3.4 Electromagnetic Spectrum
Pre-Lecture Reading 3.4
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•Astronomy Today, 8th Edition (Chaisson & McMillan)
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•Astronomy Today, 7th Edition (Chaisson & McMillan)
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•Astronomy Today, 6th Edition (Chaisson & McMillan)
Video Lecture
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•Electromagnetic Spectrum (5:14)
Supplementary Notes
Types of Light
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•See Types of Light.
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•Visible light—the light that we can see with our eyes—is only a tiny sliver of the entire electromagnetic spectrum, with wavelengths between ≈700 nm (red) and ≈400 nm (violet).
Figure 1: Image Credit: Advanced Light Source, Lawrence Berkeley National Laboratory
Light Wave Properties
Waves in general
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•See Particle vs. Wave Motion.
Light waves
Example:
If you double a light wave's frequency, you double its energy.
If you double a light wave's frequency, you double its energy.
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•Solving for λ and ν yields:
Example:
Consider a 1-m radio wave. Hence,
Consider a 1-m radio wave. Hence,
λ = 1 m
and ν =
= 3 × 108 s−1 = 3 × 108 Hz.
(3 × 108 m/s) |
(1 m) |
Example:
Consider a 108-Hz radio wave. Hence,
Consider a 108-Hz radio wave. Hence,
ν = 108 Hz
and λ =
= 3 m.
(3 × 108 m/s) |
(108 Hz) |
For λ measured in nm, µm, mm, cm, m, and km, the following values of c, respectively, can be used to simplify calculations:
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•c = 3.00 × 1017 nm/s
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•c = 3.00 × 1014 µm/s
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•c = 3.00 × 1011 mm/s
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•c = 3.00 × 1010 cm/s
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•c = 3.00 × 108 m/s
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•c = 3.00 × 105 km/s
Assignment 2
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•Do Question 2.