Topic 1 Flashcards

(42 cards)

1
Q

Occupied shells tells us

A

Period number

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2
Q

Valence shell tells us the

A

Group number

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3
Q

Emission spectra and the atom

A

When element is heated, electrons absorb energy and promoted to higher energy state (excited state)
When element relapses from excited to lower energy state (ground state), energy is released as electromagnetic radiation which we see as colour

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4
Q

Bohr model

A

Electron in given orbit has constant energy
Electrons can only occupy fixed energy levels and not exist between two levels
Orbits of larger radii (further away from nucleus) means more energy

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5
Q

How many electrons can a sub shell hold

A

2 in each orbital

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6
Q

Orbital

A

Region of space in which up to two electrons are likely to be located

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7
Q

How many electrons can p is shell hold

A

6

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8
Q

How many electrons can d sub shell hold

A

10

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9
Q

How many electrons can you hold in each orbital

A

2

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10
Q

Sub shell definition

A

A specific energy level within an electron shell

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11
Q

Order of increasing energy subshell

A

S, p, d, f

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12
Q

Pauli exclusion principle

A

States only a maximum of two electrons may be found in a given atomic orbital and if an orbital is filled, electrons will have opposite spin

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13
Q

Aufbau principle

A

States subshells are filled in order form lowest energy to highest energy and a lower energy subshell will be completely filled before electrons move into a higher energy shell

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14
Q

Hunds rule

A

States electrons in a partially filled subshell will arrange themselves so as to form the maximum number of half filled orbitals

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15
Q

Difference between atom in its ground state and atom in excited state

A

Atom in ground state has all electrons in lowest possible subshells whereas an atom in an excited state temporary has one or more electrons in higher energy subshell than the lowest possible

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16
Q

Actual configuration copper

A

1s2 2s2 2p6 3s2 3p6 4s1 3d10

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17
Q

Actual configuration chromium

A

1s2 2s2 2p6 3s2 3p6 4s1 3d5

18
Q

Trends in atomic radius-> things need to talk about

A

-core charge
- number of occupied energy levels

19
Q

Core charge

A

Measure of the net attractive force felt by valence shell electrons towards nucleus

20
Q

Core charge calculation

A

Number of protons- number of electrons in inner shells

21
Q

Trends in atomic radii down a group

A

Atomic radius increases

22
Q

Why does atomic radius increase down a group

A
  • number of occupied energy levels increases
  • core charge remains constant
23
Q

Sodium and potassium which is bigger

A

Both in g1- both have constant core charge of 1+
Sodium has 3 occupied shells whereas potassium has 4 occupied shells t/f potassium is larger

24
Q

Trends in atomic radii across a period

A

Atomic radius decreases

25
Why does atomic radius decrease across a period
Number of occupied energy levels remains constant Core charge increases-> valence electrons more strongly attracted to nucleus
26
Electronegativity definition
Strength with which atoms of an element attract electrons when chemically combined with another element
27
What does a higher electronegativity mean
Atoms are more able to pull shared electrons in covalent bond towards their nucleus
28
Electronegativity will be higher when
Atomic radius is low Core charge is high
29
Trend in electronegativity down a group
Electronegativity decreases
30
Why does electronegativity decrease down a group
Number of occupied energy shells increase-> atomic radius increases Nuclear charge and electron shielding increases Overall means outermost electron is further from the nucleus and there are more electrons between an atoms nucleus and outermost electron meaning outermost electrins are less attracted towards nucleus
31
Trend in electronegativity across a period
Electronegativity increases
32
Why does electronegativity increase across a period
Number of occupied energy shells= constant Core charge increases + Atomic radius decreases Nuclear charge increases + electron shielding= constant T/f due to inc. core charge, valence electrons more strongly attracted to nucleus t/f inc. electronegativity
33
Ionisation energy
Amount of energy required to remove an electron from each mole of gaseous atoms
34
Factors that affect ionisation energy
As electrons are neg. Charged and protons= positively charged, there is an attraction between electrons and protons. Greater the pull of the nucleus, harder it is to pull an electron away from an atom
35
As you move down a group, what happens to first ionisation energy and why
First ionisation energy decreases B/c - number of occupied energy shells increases so atomic radius increases and t/f nuclear attractions decrease - electron shielding increases and core charge= constant T/f less energy required to remove an electron
36
As you move across a period, what happens to first ionisation energy and why
Increases b/c Number of occupied energy shells= constant and atomic radius decreases t/f outermost electrons closer to nucleus Core charge inc.-> outermost electrons more strongly attracted to nucleus T/f more energy required to remove and electron
37
Electrons with low ionisation energies generally have low/high electronegativity and why
Low electronegativity b/c nuclei not exert strong attractive force on e
38
Electrons with high ionisation energies have low/high electronegativity and why
High electronegativity b.c of strong pull exerted by on electrons
39
Reactivity of metals: trends across a period
-core charge increases as we move across a period - electron shielding remains constant T/f increase energy required to remove an electron (inc. first ionisation energy) T/f reactivity of metals decreases across a period
40
Reactivity of metals down a group
Core charge stays the same Number of energy levels and electron shielding increases-> decreases energy required to remove an electron T/f Dec. reactivity of metals
41
Reactivity of non metals
Non metals with greatest attractive force will be most reactive Reactivity increases across a period Decreases down a group
42
RAM calculation
(Relative abundance x relative isotopic mass 1) + (relative abundance x relative isotopic mass 2)/100