Lesson 4 of 6 · Thermal control
Manage the paths heat takes
9 minute lesson · 3 checks along the way
Your goal for this lessonTrack heat paths and distinguish a temperature from an energy-transfer rate.
In this lesson 4 sections · 3 checks
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Read & understand
Space does not cool every object equally
In a vacuum there is no surrounding air to carry heat away by ordinary convection. A spacecraft exchanges energy with its external environment mainly through radiation, while conduction moves heat through connected solids. Sunlight, nearby planets and onboard electronics all contribute to the thermal environment.
A surface can absorb energy while also emitting it. Its temperature changes according to the net energy balance and its . “Space is cold” does not determine the temperature of an operating computer or a sunlit panel. Orientation and surface properties can matter as much as distance from a heat source.
Check 1 of 3
10 pointsUse the reading above. You can try again without losing points.
Read & understand
Build a heat-flow account
In a fictional instrument enclosure, electronics dissipate 30 W and absorbed external radiation adds 20 W. At one particular temperature, the enclosure emits 40 W and other paths are neglected. The net input is 10 W, so stored thermal energy increases. It is not in equilibrium at that moment.
If the effective thermal capacity is 2,000 J/K and those rates remain nearly constant for 60 s, the temperature rise is approximately 10 × 60 / 2,000 = 0.3 K. Emission generally changes as temperature changes; this short-interval approximation is not a forecast of unlimited linear heating.
Read & understand
Move, reject or retain heat
A thermal design can conduct energy toward a , reduce unwanted exchange with insulation, and use heaters where equipment would otherwise get too cold. These measures serve different purposes. A blanket limits exchange; it is not an active refrigerator that removes arbitrary internal heat.
The SPHEREx telescope hardware photograph shows reflective radiator stages used in its cooling architecture. Visible shininess alone cannot determine infrared emissivity. To evaluate performance, use the relevant spectral properties, geometry and temperatures. Keep a radiator’s view and unwanted illumination in the same analysis as the instrument it supports.
SPHEREx telescope and detector hardware during ground preparation, pictured in Caltech’s September 2023 account. Three reflective V-groove radiator stages sit below the telescope assembly. Their geometry helps successive stages shed energy while limiting unwanted transfer. This is a visible-light hardware photograph, not a map of infrared emission or a fully assembled spacecraft in flight.
Look closely
What would you need before deciding how efficiently these shiny structures cool the detectors?
See what to notice
Use the mission’s geometry, temperatures, and measured properties at the relevant wavelengths, along with all incoming and outgoing power. Visible shininess alone does not specify infrared emission, absorbed sunlight, or the thermal connections between stages.
Check 2 of 3
10 pointsUse the reading above. You can try again without losing points.
Read & understand
Verify local limits
A comfortable average can conceal a hot processor and a cold battery. Place sensors where the critical limits occur and test relevant operating modes. The moment just after a maneuver or a transmitter startup may differ from the eventual steady state. Temperature limits can also differ between storage and operation.
A useful diagnosis compares temperature histories with commands, and orientation. If a heater cycles more often, investigate the energy paths rather than inferring a broken sensor from one reading. Thermal control is an ongoing relationship among hardware, environment and schedule.
Check 3 of 3
10 pointsUse the reading above. You can try again without losing points.
Put it together
Your lesson progress
Each check connects to a part of the story. Complete all 3 to earn your 25-point lesson bonus.
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