/*! This file is auto-generated */ .wp-block-button__link{color:#fff;background-color:#32373c;border-radius:9999px;box-shadow:none;text-decoration:none;padding:calc(.667em + 2px) calc(1.333em + 2px);font-size:1.125em}.wp-block-file__button{background:#32373c;color:#fff;text-decoration:none} Problem 62 A spherical pot of hot coffee co... [FREE SOLUTION] | 91Ó°ÊÓ

91Ó°ÊÓ

A spherical pot of hot coffee contains \(0.75 \mathrm{~L}\) of liquid (essentially water) at an initial temperature of \(95^{\circ} \mathrm{C}\). The pot has an emissivity of \(0.60,\) and the surroundings are at a temperature of \(20.0^{\circ} \mathrm{C}\). Calculate the coffee's rate of heat loss by radiation.

Short Answer

Expert verified
The rate of heat loss by radiation is calculated using the Stefan-Boltzmann Law with given emissivity, temperatures in Kelvin, and surface area derived from volume.

Step by step solution

01

Understand the Problem

We need to calculate the rate of heat loss from the coffee, which cools by radiation. We will use the Stefan-Boltzmann Law, which relates temperature and heat loss by radiation.
02

Note Given Values

The coffee volume is 0.75 L, the initial temperature of the coffee is 95°C, the emissivity of the pot is 0.60, and the surrounding temperature is 20°C. 1 L = 0.001 m³, so the volume of the coffee is 0.00075 m³.
03

Convert Temperatures to Kelvin

Convert the temperatures from Celsius to Kelvin using the formula: \(T(\text{K}) = T(\text{C}) + 273.15\). Thus, the temperature of the coffee, \(T_c = 95 + 273.15 = 368.15\, K\), and the surrounding temperature, \(T_s = 20 + 273.15 = 293.15\, K\).
04

Calculate Surface Area of the Pot

Assuming the pot is a perfect sphere, use the volume to find the radius, then the surface area. The volume of a sphere is \(V = \frac{4}{3}\pi r^3\). Solve for \(r\) and use \(A = 4\pi r^2\) for surface area.\[\begin{align*} V &= \frac{4}{3} \pi r^3 = 0.00075 \ r &= \left(\frac{3 \times 0.00075}{4 \pi}\right)^{1/3} \ A &= 4\pi r^2. \end{align*}\]
05

Apply the Stefan-Boltzmann Law

The rate of heat loss \(P\) is calculated using \(P = \varepsilon \sigma A (T_c^4 - T_s^4)\), where \(\varepsilon = 0.60\) is the emissivity, \(\sigma = 5.67 \times 10^{-8} \, \text{W/m}^2\text{K}^4\) is the Stefan-Boltzmann constant. Calculate using values derived earlier for \(A\), \(T_c\), and \(T_s\).
06

Compute Results

Using the calculated values from previous steps, plug these into the Stefan-Boltzmann Law formula to solve for \(P\). Ensure all units are consistent for accuracy.

Unlock Step-by-Step Solutions & Ace Your Exams!

  • Full Textbook Solutions

    Get detailed explanations and key concepts

  • Unlimited Al creation

    Al flashcards, explanations, exams and more...

  • Ads-free access

    To over 500 millions flashcards

  • Money-back guarantee

    We refund you if you fail your exam.

Over 30 million students worldwide already upgrade their learning with 91Ó°ÊÓ!

Key Concepts

These are the key concepts you need to understand to accurately answer the question.

Heat Transfer
Heat transfer is the process by which thermal energy is exchanged between physical systems. It can occur via three primary mechanisms: conduction, convection, and radiation. In this particular problem, heat loss from the coffee occurs through radiation, which is the emission of energy as electromagnetic waves or as moving subatomic particles. Radiation does not require a medium, such as air or water, to transfer heat. This means that it can occur even in a vacuum.

In many real-world scenarios, different modes of heat transfer can happen simultaneously. However, in this exercise, the focus is on radiative heat transfer. Understanding how and why heat is transferred is essential in developing systems for heating, cooling, and managing energy efficiency across various applications.
Radiation
Radiation is one of the core processes for heat transfer, where energy is emitted by a body in the form of electromagnetic waves. Every body with a temperature above absolute zero emits some form of thermal radiation. The amount of energy radiated depends on the temperature and surface properties of the object.

