Lecture 15 Flashcards

1
Q

Properties of light

A

-White light is made from the whole visible spectrum
-Light is a form of energy
-Light travels at a finite speed (3x10^8m/s)

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2
Q

How does light interact with matter?

A

-Emission
-Absorption
-Transmission: transparent objects allow light to pass and opaque objects absorb light
-Reflection: changes in the light direction (but not energy)

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3
Q

Properties of waves

A

-Wavelength: distance between two peaks
-Frequency: number of times a wave vibrates up and down
-Wave speed= frequency x wavelength

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4
Q

What are photons?

A

-Particles of light
-Photons have a frequency and a wavelength
-Photon energy depends on frequency (E=hf)

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5
Q

What is spectroscopy?

A

Viewing the amount of light from each wavelength that is emitted by an object

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6
Q

What is the continuous spectrum?

A

Light produced over the range of the visible spectrum without interruption.
-Incandescent light globes produce a continuous spectrum

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7
Q

What is an emission line spectrum?

A

The different wavelengths of light emitted by unique elements.
-Low-density gas clouds emit light of specific wavelengths characteristic of the composition and temperature

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8
Q

What is an absorption specturm?

A

The opposite of an emission spectrum. Light absorbed by unique elements.

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9
Q

What is a chemical “fingerprint”?

A

The wavelengths emitted by atoms due to the unique set of energy levels of the electron shells. Each transition corresponds to a unique photon energy.
-Transitions of electrons back to their ground state produce an emission spectrum
-Transitions of electrons to higher energy levels produce an absorption spectrum

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10
Q

How do the energy levels of molecules differ from individual atoms?

A

Molecules have additional energy due to their bonds which can rotate and vibrate.

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11
Q

What does thermal radiation depend on?

A

Temperature

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12
Q

Properties of thermal radiation

A
  1. Hotter objects emit more light at all frequencies
  2. Hotter objects emit more photons with a higher average energy
  3. Thermal energy=blackbody radiation
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13
Q

What does Wien’s Law predict?

A

The peak in thermal radiation

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14
Q

How does light tell us the speed of a distant object?

A

The Doppler effect

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15
Q

How does the Doppler Effect describe the motion of objects?

A

Objects coming towards us will experience shortening of their wavelengths producing blueshift. Conversely, objects moving away from us will experience longer wavelengths producing redshift

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16
Q

How is the Doppler Effect measured?

A

It is measured from shifts in the wavelengths of the spectral lines

17
Q

How do spectral lines change in a rotating object?

A

Faster rotating objects produce wider spectral lines

18
Q

What does redshift tell us about the universe?

A

That it is expanding.