heat-pipe

Heat pipe (passive heat transport)

Component Semi-native thermal
TRL Mars
Energy intensity
Required by
0
Requires
2

Transports heat passively through a sealed wicked tube where a working fluid evaporates at the hot end and condenses at the cold end, returning by capillary action — no pump, no power, near-isothermal, and largely gravity-independent. It isothermalizes radiators, spreads heat from concentrated sources, and provides ultra-reliable thermal transport where a pumped loop's failure modes are unacceptable. Performance is bounded by capillary, boiling, and entrainment limits and by working-fluid temperature range.

Last reviewed: 2026-06-14

Governing equations

The capillary limit: the wick's pumping head (surface tension / effective pore radius) must exceed the liquid, vapor, and gravity pressure drops, or the wick dries out. The defining heat-pipe constraint. [1]

Maximum heat transport = the capillary-limited fluid circulation rate × latent heat of vaporization. Heat pipes move heat as latent energy, achieving effective conductivities far above any solid metal. [1]

Effective thermal conductivity orders of magnitude above copper — the hot and cold ends sit within a few degrees, which is why heat pipes isothermalize radiator panels and spread hot spots. [1]

When capillary pumping dominates the gravity term, orientation barely matters — heat pipes work the same on Mars, the Moon, or in orbit, a major advantage over gravity-dependent thermosiphons. [2]

Key constants & quantities

Symbol Value Units Conditions Description
Effective conductivity 10000–100000 W/m·K (effective) Apparent thermal conductivity — 25-250× copper — enabling near-isothermal heat spreading and transport.[1]
Operating temperature (fluid-dependent) -70–400 °C Range set by working fluid: ammonia/propylene for cold service, water for mid-range, alkali metals for high-temperature.[2]
End-to-end ΔT 1–10 K Temperature drop from evaporator to condenser — small, the near-isothermal behavior that defines the device.[1]
Transport length (LHP) 0.1–10 m Loop heat pipes extend transport to meters with flexible routing; classic heat pipes are shorter.[1]
Reliability 1 no moving parts (decades of passive life) No pump, no power, sealed — heat pipes have multi-decade spacecraft service records, the basis of their reliability advantage.[2]

Operating envelope

ParameterRangeUnitsSource
Operating temperature -70 – 400 °C (fluid-dependent) [2]
End-to-end ΔT 1 – 10 K [1]
Heat flux (evaporator) 1 – 100 W/cm² [1]
Transport length 0.05 – 10 m [1]
Tilt sensitivity (0.38 g) 0 – 90 ° (low for capillary-dominated) [2]

Mass balance

Basis: one radiator-isothermalizing heat pipe (functional unit)

Inputs

Sealed tube + wick 1 unit [1]
Working fluid charge 1 charge [2]
  • Sealed tube + wick: Metal envelope (Al/steel), sintered or grooved wick — machine-tools fabricable.
  • Working fluid charge: Ammonia/water/propylene per temperature range; small mass.

Outputs

Passive isothermal heat transport 1 enabling [1]
  • Passive isothermal heat transport: Moves heat / spreads it with no power; isothermalizes the radiator it serves.
TRL · Earth
9/ 9
TRL · Mars
7/ 9
Heat pipes are among the most flight-proven thermal devices — decades of service on satellites, the ISS, and planetary landers, and their gravity-independence is space-qualified. They work on Mars essentially as designed; the only adjustments are working-fluid choice for the temperature range and condenser/radiator integration.[2]
Energy budget
0 kWhe / device in service (fully passive — zero operating energy) [1]

A heat pipe consumes no energy at all — it moves heat for free, forever, with no moving parts. Its value is reliability and isothermalization, not efficiency; it complements the pumped thermal bus where passivity and zero-failure transport matter.

Variants & trade-offs

Constant-conductance heat pipe (CCHP)

[2]

The classic sealed wicked tube — fixed performance, isothermalizing and transporting heat over short-to-moderate distances.

Materials: Al/steel envelope · Sintered/grooved/screen wick · Ammonia/water working fluid
  • Simplest, most reliable; decades of flight heritage
  • Excellent radiator isothermalization and hot-spot spreading
  • Fixed conductance; limited length; can't modulate heat flow

When preferred: Radiator isothermalization, electronics/component heat spreading.

Loop heat pipe (LHP)

[1]

Separates vapor and liquid lines with the wick concentrated in a compact evaporator — flexible routing over meters, the modern spacecraft workhorse.

Materials: Compact wicked evaporator · Smooth vapor/liquid transport lines · Compensation chamber
  • Long, flexible, routable transport; high heat over meters
  • Robust against gravity orientation
  • More complex startup behavior; compensation-chamber control

When preferred: Transporting heat from a source to a distant radiator with flexible routing.

Variable-conductance heat pipe (VCHP)

[2]

A non-condensable gas reservoir that throttles the active condenser area, self-regulating to hold the source near a setpoint as load/sink vary.

Materials: NCG reservoir · Standard heat-pipe core
  • Passive temperature regulation — holds setpoint through Mars's huge day/night swing without active control
  • Protects sensitive equipment from thermal cycling
  • Reservoir sizing; slightly lower peak transport

When preferred: Equipment needing a stable temperature despite the 80-100 K diurnal swing.

