Atomic Structure Flashcards

(54 cards)

1
Q

relative masses of sub - atomic particles

A

proton: 1
neutron: 1
electron: 1/1850

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2
Q

relative charges of sub - atomic particles

A

proton: +1
neutron: 0
electron: -1

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3
Q

where are sub - atomic particles found?

A

protons and neutrons: in the nucleus
electrons: in energy levels

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4
Q

what force holds protons and neutrons together?

A

strong, nuclear force

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5
Q

what force holds protons and electrons together?

A

electrostatic FOA

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6
Q

isotope

A

atoms of the same element with the same number of protons and a different number of neutrons
have the same chemical properties (same electron configuration) and different physical properties (different mass numbers)

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7
Q

how to calculate the number of electrons in each energy level

A

2n^2 (n =2 N³ energy level)
energy levels get higher in energy as you move away from the nucleus (are quantised)

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8
Q

What does the quantum model suggest about electron orbitals?

A

electrons don’t orbit in a well - defined path
It shows complex shapes of orbitals/electron cloud (volume of space where there is likely to be an electron)
Quantum model is based on probability rather than certainty

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9
Q

how many orbitals can the s orbital hold?
how many electrons can it hold?
shape?

A

1 orbital
2 electrons
spherical

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10
Q

how many orbitals can the d orbital hold?
how many electrons can it hold?

A

5 orbitals
10 electrons

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11
Q

how many orbitals can the p orbital hold?
how many electrons can it hold?
shape?

A

3 orbitals
6 electrons
dumbbell shape (drawn as figure of 8)

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12
Q

how many orbitals can the f orbital hold?
how many electrons can it hold?

A

7 orbitals
14 electrons

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13
Q

electron spin

A

electrons have a property called spin
if 2 electrons are in the same orbital, one will spin up and one will spin down

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14
Q

When you get to the 3d sub - energy level, what happens?

A

4s is filled first as it has less energy
4s is further away from the nucleus, so when electrons are lost to form ions, they’re lost from 4s first

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15
Q

copper electron configuration

A

instead of filling 4s first, fill 3d first
1s2 2s2 2p6 3s2 3p6 4s1 3d10

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16
Q

chromium electron configuration

A

fills 1 electron in each 3d orbital to minimise repulsion and give it the lowest energy level possible
1s2 2s2 2p6 3s2 3p6 4s1 3d5

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17
Q

ionisation energy

A

energy required to remove 1 mole of electrons from 1 mole of gaseous atoms or ions to form 1 mole of positive ions
is endothermic as it needs to overcome the attraction between the nucleus and electrons
measured in kJ/mol (when plotting on a graph, use log10 function)

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18
Q

1st ionisation energy

A

enthalpy change needed to remove 1 mole of electrons from 1 mole of gaseous atoms to form 1 mole of gaseous ions with a single positive charge
Mg(g) —- Mg+(g) + e- (need to write state symbols)

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19
Q

2nd ionisation energy

A

enthalpy change needed to remove 1 mole of electrons from 1 mole of gaseous +1 ions to form 1 mole of gaseous ions with a +2 charge
Mg+(g) —- Mg2+(g) + e- (need to write state symbols)

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20
Q

enthalpy change

A

change in heat energy at constant pressure

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21
Q

factors affecting ionisation energy

A

shielding (affects it the most)
nuclear charge
electrons in orbitals

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22
Q

how shielding affects ionisation energy

A

more shielding means lower ionisation energy as there’s a weaker attraction between the outer electron and nucleus which requires less energy to overcome

23
Q

how nuclear charge affects ionisation energy

A

higher nuclear charge means greater ionisation energy as there’s a stronger attraction between the nucleus and outer electrons so it can pull the electrons more closely (decreased atomic radius)

24
Q

how electrons in orbitals affect ionisation energy

A

when electrons begin to pair in orbitals, they experience repulsion so it is easier to remove an electron, so it has a lower ionisation energy

