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PROBLEM 1.30 KNOWN: Diameter and emissivity of spherical interplanetary probe. Power dissipation within probe. FIND: Probe surface temperature. SCHEMATIC: ASSUMPTIONS: (1) Steady-state conditions, (2) Negligible radiation incident on the probe. ANALYSIS: Conservation of energy dictates a balance between energy generation within the probe and radiation emission from the probe surface. Hence, at any instant -E + E = 0out g& & ε σA T Es s4 g= & E T D 1/ 4 g s 2επ σ ⎛ ⎞= ⎜ ⎟⎜ ⎟⎝ ⎠ & ( ) 150WT 2 40.8 0.5 m 5.67 10 1/ 4 s 2 8 W/m K π ⎛ ⎞⎜ ⎟= ⎜ ⎟×⎝ ⎠− ⋅ T K.s = 254 7. < COMMENTS: Incident radiation, as, for example, from the sun, would increase the surface temperature.
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