Spectral Lines - Class 10 Review

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These flashcards are designed to help students review key concepts and information about spectral lines from their AST101 lecture.

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15 Terms

1
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What is scattering in terms of light?

Scattering is reflection in all directions.

2
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What happens to light when it is absorbed by black objects?

All colors of light are absorbed.

3
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How does a prism affect light?

The prism bends light differently for each color, revealing a spectrum.

4
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What is the relationship between wave speed, frequency, and wavelength?

The speed of a wave is its frequency times its wavelength, S = fL.

5
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What does the wavelength of light determine?

It determines the color of the light.

6
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What type of radiation do hot objects emit?

Hot objects emit thermal radiation that glows.

7
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What are emission lines?

Distinct colors of light emitted by low-pressure gas when electrically excited.

8
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What are the basic energy level transitions for electrons in the Bohr model?

Electrons can shift between energy levels, emitting or absorbing light of specific frequencies.

9
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What happens when white light shines on an atom?

Light of a specific frequency can be absorbed, causing the electron to move to a higher orbital.

10
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What is the significance of emission and absorption lines in spectra?

Both can be used as chemical fingerprints to identify different elements.

11
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What effect does temperature have on emission spectra?

Hotter things have a brighter spectrum, peaking at shorter wavelengths.

12
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What does redshift indicate about an object's movement?

Redshift indicates that the object is moving away from the observer.

13
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How does the Doppler effect apply to light?

If a light source is moving closer, it shifts to a higher frequency (blueshift); if moving away, it shifts to a lower frequency (redshift).

14
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Why are spectra from space considered to be messy?

They contain emission and absorption lines from multiple elements combined with a continuum spectrum.

15
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What indicates the presence of gases in a spectrum?

Absorption lines indicate cooler gases, while emission lines indicate warmer gases.