2.2.1: Electron structure & ionisation energy Flashcards

1
Q

Ground state

A

the lowest energy level available to the electron.

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2
Q

Energy levels converge where?

A

At n =∞

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3
Q

The higher the n…

A

the further the shell is from the nucleus

∴ the higher the energy in that shell

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4
Q

First ionisation energy

A
  • Energy required
  • To remove 1 mole of electrons
  • From 1 mole of gaseous atoms
  • To form 1 mole of gaseous unipositive cations
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5
Q

Equation for first ionisation energy

A

X (g) –ΔH–> X⁺ (g) + e-

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6
Q

Factors that affect ionisation energy

A
  • Nuclear charge
  • Shielding
  • Atomic radius (distance from nucleus)
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7
Q

Nuclear charge effect on ionisation energy

A

• Greater +ve charge (no. of protons) = harder to remove e-
∵ there is greater electrostatic attraction between e- and nucleus
• Hence greater nuclear charge = higher ionisation energy

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8
Q

Shielding effect on ionisation energy

A
  • Electrons repel each other
  • Electrons in inner shells repel those in outer shells –> reduces EFFECT OF +ve charge of the nucleus
  • Greater shielding = lower ionisation energy
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9
Q

Atomic radius effect on ionisation energy

A
  • Attractive force inversely proportional to distance squared (Coulomb’s law of electrostatics)
  • Greater distance = weaker attractive force = lower ionisation energy
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10
Q

Trends in 1st IE

A

1st IE:
↓ down group due to shielding
↑ across a period due to increasing nuclear charge

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11
Q

1st IE ______ down a group

A

decreases

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12
Q

1st IE _______ across a period

A

increases

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13
Q

Why does 1st IE decrease down a group

A

Due to increasingly shielding

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14
Q

Why do successive ionisation energies always increase?

A
  • Because electrostatic attraction between e- and nucleus increases
  • Because e- is gradually being removed from a more +ve species
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15
Q

Orbital

A

A probability region for an electron.

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16
Q

s subshell

A
  • spherically symmetric
  • 1 x orbital which holds 2 e-
  • Starts at n=1
17
Q

p subshell

A
  • Starts at n=2

* Each subshell has 3 orbitals (2e- each)

18
Q

All the p orbitals in a p subshell are __________

A

degenerate

19
Q

d subshell

A
  • starts at n=3

* Each subshell has 5 orbtials (2e- each)

20
Q

f subshell

A
  • starts at n=4

* Each subshell has 7f orbitals

21
Q

Rules for electron configuration

A

1) Each orbital can hold max 2 e- (Pauli)
2) Orbitals are occupied in order of increasing energy (Aufbau)
3) When more than one orbital of same energy available, orbitals are first occupied single (Hund’s rule)

22
Q

Trends in successive IE; consider:

A
  • Is the electron being removed from a new quantum shell –> harder
  • If the electron spin-paired with another e- in the same orbital –> they will still repel, it will be easier to remove 1 e- than expected
23
Q

Most energetically stable electron configuration:

A
  • Most energetically stable = full subshells, all electrons spin paired
  • Next most stable = half full shells (occupied singly with electron spins aligned)
24
Q

In what state can atoms be ionised?

A

Gaseous