SPACE PHILICLELP-1 · LIFE SCIENCE IN ORBIT
Experiments · 12 of 15

Immunology

Immune T-cell activation

Astronauts show immune dysregulation and reactivation of latent herpesviruses that last through 6-month ISS missions. On Earth, weak T-cell activation is also seen in older people. Since Spacelab 1 in 1983, flight experiments have found that human lymphocytes activated in suspension with the mitogen Con A respond much less in microgravity than on the ground. In a 2006 ISS study, gene expression already differed from the on-board 1 g control 1.5 hours after activation. Microgravity lets researchers weaken early T-cell activation without drugs or genetic edits, and study those early steps.

BayLarge · 5.6 kg
Power28 W peak
Temperature37 °C
Duration7 days
Launchescryopreserved (-80 C passive cassette)
Returns4 °C · lab within 144 h

Who it is for

  • University and hospital immunology labs studying T-cell signalling and immunosenescence (ageing of the immune system)
  • Space agency human-research programmes that need data on astronaut immune dysregulation and on countermeasures
  • Pharmaceutical and biotech groups testing immunomodulating compounds on a model where T-cell activation is already impaired
  • Research groups that already have ISS T-cell data and want a repeat flight with a different activator, donor set or time points

What earlier flights found

YearMissionWhat flewWhat it found
1983Spacelab 1Space Shuttle / SpacelabCultures of human lymphocytes exposed to the mitogen concanavalin A (Con A) in orbitActivation was strongly depressed. The Science paper reports less than 3 percent of the activation seen in ground controls.12
1991First Spacelab Life Sciences mission (SLS-1)Space Shuttle / SpacelabLymphocytes and monocytes attached to microcarrier beads, activated with Con AWith the cells attached to beads, DNA synthesis and interferon-gamma production more than doubled in microgravity. The authors concluded that the depression seen in earlier flights came from impaired macrophage function, not from a lymphocyte defect.23
2006Soyuz TMA-9 flight to the ISS; ESA KUBIK facility with LYCIS hardwareISSPurified human T cells from four donors, launched unfrozen at about 16-22 C and activated in orbit with Con A plus anti-CD28 at 36.5 C. A 1 g centrifuge control ran on board at the same time. Activation was stopped with RNAlater after 1.5 h, and samples returned on a Soyuz landing on 28 September 2006.Microarrays found 47 genes down-regulated twofold or more in microgravity compared with the on-board 1 g control. These included immediate early genes such as TNF, EGR1 and EGR2. Targets of Rel/NF-kB, CREB and SRF were down-regulated, and cRel binding sites were the most common among the inhibited genes.4
2014T-Cell Activation in Aging (launched on SpaceX-3)ISS (ESA KUBIK incubator, Columbus module)Isolated human T cells in experiment containers. The crew used plungers to add an activator and then a fixative. Part of the samples ran at 1 g artificial gravity as a control.The NASA page we cite describes only the design. Its stated aim was to study the mechanisms of diminished T-cell activation in ageing and in astronauts. It gives no results.5

How LELP-1 runs it

Sample. Human peripheral T cells (or PBMC, which keep the accessory cells) from 2 donors. Cells are cryopreserved before launch. They can be pre-labelled with a cell-tracking dye so proliferation can be measured after return. Container. Large bay 24-well cassette with gas-permeable lids and a filtered (about 0.4 um) outlet on each well, so supernatant can be drawn off without removing cells. Planned layout: 2 donors x 3 conditions (unstimulated; Con A + anti-CD28 to match the ISS heritage; soluble anti-CD3/anti-CD28) x 3 time points = 18 wells, plus 6 wells for imaging, viability and spares. Launch. cryopreserved (-80 C passive cassette); medium, activators and fixatives held in bay reservoirs. Light and gas. No light needed (dark incubation; the microscope LEDs run only during imaging). No CO2 supply: HEPES-buffered RPMI-type medium in sealed wells with gas-permeable lids.

  1. day -1

    Load the cryo cassette, reagent reservoirs (HEPES medium, Con A + anti-CD28, anti-CD3/anti-CD28, RNAlater, paraformaldehyde fixative) and the empty well cassette. Fix a pre-launch baseline aliquot of each donor on the ground.

