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

2.8006E+04
Reynolds Re
320.6651
Nu (Whitaker)
185.7641
Nu (Ranz-Marshall)
7862.7089
h [W/m²K]
926.3036
Heat loss Q [W]

📈 Nusselt number vs Velocity

Engine Output

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

  Reynolds Re             =     2.8006E+04
  Whitaker Nu             =     320.6651
  Ranz Nu                 =     185.7641
  Coeff h                 =    7862.7089 W/m2K
  Transfer Q              =     926.3036 W

--- VELOCITY SWEEP ---
  V[m/s]     Re           Nu_Whitaker  Nu_Ranz      h[W/m2K]   Q[W]
  -------------------------------------------------------------------------
     0.050   1.400E+03       60.582       43.091   1485.4673      175.0025
     0.215   6.010E+03      134.502       87.125   3297.9815      388.5343
     0.379   1.062E+04      184.970      115.156   4535.4715      534.3226
     0.544   1.523E+04      226.714      137.507   5559.0251      654.9072
     0.708   1.984E+04      263.418      156.661   6459.0058      760.9337
     0.873   2.445E+04      296.711      173.691   7275.3566      857.1078
     1.038   2.906E+04      327.489      189.178   8030.0334      946.0160
     1.202   3.367E+04      356.308      203.478   8736.6807     1029.2659
     1.367   3.827E+04      383.543      216.829   9404.4839     1107.9397
     1.531   4.288E+04      409.461      229.396  10039.9858     1182.8080
     1.696   4.749E+04      434.260      241.305  10648.0479     1254.4436
     1.860   5.210E+04      458.091      252.649  11232.4031     1323.2863
     2.025   5.671E+04      481.076      263.501  11795.9932     1389.6827
     2.190   6.132E+04      503.311      273.920  12341.1874     1453.9119
     2.354   6.593E+04      524.875      283.955  12869.9278     1516.2026
     2.519   7.054E+04      545.833      293.644  13383.8310     1576.7454
     2.683   7.515E+04      566.242      303.022  13884.2599     1635.7008
     2.848   7.976E+04      586.149      312.116  14372.3769     1693.2058
     3.013   8.437E+04      605.595      320.951  14849.1829     1749.3782
     3.177   8.898E+04      624.615      329.548  15315.5476     1804.3204
     3.342   9.359E+04      643.239      337.925  15772.2322     1858.1223
     3.506   9.819E+04      661.497      346.098  16219.9080     1910.8629
     3.671   1.028E+05      679.412      354.081  16659.1703     1962.6123
     3.835   1.074E+05      697.005      361.888  17090.5504     2013.4330
     4.000   1.120E+05      714.295      369.528  17514.5248     2063.3813

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:
$$Q = h A_s (T_s - T_\infty) = 39.9 \times 0.00785 \times (100-25) = 23.5\text{ W}$$