cabin-thermal-humidity-control

Cabin thermal & humidity control

Subsystem Semi-native eclss
TRL Mars
Energy intensity
Required by
0
Requires
4

Removes metabolic and equipment heat and controls humidity in habitat air by circulating it across a condensing heat exchanger, holding temperature and dew point in the comfort/safety band. The condensed water (kilograms per crew per day) is captured and routed to water recovery, so humidity control is also a water-loop input. Reject heat goes to the thermal bus and ultimately the vacuum radiator. It guards against condensation damage and microbial growth as much as against discomfort.

Last reviewed: 2026-06-14

Governing equations

Total cabin cooling load = sensible (temperature) + latent (moisture) heat, removed as the air gives up enthalpy across the condensing exchanger. The latent part is large because crew add water continuously. [1]

To dehumidify, the heat-exchanger surface must run below the cabin dew point so water condenses out — the defining requirement, and the reason a "thermal" system is also the humidity system. [2]

Latent water load per crew member (respiration + perspiration) — captured as condensate and sent to water recovery, a major reclaimed-water stream. [3]

All captured heat must ultimately leave the habitat — handed to the coolant/thermal bus and rejected by the vacuum radiator to the Martian environment. [2]

Key constants & quantities

Symbol Value Units Conditions Description
Cabin temperature 18–27 °C Crew comfort band the system holds against continuous internal heat gain.[4]
Relative humidity 25–70 % Target humidity band — high enough for comfort/health, low enough to prevent condensation and microbial growth.[4]
Latent water / crew 1.8–2.3 kg/day Respiration + perspiration water captured as condensate per crew member — a primary feed to water recovery.[3]
Metabolic heat / crew 100–150 W (avg, activity-dependent) Sensible + latent heat each crew member adds to the cabin — multiplied across crew and equipment into the cooling load.[3]
Air circulation 4–10 cabin volumes / hour Ventilation rate to avoid stagnant pockets (CO₂ buildup, condensation) — microgravity needs forced flow; Mars gravity helps but forced circulation is still required.[1]

Operating envelope

ParameterRangeUnitsSource
Cabin temperature 18 – 27 °C [4]
Relative humidity 25 – 70 % [4]
Coil surface temperature 4 – 12 °C (below dew point) [2]
Air circulation rate 4 – 10 volumes/h [1]
Cooling load per crew + equipment 0.3 – 1 kW [3]

Mass balance

Basis: crew of 4, steady-state thermal/humidity control (per day)

Inputs

Cabin air (circulated) 1 continuous flow [1]
Coolant (chilled loop) 1 loop [2]
Fan + pump power 5 kWh/day [3]
  • Cabin air (circulated): 4-10 volumes/h across the condensing exchanger.
  • Coolant (chilled loop): Provides the sub-dew-point surface; rejects to thermal bus → vacuum radiator.
  • Fan + pump power: Air-circulation fan and coolant pump for a crew of 4.

Outputs

Conditioned air (T + RH in band) 1 maintained [4]
Condensate to water recovery 8 kg/day [3]
Rejected heat 1 to radiator [2]
  • Condensate to water recovery: ~2 kg/crew·day latent water captured — a major reclaimed-water feed.
  • Rejected heat: Metabolic + equipment heat handed to the thermal bus.
TRL · Earth
9/ 9
TRL · Mars
7/ 9
Condensing-heat-exchanger thermal/humidity control is flight-proven on the ISS (the Common Cabin Air Assembly) and prior spacecraft. It transfers directly to Mars; the adjustments are exploiting Mars gravity for condensate management and balancing heat rejection against the need to keep a habitat warm in a -60 °C environment.[1]
Energy budget
5 kWhe / crew-of-4 per day (circulation fan + coolant pump) [3]

Direct power is just fans and pumps; the heat itself is moved, not created, and ultimately radiated. On cold Mars some reject heat is usefully recycled to keep the habitat warm — thermal control becomes heat MANAGEMENT, balancing rejection against recovery.

Variants & trade-offs

Condensing heat exchanger + slurper (baseline)

[1]

Air driven across a chilled finned coil; condensate forms on the fins and is collected (in microgravity by a "slurper," on Mars assisted by gravity drainage) and routed to water recovery.

Materials: Finned condensing coil · Chilled coolant loop · Condensate collection + fan
  • Combines cooling and dehumidification in one unit
  • Recovers latent water for the water loop — flight-proven
  • Wet surfaces are microbial-growth sites — biofilm control needed
  • Coolant loop and radiator dependency

When preferred: Primary habitat thermal/humidity control — the standard approach.

Desiccant dehumidification

[3]

A regenerable desiccant wheel/bed adsorbs humidity, decoupling moisture removal from the cold coil — useful where condensation control or very low humidity is wanted.

Materials: Desiccant (silica gel/zeolite) · Regeneration heat
  • Avoids cold wet surfaces (microbial benefit); reaches low humidity
  • Decouples latent from sensible load
  • Regeneration energy; desiccant is a consumable/import
  • Captured water needs a separate recovery path

When preferred: Low-humidity or condensation-sensitive zones; complements the condensing coil.

Heat-recovery (warm-side integration)

[2]

On cold Mars, reject heat from cooling is fed back to warm other habitat volumes or processes rather than simply radiated away.

Materials: Heat-recovery exchanger · Thermal bus tie-in
  • Turns "waste" cooling heat into habitat heating — net energy win in a cold world
  • Reduces both heating and radiator loads
  • Added plumbing/control complexity; balances shifting loads

When preferred: Mars settlements where habitat heating demand can absorb the rejected heat.