  2. day 0

    Launch. Cells stay in the passive -80 C cassette. Bay reservoirs are held at 4 C.

  3. day 1

    Automated thaw at 37 C, then about 1:10 dilution into warm medium to lower the DMSO level, and dispensing into the wells. Brightfield images give the starting cell count and morphology.

  4. day 2

    After an 18-24 h rest at 37 C, fix one unstimulated set (t = 0) in RNAlater. Pump the activators into the stimulated wells. Lock out arm motion for the first 2 h. At 1.5 h, add RNAlater to the early-gene wells, as in the 2006 ISS flight.

  5. day 3

    24 h after activation: draw supernatant through the well filter into a sealed sample reservoir for cytokine analysis, then fix the cells with paraformaldehyde for flow cytometry (CD69, CD25). Take brightfield images of cell clustering every 6 h from day 2.

  6. day 5

    72 h after activation: split the final wells between paraformaldehyde (proliferation, Ki-67 or dye dilution) and RNAlater. Image all wells. Set the bay to 4 C.

  7. day 7

    Bay held at 4 C through re-entry and splashdown. Fixed cassette and supernatant reservoir are handed to the customer's courier at 4 C.

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; 28 mm of height to spare
MassAS CATALOG5.60 kg in the parts, 5.60 kg in the catalog
Parts' boxes43 % of the 21.1 L inside
HousingTHIN0.36 kg of structure and containment: a 0.17 mm aluminium skin
Centre of mass-2 mm across and -12 mm front to back (+ is toward the front) from the middle, 134 mm up
Lines8 fluid lines and 3 harness runs, routed in the channel behind the front panel

