ThermalLABORATORYSPACECRAFT / THERMAL LAB
THERMAL EXPERIMENTReduced-order model · SI units
Drag to orbit · scroll to zoomIllustrative geometry. Heat flows and charts use the selected model.
HOT EQUILIBRIUM1.7°C
INTERNAL HEAT1,500W
α / ε0.25
0%Schematic motion
Hot-case absorbed power
Solar
962 W
Albedo
361 W
Infrared
839 W
Internal heat
1,500 W
Absorbed heat3,662.3 W
Hot equilibrium1.7 °C
Cold equilibrium-27.4 °C
Design window5.0 to 35.0 °C
Blackbody emission at hot T4,577.8 W

Explore thermal control and life support through public technical references and explicit study assumptions. Calculations are reduced-order models, not flight qualification or finite-element analysis.

Physical principles

  • Emissivity is relative to a blackbody. It is not the fraction of stored energy released.
  • Radiator sizing uses net heat and absolute temperature. A surface must also reject absorbed environmental heat.
  • The circular eclipse relation is derived from shadow geometry and is separate from an assumed eclipse duty cycle.
  • Ideal electrolysis uses an 8/9 oxygen-to-water mass ratio. Gas volume also depends on pressure and temperature.
  • Water-recovery performance depends on the processed streams and hardware. Radiation protection requires a dedicated analysis.

Numerical implementation

Equilibrium is algebraic. Transients use fourth-order Runge–Kutta integration with a maximum 10 s step, forcing boundaries and 601 output samples. Each node’s stored energy changes by its net heat input. Download parameters and histories for independent checks.

No local field is inferred from the decorative spacecraft mesh. Solar incidence changes the array model; the equivalent sphere always uses its projected area.