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The Lunar PlanetVac sampling head mounted at the end of Firefly's Sample Access Arm beneath the Blue Ghost lander before flight, with the open mouth of the hood taped over for protection. Two rigid gas supply lines enter the top of the hood and the flexible sample transfer hose leaves it to the upper left, running up the arm to the collection system on the lander mid-deck NASA/Firefly Aerospace. Public domain (NASA / US government work).

Lunar PlanetVac is a pneumatic sample acquisition and delivery system built by Honeybee Robotics and flown on Firefly Aerospace’s Blue Ghost Mission 1 to Mare Crisium under NASA’s Lunar Surface Instrument and Technology Payloads program [1], [5]. It has no scoop, no arm and no moving sampling element. A jet of gas inside a sampling head lofts regolith into a transfer tube, and a capture system at the far end separates the sample from the flow.

The system is three parts: the sampling head, which needs access to the surface; the transfer tubes; and the capture system, which delivers the sample to an instrument or a return container [1]. The head can be built into one or more lander footpads or deployed on a boom. On Blue Ghost it rode on a Firefly-provided Sample Access Arm released by launch lock after touchdown, with the transfer tube running up the arm to a collection system on the temperature-controlled mid-deck.

Acquisition took place on 3 March 2025, the day after landing [1].

ParameterValueSource
Subsystemssampling head, transfer tubes, capture system[1]
Working fluidgas from a standalone canister, nitrogen on this flight[2], [3]
Acquisition timeabout 5 seconds from gas release to captured sample[1]
Transport timeunder 1 second from head to collection container
Sample verificationinfrared break-beam pair at the chamber inlet, plus imaging
Capture mechanismetched screens along a labyrinth path
Particle sortingsecond gas burst, separation about 1 mm
Deployment on Blue GhostFirefly Sample Access Arm, launch-lock released

Mass, gas quantity, gas pressure, power draw and the dimensions of any part of the system are not published.

ParameterValueSource
LanderFirefly Aerospace Blue Ghost[1]
Launch15 January 2025
Landing2 March 2025, Mare Crisium
Sampling3 March 2025
Volume collectedabout 6.5 cc against a 1 cc requirement
Mass collected13 g including 5 g of rocklets about 2 mm across[2]
Sampling head positionnot flush with the surface[1], [2]

The volume and the mass come from two abstracts by the same team and are not reconciled in either; neither publishes the bulk density that would connect them, so they are two independent statements about one event rather than a consistent pair.

Gas jets inside the sampling head point downward, loft regolith and sweep it into the transfer tube [3]. The efficiency argument is that gas behaves like an explosive in vacuum, so a small quantity moves a large amount of material, and the process is indifferent to gravity. Collection finishes in seconds after a single valve command, so the power draw and the operational overhead are both small and no operator is needed in the loop.

The architectural claim is about routing rather than about digging. A scoop on a robotic arm can deliver only where the arm’s kinematics reach, and the instrument must be placed accordingly; a pneumatic transfer line can be run around obstacles, so acquisition hardware goes where sampling is best and instruments go where analysis is best [3].

The problem the design exists to solve is documented rather than asserted. In parabolic flight at one sixth g, JSC-1A lunar simulant in an hourglass hopper flowed very slowly and in some runs stopped altogether, restarting only when the assembly was tapped, shaken, bounced and hammered [3]. JSC-1A contains no agglutinates, and the authors note that real lunar soil in hard vacuum is more cohesive still. Sample delivery, not acquisition, is where several earlier missions lost science: Venera did not meet its goals because of a delivery failure, and part of the Phoenix instrument suite went unused because cohesive material could not be placed in its cups.

None. The sampling head is carried to the surface by its host’s deployment mechanism and does not move afterwards.

No power figure is published. The system’s own argument is that total draw is negligible because a single valve opens for a few seconds [3].

The sampling head and transfer tubing sit outside on the arm; the collection system is on the lander’s temperature-controlled mid-deck [1]. No operating or survival temperature limits are published.

None of its own beyond the pneumatics manifold and the break-beam sensors. The commanding and the imaging both belong to the host lander [1].

None. One command opens the manifold, and the sequence that follows is a physical process rather than a controlled one.

Through the lander.

A pair of infrared break-beam sensors at the collection container inlet captures high-speed data on material passing into the chamber, giving a non-image verification that sample arrived [1]. A camera images the collected sample, both to correlate against the break-beam data and to image dust coupons mounted on the back wall of the chamber.

Collection, then verification, then sorting. On command the manifold releases gas down the arm to the head; the gas exits the nozzles and lofts material up the tube, arriving in under a second; the break-beam pair records the passage; the sample is caught on etched screens along a labyrinth path [1]. After imaging, a second burst enters by a secondary path, vents the finest fraction with the exhaust gas and separates the remainder about 1 mm either side of a dividing wall, coarse on one side and fine on the other, because some instruments want a size-selected sample.

The lander team deployed the Sample Access Arm; the sampling itself was one commanded event [1]. No planning cycle or tooling is published.

The flight demonstrated that a pneumatic sampler works on the Moon, and it demonstrated something less expected about its robustness. The sampling hood was not flush with the surface, appearing from the video to be aggressively angled or standing off it, and it still collected several times the required volume [1]. The team’s comparison is that the result resembles off-nominal laboratory tests with the head several inches clear of the sampled surface, which is a qualitative match rather than a measured one, and no corresponding ground case is cited by name.

Two capabilities beyond acquisition were shown in the same event: verification of a delivered sample without an image, from break-beam timing alone, and particle size selection in the capture chamber using nothing but a second gas burst [1].

The unplanned result was lens cleaning. Pneumatic operation cleared accumulated dust and propellant residue from camera lenses, visible both in the capture chamber after sieving and in the collection video [1], [2].

What the flight does not establish is nominal performance. There is one acquisition, from a position that was not commanded and cannot be reconstructed, so the collected quantity cannot be attributed to a known standoff, and the builders’ assignment of technology readiness level 9 rests on that single off-nominal event [2].

References

  1. (2026). NASA: Lander to Test Vacuum Cleaner on Moon for Sample Collection. nasa.gov/missions/artemis/clps/nasa-lander-to-test-vacuum-cleaner-on-... (accessed 2026-09-02)
    BibTeX
    @misc{nasalander,
      title = {NASA: Lander to Test Vacuum Cleaner on Moon for Sample Collection},
      howpublished = {\url{https://www.nasa.gov/missions/artemis/clps/nasa-lander-to-test-vacuum-cleaner-on-moon-for-sample-collection/}},
      organization = {nasa.gov},
      year = {2026},
      urldate = {2026-09-02}
    }
  2. NASA. (2020). Cross-Program Design Specification for Natural Environments (DSNE), Revision G. NASA Marshall Space Flight Center. Source
    BibTeX
    @techreport{nasa2019cross,
      title = {Cross-Program Design Specification for Natural Environments (DSNE), Revision G},
      author = {NASA},
      year = {2020},
      institution = {NASA Marshall Space Flight Center},
      url = {https://ntrs.nasa.gov/citations/20200000867}
    }
  3. Grant H. Heiken, David T. Vaniman and Bevan M. French. (1991). Lunar Sourcebook: A User's Guide to the Moon. Cambridge University Press. Source
    BibTeX
    @book{heiken1991lunar,
      title = {Lunar Sourcebook: A User's Guide to the Moon},
      author = {Grant H. Heiken and David T. Vaniman and Bevan M. French},
      year = {1991},
      publisher = {Cambridge University Press},
      url = {https://www.lpi.usra.edu/publications/books/lunar_sourcebook/pdf/LunarSourceBook.pdf}
    }