Inside, top to bottom

  1. Top deck -80 C passive cryo cassette; controller and data storage
  2. Experiment deck imaging stack: inverted microscope, XY stage, sample
  3. Floor deck fluid pack; 2 micro-pumps, 4 valves on a manifold
  • 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. The catalog lists no stage for this microscope: it is drawn inside the microscope's mass.
  • Reagent volumes the catalog does not state are split evenly from 75 % of the reservoir item's mass.
  • Fluid pack: 6 reagent bags in 2 layers (214 x 103 x 46 mm), every port on a front edge.
  • The supernatant reservoir lies under the reagent bags and fills the room they free: they hold 750 mL, it needs 150 mL.
  • The catalog gives 0.36 kg for structure and containment; as an aluminium box that is a 0.17 mm skin on 0.11 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 deck1.00214 x 111 x 51
2 micro-pumps, 4 valves on a manifoldFloor deck1.0050 x 94 x 38
imaging stack: inverted microscope, XY stage, sampleExperiment deck1.90232 x 151 x 180
-80 C passive cryo cassetteTop deck0.80159 x 80 x 80
controller and data storageTop deck0.36132 x 96 x 28
Catalog itemkgDrawn as
24-well cassette with gas-permeable lids and filtered outlets0.70cassette
Passive -80 C cryo cassette with donor cell vials0.80cryo
Filled reagent reservoirs (medium, two activator mixes, RNAlater, paraformaldehyde, live/dead stain) plus sealed supernatant reservoir1.00bags
Fluidics: micro-pumps, valves, manifold, tubing1.00pumps
LumaScope-class inverted microscope (brightfield + 2 fluorescence channels)1.20microscope
Bay electronics, sensor harness, mounting and containment liners0.90avionics, harness, shell
Every part with mass (73)
PartRolekgSize mm
medium (125 mL)fluid0.13869 x 103 x 22
medium portfluid0.0125 x 8 x 5
activator mixes 1 (125 mL)fluid0.13869 x 103 x 22
activator mixes 1 portfluid0.0125 x 8 x 5
activator mixes 2 (125 mL)fluid0.13869 x 103 x 22
activator mixes 2 portfluid0.0125 x 8 x 5
RNAlater (125 mL)fluid0.13869 x 103 x 22
RNAlater portfluid0.0125 x 8 x 5
paraformaldehyde (125 mL)fluid0.13869 x 103 x 22
paraformaldehyde portfluid0.0125 x 8 x 5
live/dead stain (125 mL)fluid0.13869 x 103 x 22
live/dead stain portfluid0.0125 x 8 x 5
supernatant reservoir (empty at launch, 150 mL capacity), under the reagent bagsfluid0.090214 x 103 x 5
supernatant reservoir portfluid0.0105 x 8 x 5
fluid manifoldpump0.30050 x 94 x 12
micro-pump 1pump0.25020 x 20 x 26
micro-pump 2pump0.25020 x 20 x 26
valve 1pump0.0509 x 9 x 16
valve 2pump0.0509 x 9 x 16
valve 3pump0.0509 x 9 x 16
valve 4pump0.0509 x 9 x 16
microscope base: optics, filter cubes, cameraimaging0.620170 x 120 x 70
objectiveimaging0.04022 x 22 x 16
XY stage frame (travel 96.5 x 57.9 mm: every well over the objective)imaging0.162232 x 151 x 8
stage carriageimaging0.072140 x 98 x 5
X stepperimaging0.06328 x 20 x 20
Y stepperimaging0.06320 x 16 x 20
illumination columnimaging0.05416 x 16 x 90
illumination armimaging0.036112 x 16 x 12
LED head, transmitted lightimaging0.09028 x 28 x 22
cassette, 24 wells (SBS footprint, 19.3 mm pitch)sample0.574128 x 86 x 40
culture in the wellssample0.021112 x 73 x 8
cassette lid, sealed and gas-permeablesample0.084128 x 86 x 2
cassette fluid port 1sample0.0116 x 7 x 6
cassette fluid port 2sample0.0116 x 7 x 6
-80 C passive cryo cassette: vacuum-insulated bodysample0.680139 x 78 x 78
cryo cassette capsample0.12020 x 80 x 80
controller enclosure (boards, data storage)electronics0.324132 x 88 x 28
connector 1electronics0.01812 x 8 x 12
connector 2electronics0.01812 x 8 x 12
bottom panelhousing0.028313 x 191 x 2
top panelhousing0.028313 x 191 x 2
side panel Lhousing0.0322 x 191 x 362
side panel Rhousing0.0322 x 191 x 362
back panel (bay interface)housing0.052310 x 2 x 362
front panelhousing0.052310 x 2 x 362
corner post 1housing0.0098 x 8 x 362
corner post 2housing0.0098 x 8 x 362
corner post 3housing0.0098 x 8 x 362
corner post 4housing0.0098 x 8 x 362
shelf 1housing0.035310 x 158 x 2
shelf 2housing0.035310 x 158 x 2
cold wall (to the bay's thermoelectric block)thermal0.013290 x 4 x 236
blind-mate connector: power, data, videointerface0.00850 x 10 x 22
grapple fixture base (Dexter-L)interface0.00870 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 2harness0.0045 x 29 x 5
harness: controller and data storage to imaging stack: inverted microscope run 3harness0.0225 x 5 x 172
harness: controller and data storage to imaging stack: inverted microscope run 4harness0.018138 x 5 x 5
harness: controller and data storage to imaging stack: inverted microscope run 5harness0.0055 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 2harness0.0045 x 29 x 5
harness: controller and data storage to 2 micro-pumps run 3harness0.0275 x 5 x 212
harness: controller and data storage to 2 micro-pumps run 4harness0.01185 x 5 x 5
harness: controller and data storage to 2 micro-pumps run 5harness0.0175 x 130 x 5
harness: controller and data storage to 2 micro-pumps run 6harness0.0065 x 5 x 44
harness: controller and data storage to 2 micro-pumps run 7harness0.0015 x 5 x 6
harness: controller to the connector run 1harness0.0075 x 5 x 58
harness: controller to the connector run 2harness0.0125 x 91 x 5
harness: controller to the connector run 3harness0.032251 x 5 x 5
harness: controller to the connector run 4harness0.0095 x 5 x 73
harness: controller to the connector run 5harness0.0015 x 8 x 5

