Problem 62
Question
The relationship between energy \(\mathrm{E}\), of the radiation with a wavelength \(8000 \AA\) and the energy of the ra diation with a wavelength \(16000 \AA\) is (a) \(\mathrm{E}_{1}=2 \mathrm{E}_{2}\) (b) \(\mathrm{E}_{1}=4 \mathrm{E}_{2}\) (c) \(\mathrm{E}_{1}=6 \mathrm{E}_{2}\) (d) \(E_{1}=E_{2}\)
Step-by-Step Solution
Verified Answer
The correct answer is (a) \( E_1 = 2E_2 \).
1Step 1: Understanding the Energy-Wavelength Relationship
The energy of a photon is related to its wavelength by the equation \( E = \frac{hc}{\lambda} \), where \( h \) is Planck's constant, \( c \) is the speed of light, and \( \lambda \) is the wavelength of the photon.
2Step 2: Calculate Energy for Wavelength 8000 Ångströms
For radiation with a wavelength of 8000 \( \text{Å} \), the energy \( E_1 \) is given by: \[ E_1 = \frac{hc}{8000 \ Å} \] We can rewrite it using the proportionality relationship:\[ E_1 \propto \frac{1}{8000} \]
3Step 3: Calculate Energy for Wavelength 16000 Ångströms
For radiation with a wavelength of 16000 \( \text{Å} \), the energy \( E_2 \) is given by: \[ E_2 = \frac{hc}{16000 \ Å} \] We can rewrite it using the proportionality relationship:\[ E_2 \propto \frac{1}{16000} \]
4Step 4: Find the Relationship between \( E_1 \) and \( E_2 \)
Using the proportional relationship of energy to the inverse of wavelength, compare \( E_1 \) and \( E_2 \):\[ \frac{E_1}{E_2} = \frac{\frac{1}{8000}}{\frac{1}{16000}} \]Simplify this:\[ \frac{E_1}{E_2} = \frac{16000}{8000} = 2 \]Thus, \( E_1 = 2E_2 \).
Key Concepts
Photon Energy CalculationPlanck's ConstantSpeed of LightWavelength Inversion Proportionality
Photon Energy Calculation
When it comes to understanding the energy of a photon, it's all about the connection between three important values: energy, wavelength, and certain constants. A photon's energy can be calculated using the formula:
The nature of this relationship is inversely proportional, meaning as the wavelength increases, the energy decreases and vice versa. This fundamental concept is crucial for comprehending how different wavelengths affect the energy levels of photons encountered in various types of electromagnetic radiation.
- Energy, E = \( \frac{hc}{\lambda} \)
The nature of this relationship is inversely proportional, meaning as the wavelength increases, the energy decreases and vice versa. This fundamental concept is crucial for comprehending how different wavelengths affect the energy levels of photons encountered in various types of electromagnetic radiation.
Planck's Constant
Planck's constant is an essential value in the world of physics, and it plays a significant role in our calculation of photon energy. Represented as \( h \), its value is approximately \( 6.626 \times 10^{-34} \) J·s.
Planck's constant connects the energy of photons to their frequency, reinforcing the quantum nature of light.
Planck's constant connects the energy of photons to their frequency, reinforcing the quantum nature of light.
- The constant signifies that energy is quantized, meaning it's divided into discrete 'packets' or photons.
- This supports the particle-like behavior of light, similar to microscopic particles like electrons.
Speed of Light
The speed of light is another constant crucial to the equation governing photon energy. Denoted by \( c \), its precisely measured value is approximately \( 3.00 \times 10^8 \) meters per second.
This speed is the limit at which all light waves travel in a vacuum and is an integral factor in associating energy with wavelength in the formula \( E = \frac{hc}{\lambda} \).
This speed is the limit at which all light waves travel in a vacuum and is an integral factor in associating energy with wavelength in the formula \( E = \frac{hc}{\lambda} \).
- This constant ensures that the relationship between wavelength and frequency is steady and predictable.
- The speed of light's constancy across the vacuum makes it a reliable building block for equations that describe electromagnetic phenomena.
Wavelength Inversion Proportionality
The concept of wavelength inversion proportionality is pivotal to understanding how energy and wavelength are related. The equation \( E = \frac{hc}{\lambda} \) underscores that energy varies inversely with wavelength.
The shorter the wavelength, the higher the energy of the photon.
This inversion relationship is a key reason why higher-energy phenomena (like X-rays) can be more penetrating compared to longer-wavelength forms of light.
The shorter the wavelength, the higher the energy of the photon.
- For an 8000 Å photon, the energy is calculated as \( E = \frac{hc}{8000 \text{ Å}} \), whereas for a 16000 Å photon, \( E = \frac{hc}{16000 \text{ Å}} \).
- This means that if the wavelength doubles, as in going from 8000 Å to 16000 Å, the energy halves.
This inversion relationship is a key reason why higher-energy phenomena (like X-rays) can be more penetrating compared to longer-wavelength forms of light.
Other exercises in this chapter
Problem 60
The frequency of radiation emitted when the electron falls from \(\mathrm{n}=4\) to \(\mathrm{n}=1\) in a hydrogen atom will be (Given ionization energy of \(\m
View solution Problem 61
Among the following series of transition metal ions, the one where all metal ion have \(3 \mathrm{~d}^{2}\) electronic configuration is (a) \(\mathrm{Ti}^{3+},
View solution Problem 64
An electron is moving in Bohr's fourth orbit, its de-Broglie wavelength is \(X\). What is the circumference of the fourth orbit? (a) \(2 \lambda\) (b) \(2 / \la
View solution Problem 65
The correct order of number of unpaired electrons in the ion \(\mathrm{Cu}^{2+} \mathrm{Ni}^{2+}, \mathrm{Fe}^{3+}\) and \(\mathrm{Cr}^{3+}\) is (a) \(\mathrm{C
View solution