Forced Convection around a Sphere

Category: Thermal – Forced Convection | Revised 2026-10-01
CAE visualization for sphere external flow theory - technical simulation diagram
Forced Convection around a Sphere

Theory: correlations for spheres

Overview

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There seem to be several sphere heat-transfer correlations. Which should I use?

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The standard ones are Whitaker's and Ranz–Marshall's. Both start from Nu = 2 (conduction into the surroundings with no flow) and add a flow term. Up to about Re = 1000 they nearly coincide, but they diverge at higher Reynolds numbers. Ranz–Marshall came from droplet-evaporation experiments and suits small particles and droplets, while Whitaker fits larger spheres in faster flow. Let's check with a cooling steel ball and fine particles.

The two correlations

$$ Nu_{W} = 2 + \left(0.4\,Re^{1/2} + 0.06\,Re^{2/3}\right)Pr^{0.4}\left(\frac{\mu}{\mu_s}\right)^{1/4},\qquad Nu_{RM} = 2 + 0.6\,Re^{1/2}Pr^{1/3} $$

Whitaker's correlation covers Re = 3.5 to 7.6×10⁴ and Pr = 0.71 to 380. μ/μ_s is the ratio to viscosity at wall temperature, close to 1 for gases.

Cooling time by lumped capacitance

$$ \tau = \frac{\rho c\,d}{6h},\qquad \frac{T - T_\infty}{T_0 - T_\infty} = e^{-t/\tau},\qquad Bi = \frac{h\,(d/6)}{k_s} < 0.1 $$
Coffee Break Trivia

A correlation born from spray drying

The Ranz–Marshall correlation was built in 1952 by Ranz and Marshall in the US, who measured evaporation of suspended water drops for spray-dryer design. Droplet evaporation and heat transfer share the same form, so it's still used wherever particles or droplets appear: fuel sprays, spray drying, powder heating. Whitaker's correlation of 1972 re-fitted a wide body of earlier data to cover broad Reynolds and Prandtl ranges.

Worked examples

Example 1: comparing the correlations (air, Pr 0.71)

Reynolds numberWhitakerRanz-MarshallDifference
12.402.54+6%
103.353.69+10%
1006.627.35+11%
1,00018.318.9+4%
10,00061.255.5−9%
70,000183144−22%

Example 2: air-cooling a 10 mm steel ball

A 300 °C steel ball cooled to 50 °C in 20 °C air (Whitaker, no radiation). At 5 m/s: Re = 3185, Nu = 33.0, h = 86.8 W/m²K, Bi = 0.0032, time constant 71 s.

Air speedhTime to 50 °C
0.5 m/s28.0 W/m²K490 s
2 m/s54.2 W/m²K254 s
5 m/s86.8 W/m²K158 s
10 m/s126 W/m²K109 s
20 m/s184 W/m²K75 s
40 m/s271 W/m²K51 s
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Even at eight times the speed, 40 m/s, cooling only takes a third as long.

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The boundary layer thins with speed, but h grows only about as the square root of speed. So halving cooling time needs 3.6 times the speed — from 5 to about 18 m/s — and since fan power rises with the cube of speed, efficiency worsens fast. At low speed, radiation (not included here) matters too: at emissivity 0.8 it's about 16 W/m²K at 300 °C, not negligible against 28 W/m²K at 0.5 m/s. With Bi = 0.003, internal temperature differences in the ball can be ignored.

Example 3: fine particles in still air (Nu = 2)

Particle diameterh = 2k/d
50 µm1,050 W/m²K
5 µm10,500 W/m²K

Calculation tips

  1. Evaluate properties at film temperature and apply the viscosity correction.
  2. Check the Reynolds number is within the correlation's range.
  3. At low speeds add natural convection and radiation.
  4. If Bi exceeds 0.1, solve internal conduction instead of lumped capacitance.
  5. In particle clouds and packed beds, neighbours change heat transfer.
Coffee Break Trivia

“Quenching bearing balls”

Bearing balls are cooled in oil or air after hardening. Smaller balls have higher heat transfer coefficients and more surface per volume, so they cool faster. Doubling diameter cuts h to about 0.7 times while the time constant grows with diameter, so cooling takes about three times longer. That's why, cooled under identical conditions, only the larger balls may lack hardness — and cooling conditions are adjusted to ball size.

Common mistakes

Mistakes and fixes

MistakeEffectFix
Ranz–Marshall at high ReAbout 20% lowUse Whitaker
Forgetting Nu = 2Too low at low ReInclude conduction term
Ignoring radiationHot cooling underestimatedAdd radiation
Unchecked BiInternal gradients missedCheck Bi < 0.1
Radius as length scaleRe halvedUse diameter
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