Experiment No09 - Procedure for Simulation: 1. The variable menu contains two drop down combo PDF

Title Experiment No09 - Procedure for Simulation: 1. The variable menu contains two drop down combo
Course Heat and mass transfer
Institution University of Engineering and Technology Peshawar
Pages 6
File Size 314.3 KB
File Type PDF
Total Downloads 65
Total Views 155

Summary

Procedure for Simulation:
1. The variable menu contains two drop down combo boxes and two buttons. The user can
select the desired material and liquid from these combo boxes.
2. Here select the material (say 'Brass') and liquid (say 'Water'), then click on the Start Heating
b...


Description

Experiment No.09 Determination of Stefan- Boltzmann constant σ. Objective. Determination of Stefan- Boltzmann constant σ.

Apparatus: Heater, temperature-indicators, box containing metallic hemisphere with provision for waterflow through its annulus, a suitable black body which can be connected at the bottom of this metallic hemisphere.

Theory: A black body is an ideal body which absorbs or emits all types of electromagnetic radiation. The term ‘black body’ was first coined by the German physicist Kirchhoff during 1860’s. Black body radiation is the type of electromagnetic radiation emitted by a black body at constant temperature. The spectrum of this radiation is specific and its intensity depends only on the temperature of the black body. It was the study of this phenomenon which led to a new branch of physics called Quantum mechanics. According to Stefan’s Boltzmann law (formulated by the Austrian physicists, Stefan and Boltzmann), energy radiated per unit area per unit time by a body is given by, e Austrian physicists, Stefan and Boltzmann), energy radiated per unit area per unit time by a body is given by, R= Є σT4 Where R = energy radiated per area per time, Є = emissivity of the material of the body, σ = Stefan’s constant = 5.67x10-8 Wm-2K-4, and T is the temperature in Kelvin scale. For an ideal black body, emissivity Є=1, and equation becomes, R= σT4 The block diagram of experimental set up to study the blackbody radiation is given below.

This setup uses a copper disc as an approximation to the black body disc which absorbs radiation from the metallic hemisphere as shown in fig (1). Let T d and Th is the steady state temperatures of copper disc and metallic hemisphere respectively. Now according to the equation (2), the net heat transfer to the copper disc per second is,

Where A is the area of the copper disc and ΔQ= (Qh-Qd). Now, we have another equation from thermodynamics for heat transfer as,

Where ‘m’ mass of the disc, ‘Cp’’ specific heat of the copper, dT/dt is the change in temperature per unit time. Equating equations (3) and (4),

Hence,

Applications: 1. Determination of temperature of Sun from its energy flux density. 2. Temperature of stars other than Sun, and also their radius relative to the Sun, can be approximated by similar means. 3. We can find the temperature of Earth, by equating the energy received from the Sun and the energy transmitted by the Earth under black body approximation

Procedure for performing real lab: 1. Remove the disc from the bottom of the hemisphere and switch on the heater and allow the water to flow through it. 2. Allow the hemisphere to reach the steady state and note down the temperature T1, T2, T3 . 3. Fit the disc (black body) at the bottom of the hemisphere and note down its rise in temperature with respect to time till steady state is reached. 4. A graph is plotted with temperature of disc along Y-axis and time along X-axis as shown

5. Find out the slope dT/dt from the graph.

Procedure for Simulation: 1. Choose desirable values of water temperature, surrounding temperature, mass and radius of the disc using the sliders. 2. Click the "Power ON" button and wait till T1, T2 ,T3 reach steady state. Note down its values. 3. Putting T4 button, click "Fit the disc'' option. 4. Note down T4 at different intervals of time till it reaches steady state. 5. Plot Temperature-Time graph and determine its slope dT/dt. 6. Determine Stefan's constant ' σ ' using the given formula.

Observations: Td

Td(K)

339.91

350 340

f(x) = 0.04 x + 303.02

330

Td(K) Linear (Td(K)) Linear (Td(K)) Linear (Td(K))

320 310 300 290 280

0

100 200 300 400 500 600 700 800 900 1000

6 7 8 9 10 11 12 13 14 15

360 420 480 540 600 660 720 780 840 900

45.15 48.03 50.17 53.18 55.32 57.9 60.9 63.48 65.62 66.91

318.15 321.03 323.17 326.18 328.32 330.9 333.9 336.48 338.62 339.91

Calculations: Mass of the copper disc = 5 g Specific heat of copper = 380 Jkg-1 Radius of the disc = 0.01 m Area of the disc = 0.00314 m2 Slope of the graph dT/dt= 0.0422 Ks-1 Substituting the values in the given expression,

s=(5*380*0.0422)/{0.000314*(3434-339.914)} s=1.6294*10-7 Wm-2K-4 Result: Stefan-Boltzmann’s constant σ = 1.6294 x 10-8 Wm-2 K-4...


Similar Free PDFs