Measured in orbit

  • Cell number, morphology and clustering (activated T cells form clusters) Brightfield time-lapse with the bay's LumaScope-class microscope, every 6 h from thaw to the last fixation
  • Post-thaw viability Two-colour live/dead fluorescent stain pumped into the dedicated imaging wells and read on the 2 fluorescence channels
  • Closer look at selected wells Robotic arm moves the bay to the central 40x fluorescence microscope, outside the activation and fixation windows
  • Exact activation and fixation times Time-tagged fluidics valve and pump log
  • Thermal, radiation and acceleration history Bay temperature, pressure and humidity sensors, active silicon dosimeter plus passive TLDs, and the accelerometer log (to flag any fixation that happened during arm motion)

Measured after the return

  • Immediate early gene expression (for example EGR1, EGR2, TNF) and later activation genes (IL2, IFNG, IL2RA) RNA extraction from RNAlater-fixed wells, then RNA-seq or microarray, with qPCR confirmation
  • Activation surface markers (CD69, CD25) and proliferation (Ki-67 or tracking-dye dilution) Flow cytometry on paraformaldehyde-fixed cells
  • Secreted cytokines (IL-2, IFN-gamma, TNF) Multiplex immunoassay on the filtered 24 h supernatants (4 C stability needs ground validation first)
  • Pathway activity (for example Rel/NF-kB, CREB and SRF targets) Analysis of transcription-factor binding sites and pathways in the gene-expression data, compared with the ground control and, if flown, the 1 g centrifuge control

Ground control

Synchronous ground control: an identical flight-model bay and cassette loaded with the same donor cell lots and reagent batches. It replays the same timeline (offset by a few hours) and the recorded flight temperature profile, including the -80 C hold, thaw, 37 C phases and the 4 C return hold. If possible, it also gets a launch vibration profile on a shaker table. Add a pre-launch baseline fixed on the ground. The key flight control in the 2006 and 2014 ISS studies was an on-board 1 g centrifuge running at the same time in KUBIK, which separates microgravity from radiation, launch and handling effects. LELP-1 should fly one (see needs). Without it, the result is flight versus ground only. Because the 2006 flight launched live cells unfrozen, the cryopreserved-launch step should also be checked against fresh cells on the ground.

Coming home

All cells are chemically fixed in orbit, so nothing needs to come back alive. The manufacturer states RNAlater stabilises RNA for 1 month at 4 C (and indefinitely at -20 C), which easily covers the return. The 144 h limit is our estimate and is set by the unfrozen 24 h supernatants: drawn on day 3, they spend about 4 days in orbit, then about 20 min to courier pickup and 1-2 days in transit, so about 6 days at 4 C. The last paraformaldehyde-fixed cells (day 5) reach the lab after about 3-4 days. The bay cannot go below 4 C, so supernatants cannot be frozen in orbit; their cytokine stability for 6 days at 4 C must be checked on the ground before flight. Keep everything at 4 C in transit and avoid temperatures above 25 C.

Limits of this flight

  • Without the added 1 g centrifuge, LELP-1 cannot tell microgravity effects apart from launch, radiation and handling effects. The 2006 and 2014 ISS studies used this control.
  • LELP-1 has no crew and no way to pellet cells. Thawed cells are diluted rather than washed, so some DMSO stays in the medium. Medium changes must go through filters, and activator or fixative mixing relies on pumped flow because there is no sedimentation or convection.
  • Bead-based activators need bead-cell contact, which in microgravity depends on mixing. The protocol therefore uses soluble activators (Con A + anti-CD28, soluble anti-CD3/CD28). Results with bead activation are not directly comparable.
  • Cell attachment changes the outcome: on SLS-1, bead-attached lymphocytes and monocytes responded more in microgravity, not less. Results from suspension wells apply to suspension culture only.
  • There is no CO2 supply. HEPES-buffered medium in sealed wells can drift in pH over several days of activated, high-metabolism culture, so 72 h is about the practical limit without a medium exchange.
  • No in-flight flow cytometry, cytokine assay or RNA readout. In flight, the satellite only gives images and environment logs; the molecular answers come after return.
  • Supernatants cannot be frozen (the bay minimum is 4 C), so cytokine values depend on about 6 days of stability at 4 C.
  • A 2-14 day free-flyer studies isolated cells in vitro. It cannot reproduce astronaut immune changes in the body over months, latent virus reactivation, stress hormones or the role of other tissues.
  • Few donors per flight (2 planned), so donor-to-donor variability limits the statistics. Several flights or more donors in a second bay may be needed.
  • The radiation environment at 550 km sun-synchronous orbit differs from the ISS, so dose comparisons with ISS heritage data need the on-board dosimeter record.