The Stefan-Boltzmann Law is a fundamental principle used to calculate the heat transfer by radiation. The law states that the power radiated by a black body is directly proportional to the fourth power of its absolute temperature. For real objects, which are not perfect black bodies, this concept is refined by using a factor called emissivity. Hence, energy radiated can be calculated using the formula: \(
P = \varepsilon \sigma A (T_c^4 - T_s^4)\)
Where:
  • \(P\) is the rate of heat loss (Watt),
  • \(\varepsilon\) is emissivity (a unitless measure ranging from 0 to 1),
  • \(\sigma\) is the Stefan-Boltzmann constant \((5.67 \times 10^{-8} \, \text{W/m}^2 \text{K}^4)\),
  • \(A\) is the surface area (\(\text{m}^2\)),
  • \(T_c\) and \(T_s\) are the temperatures of the coffee and surroundings in Kelvin, respectively.
Temperature Conversion
To perform calculations involving temperature, converting between different temperature scales is crucial in ensuring precision. The Celsius scale is commonly used in everyday applications, while Kelvin is the SI unit for thermodynamic temperature and is widely used in scientific calculations. Converting from Celsius to Kelvin is straightforward and is achieved with the formula:

\(T(\text{K}) = T(\text{°C}) + 273.15\)

In this problem, the temperatures of both the coffee and the surroundings need to be converted from Celsius to Kelvin. This conversion is necessary because the Stefan-Boltzmann Law requires absolute temperatures in Kelvin for accurate calculations of radiative heat transfer. Understanding how to convert temperatures is a fundamental skill to prevent common calculation errors in physics and engineering problems.
Emissivity
Emissivity is a measure of an object's ability to emit infrared energy compared to that of a perfect black body. It is a dimensionless value ranging between 0 and 1. A black body has an emissivity of 1, meaning it emits the maximum possible radiation at a given temperature. In contrast, an object with an emissivity of 0 does not radiate at all.

The pot in this exercise has an emissivity of 0.60, indicating that it emits 60% of the radiation a perfect black body would at the same temperature. Emissivity affects how efficiently an object can radiate heat energy and is an essential factor in calculations using the Stefan-Boltzmann Law. It is influenced by factors like the material’s surface structure, texture, and temperature. Without accounting for emissivity, heat transfer calculations would be inaccurate, leading to potential errors in understanding energy dynamics in various systems.

One App. One Place for Learning.

All the tools & learning materials you need for study success - in one app.

Get started for free

Most popular questions from this chapter

An insulated beaker with negligible mass contains \(0.250 \mathrm{~kg}\) of water at a temperature of \(75.0^{\circ} \mathrm{C}\). How many kilograms of ice at a temperature of \(-20.0^{\circ} \mathrm{C}\) must be dropped in the water so that the final temperature of the system will be \(30.0^{\circ} \mathrm{C} ?\)

Convert the following Kelvin temperatures to the Celsius and Fahrenheit scales: (a) the midday temperature at the surface of the moon \((400 \mathrm{~K}) ;\) (b) the temperature at the tops of the clouds in the atmosphere of Saturn \((95 \mathrm{~K}) ;\) (c) the temperature at the center of the sun \(\left(1.55 \times 10^{7} \mathrm{~K}\right)\)

A picture window has dimensions of \(1.40 \mathrm{~m} \times 2.50 \mathrm{~m}\) and is made of glass \(5.20 \mathrm{~mm}\) thick. On a winter day, the outside temperature is \(-20.0^{\circ} \mathrm{C},\) while the inside temperature is a comfortable \(19.56^{\circ} \mathrm{C}\). (a) At what rate is heat being lost through the window by conduction? (b) At what rate would heat be lost through the window if you covered it with a \(0.750-\mathrm{mm}\) -thick layer of paper (thermal conductivity \(0.0500 \mathrm{~W} /(\mathrm{m} \cdot \mathrm{K})) ?\)

The basal metabolic rate is the rate at which energy is produced in the body when a person is at rest. A \(75 \mathrm{~kg}\) (165 lb) person of height \(1.83 \mathrm{~m}\) (6 ft) would have a body surface area of approximately \(2.0 \mathrm{~m}^{2}\). (a) What is the net amount of heat this person could radiate per second into a room at \(18^{\circ} \mathrm{C}\) (about \(65^{\circ} \mathrm{F}\) ) if his skin's surface temperature is \(30^{\circ} \mathrm{C}\) ? (At such temperatures, nearly all the heat is infrared radiation, for which the body's emissivity is \(1.0,\) regardless of the amount of pigment.) (b) Normally, \(80 \%\) of the energy produced by metabolism goes into heat, while the rest goes into things like pumping blood and repairing cells. Also normally, a person at rest can get rid of this excess heat just through radiation. Use your answer to part (a) to find this person's basal metabolic rate.

A thirsty nurse cools a \(2.00 \mathrm{~L}\) bottle of a soft drink (mostly water) by pouring it into a large aluminum mug of mass \(0.257 \mathrm{~kg}\) and adding \(0.120 \mathrm{~kg}\) of ice initially at \(-15.0^{\circ} \mathrm{C}\). If the soft drink and mug are initially at \(20.0^{\circ} \mathrm{C},\) what is the final temperature of the system. assuming no heat losses?

See all solutions

Recommended explanations on Physics Textbooks

View all explanations

What do you think about this solution?

We value your feedback to improve our textbook solutions.

Study anywhere. Anytime. Across all devices.