. 
    
    This paper will discuss the latest systems-level integration activities by the VIPER team, following our initial introduction to this mission at IAC2021[2] . The VIPER team successfully passed its Systems Integration Review (SIR) in late-2022, and in early 2023, began system-level surface segment (rover) flight hardware assembly. 
    
    VIPER is managed within NASA’s Science Mission Directorate (SMD), utilizing the Commercial Lunar Payload Services (CLPS) lunar delivery model with partner, Astrobotic, Inc.}
    }
  10. Stukes, S. A., Hihn, J., Allan, M., Bajjalieh, G., Deans, M., Fong, T. and Utz, H. (2021). An Innovative Approach to Modeling VIPER Rover Software Life Cycle Cost . IEEE Aerospace Conference. Source
    BibTeX
    @inproceedings{stukes2021innovative,
      title = {An Innovative Approach to Modeling VIPER Rover Software Life Cycle Cost},
      author = {Stukes, Sherry A and Hihn, Jairus and Allan, Mark and Bajjalieh, Georgia and Deans, Matthew and Fong, Terry and Utz, Hans},
      booktitle = {IEEE Aerospace Conference},
      publisher = {IEEE},
      year = {2021},
      doi = {10.1109/aero50100.2021.9438347},
      abstract = {NASA's “Volatiles Investigating Polar Exploration Rover” (VIPER) will be the first robotic mission to prospect for water ice near the south pole of the Moon in late 2023 on a 100-Earth-day mission. The information that the VIPER rover provides will help improve understanding of the composition, distribution, and accessibility of Lunar polar volatiles and will help determine how the Moon's resources can support future human space exploration. VIPER, however, represents a radical departure from the way that NASA has traditionally developed planetary robotic missions. A key consequence of these differences is that estimating the cost of VIPER's rover software is challenging and complex. For example, VIPER is being developed using management procedures typically applied to NASA research and technology projects, rather than space flight programs. In addition, key portions of the rover's software are being designed as ground software to run on mission control computers (rather than onboard the rover as flight software as with prior planetary missions) taking advantage of continuous, interactive data communications between the Moon and Earth and higher performance computing available on the ground. Moreover, the rover's software is being engineered using Agile software development practices and incorporates a significant amount of open-source code, rather than following traditional (spiral, waterfall, etc.) development methods and in-house code. In this paper, we present an innovative process to estimate the life cycle cost of VIPER's rover software. We first describe how we modeled the architecture and code counts for three software elements: Rover Flight Software (RFSW), Rover Ground Software (RGSW), and Rover Simulation Software (RSIM). We then discuss key challenges and unique aspects of our approach, such as the lack of Lunar rover analogies, the need to integrate and test large open source software, and the strategies developed to account for use of non-space flight management practices and the impact of the COVID-19 pandemic. We conclude with a summary of our results, including cumulative distribution, nearest neighbors and cluster analysis, as well as heuristics used to confirm the reasonableness of the cost estimate.}
    }
  11. (2026). Astrolab: FLIP Rover. astrolab.space/flip-rover
    BibTeX
    @misc{astrolabflip,
      title = {Astrolab: FLIP Rover},
      organization = {astrolab.space},
      year = {2026},
      url = {https://www.astrolab.space/flip-rover/}
    }
  12. (2025). Astrobotic: Astrolab's FLIP rover joins Astrobotic's Griffin-1 to the Moon. astrobotic.com/astrolabs-flip-rover-joins-astrobotics-griffin-1-to-th...
    BibTeX
    @misc{astroboticastrolabs,
      title = {Astrobotic: Astrolab's FLIP rover joins Astrobotic's Griffin-1 to the Moon},
      organization = {astrobotic.com},
      year = {2025},
      url = {https://www.astrobotic.com/astrolabs-flip-rover-joins-astrobotics-griffin-1-to-the-moon/}
    }