Failure modes

Mode Cause Detection Mitigation
Microbial / mold growth on wet surfaces[1] Condensing surfaces and humid pockets are perfect microbial habitat; biofilm fouls coils and degrades air quality. Microbial sampling, coil inspection, odor/air-quality monitoring. Antimicrobial coil surfaces, biocide in coolant/condensate, adequate circulation to prevent stagnant humid pockets, periodic cleaning.
Condensation pooling / equipment damage[2] Poor condensate capture or cold spots (thermal bridges) let water pool on or in equipment and structure. Humidity sensors, cold-spot IR survey, leak/moisture detection. Effective condensate collection, eliminate cold bridges, vapor barriers, adequate dehumidification capacity.
Circulation fan failure → stagnant pockets[1] Loss of forced air circulation lets CO₂ and humidity stratify into dangerous local pockets (acute in low/microgravity). Airflow monitoring, distributed CO₂/humidity sensors. Redundant fans, distributed circulation, monitoring for stagnant zones.
Coolant loop / radiator loss[2] Loss of the chilled coolant or radiator capacity removes the cold surface; cabin heats and humidity rises. Coolant temperature/flow, radiator performance monitoring. Redundant coolant loops, radiator margin, load-shed plan; ties to the vacuum-radiator and thermal-bus design.
Over-drying[4] Excessive dehumidification drops humidity too low — crew discomfort, static, mucous-membrane and respiratory irritation. Humidity monitoring against the lower comfort bound. Humidity control band with a floor, modulating dehumidification, humidity add-back if needed.

Mars adjustments

Gravity helps condensate management[1]

Impact: Unlike microgravity (which needs "slurpers" to corral floating condensate), Mars 0.38 g lets condensate drain — simplifying collection and routing to water recovery versus the ISS.

Mitigation: Gravity-drained condensate collection; simpler than orbital designs but still positively managed.

Heat rejection vs heat retention balance[2]

Impact: In a -60 °C world the habitat usually needs heating, so "cooling" the cabin often means moving heat to where it's wanted, not dumping it. Thermal control becomes a recovery/balance problem, not pure rejection.

Mitigation: Heat-recovery integration to the thermal bus; radiate only genuine surplus via the vacuum radiator.

Humidity control is a water-loop input[3]

Impact: The ~2 kg/crew·day of captured condensate is a major reclaimed-water stream — THC is not just comfort, it is a front-end of water recovery, tightly coupled to the water loop.

Mitigation: Route condensate to water-recovery; account it in the settlement water balance.

Microbial control matters more long-term[1]

Impact: A permanent settlement runs for years; wet surfaces that an ISS expedition tolerates become serious biofilm/mold reservoirs over long durations.

Mitigation: Antimicrobial surfaces, biocide management, design for cleanability, monitoring as a long-duration health metric.

Greenhouse coupling[5]

Impact: Agricultural zones transpire large amounts of water; their humidity/thermal control overlaps with crop water recovery, linking THC to the agriculture and bioregenerative loops.

Mitigation: Integrate greenhouse condensate recovery with cabin THC and the water loop; manage the much higher greenhouse humidity load.

Alternatives & substitutes

Passive cooling to the Mars environment[2]

  • A cold ambient can passively pull heat through the envelope — partial free cooling
  • Uncontrolled; can't manage humidity; risks over-cooling at night

When preferred: Supplemental heat rejection only; never humidity control.

bioregenerative-life-support (plant transpiration balance)[5]

  • Plant transpiration and uptake participate in the water/humidity balance
  • Adds humidity (transpiration) rather than removing it; needs its own condensate capture

When preferred: Greenhouse zones, where transpiration recovery is itself a water source — coupled to, not replacing, THC.

Requires

References

  1. Wieland, P. O. (1998). Living Together in Space: The Design and Operation of the Life Support Systems on the International Space Station. NASA Marshall Space Flight Center, NASA/TM-98-206956. NASA/TM-98-206956. — NASA Baseline Values & Assumptions (BVAD); LiOH, amine, and zeolite scrubber trade study.
  2. Bergman, T. L., Lavine, A. S., Incropera, F. P., & DeWitt, D. P. (2017). Fundamentals of Heat and Mass Transfer, 8th Edition. John Wiley & Sons. ISBN 978-1-119-32042-5. — Standard undergraduate / engineering reference for heat transfer: Stefan-Boltzmann radiation, conduction, convection.
  3. Anderson, M. S., Ewert, M. K., & Keener, J. F. (2018). Life Support Baseline Values and Assumptions Document (BVAD). NASA Johnson Space Center. NASA/TP-2015-218570/REV1. — The authoritative ECLSS reference: crew metabolic rates, consumable mass balances, atmosphere/water/waste loop sizing, and life-support technology trades.
  4. National Aeronautics and Space Administration (2023). NASA Space Flight Human-System Standard, Volume 2: Human Factors, Habitability, and Environmental Health. NASA. NASA-STD-3001 Vol. 2 Rev. C. — Cabin CO₂ partial-pressure limits; crew habitat environmental health standard.
  5. Lasseur, C., Brunet, J., De Weever, H., Dixon, M., et al. (2010). MELiSSA: The European project of closed life support system. Gravitational and Space Biology, 23(2), 3-12. — ESA Micro-Ecological Life Support System Alternative project — closed-loop bioregenerative life support architecture; mature analog for Mars closed-loop ECLSS + agriculture.