SPACE PHILICLELP-1 · LIFE SCIENCE IN ORBIT
Experiments · 14 of 15

Muscle biology / ageing

C. elegans muscle and ageing

Astronauts lose muscle in orbit, and people on Earth lose muscle with age, disuse and diseases such as Duchenne muscular dystrophy. The worm C. elegans grows from larva to adult in about four days, has well-mapped genetics, and has been studied in space for more than 20 years. On ISS flights, worms grown in microgravity had less myosin heavy chain, smaller body-wall muscle cells and less strength, and similar gene changes appeared across missions. An uncrewed free-flyer could repeat these runs more often, without waiting for crew time, to test which genes and drugs protect muscle.

BayLarge · 5.6 kg
Power28 W peak
Temperature20 °C
Duration14 days
LaunchesLive, starved L1 larvae arrested in buffer (M9…
Returns4 °C · lab within 336 h

Who it is for

  • University C. elegans and muscle biology groups studying spaceflight muscle loss and ageing
  • Space agency life-science and astronaut countermeasure programmes
  • Pharma and biotech teams screening drugs against muscle wasting, sarcopenia or muscular dystrophy in a whole animal
  • Companies that make C. elegans phenotyping tools (for example microfluidic strength or imaging assays) and want flight data

What earlier flights found

YearMissionWhat flewWhat it found
2004ICE-First (International C. elegans Experiment First), flown during the ESA DELTA missionISS (carried on a Soyuz that docked with the ISS)Mixed-stage wild-type and transgenic C. elegans in chemically defined medium (CeMM) in gas-permeable culture bags inside a vented Biorack experiment container. Worms spent 2 days at 12 C in transit, then 9 days on the ISS at 20 C, and were frozen in liquid nitrogen within 2 h of landing.Myosin heavy chain fell in body-wall and pharyngeal muscle, with lower expression of the myogenic factors HLH-1, PEB-1, CEH-22 and PHA-4. Flown worms moved more slowly after return. A later analysis of the same flight found fewer polyglutamine (Q35::YFP) aggregates in body-wall muscle, and seven genes down-regulated in space extended lifespan when inactivated on the ground.12
2009CERISE (C. elegans RNA Interference in Space Experiment), JAXAISS Japanese Experiment Module, Cell Biology Experiment Facility; up on Space Shuttle Atlantis STS-129 (16 November 2009), down on Space Shuttle Endeavour STS-130 (21 February 2010)Synchronised L1 larvae held in stasis in M9C buffer, then given bacterial food on the ISS (start 20 November 2009) and grown 4 days at 20 C in microgravity and on a 1 G centrifuge. Movies were downlinked. Samples were frozen at -80 C in the ISS freezer (MELFI) and returned.Gene and protein levels for muscle thick filaments, cytoskeleton and mitochondrial enzymes fell in microgravity worms compared with the 1 G centrifuge worms. Swimming frequency differed, body length was about 5.5% shorter, and fat storage was lower.3
2018Molecular Muscle Experiment (MME), University of Nottingham with Exeter and LancasterISS (launched on a SpaceX Falcon 9, 5 December 2018)Wild-type N2 and unc-70 mutant worms (the strains used in the muscle analysis), about 500 synchronised L1 larvae per polyethylene bag in 6.5 mL with freeze-dried E. coli OP50. Bags were cold-stowed at 8-13 C until arrival, incubated 5 days on the ISS, then frozen at -80 C. The project also used gene changes and drugs.Ground tests for the hardware showed that gas exchange limits worm growth in sealed plastic bags, with best growth at 5-7 mL (MME bags about 8.4 cm2/mL surface area to volume; ICE-First bags about 10 cm2/mL). In flight worms, the ratio of body-wall muscle length to body length was 29.7% lower in wild type and 27.4% lower in unc-70.456
Not stated in the sources we checkedNIS (Neural Integration System), JAXAISS, with an on-board 1 G centrifuge controlAbout 200 synchronised wild-type L1 larvae per sample in M9 buffer with cholesterol and E. coli food, grown at 20 C for 12 days in total. FUdR (75 uM) was added to stop new offspring. The astronaut fixed half of each sample in 0.7% paraformaldehyde at day 1 and day 10 of adulthood. Samples were kept at 4 C.Supported the MME result: wild-type body-wall muscle cell area was 23.4% smaller in microgravity than in the space 1 G control.6
2021micro-16ISS (launched on Northrop Grumman NG-15, 20 February 2021)Wild-type and dys-1 (BZ33, a Duchenne model) worms in FEP bags, from cultures kept in chemically defined medium (CeMM), handed over at 15 C and grown at 20 C on the ISS. Strength was measured in the second generation: crew loaded worms, including adults, into NemaFlex-S micropillar devices and recorded 1-minute videos. Bags were frozen at -80 C in MELFI for transcript analysis.Strength was 16.6% lower in flight worms than in ground controls. In flight, dys-1 worms were 23% weaker than wild-type worms. Transcripts showed more stress-response activity, lower mitochondrial and cytoskeletal activity, and links to neuronal calcium and acetylcholine signalling.7

