/*! 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 12 A glass plate has a mass of 0.50... [FREE SOLUTION] | 91Ó°ÊÓ

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A glass plate has a mass of 0.50 \(\mathrm{kg}\) and a specific heat capacity of 840 \(\mathrm{J} /\left(\mathrm{kg} \cdot \mathrm{C}^{\circ}\right) .\) The wavelength of infrared light is \(6.0 \times 10^{-5} m\) , while the wavelength of blue light is \(4.7 \times 10^{-7} \mathrm{m}\) . Find the number of infrared photons and the number of blue photons needed to raise the temperature of the glass plate by \(2.0 \mathrm{C}^{\prime},\) assuming that all the photons are absorbed by the glass.

Short Answer

Expert verified
The number of infrared photons needed is approximately 840 and the number of blue photons is close to 10,840.

Step by step solution

01

Calculate Heat Required

To raise the temperature of the glass plate, the amount of heat required (\( Q \)) can be calculated using the formula: \( Q = m \cdot c \cdot \Delta T \), where \( m = 0.50 \) kg, \( c = 840 \, \mathrm{J/kg \cdot C^\circ} \), and \( \Delta T = 2.0 \) C. Plugging in the values, we get: \[ Q = 0.50 \times 840 \times 2.0 = 840 \, \text{Joules} \]

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Key Concepts

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

Specific Heat Capacity
Specific heat capacity is a property of a material that indicates how much heat energy is needed to raise the temperature of a unit mass of the substance by one degree Celsius. For the glass plate in this exercise, the specific heat capacity is given as 840 \( \mathrm{J} / (\mathrm{kg} \cdot \mathrm{C}^{\circ}) \). This means that 840 joules of energy are required to increase the temperature of 1 kilogram of glass by 1 degree Celsius.
Understanding specific heat capacity is crucial for solving problems involving temperature changes. It helps to determine the quantity of heat energy needed to achieve the desired change.
Given a mass \( m \) and a temperature change \( \Delta T \), the total heat \( Q \) needed can be calculated using the formula:
  • \( Q = m \cdot c \cdot \Delta T \)
Here, \( c \) represents the specific heat capacity. In our problem, using the given values resulted in \( Q = 840 \) Joules, indicating the heat energy needed to raise the glass plate's temperature by 2 degrees Celsius.
Photon Energy
Photons are tiny packets of energy that travel at the speed of light. The energy of a photon depends on its wavelength—the shorter the wavelength, the higher the energy. To find how many photons are needed to raise the temperature of the glass plate, we need to understand the energy each type of photon carries.
The energy of a photon \( E \) can be calculated using the equation:
  • \( E = \frac{hc}{\lambda} \)
Here, \( h \) is Planck's constant \( (6.626 \times 10^{-34} \mathrm{J} \cdot \mathrm{s}) \), \( c \) is the speed of light \( (3 \times 10^{8} \mathrm{m/s}) \), and \( \lambda \) is the wavelength of the photon.
Photon energy is vital in this context because it allows us to determine how many photons are needed to provide the required thermal energy. By taking the heat requirement from the glass plate formula and dividing it by the energy per photon, we obtain the number of photons needed.
Wavelength
Wavelength is a critical feature of light that determines its energy. Light can be categorized into different types, such as infrared and blue light, based on its wavelength.
In this exercise, the infrared light has a wavelength of \( 6.0 \times 10^{-5} \) meters, while blue light has a shorter wavelength of \( 4.7 \times 10^{-7} \) meters. The shorter wavelength of blue light indicates it has more energy per photon compared to infrared light.
Wavelength is directly related to photon energy by the photon equation:
  • \( E = \frac{hc}{\lambda} \)
Thus, knowing the wavelength helps us figure out how much energy each photon carries, which is crucial for calculating how many photons are needed to achieve a certain amount of energy, like raising the glass plate temperature in our case.
Temperature Change
Temperature change refers to the difference in temperature that is being targeted after the glass absorbs the energy provided by photons.
In our given problem, the target temperature change \( \Delta T \) is 2 degrees Celsius. Temperature change is a driving factor for calculating the amount of heat required, as it appears in the heat calculation formula:
  • \( Q = m \cdot c \cdot \Delta T \)
Without specifying the temperature change, it wouldn't be possible to calculate the energy requirement to warm the glass.
Understanding the relationship between the heat provided by the photons and the resulting temperature change is fundamental to solving real-world thermodynamics problems. This knowledge enables us to predict how much energy is needed and, consequently, how many photons are required to achieve the desired thermal effect.

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Most popular questions from this chapter

Light is shining perpendicularly on the surface of the earth with an intensity of 680 \(W/ m^{2} .\) Assuming that all the photons in the light have the same wavelength (in vacuum) of 730 nm, determine the number of photons per second per square meter that reach the earth.

An owl has good night vision because its eyes can detect a light intensity as small as \(5.0 \times 10^{-13} W/m^{2}\) . What is the minimum number of photons per second that an owl eye can detect if its pupil has a diameter of 8.5 mm and the light has a wavelength of 510 nm?

Two sources produce electromagnetic waves. Source B produces a wavelength that is three times the wavelength produced by source A. Each photon from source A has an energy of \(2.1 \times 10^{-18} \mathrm{J}\) . What is the energy of a photon from source B?

Some scientists have suggested that spacecraft with sails of the kind described in Conceptual Example 4 could be propelled by lasers. Suppose that such a sail is constructed of a highly reflective material thin enough so that one square meter of the sail has a mass of just \(3.0 \times 10^{-3} \mathrm{kg}\) . The sail is to be propelled by an ultraviolet laser beam (wavelength \(=225 \mathrm{nm}\) ) that will strike its surface perpendicularly. (a) Use the impulse-momentum theorem (Section 7.1\()\) determine the number of photons per second that must strike each square meter of the sail in order to cause an acceleration of \(9.8 \times 10^{-6} \mathrm{m} / \mathrm{s}^{2},\) which is one million times smaller than the gravitational acceleration at the earth’s surface. Assume that no other forces act on the sail, and that all the incident photons are reflected. (b) Determine the intensity (power per unit area) that the laser beam must have when it strikes the sail.

When light with a wavelength of 221 nm is incident on a certain metal surface, electrons are ejected with a maximum kinetic energy of \(3.28 \times 10^{-19} J.\) Determine the wavelength (in nm) of light that should be used to double the maximum kinetic energy of the electrons ejected from this surface.

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