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Thermal Simulation

Simulate thermal behavior of compute hardware in orbital environments, including eclipse cycles and varying solar flux.
Status: Early Access — Request API key

Overview

Space presents unique thermal challenges:
  • No convection — Heat can only be rejected via radiation
  • Eclipse cycles — Periodic loss of solar heating
  • Solar flux variation — Changes with orbit and season
  • Internal heat — Compute generates significant waste heat

Quick Start

Parameters

string
required
Orbit specification. Options:
  • LEO-400 to LEO-600 — Low Earth Orbit at specified altitude
  • MEO-2000 to MEO-20000 — Medium Earth Orbit
  • GEO — Geostationary orbit
  • Custom: {"altitude_km": 550, "inclination_deg": 53}
number
required
Internal heat generation in watts
number
required
Radiator surface area in square meters
number
Internal thermal mass in kg (affects transient response)
number
default:"0.9"
Radiator emissivity (0-1)
number
default:"0.3"
Solar absorptivity (0-1)

Response

Thermal Profiles

LEO Thermal Cycle

Operating Limits

Advanced: Time-Series Simulation

Get detailed thermal behavior over multiple orbits:

Design Considerations

Larger radiators = lower steady-state temperature but more mass and cost. Rule of thumb: 0.1-0.2 m² per 100W dissipation for LEO.
Ensure minimum temperature stays above component limits. May require heaters or thermal mass.
Consider worst-case solar flux (perihelion + beta angle = 0). Add 10-15% margin to maximum temperature.

Next Steps

Latency Simulation

Model network latency for your orbit

Power Budgeting

Plan power generation and storage