Forced Convection Over Spheres

Determine boundary layer heat transfer coefficients and total heat rate for flows over spherical surfaces.

Flow (V) Ts Diameter D

External Flow Over Sphere

Similar to crossflow over cylinders, flow separates from the rear side of spheres, creating a low-pressure wake region. Convection is analyzed using empirical correlations that account for the fluid viscosity change near the surface ($\mu/\mu_s$).

Parameters Setup

📐 Geometry & Flow
🌡️ Temperatures
💧 Fluid Properties

Results & Curves

5.2200E+02
Reynolds Re
521.5707
Nu (Whitaker)
110.8036
Nu (Ranz-Marshall)
730.1990
h [W/m²K]
2752.7855
Heat loss Q [W]

📈 Nusselt number vs Velocity

Engine Output

============================================
  CONVECTION OVER SPHERE ENGINE
============================================

  Reynolds Re             =     5.2200E+02
  Whitaker Nu             =     521.5707
  Ranz Nu                 =     110.8036
  Coeff h                 =     730.1990 W/m2K
  Transfer Q              =    2752.7855 W

--- VELOCITY SWEEP ---
  V[m/s]     Re           Nu_Whitaker  Nu_Ranz      h[W/m2K]   Q[W]
  -------------------------------------------------------------------------
     0.050   8.700E+01      197.765       46.419    276.8707     1043.7781
     0.098   1.704E+02      283.747       64.160    397.2454     1497.5799
     0.146   2.538E+02      352.002       77.860    492.8033     1857.8247
     0.194   3.371E+02      410.786       89.439    575.0999     2168.0756
     0.242   4.205E+02      463.401       99.654    648.7614     2445.7729
     0.290   5.039E+02      511.576      108.898    716.2060     2700.0329
     0.337   5.872E+02      556.350      117.404    778.8896     2936.3447
     0.385   6.706E+02      598.408      125.324    837.7710     3158.3221
     0.433   7.540E+02      638.230      132.766    893.5216     3368.4971
     0.481   8.374E+02      676.167      139.806    946.6341     3568.7266
     0.529   9.208E+02      712.488      146.504    997.4827     3760.4213
     0.577   1.004E+03      747.400      152.904   1046.3597     3944.6833
     0.625   1.088E+03      781.071      159.044   1093.4989     4122.3936
     0.673   1.171E+03      813.636      164.953   1139.0904     4294.2695
     0.721   1.254E+03      845.208      170.655   1183.2918     4460.9051
     0.769   1.338E+03      875.882      176.171   1226.2354     4622.7984
     0.817   1.421E+03      905.738      181.517   1268.0332     4780.3725
     0.865   1.504E+03      934.844      186.708   1308.7815     4933.9900
     0.912   1.588E+03      963.260      191.758   1348.5636     5083.9651
     0.960   1.671E+03      991.037      196.676   1387.4522     5230.5716
     1.008   1.754E+03     1018.222      201.473   1425.5111     5374.0504
     1.056   1.838E+03     1044.855      206.158   1462.7969     5514.6145
     1.104   1.921E+03     1070.971      210.737   1499.3598     5652.4534
     1.152   2.005E+03     1096.603      215.218   1535.2449     5787.7368
     1.200   2.088E+03     1121.780      219.607   1570.4925     5920.6171

Calculation Methodology

Mathematical Model & Theory

Convective heat transfer over a spherical object is evaluated using two primary models:

1. Whitaker Correlation: $$\text{Nu}_D = 2 + \left(0.4 \text{Re}_D^{1/2} + 0.06 \text{Re}_D^{2/3}\right) \text{Pr}^{0.4} \left(\frac{\mu}{\mu_s}\right)^{1/4}$$ where fluid properties (except $\mu_s$) are evaluated at the free-stream temperature $T_\infty$.

2. Ranz-Marshall Correlation: $$\text{Nu}_D = 2 + 0.6 \text{Re}_D^{1/2} \text{Pr}^{1/3}$$ This correlation is a classical simplification widely used for droplets and evaporating sprays.

Academic References:

  1. Incropera, F. P., & DeWitt, D. P. (2011). Fundamentals of Heat and Mass Transfer. 7th Edition, John Wiley & Sons.
  2. Whitaker, S. (1972). Forced Convection Heat Transfer Correlations for Flow in Pipes, Past Flat Plates, Single Cylinders, Single Spheres, and for Flow in Packed Beds and Tube Bundles. AIChE J.

Worked Engineering Example

Problem Statement:
Air at $25^\circ\text{C}$ flows at $5.0\text{ m/s}$ past a $50\text{ mm}$ sphere maintained at $100^\circ\text{C}$. Find the convective heat loss ($T_\infty = 25^\circ\text{C}$).

Step-by-step Solution:
1. Evaluate air properties at free-stream temp $25^\circ\text{C}$:
- $\rho = 1.177\text{ kg/m}^3, \mu = 1.85 \times 10^{-5}\text{ Pa·s}, k = 0.0263\text{ W/m·K}, Pr = 0.71$.
- At $T_s = 100^\circ\text{C}$, $\mu_s \approx 2.18 \times 10^{-5}\text{ Pa·s}$.
2. Calculate Reynolds number:
$$\text{Re}_D = \frac{\rho V D}{\mu} = \frac{1.177 \times 5.0 \times 0.05}{1.85 \times 10^{-5}} = 15,905$$ 3. Evaluate Nusselt number via Whitaker correlation:
$$\text{Nu}_D = 2 + \left[0.4 \times (15,905)^{1/2} + 0.06 \times (15,905)^{2/3}\right] \times (0.71)^{0.4} \times \left(\frac{1.85}{2.18}\right)^{1/4}$$ $$\text{Nu}_D = 2 + \left[50.4 + 37.9\right] \times 0.87 \times 0.96 = 75.8$$ 4. Convection coefficient $h$:
$$h = \frac{\text{Nu}_D k}{D} = \frac{75.8 \times 0.0263}{0.05} = 39.9\text{ W/m}^2\text{K}$$ 5. Surface area $A_s = \pi D^2 = \pi \times 0.05^2 = 0.00785\text{ m}^2$. Total heat loss:
$$Q = h A_s (T_s - T_\infty) = 39.9 \times 0.00785 \times (100-25) = 23.5\text{ W}$$