Chem Unit 1 Flashcards

(36 cards)

1
Q

Define electromagnetic spectrum

A

electromagnetic radiation (light) is a way energy moves. Light energy travels in waves, at the speed of light.

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2
Q

In what way do waves move?

A

Perpendicular to the way it travels

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3
Q

Define amplitude

A

The distance between a wave’s zero to it’s crest

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4
Q

Define crest

A

the highest point of a wave

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5
Q

define trough.

A

the lowest point of a wave

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6
Q

define wavelength

A

the distance between crests; the length of one complete wave cycle

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7
Q

define frequency

A

the number of wave cycles to pass a given point, per unit of time

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8
Q

what is the mathematical relationship between wavelength and frequency?

A

they are inversely proportional/related.

c = speed of light (m/s) —–> 3.0 * 108 m/s
λ = wavelength (m)
v = frequency (hertz, 1/s)

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9
Q

describe the relationship between frequency, wavelength, and energy.

A

lower frequency = lower energy = longer wavelength

higher frequency = higher energy = shorter wavelength

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10
Q

atomic emission spectra

A
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11
Q

how do atoms arrange themselves?

A

electrons arrange themselves to be in the lowest possible energy state.

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12
Q

what is the lowest state?

A

the closest an electron can be to the nucleus.

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13
Q

in what way do electrons move when absorbing energy?

A

they move to a higher energy level, and then as they come back down they emit the energy.

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14
Q

define quantized energy.

A

quantized energy means the electrons can possess only certain, discrete energy values; values between those quantized values are not permitted.

Electron must move from one energy level to another in distinct steps, rather than moving continuously

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15
Q

what is an excited state of an atom?

A

a state where its potential energy is higher than the ground state
–> unstable

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16
Q

what happens when the electron returns back to the ground state?

A

it releases energy that it previously gained in the form of electromagnetic radiation (light).

17
Q

how do atoms gain energy?

A

tubes filled with gas at low pressure pass through an electric current. Electrons in the gaseous atoms become excited, and then fall back to lower energy levels, emitting a light of distinctive colour.

18
Q

why do gas discharge tubes glow with a different, distinct colour?

A

electron energy levels are unique for each element

Different types of light are based on how many energy levels there are.

19
Q

list the two steps of an electron gaining energy.

A
  1. excited electrons jump to a new energy level.
  2. they fall back down, emitting the distinct colour, as they can only occupy specific spaces and therefore give different emissions
20
Q

when are atomic emission spectras produced?

A

when excited electrons return to ground state.

discrete photons carrying discrete amounts of energy

21
Q

describe the visible EMISSION spectrum for hydrogen

A

composed of 4 lines: converge at high frequency.

gas discharge tube, light goes through a slit, which hits a prism, which creates the emission spectrum

v = 410
i = 440
g = 490
r = 660

22
Q

define/describe the continuous spectrum.

A
  • all wavelengths (frequencies within a particular region) are seen
  • often represented as the complete ROYGBIV
23
Q

what two regions can you have continuous spectrum in?

24
Q

describe white light.

A

white light contains all frequencies in the visible spectrum, so it can be split into a continuous spectrum by a prism

25
what does emissions only existing at certain wavelengths tell us?
electrons cannot occupy anywhere around the spectrum. [?]
26
define a line spectrum
- has two types - emitted radiation is split into a spectrum that only contains emissions at particular wavelengths - gas absorbs different wavelengths that correspond to their energy levels, everything else passes through
27
define an absorption spectrum
- is a kind of LINE spectrum - a heat source that emits a continuous spectrum is placed BEHIND a COLD and transparent cloud of gas - gas absorbs some colours/specific wavelengths - displays missing black lines - the black lines that are "missing" correspond to the emission spectrum In the absorption spectrum there will be gaps. The absorbed photons show up as black lines because the photons of these wavelengths have been absorbed and do not show up.
28
define an emission spectrum
- the gas is heated directly - cloud of hot, transparent gas emitting certain colours - displays coloured lines coloured lines correspond with absorption spectrum
29
describe the Hg, Ne spectrums
Hg: 2v, 1i, 2g, 3y, 2o, 1r (11) Ne: 2i, 3g, 6y, 5o, 4r (20)
30
there is a [limited/non-limited], [specific/non-specific] number of energy quantities (deltaE) that the e- in an atom can lose.
limited, specific
31
falling down a specific distance will always give off the [same/different] amount of energy
same - The “gap” the electron falls down by is dictated by the energy level - Electrons can only be found in specific energy levels, and must remain there except when energy change is applied
32
what are the four different components of energy levels?
1. ground state (n = 1; shell closest to the nucleus) 2. excitation (excited state): give light/heat, somewhere between n = 1 and the largest shell 3. emission: eventually returns back to ground state 4. ionization: when the electron completely leaves an atom due to an excess of energy
33
be able to draw the diagram of energy levels.
34
list the 3 kinds of spectrums that the light emits.
a) LYMAN: electrons returning down to n = 1 emit UV light (HIGH energy). --> biggest amount of energy released b) BALMER: electrons returning down to n = 2 emit visible light c) PASCHEN: electrons returning down to n = 3 emit IR light (LOW energy)
35
define ground state, first excited state, second excited state.
ground state: n = 1 (closest shell to nucleus) first excited state: n = 2 second excited state: n = 3
36
what is the trend for energy levels?
CONVERGENCE: the lines, as demonstrated by energy level diagrams, get closer and closer together, as frequency increases (wavelength decreases) more energy = the higher the energy level (approaching n = infinity). corresponds with the difference of far out electron shells: closer and closer --> as you move away from the nucleus, do not feel attraction as much