Analyzing Light

Flashcard
•
Science
•
9th Grade
•
Hard
Wayground Content
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15 questions
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1.
FLASHCARD QUESTION
Front
What is blackbody radiation?
Back
Blackbody radiation refers to the electromagnetic radiation emitted by an idealized object that absorbs all incident radiation, regardless of frequency or angle of incidence. It is characterized by a specific spectrum that depends only on the object's temperature.
2.
FLASHCARD QUESTION
Front
What does the peak of a blackbody radiation curve indicate?
Back
The peak of a blackbody radiation curve indicates the wavelength at which the object emits the most radiation. This peak shifts to shorter wavelengths as the temperature of the object increases, according to Wien's Displacement Law.
3.
FLASHCARD QUESTION
Front
What is Wien's Displacement Law?
Back
Wien's Displacement Law states that the wavelength at which the emission of a blackbody spectrum is maximized is inversely proportional to the temperature of the blackbody. Mathematically, it is expressed as λ_max = b/T, where b is a constant.
4.
FLASHCARD QUESTION
Front
How do scientists use spectroscopes to analyze light?
Back
Scientists use spectroscopes to separate light into its component colors (spectrum) and analyze the intensity of each wavelength. This helps in identifying the composition of stars and other celestial objects based on their emission or absorption lines.
5.
FLASHCARD QUESTION
Front
What are emission and absorption lines?
Back
Emission lines are bright lines in a spectrum that correspond to specific wavelengths of light emitted by atoms or molecules. Absorption lines are dark lines that appear in a spectrum when light passes through a cooler gas, which absorbs specific wavelengths.
6.
FLASHCARD QUESTION
Front
What is the electromagnetic spectrum?
Back
The electromagnetic spectrum is the range of all types of electromagnetic radiation, including radio waves, microwaves, infrared, visible light, ultraviolet, X-rays, and gamma rays, ordered by wavelength or frequency.
7.
FLASHCARD QUESTION
Front
What is infrared light and why is it important in astronomy?
Back
Infrared light is a type of electromagnetic radiation with wavelengths longer than visible light. It is important in astronomy because it can penetrate dust and gas clouds, allowing astronomers to observe celestial objects that are otherwise obscured.
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