1.5 Atomic Spectroscopy Flashcards

(30 cards)

1
Q

Main group number

A

Number of electrons in valence shell in one atom of that element

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2
Q

Period number

A

Number of occupied shells in one atom of that element

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3
Q

Periodic table blocks (s, p, d, f)

A

Identity of highest energy subshell

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4
Q

Maximum number of electrons each orbital can hold

A

2

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5
Q

Maximum number of electrons s-subshell can hold

A

2

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6
Q

Maximum number of electrons p-subshell can hold

A

6

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7
Q

Maximum number of electrons d-subshell can hold

A

10

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8
Q

Maximum number of electrons f-subshell can hold

A

14

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9
Q

Aufbau principle

A

Electrons fill subshells in order of increasing energy; low -> high.

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10
Q

Ions

A

Charged particles formed from gain/loss of electrons. Electrons added/removed from highest energy subshell (highest n-value) in an atom.

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11
Q

2 exceptions to electron subshell configuration

A

Chromium (Cr)
Copper (Cu)

Contain half-filled 4s subshell (4s1, not 4s2), allowing each orbital in 3d subshell to be half/completely filled, which is a more stable configuration for them.

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12
Q

Ground state

A

Lowest energy level; most stable, so electrons occur naturally in this state. Singular.

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13
Q

Excited state

A

Electrons promoted to higher energy levels through absorption of photons. Unstable and temporary. Numerous.

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14
Q

Photon

A

Discrete quantised amount of energy, supplied as light, heat, or electrical energy.

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15
Q

Octet rule

A

Tendency of atoms to prefer to have eight electrons in their valence shell.
Will share, gain, lose electrons to do so.
Noble gas configuration.

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16
Q

Electromagnetic emissions

A

Excited state is unstable, so electrons will return to lower energy levels by emitting energy equivalent to the transition, and so the photon’s energy, as electromagnetic radiation.
These emitted photons have specific frequencies and wavelengths related to their energies; so, emissions are characteristic of certain elements.

17
Q

Transition metals forming ions

A

Transition metals (d-block) lose electrons from valence shell (highest quantum number).

18
Q

Isoelectric

A

Same number of electrons.

Number and distribution of electrons in cation’s or anion’s outermost shells match the electron configuration of the nearest preceding noble gas (isoelectric with noble gas configuration).

19
Q

Line emission spectrum

A

Black background with colourful lines

20
Q

Line absorption spectrum

A

Colourful background with black lines

21
Q

Purpose of atomic absorption spectroscopy (AAS)

A

Detection of metal ions in small quantities - that is, in the ppm and ppb range. Uses absorption of light to measure the concentration of metal in a mixture.

22
Q

Metals forming ions

A

Tend to lose electrons from valence shell

23
Q

Non-metals forming ions

A

Tend to gain electrons to fill valence shell

24
Q

Hollow cathode lamp

A

Emits light at specific wavelengths of the target element for absorption measurement.

25
Detector
Measures intensity of light - both incident and transmitted - to determine how much was absorbed.
26
Fuel
Sample aspirated into this fuel to undergo desolvation; so, sample dehydrated and solvent removed.
27
Atomiser
Causes sample molecules to dissociate into atoms and convert to atomic vapour (gas-phase).
28
Monochromator
Consists of a diffraction grating or prism. Enables selection of one specific wavelength of light for detection, which is unique to the element of interest.
29
Relationship between absorbance and concentration
A ∝ C
30
Formula for absorbance
A = log10 (I0/I) where I0 = incident light I = transmitted light