22-Mec-A1 Applied Thermodynamics and Heat Transfer · December 2016
Question 7 of 8: Electrically Heated Pipe — Power to Hold 30 °C
Nivaar worked solution (AI-drafted; not reviewed by a licensed engineer)
Notes on this paper
Reference texts: Çengel & Boles, Thermodynamics: An Engineering Approach (9th ed., McGraw-Hill) — closed- and open-system energy balances, boundary work, reciprocating-compressor and vapour/gas power cycles, and gas-turbine refrigeration; Çengel & Ghajar, Heat and Mass Transfer (6th ed.) and Incropera, DeWitt, Bergman & Lavine, Fundamentals of Heat and Mass Transfer (8th ed., Wiley) — radial composite-wall conduction, internal-flow decay, natural convection with radiation from a horizontal cylinder, and the ε–NTU cross-flow heat-exchanger method. Air and steam properties are evaluated from IAPWS-IF97 / ideal-air data; the gas-turbine cycle uses cold-air-standard constant specific heats.
Paper format: National Examination 07-Mec-A1, December 2016, 3 hours, open book. Part A — Thermodynamics (Q1–4); Part B — Heat Transfer (Q5–8). Each answer carries equal value; a complete paper is any five (three from one part and two from the other). All eight questions are solved in full below.
Question 7: Electrically Heated Pipe — Power to Hold 30 °C (equal value)
Figure 7 — The heated horizontal pipe loses heat by natural convection to the 20 °C air and by radiation to the 25 °C surroundings; the electrical input per metre must balance the sum of the two.
Approach. At steady state the electrical power per metre equals the natural-convection loss (Churchill–Chu horizontal-cylinder correlation) plus the radiation loss to the surroundings.
Rayleigh number. At film temperature $T_f=25$ °C, with $\beta=1/T_f$ and $\Delta T=10$ °C,
$$Ra_D=\frac{g\beta\,\Delta T\,D^3}{\nu\alpha}=2.59\times10^{7}$$
Convective loss per metre. $q'_\text{conv}=h(\pi D)(T_s-T_\infty)=3.28(\pi\cdot0.3)(10)=30.9$ W/m.
Radiative loss per metre.
$$q'_\text{rad}=\varepsilon\sigma(\pi D)\big(T_s^4-T_\text{sur}^4\big)=0.8(5.67\times10^{-8})(\pi\cdot0.3)(303.15^4-298.15^4)=23.2\ \text{W/m}$$
Total electrical power per metre.
$$q'=q'_\text{conv}+q'_\text{rad}=30.9+23.2$$
==**$q'\approx54$ W/m must be supplied.**==
Check
Radiation contributes ≈ 43 % of the loss here even though $\Delta T$ is only 5–10 °C — at near-ambient temperatures the two mechanisms are comparable, so neglecting radiation would under-size the heating by nearly half. Air properties are at the 25 °C film temperature; the small 10 °C driving difference keeps $h$ modest (≈ 3.3 W/m²·K).