electrons and ionisation energy

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23 Terms

1
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what are shells made up of?

atomic orbitals - region around the nucleus that holds up 2e- with opposite spins

2
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types of atomic orbitals

s, p, d, f

3
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s-orbital

  • electron cloud of a sphere

  • can hold up to 2 e-

  • greater the shell number, greater radius of s-orbital

<ul><li><p>electron cloud of a sphere</p></li><li><p>can hold up to 2 e-</p></li><li><p>greater the shell number, greater radius of s-orbital</p></li></ul><p></p>
4
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p-orbitals

  • electron cloud shape of dumb-bell

  • one orbital can hold up 2e-

  • the subshells (px, py, pz) hold 6e-

  • greater shell no. the further the p-orbital is from the nucleus

<ul><li><p>electron cloud shape of dumb-bell</p></li><li><p>one orbital can hold up 2e-</p></li><li><p>the subshells (px, py, pz) hold 6e-</p></li><li><p>greater shell no. the further the p-orbital is from the nucleus</p></li></ul><p></p>
5
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aufbau principle

electrons fill the lowest energy orbitals first before moving to higher ones

6
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pauli exclusion principle

an orbital can hold a maximum of 2e- and must have opposite spins

7
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hunds rule

electrons fill orbitals of equal energy singly first before pairing up

8
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how many electrons can each orbital hold

s → 2

p → 6

d → 10

f → 14

9
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ionisation energy

how easily an e- loses to form positive ions

10
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first ionisation energy

the energy required to remove one e- from each atom in one mole of a gaseous atom of an element to form one mole of gaseous 1+ ions

11
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units of ionisation energy

kJ mol⁻¹

12
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What are the main factors affecting ionisation energy?

  1. Nuclear charge (number of protons)

  2. Distance of outer electron from nucleus

  3. Electron shielding

  4. Electron–electron repulsion (sub-shell effects)

13
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What is meant by successive ionisation energies?

The energies required to remove each electron in turn from the same atom.

14
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Why is the 2nd ionisation energy always higher than the 1st?

Because the electron is removed from a positive ion, so there’s greater attraction between the nucleus and remaining electrons.

15
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What happens to ionisation energy across a period (e.g. Na → Ar)?

increases overall

16
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Why does ionisation energy increase across a period?

  • Nuclear charge increases (more protons)

  • Same shielding

  • Electrons closer to nucleus (atomic radius decreases)
    → Stronger attraction → more energy needed to remove an electron.

17
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What are the exceptions to the trend in ionisation energy across Period 2?

  • Boron (B) has lower IE than Be → electron removed from 2p, higher energy sub-shell.

  • Oxygen (O) has lower IE than N → due to paired electrons in 2p orbital causing extra repulsion.

18
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What causes a drop in ionisation energy between Be → B and N → O?

  • Be → B: change from 2s → 2p, higher energy, easier to remove.

  • N → O: electron pairing in p orbital increases repulsion.

19
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What happens to ionisation energy down a group?

decreases

20
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Why does ionisation energy decrease down a group?

  • More electron shells → increased shielding

  • Outer electrons further from nucleus

  • Attraction weaker, despite increased nuclear charge.

21
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Which factor has the greatest influence down a group?

Increased distance and shielding outweigh increased nuclear charge.

22
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What does a large jump in successive ionisation energies show?

A change of shell — the electron is now being removed from a closer, more strongly attracted shell.

23
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How can successive ionisation energies identify an element?

The pattern shows how many electrons are in the outer shell (e.g., a big jump after 3 electrons → element is in Group 3).