Difficulty: Easy
Correct Answer: 123 K
Explanation:
Introduction / Context:When a spacecraft passes into Earth’s shadow, the Sun's radiant heating suddenly disappears. The thermal balance shifts to internal dissipation and deep-space radiation. This question checks fundamental awareness of eclipse temperatures for communication satellites and the typical order-of-magnitude value used in basic satellite engineering courses and competitive exams.
Given Data / Assumptions:
Concept / Approach:
Spacecraft surface temperature is governed by radiative balance: absorbed power equals radiated power. Without solar input, temperatures rapidly drop until a new equilibrium is reached. Classic first-order figures used in many texts put “cold case” external temperatures around 120 K to 130 K for unheated surfaces, which is a helpful design anchor for thermal control systems (MLI, louvers, heaters).
Step-by-Step Solution:
Recognize eclipse eliminates dominant solar heat (~1361 W/m^2 at 1 AU).Remaining inputs: internal dissipation + weak Earth IR; outputs: thermal radiation to space.Standard reference “cold case” value widely rounded to ~120 K.Among the choices, 123 K is closest to this canonical number.Verification / Alternative check:
Thermal analyses vary by coating emissivity/absorptivity and geometry. However, exam-centric values often cite ~120 K as a representative eclipse external temperature, validating selection of 123 K over higher values like 170–273 K.
Why Other Options Are Wrong:
Common Pitfalls:
Confusing average internal avionics temperature (actively controlled) with uncontrolled outer surface skin temperatures in eclipse; also forgetting that coatings and MLI can push actual values up or down around the textbook baseline.
Final Answer:
123 K
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