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Heat and Thermodynamics question

2023 · Shift 2 · Q50
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Heat and Thermodynamics question

2023 · Shift 2 · Q50

JEE AdvancedPhysicsHeat and ThermodynamicsNumerical+3 / −1
A cylindrical furnace has height (H)(H)(H) and diameter (D)(D)(D) both 1 m1 \mathrm{~m}1 m. It is maintained at temperature 360 K360 \mathrm{~K}360 K. The air gets heated inside the furnace at constant pressure PaP_aPa​ and its temperature becomes T=360 KT=360 \mathrm{~K}T=360 K. The hot air with density ρ\rhoρ rises up a vertical chimney of diameter d=0.1 md=0.1 \mathrm{~m}d=0.1 m and height h=9 mh=9 \mathrm{~m}h=9 m above the furnace and exits the chimney (see the figure). As a result, atmospheric air of density ρa=1.2 kg m−3\rho_a=1.2 \mathrm{~kg} \mathrm{~m}^{-3}ρa​=1.2 kg m−3, pressure PaP_aPa​ and temperature Ta=300 KT_a=300 \mathrm{~K}Ta​=300 K enters the furnace. Assume air as an ideal gas, neglect the variations in ρ\rhoρ and TTT inside the chimney and the furnace. Also ignore the viscous effects. [Given: The acceleration due to gravity g=10 m s−2g=10 \mathrm{~m} \mathrm{~s}^{-2}g=10 m s−2 and π=3.14\pi=3.14π=3.14] JEE Advanced 2023 Paper 2 Online Physics - Heat and Thermodynamics Question 9 English ComprehensionConsidering the air flow to be streamline, the steady mass flow rate of air exiting the chimney is ‾\underline{\hspace{2cm}}​gms−1\mathrm{gm} \mathrm{s}^{-1}gms−1.
Numerical answer
View written solutionFree

Correct answer: 47.1

Step-by-step Solution:

  1. Calculate the density of hot air ( ho\ ho ho): The air inside the furnace and chimney is at a higher temperature (TTT) but is assumed to be at the same pressure as the atmosphere (PaP_aPa​). Since air is treated as an ideal gas, its equation of state is P=ρMRTP = \frac{\rho}{M}RTP=Mρ​RT, where MMM is the molar mass and RRR is the universal gas constant. For a given gas at constant pressure, density is inversely proportional to temperature: ρT=constant\rho T = \text{constant}ρT=constant.

    We can relate the density of hot air ( ho\ ho ho) at temperature T=360 KT=360\,\mathrm{K}T=360K to the density of atmospheric air ( hoa\ ho_a hoa​) at temperature Ta=300 KT_a=300\,\mathrm{K}Ta​=300K: ρT=ρaTa\rho T = \rho_a T_aρT=ρa​Ta​ ρ=ρaTaT\rho = \rho_a \frac{T_a}{T}ρ=ρa​TTa​​ Given ρa=1.2 kg m−3\rho_a = 1.2\,\mathrm{kg}\,\mathrm{m}^{-3}ρa​=1.2kgm−3, Ta=300 KT_a = 300\,\mathrm{K}Ta​=300K, and T=360 KT = 360\,\mathrm{K}T=360K: ρ=1.2×300360=1.2×56=1.0 kg m−3\rho = 1.2 \times \frac{300}{360} = 1.2 \times \frac{5}{6} = 1.0\,\mathrm{kg}\,\mathrm{m}^{-3}ρ=1.2×360300​=1.2×65​=1.0kgm−3

  2. Apply Bernoulli's Principle and the concept of Stack Effect: The upward flow of hot air is driven by the pressure difference caused by the lower density of the hot air column inside the chimney compared to the colder, denser atmospheric air outside. This is known as the stack effect or chimney effect. The driving pressure difference (\\[Delta\] P) is due to the difference in weight of the air columns.

    A standard model for the stack effect considers the buoyant force to be generated over the height of the chimney, hhh. This driving pressure is converted into the kinetic energy of the flowing gas. The pressure difference is given by: \[Delta\] P = (\rho_a - \rho) g h This pressure difference is equal to the dynamic pressure of the exiting air, assuming the initial velocity inside the large furnace is negligible: \[Delta\] P = \frac{1}{2}\rho v^2 where vvv is the exit velocity of the hot air.

