Step 1: Understanding the Question:
Determine how radiated power changes when the absolute temperature of a body is scaled by a given factor.
Step 2: Key Formula or Approach:
According to the Stefan-Boltzmann Law, the power radiated per unit area is proportional to the fourth power of absolute temperature: P ∝ T⁴. For any temperature multiplier n, the power scales by n⁴.
Step 3: Detailed Explanation:
If the temperature doubles (multiplier = 2), the radiated power increases by 2⁴ = 16 times. Had the temperature tripled instead, the factor would jump to 3⁴ = 81. This exponential dependence means even modest temperature increases produce dramatic rises in radiative output. Remembering this T⁴ proportionality provides a rapid mental shortcut for any thermal radiation scaling problem.
Step 4: Final Answer:
Doubling the temperature multiplies radiated power by 16.