Temperature is a measure of the average translational kinetic energy of the particles in a substance. We cannot observe individual molecular motion directly, but we can measure its macroscopic effect: the tendency to spontaneously exchange energy with surroundings.
Definition 10.1 — Zeroth Law of Thermodynamics
If two systems A and B are each in thermal equilibrium with a third system C, then A and B are in thermal equilibrium with each other. This law — logically prior to the other three — is the basis for temperature as a meaningful, transitive quantity, and for the operation of thermometers.
The three common temperature scales relate by exact conversions:
TK=TC+273.15TF=59TC+32(10.1)
The Kelvin scale is the fundamental one — it starts at absolute zero, the temperature at which thermal motion would theoretically cease. All thermodynamic formulas require Kelvin.
10.2 Heat Transfer and Specific Heat
Heat Q is energy in transit — it flows from a hotter body to a cooler one until thermal equilibrium is reached. Heat is not stored; temperature is. When Q joules of heat enter a substance of mass m, the temperature change ΔT depends on the material:
Q=mcΔT(10.2)
where c is the specific heat capacity (J/kg·K) — how much energy per kilogram per degree it takes to warm that material. Water has an unusually high c = 4186 J/kg·K, which is why oceans moderate coastal climates. Metals are far lower (aluminum: 900, iron: 450).
Example 10.1 — Mixing Hot and Cold Water
200 g of water at 80°C is mixed with 300 g of water at 20°C in an insulated container. Find the final temperature.
Conduction — through direct molecular contact. Heat flux: Q/t = kA(ΔT/d), where k is thermal conductivity (W/m·K), A is area, and d is thickness.
Convection — by bulk fluid motion. Hot fluid rises, carrying energy. Responsible for ocean circulation and atmospheric weather.
Radiation — via electromagnetic waves (photons), requiring no medium. A blackbody emits power P = σT⁴A (Stefan-Boltzmann law, σ = 5.67×10⁻⁸ W/m²·K⁴).
Pconduction=kAdΔTPradiation=εσAT4(10.3)
10.4 Phase Changes and Latent Heat
When a substance changes phase (solid ↔ liquid ↔ gas), energy is absorbed or released at constant temperature. This energy goes into rearranging molecular bonds, not increasing kinetic energy:
Q=mL(10.4)
where L is the latent heat (J/kg). For water: L_fusion = 334 kJ/kg (melting ice), L_vaporization = 2257 kJ/kg (boiling water). The enormous L_vap is why sweating cools you so effectively — evaporating 1 g of sweat removes 2257 J from your skin.
Definition 10.2 — Thermal Equilibrium Condition
When an isolated system reaches thermal equilibrium, all heat exchange has ceased. For two objects mixing: the total enthalpy is conserved (no work done, no phase change):∑mici(Tf−Ti)=0Each term is positive if the object gains heat, negative if it loses heat. The sum is exactly zero for a perfectly insulated system.
10.5 Kinetic Theory of Temperature
At the microscopic level, temperature is a measure of average translational kinetic energy per particle. For an ideal gas of N molecules, the equipartition theorem gives:
21mvrms2=23kBTvrms=m3kBT(10.5)
where k_B = 1.38×10⁻²³ J/K is Boltzmann's constant. At room temperature (T = 293 K), nitrogen molecules move at v_rms ≈ 511 m/s — faster than a rifle bullet. The simulation below shows this directly: faster particles appear redder.
Figure 10.1. Kineticgassimulation.Eachdotisamolecule.Colorencodesspeed(blue=slow,red=fast. Raise the temperature to watch the speed distribution shift. Compress the volume (move the piston) to see pressure increase — Boyle's law in action.
Example 10.2 — RMS Speed of Oxygen
Find the rms speed of O_{2} molecules at T = 300 K. (m_O_{2} = 32 u = 5.31\times10^{-26} kg
Formula:vrms=(3kBT/m
Calculate:vrms=(3×1.38×10−23×300/5.31×10−26)=(2.34×105)=484 m/s
Definition 10.3 — Common Traps
Heat is not temperature: heat is energy crossing a boundary; temperature is a state variable.
Use Kelvin for proportional laws: Celsius differences are fine, but absolute temperature formulas need kelvin.
Phase changes happen at constant temperature: during melting or boiling, added energy changes phase before raising T.
Radiation depends on absolute temperature:Stefan−BoltzmannusesTinkelvinandscalesasT4
5.A10gleadbullet(c=128J/kg\cdotK)movingat300m/sembedsina0.5kgwoodblock(c=1700J/kg\cdotK).Assumingallkineticenergyconvertstoheat,estimatethetemperatureriseof the bullet.
Challenging
Key Takeaways
Temperature is average molecular KE; heat is energy in transfer — they are not the same thing.