    Note: A more detailed analysis might include the height of the furnace HHH as well, leading to a driving height of (H+h)(H+h)(H+h). However, using only the chimney height hhh is a common simplification and, as we will see, leads to the intended answer.

  3. Calculate the exit velocity (vvv): Equating the two expressions for \\[Delta\] P: 12ρv2=(ρa−ρ)gh\frac{1}{2}\rho v^2 = (\rho_a - \rho) g h21​ρv2=(ρa​−ρ)gh v2=2(ρa−ρ)ghρv^2 = \frac{2(\rho_a - \rho) g h}{\rho}v2=ρ2(ρa​−ρ)gh​ Substituting the known values:

    • ρa=1.2 kg m−3\rho_a = 1.2\,\mathrm{kg}\,\mathrm{m}^{-3}ρa​=1.2kgm−3
    • ρ=1.0 kg m−3\rho = 1.0\,\mathrm{kg}\,\mathrm{m}^{-3}ρ=1.0kgm−3
    • g=10 m s−2g = 10\,\mathrm{m}\,\mathrm{s}^{-2}g=10ms−2
    • h=9 mh = 9\,\mathrm{m}h=9m v2=2(1.2−1.0)×10×91.0=2(0.2)×901.0=0.4×90=36 m2 s−2v^2 = \frac{2(1.2 - 1.0) \times 10 \times 9}{1.0} = \frac{2(0.2) \times 90}{1.0} = 0.4 \times 90 = 36\,\mathrm{m^2}\,\mathrm{s}^{-2}v2=1.02(1.2−1.0)×10×9​=1.02(0.2)×90​=0.4×90=36m2s−2 v=36=6 m s−1v = \sqrt{36} = 6\,\mathrm{m}\,\mathrm{s}^{-1}v=36​=6ms−1
  4. Calculate the steady mass flow rate (\\[dot\] m): The mass flow rate is the product of the density of the exiting fluid, the cross-sectional area of the exit, and the exit velocity. m˙=ρAv\dot{m} = \rho A vm˙=ρAv The cross-sectional area AAA of the chimney is: A=π(d2)2A = \pi \left(\frac{d}{2}\right)^2A=π(2d​)2 Given diameter d=0.1 md=0.1\,\mathrm{m}d=0.1m and π=3.14\pi = 3.14π=3.14: A=3.14×(0.12)2=3.14×(0.05)2=3.14×0.0025=0.00785 m2A = 3.14 \times \left(\frac{0.1}{2}\right)^2 = 3.14 \times (0.05)^2 = 3.14 \times 0.0025 = 0.00785\,\mathrm{m}^2A=3.14×(20.1​)2=3.14×(0.05)2=3.14×0.0025=0.00785m2 Now, calculate the mass flow rate in kg/s: m˙=(1.0 kg m−3)×(0.00785 m2)×(6 m s−1)\dot{m} = (1.0\,\mathrm{kg}\,\mathrm{m}^{-3}) \times (0.00785\,\mathrm{m}^2) \times (6\,\mathrm{m}\,\mathrm{s}^{-1})m˙=(1.0kgm−3)×(0.00785m2)×(6ms−1) m˙=0.0471 kg s−1\dot{m} = 0.0471\,\mathrm{kg}\,\mathrm{s}^{-1}m˙=0.0471kgs−1

  5. Convert the mass flow rate to grams per second: The question asks for the answer in gm s−1\mathrm{gm}\,\mathrm{s}^{-1}gms−1. m˙=0.0471×1000 g s−1=47.1 g s−1\dot{m} = 0.0471 \times 1000\,\mathrm{g}\,\mathrm{s}^{-1} = 47.1\,\mathrm{g}\,\mathrm{s}^{-1}m˙=0.0471×1000gs−1=47.1gs−1

    The steady mass flow rate of air exiting the chimney is 47.1 gm s−147.1\,\mathrm{gm}\,\mathrm{s}^{-1}47.1gms−1.

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