25
successive ionisation energy
energy required to remove electrons 1 by 1 from the same atom/ion each time, forming a more highly charged ion F(g) ---- F+(g) + e- F+(g) ---- F2+(g) + 2e- F2+(g) ---- F3+(g) + 3e- F3+(g) ---- F4+(g) + 4e-
26
What is the evidence for different energy levels and the number of electrons in each energy level?
plotting successive ionisation energies show existence of different energy levels and electrons in these energy levels As more electrons are removed, there are large jumps in ionisation energy, which reveal electrons are being removed in the next energy level
27
How to identify the group number the element belongs to, judging from a successive ionisation energy graph
the number of electrons before the first big jump shows the group number of the element If there is no big jump, the element is in group 0 EG: 736 1450 7740 10500 (element is in group 2)
28
trend of ionisation energy across a period
up, down, up, up, down, up, up
29
explain the dip in 1st ionisation energy between beryllium and boron (Be: 1s2 2s2) (B: 1s2 2s2 2p1)
Boron has more energy levels; its outer electron is in the 2p energy level which is further away from the nucleus, so it's easier to remove the electron, so it has a lower ionisation (must write electron configuration)
30
explain the dip in 1st ionisation energy between phosphorus and sulphur (P: 1s2 2s2 2p6 3s2 3p3) (S: 1s2 2s2 2p6 3s2 3p4)
In phosphorus, in the p energy level, electrons are arranged singly in orbitals but in sulphur, they begin to pair and experience repulsion, so electrons are easier to remove, so it has a lower ionisation energy
31
trend of ionisation energies down a group
general decrease due to increase in shielding steep line from Be to Ca then it becomes less steep
32
trend in ionisation from H to Mg
up, down, up, down, up, up, down, up, up, down, up
33
Which ion has the highest ionisation energy? Na: 1s2 2s2 2p6 3s1 Mg+: 1s2 2s2 2p6 3s1
same amount of shielding and number of electrons but magnesium has a higher nuclear charge so it has a higher ionisation energy since there's a stronger attraction between the nucleus and outer electrons
34
trends across period 3: atomic radius 1st ionisation energy electronegativity
atomic radius: decreases 1st ionisation energy: generally increases electronegativity: increases
35
why does the atomic radius of elements decrease across period 3?
higher nuclear charge so the protons are able to attract the electrons more closely (has the same shielding)
36
why does the 1st ionisation energy increase across period 3?
higher nuclear charge with similar shielding so there's a stronger electrostatic attraction between protons and electrons which takes more energy to overcome
37
why does electronegativity increase across period 3?
higher nuclear charge and similar shielding so it can attract electrons more strongly
38
how does melting and boiling point change across period 3?
increases from sodium to silicon (metals increase due to size of ion and having more electrons, and silicon is giant covalent) decreases to phosphorus (P4) then increases to sulfur (S8) as it has more vdW then decreases to chlorine and argon
39
significance of mass spectrometry:
allows us to figure out the Mr of substances helps us see which isotopes make up a certain sample
40
stages of time of flight mass spectrometry:
ionisation acceleration detection
41
conditions of time of flight mass spectrometry:
vacuum (stops electrons from being absorbed by molecules in the air) atoms must be gaseous
42
2 types of ionisation in time of flight mass spectrometry
electron impact (used for elements and low Mr compounds) electrospray (used for high Mr compounds to prevent fragmentation)
43
electron impact ionisation in time of flight mass spectrometry
substance has to be gaseous high energy electrons are fired from an electron gun at the sample to knock off an electron from each atom to form a +1 ion X(g) --- X+ (g) + e-
44
electrospray ionisation in time of flight mass spectrometry
sample dissolved in volatile solvent and injected into a hypodermic needle where particles gain a proton when they leave the needle as a fine mist X + H+ --- XH+ when calculating m/z, you need to take away 1 from each peak as this includes H+ (same for TOF calculations)
45
acceleration in time of flight mass spectrometry
all particles are accelerated so they have the same kinetic energy (only ionised molecules can interact and be accelerated) in the flight tube, ions are accelerated towards a negative plate; their TOF depends on velocities which depend on mass
46
detection in time of flight mass spectrometry
ion picks up electron from a detector to complete the circuit Mg+(g) + e- --- Mg(g) current and abundance are proportional (the higher the current, the greater the abundance of the isotope)
47
m/z ratio in time of flight mass spectrometry
is mass of isotope since charge is +1 (mass/charge) sometimes, 2 electrons can be knocked off in ionisation so the mass is 1/2 than usual
48
RAM equation
(abundance x isotope) + (abundance x isotope)/total abundance
49
how to find the mass of an ion in kg
mr x 10^-3/avogadro's constant
50
molecular ion peak on a mass spectrum
peak with the largest m/z ratio (is the complete molecule that hasn't undergone fragmentation) small peaks on the right of this peak may be due to isotopes such as C13 or H3
51
2 common isotopes of chlorine
Cl35 and Cl37 abundance of 35: 75% abundance 37: 25% relative abundances of Cl35, Cl37 and mix: 9:1:6 (on mass spectrum its m/z ratio is 70, 72 and 74 as it is diatomic and some atoms form in ratio of 3:1)
52
common isotopes of bromine:
Br79 and Br81 abundance of 81 and 79: 50% relative abundance ratio of 79, 81 and mix: 1:1:2 (on mass spectrum its m/z ratio is 158, 160 and 162 as it is diatomic and some atoms form in ratio 1:1)
53
Why do all atoms and compounds have to be ionised in the time of flight spectrometer?
so they can be accelerated by the electric field so ions can create a current when they hit the detector
54
how can you change the acceleration of ions in the spectrometer flight tube?
change the electric field