How LELP-1 runs it

Sample. C. elegans hermaphrodites: wild-type N2 plus one muscle-relevant strain chosen by the customer, for example dys-1 (BZ33), a body-wall muscle GFP reporter, or the Q35::YFP polyglutamine line. Each well holds about 50-100 age-synchronised L1 larvae. Container. 24-well gas-permeable culture cassette (about 0.5 mL liquid per well, thin gas-permeable film lid) inside the sealed bay. Two identical large modules fly: Module A (young-adult time point) and Module B (aged time point). Each bay block holds only one temperature, so the two time points need separate bays. Launch. Live, starved L1 larvae arrested in buffer (M9 with cholesterol) without food, held at 12 C. CERISE used a similar approach: L1 larvae held in stasis in buffer, then fed on orbit to start the experiment. Light and gas. Dark, except for short LED pulses during imaging. Air headspace through the gas-permeable lid in the sealed bay; no CO2 needed. Worm number and liquid volume are kept low because MME ground tests found gas exchange limits growth in sealed bags.

  1. day -2

    Ground: bleach gravid adults, hatch eggs overnight in buffer to get synchronised L1 larvae, load each well, seal the cassettes, close the triple containment. Load reservoirs: freeze-dried E. coli OP50 food, FUdR, paraformaldehyde fixative, RNA preservation solution. Hold at 12 C.

  2. day 0

    Launch. Both modules hold 12 C; larvae stay arrested without food.

  3. day 1

    After orbit checkout and once the arm is parked (quasi-steady microgravity), raise both modules to 20 C. Pump bacterial food into every well to start development. Take baseline brightfield images of each well.

  4. day 2

    Daily, both modules: 30-60 s brightfield video per well (swimming frequency, body length, stage); fluorescence images if a reporter strain flies. Downlink a compressed subset.

  5. day 3

    Worms near L4: add FUdR to both modules (NIS used 75 uM) to stop new offspring before egg laying starts. Top up food.

  6. day 5

    Module A (about day 1 of adulthood): final video and fluorescence imaging. Then fix 12 wells with paraformaldehyde (for muscle staining and body length) and fill 12 wells with RNA preservation solution (for gene expression). Drop Module A to 4 C and hold it there until the courier hands it over.

  7. day 7

    Module B: top up food and FUdR. Continue daily imaging. Repeat every 2-3 days.

  8. day 13

    Module B (about day 9 of adulthood): final video and fluorescence imaging. Fix 12 wells and preserve 12 wells for RNA, as in Module A. Drop Module B to 4 C.

  9. day 14

    Deorbit and splashdown with both modules at 4 C. Recovery ship hands the sealed modules to the customer's courier (about 20 min after splashdown); cold transport at 4 C to the lab (about 1-2 days).

The payload module, in CAD

Every item in the module sheet, drawn and packed into the large bay deck by deck. The back face mates with the bay: blind-mate connector, and a cold wall against the bay's thermoelectric block. The front face carries Dexter-L's grapple fixture, and the fluid lines run down a channel just behind it. What you load before launch is marked blue in the configurator's payload guide.

