Continuous Spectra Flashcards

1
Q

What is the spectrum of white light?

A

Continuous

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2
Q

What is each line in a line spectrum caused by?

A

Each line in a line spectrum is due to light of a certain color and therefore a certain wavelength.

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3
Q

What are some features of the wavelength of lines of a line spectrum?

A

• They are a characteristic of the atoms of that element.

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4
Q

How can you identify the element that produced the light?

A
  • The wavelength of lines of a line spectrum of an element are characteristic of the atoms of that element.
  • By measuring the wavelengths of a line spectrum, you can identify the element the element that produced the light.
  • No other element produces the same pattern of light wavelengths.
  • This is because the energy levels of each type of atom are unique to that atom, so photons that are emitted a characteristic of the atom.
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5
Q

When do you get a line absorption spectrum?

A

When light with a continuous spectrum of energy passes through a cool gas.

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6
Q

What happens at low temperatures?

A

Most of the electrons in the gas atoms will be in their ground states.

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7
Q

what happens to the photons?

A
  • Electrons can only absorb photons with energies equal to the difference between two energy levels
  • Photons of the corresponding wavelengths are absorbed by the electrons to excite them to higher energy levels.=
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8
Q

Why are the wavelengths missing from the continuous spectrum when it passes through the cool gas?

A
  • Most of the electrons in the gas atoms will be in their ground states.
  • Electrons can only absorb photons with energies equal to the difference between two energy levels
  • Photons of the corresponding wavelengths are absorbed by the electrons to excite them to higher energy levels.=
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9
Q

What do the black lines represent in the excited gas?

A
  • A continuous spectrum appears with black lines in it corresponding to the absorbed wavelengths.
  • Comparisons of absorption and emission spectra of a particular gas, shows that the black lines in the absorption spectrum match up to the bright lines in the emission spectrum.
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