1.2 Atoms Flashcards

1
Q

Define an atomic orbital

A
  • region of space around the nucleus of an atom where there is a high probability of finding an electron of a given energy
  • up to 2 electrons with opposite spins
How well did you know this?
1
Not at all
2
3
4
5
Perfectly
2
Q

What are the different types of orbitals?

A
  • s orbital
  • p orbitals
  • d orbitals
  • f orbitals
How well did you know this?
1
Not at all
2
3
4
5
Perfectly
3
Q

Define ionisation

A
  • the process of removing one or more electrons from an atom to form a positively charged ion
  • there is a first, second and third ionisation energy
How well did you know this?
1
Not at all
2
3
4
5
Perfectly
4
Q

Define the (molar) first ionisation energy

A
  • the energy required to remove one electron from each atom in one mole of its gaseous atoms
  • kJ/mol
How well did you know this?
1
Not at all
2
3
4
5
Perfectly
5
Q

Outline the factors affecting ionisation energy

A
  • attraction of the nucleus (more protons = greater attraction = more IE)
  • distance of electrons from the nucleus (force between decreases as the distance increases - further away = lower IE)
  • shielding of the nucleus
How well did you know this?
1
Not at all
2
3
4
5
Perfectly
6
Q

Define and explain the shielding affect

A
  • the repulsion between electrons in different shells.
  • inner shell electrons repel outer shell electrons and reduce the effect of the positive nuclear charge
    -the more filled inner shells there are, the smaller the attractive force on the outer electron and therefore the lower the IE
How well did you know this?
1
Not at all
2
3
4
5
Perfectly
7
Q

What is effective nuclear charge?

A

The total positive charge pulling the electrons to the nucleus. lt is affected by atomic radius and shielding

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
8
Q

Explain the impact of atomic radius on IE

A

The greater the atomic radius the more electron shielding meaning the outer electrons of the atom are easier to remove, resulting in overall lower effective nuclear charge thus IE.

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
9
Q

What happens to IE as you descend a group?

A
  • decreases
  • more shells
  • increase in shielding due to shell number and so decreases attraction between +ve nucleus and -ve electrons, therefore easier to remove the outer electron
How well did you know this?
1
Not at all
2
3
4
5
Perfectly
10
Q

What happens to IE as you go across a period

A

IE increase across a group as there’s no change in shells or electron shielding but the increase number of electrons and protons increases the attraction of the nucleus making it harder to remove an outer electron

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
11
Q

Why is the 1st IE of N higher than that of O?

A

In oxygens electronic configuration it has a paired electron that N does not have. This means that due to the repulsion, it is easier to lose this electron in the first ionisation energy stage than it is in N, making the IE of O lower.

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
12
Q

What is atomic spectrum?

A
  • spectrum of frequencies of EM radiation that is admitted or absorbed during transitions of electrons between energy levels within in atom
How well did you know this?
1
Not at all
2
3
4
5
Perfectly
13
Q

How does an absorption spectra form?

A
  • white light shone through vapour of element
  • black lines appear in the spectrum where the light
    of some wavelengths has been absorbed
  • the wavelengths of these lines correspond to the energy taken in by atoms to promote electrons to higher energy levels
How well did you know this?
1
Not at all
2
3
4
5
Perfectly
14
Q

How is emission spectra formed?

A
  • atom absorbs white light through its vapour which gives the atom energy, exciting it
  • promotes electron to a higher energy level which it is unable to stay at for long as energy levels are quantised
  • leaves the excited state and falls to a lower energy level, emitting photons of light
How well did you know this?
1
Not at all
2
3
4
5
Perfectly
15
Q

The hydrogen emission spectrum

A
  • only 1 electron and so simplest emission spectrum
  • consists of separate series of lines mainly in the UV, visible and infrared regions
  • only Balmer series in in visible region
How well did you know this?
1
Not at all
2
3
4
5
Perfectly
16
Q

What is electronic transition?

A

When an electron moves from one energy level to another

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
17
Q

The lower an electron falls,

A

The lower the wavelength and therefore the more energy

18
Q

What is the convergence limit?

A

The point at which the energy of an electron is no longer quantised as the atom is ionised

19
Q

How do you calculate the IE of a hydrogen atom from the atomic emission spectrum?

A
  • record the convergent frequency from the Lyman series
  • use E=hf to calculate the energy of 1 atom
  • multiply by avogadros constant for 1st molar IE
20
Q

Equations for E (always in kJ)

A

E = hf

E = Lhc/y

21
Q

What is radioactive decay?

A

Where atoms are unstable due to an imbalance of protons and neutrons in the nucleus and so undergo radioactive decay to produce stable fragments

22
Q

Explain alpha decay

A
  • helium nuclei (2P, 2N)
  • least penetrating - stopped by paper and skin and only travel few cm in air
  • most ionising in the body
  • mass decrease by 4 and atomic number decrease by 2
23
Q

Explain gamma decay

A
  • high energy EM wave
  • no impact on mass or atomic number
  • most penetrating - stopped by lead and concrete and travels a few m in air
  • least ionising in body
24
Q

Explain beta decay

A
  • regular and inverse ( beta plus and beta minus)
  • high speed, high energy electrons
  • atomic number increase by 1
25
Q

Explain beta minus

A
  • electron capture
  • orbital electrons captured by a proton leading to the formation of a neutron and the emission of an electron neutrino (ve) (similar to an electron but no charge)
  • atomic number minus 1, +ve
26
Q

Explain beta plus

A
  • proton converted into a neutron while releasing a positron (B+ particle similar to electron but +ve charge) and an electron neutrino
  • atomic number minus one, + B+ + ve
27
Q

Define first ionisation energy

A
  • energy required to remove one electron from each atom in one mole of its gaseous atoms
28
Q

f=

A

speed of light
———————
wavelength

29
Q

Explain why it is unlikely that stable atoms of (ION) will form

A

Large increase between 1st and 2nd IE due to shells/electrons being much closer to nucleus. Energy required is unlikely to occur naturally

30
Q

Why do H atoms emit definite frequencies of light?

A

Frequency of light depends on the energy absorbed to promote an electron from lower to higher energy levels. Energy levels are quantised so frequency emitted is definite

31
Q

Why are there several series of lines?

A

Electrons falling to different energy levels when leave excited state

32
Q

Why do the lines within the series converge?

A

Energy differences decreases and so they eventually merge into 1

33
Q

How does gamma react to an electric/magnetic field?

A

It is undeflected as it has no charge. A straight line.

34
Q

How does alpha react to electric/magnetic field?

A

Deflects toward the negative because helium nuclei is positively charged. Gradual and slow deflection due to weight

35
Q

How does beta react to electric/magnetic field?

A

Deflects to positive pole as it’s a negative particle. Deflects quickly as it’s light

36
Q

Define half life

A

Time taken for half of the unstable atoms of an isotope to decay

37
Q

What does radiation do to cells?

A

Damages the DNA of cells which leads to mutations and uncontrolled cell division, resulting in cell death or cancerous tumours forming

38
Q

Uses of radioactive isotopes

A
  • medicine: radiotherapy and medical tracers
  • carbon and radiodating
  • industry to analyse thickness of foil or paper
39
Q

Frequency and wavelength are

A

Inversely proportional

40
Q

Frequency is (….) to energy

A

Directly proportional