CAD generated by cad/build_modules.py (CadQuery, OpenCascade kernel) from the catalog's module items: concept geometry, not a released design. Standard parts keep their real formats; the rest are sized from their catalog mass. The front panel and grapple fixture are left off in the 3-D view and are in the STEP.

Checks

Fits the large bayFITS313 x 191 x 365 mm envelope; 122 mm of height to spare
MassAS CATALOG5.60 kg in the parts, 5.60 kg in the catalog
Parts' boxes37 % of the 21.1 L inside
HousingTHIN0.80 kg of structure and containment: a 0.38 mm aluminium skin
Centre of mass-3 mm across and -4 mm front to back (+ is toward the front) from the middle, 107 mm up
Lines6 fluid lines and 3 harness runs, routed in the channel behind the front panel

Inside, top to bottom

  1. Experiment deck imaging stack: inverted microscope, XY stage, sample; dosimeter; 2 micro-pumps, 4 valves on a manifold
  2. Floor deck fluid pack; controller and data storage
  • The XY stage travels 96.5 x 57.9 mm, so every one of the 24 wells reaches the objective; with the stage the imaging stack is 232 x 151 mm, which sets the module's depth budget.
  • Reagent volumes the catalog does not state are split evenly from 75 % of the reservoir item's mass. The waste bag holds the spent medium and washes; fixatives and stabilisers stay in the wells and come home.
  • Fluid pack: 4 reagent bags in 2 layers (164 x 120 x 46 mm), every port on a front edge.
  • The waste bag lies under the reagent bags and fills the room they free: they hold 675 mL, it needs 169 mL.
  • The catalog gives 0.80 kg for structure and containment; as an aluminium box that is a 0.38 mm skin on 0.24 kg of posts and shelves. Thin: the bay rails have to carry the launch loads, or the module needs more structure mass.
  • The grapple fixture stands 26 mm proud of the front panel, into the bay opening; everything else is inside the bay envelope.
Components (5) and how each catalog item was drawn
ComponentDeckkgBox mm
fluid packFloor deck0.90164 x 128 x 51
controller and data storageFloor deck0.32125 x 91 x 28
imaging stack: inverted microscope, XY stage, sampleExperiment deck2.70232 x 151 x 174
dosimeterExperiment deck0.1054 x 32 x 14
2 micro-pumps, 4 valves on a manifoldExperiment deck0.7050 x 94 x 38
Catalog itemkgDrawn as
24-well gas-permeable culture cassette with worms and buffer0.60cassette
Reservoirs and lines: bacterial food, FUdR, paraformaldehyde fixative, RNA preservation solution, waste0.90bags
Micropumps and valve manifold0.70pumps
LumaScope-class inverted microscope, brightfield plus 2 fluorescence channels1.50microscope
XY stage to move the cassette under the objective0.60stage
Controller board, camera interface and cabling0.40avionics, harness
Containment housing, seals and mounting structure0.80shell
Passive TLDs and extra in-cassette temperature probes0.10dosimeter
Every part with mass (68)
PartRolekgSize mm
bacterial food (169 mL)fluid0.18680 x 120 x 22
bacterial food portfluid0.0165 x 8 x 5
FUdR (169 mL)fluid0.18680 x 120 x 22
FUdR portfluid0.0165 x 8 x 5
paraformaldehyde fixative (169 mL)fluid0.18680 x 120 x 22
paraformaldehyde fixative portfluid0.0165 x 8 x 5
RNA preservation solution (169 mL)fluid0.18680 x 120 x 22
RNA preservation solution portfluid0.0165 x 8 x 5
waste bag (empty at launch, 169 mL capacity), under the reagent bagsfluid0.081164 x 120 x 5
waste bag portfluid0.0095 x 8 x 5
controller enclosure (boards, data storage)electronics0.288125 x 83 x 28
connector 1electronics0.01612 x 8 x 12
connector 2electronics0.01612 x 8 x 12
microscope base: optics, filter cubes, cameraimaging1.156170 x 120 x 70
objectiveimaging0.07422 x 22 x 16
XY stage frame (travel 96.5 x 57.9 mm: every well over the objective)imaging0.270232 x 151 x 8
stage carriageimaging0.120140 x 98 x 5