High-temperature (alkali-metal) heat pipe

[1]

Sodium or potassium working fluid for 500-1000+ °C service — isothermalizing reactor, kiln, or concentrator receivers.

Materials: Refractory envelope · Na/K working fluid
  • Isothermalizes very-high-temperature sources (reactor, solar receiver)
  • Extreme effective conductivity at high T
  • Material compatibility and startup challenges; specialist fabrication

When preferred: High-temperature heat spreading — nuclear reactor and solar-concentrator receivers.

Failure modes

Mode Cause Detection Mitigation
Capillary dryout[1] Heat load exceeds the capillary limit; the wick can't return liquid fast enough, the evaporator dries, and temperature spikes. Evaporator temperature excursion; conductance drop. Operate below the capillary limit with margin, wick design for the duty, LHP for long transport; orientation help at 0.38 g.
Non-condensable gas generation[2] Corrosion or material incompatibility generates non-condensable gas that blankets the condenser and degrades performance over time. Gradual conductance decline; condenser-end cold spot. Compatible envelope/fluid pairs, clean fabrication, proven material combinations (the classic heat-pipe compatibility tables).
Working-fluid freezing[3] A heat pipe whose fluid freezes (e.g. water-charged pipe exposed to Mars cold) can't start and may be damaged by freeze expansion. Failure to start; temperature monitoring. Choose fluids with freeze points below the cold-end minimum (ammonia/propylene for cold service), startup heaters if needed.
Envelope breach[2] Micrometeorite, corrosion, or mechanical damage punctures the sealed tube; the working fluid escapes and the pipe dies. Performance loss; pressure/leak indication. Robust/shielded envelopes, redundant pipes on critical paths, non-toxic fluids where breach reaches crew areas.
Startup difficulty (LHP / high-T)[1] Loop and alkali-metal heat pipes can have finicky cold-start behavior (frozen/over-loaded startup). Startup temperature behavior monitoring. Startup heaters, proper charge and compensation-chamber sizing, validated startup procedures.

Mars adjustments

Gravity-independence is proven and valuable[2]

Impact: Heat pipes work the same at 0.38 g as at 1 g (capillary-dominated), and their space heritage de-risks them completely — they are among the lowest-risk thermal technologies for Mars.

Mitigation: Use heat pipes wherever passive, orientation-free transport is wanted; lean on flight heritage.

The reliable passive backbone[1]

Impact: For decade-long unattended operation, a device with no moving parts and no power need is invaluable — heat pipes carry critical thermal paths (radiator isothermalization, reactor/receiver spreading) where a pump failure would be unacceptable.

Mitigation: Put heat pipes on the highest-reliability thermal paths; complement the active bus with passive redundancy.

Working-fluid choice for the cold[3]

Impact: Water-charged pipes freeze in Mars cold; cold-service paths need ammonia/propylene-class fluids with low freeze points, or startup heaters.

Mitigation: Select working fluid for the full temperature range including the cold-end minimum; VCHPs for setpoint stability.

Passive setpoint regulation through the diurnal swing[2]

Impact: Variable-conductance heat pipes hold equipment near a setpoint through Mars's 80-100 K day/night swing with no active control — a free thermal stabilizer for sensitive hardware.

Mitigation: Use VCHPs on temperature-sensitive equipment exposed to the diurnal cycle.

Locally fabricable, fluid is the import[1]

Impact: The metal envelope and wick are machine-tools products; the working-fluid charge and precision sealing are the demanding parts.

Mitigation: Local envelope/wick fabrication, imported/charged working fluids and seals, standardized pipe families.

Alternatives & substitutes

thermal-bus (pumped fluid loop)[2]

  • Settlement-scale, flexible routing, variable distribution to many users
  • Needs pumps and power; has active failure modes a heat pipe doesn't

When preferred: Large-scale variable heat distribution; heat pipes handle passive spot transport.

Solid conduction (metal straps)[4]

  • Utterly simple and reliable for short distances
  • Orders of magnitude lower effective conductivity; heavy for any real distance

When preferred: Very short, low-power thermal paths.

Pumped two-phase loop[1]

  • Combines latent-heat transport with active pumping for long range + high flux
  • Active components; more complex than a passive pipe

When preferred: High-flux sources needing long-range active two-phase transport.

Requires

References

  1. Faghri, A. (2016). Heat Pipe Science and Technology, 2nd Edition. Global Digital Press. ISBN 978-1-4939-2503-2. — Comprehensive heat-pipe engineering: capillary and loop heat pipes, working-fluid selection, capillary/boiling/entrainment limits, variable-conductance designs.
  2. Gilmore, D. G. (Ed.) (2002). Spacecraft Thermal Control Handbook, Vol. 1: Fundamental Technologies, 2nd Edition. The Aerospace Press / AIAA. ISBN 978-1-884989-11-7. — The definitive spacecraft thermal-control reference: thermal surfaces and coatings (α/ε), heat pipes, radiators, louvers, loops, and thermal-balance design.
  3. Haberle, R. M., Clancy, R. T., Forget, F., Smith, M. D., & Zurek, R. W. (Eds.) (2017). The Atmosphere and Climate of Mars. Cambridge University Press. ISBN 978-1-107-01618-7. — Reference handbook for Mars atmospheric pressure, temperature, dust climatology.
  4. 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.