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Heat Transfer
Convection & Radiation
GATE 2017
Easy

The emissive power of a blackbody is P. If its absolute temperature is doubled, the emissive power becomes

  • A2P
  • B4P
  • C8P
  • 16P

Explanation

By the Stefan-Boltzmann law, emissive power E ∝ T⁴. Doubling T multiplies E by 2⁴ = 16, so the new emissive power is 16P.

Source: GATE ME 2017 Session 2 (ME-2) (2017)

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