X stepperimaging0.10528 x 20 x 20
Y stepperimaging0.10520 x 16 x 20
illumination columnimaging0.08116 x 16 x 84
illumination armimaging0.054112 x 16 x 12
LED head, transmitted lightimaging0.13528 x 28 x 22
cassette, 24 wells (SBS footprint, 19.3 mm pitch)sample0.492128 x 86 x 34
culture in the wellssample0.018112 x 73 x 8
cassette lid, sealed and gas-permeablesample0.072128 x 86 x 2
cassette fluid port 1sample0.0096 x 7 x 6
cassette fluid port 2sample0.0096 x 7 x 6
TLD and temperature-probe holdersensor0.07040 x 32 x 12
passive TLD holdersensor0.03012 x 12 x 14
fluid manifoldpump0.21050 x 94 x 12
micro-pump 1pump0.17520 x 20 x 26
micro-pump 2pump0.17520 x 20 x 26
valve 1pump0.0359 x 9 x 16
valve 2pump0.0359 x 9 x 16
valve 3pump0.0359 x 9 x 16
valve 4pump0.0359 x 9 x 16
bottom panelhousing0.061313 x 191 x 2
top panelhousing0.061313 x 191 x 2
side panel Lhousing0.0712 x 191 x 362
side panel Rhousing0.0712 x 191 x 362
back panel (bay interface)housing0.117310 x 2 x 362
front panelhousing0.117310 x 2 x 362
corner post 1housing0.0218 x 8 x 362
corner post 2housing0.0218 x 8 x 362
corner post 3housing0.0218 x 8 x 362
corner post 4housing0.0218 x 8 x 362
shelf 1housing0.156310 x 158 x 2
cold wall (to the bay's thermoelectric block)thermal0.028290 x 4 x 352
blind-mate connector: power, data, videointerface0.01750 x 10 x 22
grapple fixture base (Dexter-L)interface0.01770 x 4 x 70
harness: controller and data storage to imaging stack: inverted microscope run 1harness0.0015 x 6 x 5
harness: controller and data storage to imaging stack: inverted microscope run 2harness0.0015 x 28 x 5
harness: controller and data storage to imaging stack: inverted microscope run 3harness0.0045 x 5 x 86
harness: controller and data storage to imaging stack: inverted microscope run 4harness0.007142 x 5 x 5
harness: controller and data storage to imaging stack: inverted microscope run 5harness0.0025 x 38 x 5
harness: controller and data storage to imaging stack: inverted microscope run 6harness0.0015 x 6 x 5
harness: controller and data storage to 2 micro-pumps run 1harness0.0015 x 6 x 5
harness: controller and data storage to 2 micro-pumps run 2harness0.0015 x 28 x 5
harness: controller and data storage to 2 micro-pumps run 3harness0.0115 x 5 x 228
harness: controller and data storage to 2 micro-pumps run 4harness0.00599 x 5 x 5
harness: controller and data storage to 2 micro-pumps run 5harness0.0045 x 86 x 5
harness: controller and data storage to 2 micro-pumps run 6harness0.0085 x 5 x 166
harness: controller and data storage to 2 micro-pumps run 7harness0.0015 x 5 x 6
harness: controller to the connector run 1harness0.0025 x 5 x 30
harness: controller to the connector run 2harness0.0055 x 95 x 5
harness: controller to the connector run 3harness0.012248 x 5 x 5
harness: controller to the connector run 4harness0.0155 x 5 x 293
harness: controller to the connector run 5harness0.0015 x 8 x 5

Measured in orbit

  • Swimming (thrashing) frequency and wave shape Brightfield video from the bay's inverted microscope, tracked frame by frame. CERISE measured swimming from downlinked movies.
  • Body length and developmental stage Brightfield images per well, measured with image analysis. CERISE found body length about 5.5% shorter in microgravity.
  • Population and survival per well Count moving and still worms from video; check for contamination or starvation.
  • Muscle reporter fluorescence or polyglutamine aggregates Bay fluorescence channel for a GFP or YFP muscle reporter. Aggregate counts and muscle cell detail need the 40x central microscope, reached by moving the bay with the arm.
  • Environment log Bay temperature, pressure, humidity and acceleration sensors; active silicon dosimeter and passive TLDs for radiation dose.

