Atomic structure Flashcards

1
Q

What are the 3 subatomic particles?

A

Proton, neutron, electron

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2
Q

What are the charges and location of protons and electrons?

A

Proton: +1, in the nucleus
Electron: -1, in orbitals around the nucleus

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3
Q

What is the role of neutrons in the nucleus?

A

They add mass and help stabilise the nucleus

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4
Q

What is an ion?

A

An atom or molecule with a charge due to losing or gaining electrons

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5
Q

What is a cation?

A

A positively charged ion formed by losing electrons

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6
Q

What is an anion?

A

A negatively charged ion formed by gaining electrons

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7
Q

What is an electrolyte?

A

A substance that conducts electricity in solution by releasing ions

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8
Q

What is the maximum number of electrons in an S orbital?

A

2

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9
Q

What is the order of orbital filling?

A

1s, 2s, 2p, 3s, 3p, 4s, 3d, 4p, 5s, 4d, 5p, 6s, 4f……

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10
Q

What are the 4 quantum numbers?

A

n (shell)
I (subshell)
m (orbital orientation)
s (spin)

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11
Q

Name the state symbols

A

aq (Aqueous)
s (Solid)
g (Gas)
l (Liquid)

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12
Q

What is the formula for concentration in mol/dm³?

A

C = n/V

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13
Q

What is the formula for moles using mass?

A

n = m/Mr

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14
Q

How many particles are in one mole? (Avogadro’s number)

A

6.022 × 10²³

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15
Q

What is the molar volume of gas at room temp?

A

24 dm³/mol (at 20°C and 1 atm)

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16
Q

What is the formula to convert g/dm³ to mol/dm³?

A

C = m/(Mr x V)

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17
Q

What is ionisation energy?

A

The energy needed to remove one mole of electrons from one mole of gaseous atoms

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18
Q

Why is the second ionisation energy higher than the first?

A

Because it’s harder to remove an electron from a positively charged ion

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19
Q

What factors affect ionisation energy?

A

Atomic radius, nuclear charge, shielding, orbital stability

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20
Q

How does atomic radius affect ionisation energy?

A

Larger atoms = lower ionisation energy (electrons are further away)

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21
Q

How does nuclear charge affect ionisation energy?

A

More protons = higher attraction = higher ionisation energy

22
Q

How does shielding affect ionisation energy?

A

More inner shells = more shielding = lower ionisation energy

23
Q

Why is it easier to remove paired electrons?

A

They repel each other slightly

24
Q

What is relative atomic mass (Ar)?

A

The average mass of isotopes compared to 1/12 of carbon-12

25
What is the relative molecular mass (Mr)?
The sum of Ar values in a molecule
26
What is radioactivity?
Spontaneous emission of radiation from an unstable nucleus
27
What are the three types of radiation?
Alpha, Beta, Gamma
28
What is alpha radiation?
2 protons + 2 neutrons (He nucleus) (low penetration)
29
What is beta radiation?
High-speed electron from nucleus. (medium penetration)
30
What is gamma radiation?
High-energy wave, no mass or charge. (high penetration)
31
What is a radioactive isotope?
An unstable isotope that emits radiation to become stable
32
What is a half life?
The time required for a substance to reduce to half of its initial value
33
How do you calculate decay?
N = N₀ × (½)ⁿ, where n = number of half-lives
34
What is radioactivity?
Radioactivity is the spontaneous emission of particles or electromagnetic radiation from an unstable atomic nucleus.
35
What factors influence the stability of an atomic nucleus?
The neutron/proton (n/p) ratio, total nuclear charge, and whether the nucleus is light or heavy.
36
How does the n/p ratio affect nuclear stability?
Light nuclei are more stable with n/p ≈ 1. Heavy nuclei require higher n/p ratios for stability. An odd n/p ratio often leads to instability.
37
What are the main types of radioactive decay and their associated radiations?
Alpha decay (α): emission of helium nucleus; Beta decay (β): neutron/proton conversion; Gamma radiation (γ): emission of high-energy photons; Positron emission (β⁺): for light nuclei with n/p < 1; Electron capture (EC): proton turns into neutron by capturing orbital electron.
38
What occurs during electron capture?
An inner-shell electron is captured by the nucleus, converting a proton into a neutron and emitting a neutrino (νₑ) and an X-ray.
39
What are the modern and old units for measuring radiation activity?
New: Becquerel (Bq) = 1 disintegration/sec. Old: Curie (Ci) = 3.7 × 10¹⁰ disintegrations/sec.
40
What are the modern and old units for absorbed radiation dose?
New: Gray (Gy) = 1 J/kg. Old: rad. 1 rad = 0.01 Gy.
41
What are the modern and old units for biological damage from radiation?
New: Sievert (Sv). Old: rem. 1 rem = 0.01 Sv.
42
What are the radiation weighting factors used in Sievert calculations?
1 for β, γ, and X-rays; 10 for high-energy protons and neutrons; 20 for α-radiation.
43
What is the general form of the radioactive decay equation?
ln[N] = ln[N₀] - λt. ## Footnote Example: ln[¹³¹I] = 2.9957 - 0.0866·t
44
What is half-life?
The time it takes for half of the radioactive nuclei in a sample to decay.
45
How are natural radioisotopes formed?
They originate from long-lived isotopes and can be produced by cosmic ray interactions.
46
How are artificial radioisotopes produced?
By transmutation: bombarding stable isotopes with α-particles, protons, or neutrons.
47
What are some applications of radioactive isotopes?
Carbon dating, radioimmunoassay, medical imaging and treatment, nuclear energy generation.
48
What’s the difference between nuclear fission and fusion?
Fission splits heavy nuclei to release energy. Fusion combines light nuclei to form a heavier nucleus, releasing energy.
49
Why are heavy nuclei typically unstable?
Heavy nuclei have many protons, which create strong electrostatic repulsion. ## Footnote More neutrons are needed to add nuclear binding through the strong force.
50
What happens if the neutron-to-proton (n/p) ratio isn't high enough?
The nucleus becomes unstable and undergoes radioactive decay.