light and matter

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27 Terms

1
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watt

flow of energy per unit time; 1 Joule/second

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components of white light

all rainbow colors

3
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photon’s energy depends on

frequency

4
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light has _ fields which oscillate in _

electric and magnetic; opposite directions

5
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what do waves carry and not carry

energy, not matter

6
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atmospheric transmission

some wavelengths are blocked by Earth’s atmosphere, others aren’t

7
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what do transparent and opaque objects do

transmit vs block light

8
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atomic number

number of protons

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atomic mass number

number of protons + neutrons

10
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different isotopes have same number of _ but different

protons, neutrons

11
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continuous spectrum

e.g a common lightbulb spanning all visible wavelengths, white noise

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emission spectrum

specific wavelength depending on composition and temperature

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absorption spectrum

can absorb light of specific wavelengths, leaving dark absorption lines in the spectrum

14
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solid sphere model

Dalton, Greek idea of an indivisible, identical elemental sphere

15
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plum pudding model

Thomson, electrons scattered throughout a sphere of + charge

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nuclear model

rutherford, atoms are mostly empty space, with most mass in nucleus and electrons orbiting

17
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planetary model

bohr, orbits have quantized sizes and energies

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quantum model

Schrödinger, electrons move in waves instead of set paths, clouds of probability instead of knowing exact location

19
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vibrational and rotational lines

movement of molecules that complicates their spectra, many of which are the infrared range

20
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blackbody spectrum

thermal emission’s continuous spectrum, its peak tells us object’s temperature

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thermal radiation

emitted by nearly all large or dense objects, depends on temperature (poker in fireplace getting white-hot

22
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doppler shift

light as well as sound → red and blue-shifting; tells you about the relative motion of distant objects

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we measure doppler effect from

shifts in wavelengths of spectral lines; tells us an object’s speed toward or away from us, but only if there’s a component of its motion parallel to our line of sight

<p>shifts in wavelengths of spectral lines; tells us an object’s speed toward or away from us, but only if there’s a component of its motion parallel to our line of sight</p>
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doppler shift and rotating objects

different sides of a rotating object spread out its spectral lines, wider when an object rotates faster

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doppler broadening in gas

random motions in gas particles caused by a higher temperature broadens the spectral lines

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cosmological redshift (not doppler)

light shifts lower in frequency due to Universe’s and the wave’s expansion

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velocity of molecule and spectral lines

NO CONTRIBUTION; while it can cause doppler broadening or shifts, it doesn’t create unique spectral lines