Difficulty: Easy
Correct Answer: equilibrium temperature
Explanation:
Introduction / Context:
Earth’s climate system is governed by the balance between absorbed solar radiation and emitted longwave radiation. A useful conceptual quantity is the equilibrium temperature implied by this balance, often used in simple zero-dimensional energy budget models.
Given Data / Assumptions:
Concept / Approach:
Equilibrium temperature (sometimes “effective radiating temperature”) is obtained by equating absorbed shortwave to emitted longwave. In a basic model: (1 − albedo) * S0/4 = sigma * Te^4, where S0 is the solar constant and sigma is the Stefan–Boltzmann constant. This yields Te around 255 K for Earth absent greenhouse enhancement, whereas the observed global mean surface temperature is ~288 K because greenhouse gases and clouds trap outgoing longwave radiation.
Step-by-Step Solution:
Identify the conceptual focus: radiative balance, not measured surface readings.Select the term explicitly tied to balance: equilibrium temperature.Differentiate from “mean global surface temperature,” an observed climatological statistic.
Verification / Alternative check:
Introductory climate texts compute Earth’s effective radiating temperature near 255 K, demonstrating the greenhouse effect by comparison with the observed ~288 K.
Why Other Options Are Wrong:
Common Pitfalls:
Equating effective radiating temperature with surface temperature; they differ due to atmospheric absorption and emission.
Final Answer:
equilibrium temperature
Discussion & Comments