Problem 7
Question
What kinds of photons are absorbed by typical dust grains? a. infrared b. visible c. ultraviolet d. radio e. microwave
Step-by-Step Solution
Verified Answer
Typical dust grains absorb ultraviolet photons.
1Step 1: Understanding Photon Absorption by Dust Grains
Dust grains in space absorb different kinds of photons depending on their sizes and composition. The efficiency of absorbing certain wavelengths is key to determining what kinds of photons a typical dust grain would absorb.
2Step 2: Analyzing the Wavelengths
Photons have different energy levels based on their wavelengths. Ultraviolet (UV) photons have shorter wavelengths and higher energy compared to visible, infrared, microwave, and radio photons.
3Step 3: Absorption by Dust Grains
Typical interstellar dust grains are most effective at absorbing shorter wavelengths. These grains absorb UV and visible light more readily because their size is comparable to these wavelengths, leading to efficient scattering and absorption.
4Step 4: Conclusion
Since dust grains efficiently absorb shorter wavelengths, they are particularly adapted to absorbing ultraviolet photons, which have a shorter wavelength and higher energy compared to the others listed.
Key Concepts
Ultraviolet PhotonsInterstellar Dust GrainsWavelengths and Energy LevelsPhoton Scattering and Absorption
Ultraviolet Photons
Ultraviolet (UV) photons are packets of light energy with wavelengths shorter than visible light. These photons possess higher energy than their visible or infrared counterparts. The energy of a photon is inversely proportional to its wavelength, meaning that shorter wavelengths equate to higher energy levels. UV photons play a significant role in many astronomical processes and are particularly impactful in the context of interstellar dust.
- Higher energy levels due to shorter wavelengths.
- Invisible to the human eye, but detectable with specialized instruments.
- Associated with processes such as star formation and chemical reactions in space.
Interstellar Dust Grains
Interstellar dust grains are tiny particles found between stars, often consisting of a mix of carbon, silicates, ice, and metals. Despite their small size, they have a critical role in the cosmos by contributing to the cloudiness of space and affecting the propagation of light.
These dust grains are usually about the size of a thousandth of a millimeter, enabling them to interact efficiently with ultraviolet and visible light. They not only absorb these wavelengths but also scatter them, impacting the appearance and behavior of astronomical objects.
- Composed of carbon, silicates, ice, and metals.
- Size makes them effective at absorbing and scattering light.
- Easily absorb UV and visible light due to size-wavelength interaction.
Wavelengths and Energy Levels
The wavelength of light refers to the distance between successive peaks of a wave. This distance determines the energy level of the photon, with shorter wavelengths correlating to higher energy.
Different regions of the electromagnetic spectrum are characterized by varying wavelengths and energy levels:
- Radio waves: Longest wavelengths, lowest energy.
- Microwaves: Slightly shorter wavelengths, still low energy.
- Infrared: Moderate wavelengths, moderate energy.
- Visible light: Shorter wavelengths than infrared, moderately high energy.
- Ultraviolet light: Even shorter wavelengths, high energy.
Photon Scattering and Absorption
Photon scattering and absorption are key processes when discussing how light interacts with matter like interstellar dust.
"Scattering" occurs when photons are deflected in many directions after hitting particles. This does not remove the photons from the beam of light but changes their path. "Absorption," on the other hand, involves photons transferring their energy to the particles, which essentially removes these photons from the beam of light.
- Scattering deflects photons without removing them from light.
- Absorption transfers photon energy to matter, reducing light intensity.
- Both are influenced by the size and composition of the dust grains.
Other exercises in this chapter
Problem 5
Which phase of the ISM is found near hot, young stars? a. H I region b. H II region c. molecular cloud d. WISM e. coronal gas
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Which of the following is not a quality that all phases of the ISM share? a. absence of free electrons as part of gas b. more gas than dust c. more hydrogen tha
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Why does interstellar dust play a vital role in the chemistry of the galaxy? a. It allows gamma rays to penetrate into dark clouds. b. When it breaks apart, it
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How do molecular clouds provide protection from ultraviolet photons that can dissociate molecules? a. Their thermal energy deflects the ultraviolet photons. b.
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