3.3 Flashcards

1
Q

define continuous spectrum

A

the colours white light is split into after going through a prism

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2
Q

how do you know the energy of an atom is quantized

A

only certain frequencies are released when sparked ect. so only certain energy levels for atoms

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3
Q

equation for energy levels of an atom

A

hv = E2 - E1

plancks constant x frequency = higher energy - lower energy

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4
Q

which energy transitions lead to the paschen series

A

n = 7,6,5,4 to n = 3

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5
Q

which energy transitions lead tot he Balmer series

A

n = 6,5,4,3 to n = 2

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6
Q

which transitions lead to the Lyman series

A

n = 5,4,3,2 to n = 1

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7
Q

Blamer’s frequency expression

A

v is proportional to 1/4 - 1/n^2

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8
Q

what is the Rydberg equation used for the lyman series

A
v = Rh[1/n1^2 - 1/n2^2]
frequency = Rydberg constant [ 1/lower energy level squared - 1/higher energy level squared]
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9
Q

define ionisation energy

A

the minimum energy required to to completely remove the electron from the atom

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10
Q

when does the spectral lines for hydrogen converge into a continuum

A

at n = infinity

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11
Q

what sort of spectra emit electromagnetic waves

A

emission spectra

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12
Q

what sort of spectra absorb electromagnetic waves

A

absorption spectra

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13
Q

which photons are absorbed by absorption spectra

A

the ones with energy that corresponds to transitions between the ground state and excited state

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14
Q

what do absorption spectra look like

A

dark lines on a bright background

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15
Q

what does the bohr model of an atom suggest

A

electrons have specific orbits and a nucleus in the centre

emitting energy is electron moving between orbits

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16
Q

simplified bohr equation

A

E = -k/n^2
k is a constant
E is energy
n is a quantum integer where n = 1 is ground state

17
Q

why did bohrs equation to explain the spectra not work?

A

it only applied to hydrogen