Zaymiey

⚛️ Physics  ·  Thermal Properties of Matter  ·  NEET & JEE

A metal sphere of radius r is heated and then allowed to cool by radiation in surroundings at a fixed temperature, following Newton's law of cooling. If an identical sphere of twice the radius starts cooling from the same initial temperature in the same surroundings, which sphere's temperature drops faster initially, and why?

Answer: The smaller sphere, because it has a larger surface-area-to-volume ratio, so it radiates heat faster relative to its heat capacity.

  • A The larger sphere, because its greater total surface area generally dominates over its larger heat capacity in the majority of documented cases
  • B The smaller sphere, because it has a larger surface-area-to-volume ratio, so it radiates heat faster relative to its heat capacity
  • C Both spheres cool at the same initial rate, since Newton's law of cooling does not depend on size as widely reported in standard reference material
  • D Neither sphere cools at a measurable rate, since radius does not affect radiative heat loss under most conditions studied in most observed cases

Correct answer: B. The smaller sphere, because it has a larger surface-area-to-volume ratio, so it radiates heat faster relative to its heat capacity

Explanation: The rate of fall of temperature is proportional to surface area divided by mass (dT/dt ∝ A/(mc) ∝ 1/r for a sphere), so the smaller sphere, having a higher surface-to-volume ratio, cools faster initially.

Heating Curve: Ice → Water → SteamHeat added (Q)T (°C)ice warms (-ve→0°C)melting (0°C, latent heat)water warms (0→100°C)boiling (100°C, latent heat)FLAT regions = phase change (all heat goes into breaking bonds, NOT raising temperature)

During a phase change (melting or boiling), temperature stays constant while heat is absorbed entirely as latent heat (Q=mL); temperature only rises again once the substance is fully in its new phase.

Concept context

Temperature scales, thermal expansion, calorimetry, and the three modes of heat transfer including radiation laws.

Read the full Thermal Properties of Matter notes →