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

SP-IMM is a 133 kg free-flyer. Only the samples come home: 3.6 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, the centrifuge drive stay in the service module and burn up with it, and a small mechanism moves the fixed cassette off the rotor into the capsule first. Why B: all cells are fixed in orbit; the unfrozen day-3 supernatants set the return clock.

See SP-IMM in 3-D

Comes home · capsule

24-well cassette0.70
1 g rotor cassette0.80
reagent block with the sealed supernatant reservoir1.00
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 reservoirs3.90
centrifuge drive and structure4.50
cassette transfer mechanism (rotor to capsule)1.00
Service module dry, with power, radios, attitude, propulsion76.4

Budgets · estimate

Launch mass132.8 kg
Propellant for 190 m/s11.4 kg
Average / peak load82 / 155 W
Array, worst eclipse season179 W
Battery (sized by ascent)350 Wh
Deorbit burn2 × 22 N, 573 s

Tailored for this experiment

  • In-flight 1 g centrifuge control (not part of the standard bay): a second identical cassette on a small rotor. At 5 cm radius, 1 g needs about 134 rpm. Without it, the core control from the ISS heritage is missing.
  • Filtered well outlets and a sealed supernatant reservoir, so medium can be harvested in microgravity without drawing up the cells
  • Arm-motion lockout (keeping the vehicle in the 1e-6 g regime) for about 2 h after activator addition and during each fixation
  • A -80 C passive cassette hold time that covers the launch campaign plus 1 day in orbit, with the cassette temperature logged
  • Fixation events time-stamped against the accelerometer and dosimeter logs

Bay or satellite?

The capsule is the floor: no capsule much smaller than about 45 kg has been recovered yet, so 3.6 kg of samples need 133 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. Cogoli A, Tschopp A, Fuchs-Bislin P. 1984. Cell sensitivity to gravity. Science 225:228-230. doi:10.1126/science.6729481 https://www.ebi.ac.uk/europepmc/webservices/rest/search?query=EXT_ID:6729481%20AND%20SRC:MED&resultType=core&format=json
  2. Cogoli-Greuter M, Bechler B, Lorenzi G, Cogoli A, Sciola L, Pippia P, Sechi G. Mitogen binding, cytoskeleton patterns and motility of T lymphocytes in microgravity. In: ESA SP-1206, European Space Agency, April 1997 https://www.esa.int/esapub/sp/sp1206/cogol.htm
  3. Bechler B, Cogoli A, Cogoli-Greuter M, Muller O, Hunzinger E, Criswell SB. 1992. Activation of microcarrier-attached lymphocytes in microgravity. Biotechnology and Bioengineering 40(8). NASA NTRS record https://ntrs.nasa.gov/citations/20040089971
  4. Chang TT, Walther I, Li CF, Boonyaratanakornkit J, Galleri G, Meloni MA, Pippia P, Cogoli A, Hughes-Fulford M. 2012. The Rel/NF-kB pathway and transcription of immediate early genes in T cell activation are inhibited by microgravity. J Leukoc Biol 92(6):1133-1145. doi:10.1189/jlb.0312157 https://pmc.ncbi.nlm.nih.gov/articles/PMC3501893
  5. NASA Ames Research Center. T-Cell Activation in Aging (SpaceX-3). NASA Space Biosciences web page https://www.nasa.gov/ames/research/space-biosciences/t-cell-activation-in-aging-spacex-3
  6. Crucian BE, Chouker A, Simpson RJ, et al. 2018. Immune System Dysregulation During Spaceflight: Potential Countermeasures for Deep Space Exploration Missions. Frontiers in Immunology 9:1437. doi:10.3389/fimmu.2018.01437 https://www.frontiersin.org/journals/immunology/articles/10.3389/fimmu.2018.01437/full
  7. Thermo Fisher Scientific. RNAlater Stabilization Solution, product page (AM7020) https://www.thermofisher.com/order/catalog/product/AM7020

Fact-check: 17 claims and sources checked, 8 confirmed, 9 corrected, 0 removed · confidence high