Problem 4
Question
Explain why the absorption lines of an element have the same wavelengths as the emission lines of that element.
Step-by-Step Solution
Verified Answer
Absorption and emission lines match because they involve equal energy level changes in opposite directions.
1Step 1: Understanding Emission and Absorption
Atoms consist of electrons orbiting a nucleus. When an electron gains energy, it moves to a higher energy level, a process associated with emission. Conversely, when an electron releases energy, it falls back to a lower energy level, corresponding to absorption.
2Step 2: Recognizing Energy and Wavelength Relationship
The energy of photons absorbed or emitted by an electron is directly related to their frequency and inversely related to their wavelength by the equation: \( E = h u = \frac{hc}{\lambda} \), where \( E \) is energy, \( u \) is frequency, \( \lambda \) is wavelength, \( h \) is Planck's constant, and \( c \) is the speed of light.
3Step 3: Identifying Specific Wavelengths
Each element has discrete energy levels, and when electrons transition between these levels, they absorb or emit photons of specific energy, thus specific wavelengths unique to that element.
4Step 4: Connecting Emission and Absorption Wavelengths
When an atom absorbs a photon, causing an electron to jump to a higher energy level, it does so at the same wavelength as it would emit when the electron falls back to the original or another lower energy level. This is because the difference in energy levels (determining the transition's wavelength) is the same in both directions.
Key Concepts
Energy Levels in AtomsPhoton WavelengthPlanck's Constant
Energy Levels in Atoms
Atoms are like tiny solar systems where electrons orbit a central nucleus. These electrons can only exist at specific energy levels, like rungs on a ladder. Each level is a set distance from the nucleus, and electrons need a specific amount of energy to jump to a higher level or drop to a lower one.
- Exciting Electrons: When an electron absorbs energy, it moves to a higher energy level. This process is called absorption.
- Releasing Energy: Conversely, when an electron drops to a lower energy level, it emits energy in the form of a photon. This is known as emission.
Photon Wavelength
Photons are packets of light energy, and each has a specific wavelength, determining its color and energy. The wavelength of a photon is inversely related to its energy.
- Collision of Concepts: Energy and wavelength are linked by the equation \( E = \frac{hc}{\lambda} \), where \( \lambda \) is wavelength, \( h \) is Planck's constant, and \( c \) is the speed of light.
- Color Code: Shorter wavelengths correspond to higher energy and tend to be more towards the blue end of the spectrum, while longer wavelengths are lower in energy and appear more red.
Planck's Constant
Named after the physicist Max Planck, Planck's constant \( h \) is a crucial figure in the field of quantum mechanics. It establishes the scale of energy that photons carry.
- Fundamental Value: \( h \) is approximately \( 6.626 \times 10^{-34} \text{ J}\cdot\text{s} \).
- Role in Equations: It appears in the equation \( E = hu \), linking energy \( E \) with frequency \( u \), and in \( E = \frac{hc}{\lambda} \), connecting energy to wavelength.
Other exercises in this chapter
Problem 2
Both parallax and proper motion are changes in the apparent positions of stars. Describe how observations carried out over many years could be used to distingui
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Suppose the Sun moved through space much faster than it actually does. What effect would this have on the directions of the apex and antapex of the Sun's motion
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Why is it impossible for a gas composed of atoms that all have their electrons in the ground state to produce an emission line?
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Why are Balmer lines weaker in the spectra of \(\mathrm{O}\) stars than they are in the spectra of A stars?
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