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Heat transfer and thermal systems

Lumped radiative cooling towards a cold sink

Time for a lumped body to cool from Ti to Tf by radiation alone to a sink so cold that its irradiation is negligible.

Ref
HTS-50
Rev
v1
Field
Heat transfer and thermal systems
Result
t [s]

A body cooling only by radiation to a very cold sink has C dT/dt = −εσAT⁴. Integrating from Ti to Tf gives the cooling time t ≈ C(Tf⁻³ − Ti⁻³)/(3εσA). It neglects irradiation from the sink, so the sink must be far colder than Tf, and needs a uniform body temperature. Doubling the absolute temperature range does not simply scale the time, because of the cube.

Time for a lumped body to cool from Ti to Tf by radiation alone to a sink so cold that its irradiation is negligible. Needs a uniform body temperature, constant properties and Tf above the sink temperature.

Calculator

Solve for
s
J/K
1100,000
m²
0.00110
0.051
K
5002,000
K
100499
  • Initial radiated power, εσAT_i⁴283.5 W
  • Final radiated power, εσAT_f⁴116.1 W
  • Mean cooling power, C(Ti − Tf)/t178.5 W

What drives the result

Each variable is moved across its typical range while the others stay at the values above. The longest bar is the key driver.

Cooling time (s) current value 56.03 s
CThermal capacitanceKey driver
0.5656,000
TfFinal temperature
0.3547,290
ARadiating area
0.565,600
εEmissivity
44.8896
TiInitial temperature
114
  • The body takes 56.03 s to cool from 500 K to 400 K, radiating 283.5 W at first and 116.1 W at the end.
  • Cooling gets slower as it proceeds: most of the time is spent at the low end, where radiation is weakest.
Chart data as tables

Ranked variables

VariableTypical rangeLowest resultHighest resultSwing (s)Local stepChange in result
C Thermal capacitance1 to 100,000 J/K0.560356,03056,030+10%+10 %
Tf Final temperature100 to 499 K0.35417,2897,289+10%−51 %
A Radiating area0.001 to 10 m²0.56035,6035,602+10%−9.09 %
ε Emissivity0.05 to 1 44.82896.5851.6+10%−9.09 %
Ti Initial temperature500 to 2,000 K56.03113.957.87+10%+26.1 %

Sweep of Final temperature

Final temperature (K)Cooling time (s)
1007,289
149.92,124
199.8863.2
249.6413.6
299.5214.7
349.4113.5
399.356.68
449.122.33
4990.3541

Sweep one variable

Cooling time (s)Hover, touch, or use the arrow keys on the chart
0200040006000 100200300400 Final temperature (K) now 56.03

Variables and how each one contributes

t

Cooling time

Result · s

What the equation gives you. Everything else feeds it.

C

Thermal capacitance

J/K · typical 1 to 100,000

The thermal capacitance of the body, in J/K. Raises the cooling time in direct proportion. Raising it by 10 % (to 110) moves the result by +10 %, from 56.03 to 61.63 s.

A

Radiating area

m² · typical 0.001 to 10

The radiating area, in m². Lowers the cooling time in inverse proportion. Raising it by 10 % (to 0.11) moves the result by −9.09 %, from 56.03 to 50.94 s.

ε

Emissivity

· typical 0.05 to 1

The emissivity of the surface. Lowers the cooling time in inverse proportion. Raising it by 10 % (to 0.88) moves the result by −9.09 %, from 56.03 to 50.94 s.

Ti

Initial temperature

K · typical 500 to 2,000

The initial temperature, in K. A hotter start raises the time slightly, since the hottest period passes quickly. Raising it by 10 % (to 550) moves the result by +26.1 %, from 56.03 to 70.65 s.

Tf

Final temperature

K · typical 100 to 499

The final temperature, in K. A lower final temperature raises the time greatly, since radiation falls as T⁴. Raising it by 10 % (to 440) moves the result by −51 %, from 56.03 to 27.48 s.

Worked example with the values above

  1. Temperature terms: Tf⁻³ = 1.5625×10−8, Ti⁻³ = 8×10−9; difference = 7.625×10−9 K⁻³.
  2. Denominator: 3εσA = 3 × 0.8 × 5.67037×10−8 × 0.1 = 1.3609×10−8.
  3. t = 100 × 7.625×10−9 / 1.3609×10−8 = 56.03 s.

Assumptions and limits

  • Constant properties in each phase, a single melting temperature and no losses unless stated.
  • Steady or quasi-steady balances, with absolute temperatures where logarithms or powers are used.

Common mistakes

  • Forgetting the latent heat term, or counting it twice.
  • Using °C in an entropy or radiation formula.
  • Using these simple formulas when the Stefan number is not small.

Statistics and uncertainty

Latent heats and specific heats are tabulated to a few per cent, but real storage materials melt over a range and lose heat, so real systems typically deliver 5 % to 20 % less than the ideal values.

Where it is used

  • Sizing thermal storage, ice banks and phase-change units.
  • Checking exchanger data, mixing streams and cooling times.

Maths you need

  • Latent heat: energy per kilogram to change phase
  • Heat-capacity rate: C = ṁcp
  • Second law: entropy generation cannot be negative

Related formulas

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