Measured after the return

  • Body-wall muscle cell area and muscle-to-body-length ratio Phalloidin staining of fixed worms and fluorescence microscopy, as in the MME and NIS analysis
  • Myosin heavy chain and other muscle protein levels Quantitative western blot or mass-spectrometry proteomics, as in ICE-First and CERISE
  • Gene expression (myogenic factors, mitochondrial, cytoskeletal, synaptic and longevity genes) RNA sequencing or qPCR on RNA-preserved wells, compared with the ground control
  • Young versus aged comparison Compare Module A (day 1 adult) with Module B (about day 9 adult), flight against ground, for muscle structure and transcripts
  • Polyglutamine aggregate count (if Q35::YFP flies) Fluorescence microscopy count of aggregates per worm, as in the ICE-First follow-up analysis
  • Radiation dose TLD readout to report the total dose the worms received

Ground control

Two identical ground modules with the same worm batches, food, reservoirs and cassette lots, run in a flight-like bay. Each step follows the flight timeline, with the bay's recorded temperature profile replayed about 1-2 days behind the flight (micro-16 replicated the flight temperature profile on a two-day delay). Ground modules are fixed, preserved, chilled and shipped the same way. This control cannot separate microgravity from space radiation or launch and re-entry loads. That needs an in-flight 1 G centrifuge control, as flown on CERISE and NIS.

Coming home

Fixed and RNA-preserved worms return sealed at 4 C. Module A samples are about 9 days past preservation at splashdown and about 10-11 days by the time they reach the lab. The 336 h (14 day) window is OUR ESTIMATE, and the customer must check it on the ground for both the fixative and the RNA solution. Heritage flights froze worms for gene and protein work: liquid nitrogen within 2 h of landing on ICE-First, and -80 C on orbit on CERISE, MME and micro-16. Only the NIS morphology samples were PFA-fixed and held at 4 C. If live worms are wanted for after-flight motility or lifespan tests, an extra well set must return unfixed at 15-20 C and reach the lab within about 48 h; this is also our estimate.

Limits of this flight

  • 14 days of lab time covers development and early ageing (to about day 9 of adulthood) only; the worms' full lifespan cannot be followed in orbit
  • No on-orbit freezing to -80 C. All the heritage gene and protein datasets we checked came from frozen worms, so chemical preservation (RNA solution, paraformaldehyde) at 4 C is a change that must be validated on the ground
  • No crew, so the micro-16 strength assay (crew loaded worms into micropillar devices) cannot be repeated as flown; strength would need a new automated chip
  • Without an in-flight 1 G centrifuge, the experiment cannot separate microgravity from radiation and launch or re-entry effects; CERISE and NIS had this control
  • Sealed wells limit oxygen and food, so worm number per well must stay low; MME ground tests found gas exchange limited growth in sealed bags, and a lid-only well has less gas-exchange area per mL than the heritage bags
  • The bay microscope is low magnification; sarcomere and mitochondrial detail needs the 40x central microscope or post-flight staining
  • Arm moves raise acceleration to about 1e-4 to 1e-3 g, which may disturb swimming measurements; imaging must avoid those periods
  • About 2 h to hand-over and 1-2 days to the lab means live worms partly readapt to 1 g before any post-flight motility test
  • Worm muscle has no satellite stem cells and differs from human muscle; results point to mechanisms and need follow-up in mammalian models
  • Two L bays per run use a large share of the 16 large bays

A satellite of its own: SP-WORM B · samples return, hardware burns up

SP-WORM is a 137 kg free-flyer. Only the samples come home: 2.3 kg ride in a 45 kg capsule in a drawer behind an optical window; the microscope looks through the window from the service module, and fluid lines cross through dry-break couplings that part at separation once the last fluid step is done. The microscope, pumps and reservoirs stay in the service module and burn up with it. Why B: two modules fly (young and aged); both cassettes come home, fixed or RNA-preserved.

