📋 Case Study

Thermal Design of Satellite Payload Radiator for Lunar Orbit Mission

Extreme radiative environment: solar flux up to 1360 W/m², albedo up to 0.12, IR emission from hot regolith (~390 K)

🏗️ Project Overview

NASA CLPS payload requiring stable 20±2°C operation during 14-day lunar day/night cycle

🎯 Challenge

Extreme radiative environment: solar flux up to 1360 W/m², albedo up to 0.12, IR emission from hot regolith (~390 K)

🔧 Design Approach

Deployable high-emissivity (ε = 0.92) radiator with variable-emittance coatings (VEC) and thermal louvers controlled by bi-metallic actuators

📐 Design Diagram

Thermal Radiator Design — Lunar Orbit MissionSatellite BusRadiator Panel (ε=0.92)Louvers (f_open=0.35 day / 1.0 night)Bi-Metallic ActuatorQ_in = +128 W/m² (day)Q_out = −18 W/m² (night)SunG_solar = 1360 W/m²RegolithIR (390 K)Albedo (0.12)Q_net = εσ(T⁴−T_space⁴) − αG_solar − αG_albedoDay: −128 W/m² | Night: +18 W/m²

AI-generated project design illustration

📐 Key Calculations

Net Radiative Balance

Q_net = εσ(T_rad⁴ − T_space⁴) − αG_solar − αG_albedo
Result: −128 W/m² (day), +18 W/m² (night)
Drives radiator area sizing

Louvers Open Fraction

f_open = (T_rad − T_set)/ΔT_range
Result: 0.35 (day), 1.0 (night)
Passive thermal regulation without power

📊 Results

Payload temperature stability achieved across full orbit: 19.8–20.3°C; no heater use required during night; mass penalty <1.2 kg

💡 Lessons Learned

  • Second-surface optics modeling essential for albedo reflection paths
  • VEC hysteresis must exceed orbital thermal lag to prevent oscillation

Key Takeaways

  • 1Second-surface optics modeling essential for albedo reflection paths
  • 2VEC hysteresis must exceed orbital thermal lag to prevent oscillation