See SP-WORM in 3-D

Comes home · capsule

worm culture cassette 10.60
worm culture cassette 20.60
sample drawer, optical window, dry-break couplings0.50
drawer thermoelectric block0.60
Capsule at entry (with heat shield, parachute, hold battery, margin)45.0

Stays · service module

experiment instruments, pumps and reservoirs10.00
Service module dry, with power, radios, attitude, propulsion79.9

Budgets · estimate

Launch mass136.7 kg
Propellant for 190 m/s11.8 kg
Average / peak load96 / 166 W
Array, worst eclipse season208 W
Battery (sized by ascent)350 Wh
Deorbit burn3 × 22 N, 394 s

Tailored for this experiment

  • Two large bays at once (one per time point), because each bay block holds a single temperature setpoint
  • Launch hold at 12 C from handover until orbit, then a step to 20 C, then 4 C after preservation and through re-entry and recovery (all inside the 4-45 C range, but the bay must be powered during ascent and descent)
  • Video imaging: 30-60 s brightfield clips per well each day, with some downlink bandwidth for compressed video
  • Arm transfer of each module to the central 40x fluorescence microscope for muscle reporter and aggregate imaging, scheduled so arm moves do not overlap the daily swimming videos
  • Optional: a small 1 G centrifuge position for an in-flight gravity control (not part of the standard bay)

Bay or satellite?

The capsule is the floor: no capsule much smaller than about 45 kg has been recovered yet, so 2.3 kg of samples need 137 kg of satellite. On LELP-1 the same samples share one capsule, the whole lab, with 31 other bays. A dedicated satellite earns its place when the experiment needs the schedule to itself, a quieter ride (about 7.3 × 10⁻⁸ g quasi-steady, no robotic arm), or power a bay cannot give.

First-order sizing with a 20 % margin by one model for every experiment, reviewed independently; caveats and sources. The smallest recovered capsule so far (Varda W-1) is under 90 kg, so treat these masses as optimistic.

References

  1. Higashibata A, Szewczyk NJ, Conley CA, et al., 2006. Decreased expression of myogenic transcription factors and myosin heavy chains in Caenorhabditis elegans muscles developed during spaceflight. Journal of Experimental Biology 209(16):3209-3218 https://doi.org/10.1242/jeb.02365
  2. Honda Y, Higashibata A, Matsunaga Y, et al., 2012. Genes down-regulated in spaceflight are involved in the control of longevity in Caenorhabditis elegans. Scientific Reports 2:487 https://doi.org/10.1038/srep00487
  3. Higashibata A, Hashizume T, Nemoto K, et al., 2016. Microgravity elicits reproducible alterations in cytoskeletal and metabolic gene and protein expression in space-flown Caenorhabditis elegans. npj Microgravity 2:15022 https://doi.org/10.1038/npjmgrav.2015.22
  4. Pollard AK, Gaffney CJ, Deane CS, et al., 2020. Molecular Muscle Experiment: Hardware and Operational Lessons for Future Astrobiology Space Experiments. Astrobiology 20(8):935-943 https://doi.org/10.1089/ast.2019.2181
  5. University of Nottingham, 2018. Blast off for first UK-led experiment on the International Space Station (press release) https://www.nottingham.ac.uk/news/pressreleases/2018/december/blast-off-for-first-uk-led-experiment-on-the-international-space-station.aspx
  6. Kim BS, Alcantara AV Jr, Moon JH, et al., 2023. Comparative Analysis of Muscle Atrophy During Spaceflight, Nutritional Deficiency and Disuse in the Nematode Caenorhabditis elegans. International Journal of Molecular Sciences 24(16):12640 https://doi.org/10.3390/ijms241612640
  7. Soni P, Edwards H, Anupom T, et al., 2023. Spaceflight Induces Strength Decline in Caenorhabditis elegans. Cells 12(20):2470 https://doi.org/10.3390/cells12202470

Fact-check: 23 claims and sources checked, 12 confirmed, 11 corrected, 0 removed · confidence high