The how and why
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Transcript of The how and why
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The how and whyThe how and why
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History Russian scientist Dmitri MendeleevDmitri Mendeleev
taught chemistry in terms of properties.
Mid 1800 - molar masses of elements were known.
Wrote down the elements in order of increasing mass.
Found a pattern of repeating properties.
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Mendeleev’s Table Grouped elements in columns by similar
properties in order of increasing atomic mass.
Found some inconsistencies - felt that the properties were more important than the mass, so switched order.
Found some gaps. Must be undiscovered elements. Predicted their properties before they
were found.
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The modern table Elements are still grouped by
properties. Similar properties are in the same
column. Order is in increasing atomic number. Added a column of elements Mendeleev
didn’t know about. The noble gases weren’t found because
they didn’t react with anything.
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Horizontal rows are called Periods There are 7 periods
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Vertical columns are called Groups.
Elements are placed in columns by similar properties.
Also called families
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1A
2A 3A 4A 5A 6A7A
8A0
The elements in the A groups are called the representative elements
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The group B are called the transition elements
These are called the inner transition elements and they belong here
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Group 1A are the alkali metals Group 2A are the alkaline earth metals
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Group 7A is called the Halogens Group 8A are the noble gases
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Why? The part of the atom another atom
sees is the electron cloud. More importantly the outside
orbitals. The orbitals fill up in a regular
pattern. The outside orbital electron
configuration repeats. The properties of atoms repeat.
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1s1
1s22s1
1s22s22p63s1
1s22s22p63s23p64s1
1s22s22p63s23p64s23d104p65s1
1s22s22p63s23p64s23d104p65s24d10 5p66s1
1s22s22p63s23p64s23d104p65s24d105p66s2
4f145d106p67s1
H1
Li3
Na11
K19
Rb37
Cs55
Fr87
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He2
Ne10
Ar18
Kr36
Xe54
Rn86
1s2
1s22s22p6
1s22s22p63s23p6
1s22s22p63s23p64s23d104p6
1s22s22p63s23p64s23d104p65s24d105p6
1s22s22p63s23p64s23d104p65s24d10
5p66s24f145d106p6
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Alkali metals all end in s1
Alkaline earth metals all end in s2
really have to include He but it fits better later.
He has the properties of the noble gases.
s2s1 S- block
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Transition Metals -d block
d1 d2 d3 d5 d5 d6 d7 d8 d9 d10
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The P-block p1 p2 p3 p4 p5 p6
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F - block inner transition elements
f1 f5f2 f3 f4
f6 f7 f8 f9 f10 f11 f12 f14
f13
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Each row (or period) is the energy level for s and p orbitals.
1
2
3
4
5
6
7
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D orbitals fill up after previous energy level so first d is 3d even though it’s in row 4.
1
2
3
4
5
6
7
3d
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f orbitals start filling at 4f
1
2
3
4
5
6
7 4f
5f
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Writing Electron configurations the easy way
Yes there is a shorthandYes there is a shorthand
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Electron Configurations repeat The shape of the periodic table is a
representation of this repetition. When we get to the end of the
column the outermost energy level is full.
This is the basis for our shorthand.
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The Shorthand Write the symbol of the noble gas
before the element. Then the rest of the electrons. Aluminum - full configuration. 1s22s22p63s23p1
Ne is 1s22s22p6
so Al is [Ne] 3s23p1
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More examples Ge = 1s22s22p63s23p64s23d104p2
Ge = [Ar] 4s23d104p2
Hf=1s22s22p63s23p64s23d104p65s2
4d105p66s24f145d2
Hf=[Xe]6s24f145d2
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The Shorthand Again
Sn- 50 electrons
The noble gas before it is Kr
[ Kr ]
Takes care of 36
Next 5s2
5s2
Then 4d10
4d10Finally 5p2
5p2
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Atomic Size First problem where do you start
measuring. The electron cloud doesn’t have a
definite edge. They get around this by measuring
more than 1 atom at a time.
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Atomic Size
Atomic Radius = half the distance between two nuclei of a diatomic molecule.
}Radius
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Trends in Atomic Size Influenced by two factors. Energy Level Higher energy level - electrons
are further away from nucleus. Charge on nucleus More charge (# of protons) pulls
electrons in closer.
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Group trends As we go down a
group Each atom has
another energy level,
So the atoms get bigger.
HLi
Na
K
Rb
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Periodic Trends As you go across a period the radius
gets smaller. Same energy level. More nuclear charge = more protons. Outermost electrons are closer.
Na Mg Al Si P S Cl Ar
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Overall
Atomic Number
Ato
mic
Rad
ius
(nm
)
H
Li
Ne
Ar
10
Na
K
Kr
Rb
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Ionization Energy The amount of energy required to
completely remove an electron from a gaseous atom.
Removing one electron makes a +1 ion.
The energy required is called the first ionization energy.
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Ionization Energy The second ionization energy is the
energy required to remove the second electron.
Always greater than first IE. The third IE is the energy required to
remove a third electron. Greater than 1st of 2nd IE.
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Symbol First Second ThirdHHeLiBeBCNO F Ne
1312 2731 520 900 800 1086 1402 1314 1681 2080
5247 7297 1757 2430 2352 2857 3391 3375 3963
11810 14840 3569 4619 4577 5301 6045 6276
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Symbol First Second ThirdHHeLiBeBCNO F Ne
1312 2731 520 900 800 1086 1402 1314 1681 2080
5247 7297 1757 2430 2352 2857 3391 3375 3963
11810 14840 3569 4619 4577 5301 6045 6276
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What determines IE The greater the nuclear charge the
greater IE. Distance form nucleus increases IE Filled and half filled orbitals have
lower energy, so achieving them is easier, lower IE.
Shielding
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Shielding The electron on the
outside energy level has to look through all the other energy levels to see the nucleus
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Shielding The electron on the
outside energy level has to look through all the other energy levels to see the nucleus.
A second electron has the same shielding.
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Group trends As you go down a group first IE
decreases because The electron is further away. More shielding.
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Periodic trends All the atoms in the same period
have the same energy level. Same shielding. Increasing nuclear charge So IE generally increases from left to
right. Exceptions at full and 1/2 fill orbitals.
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Firs
t Ion
izat
ion
ener
gy
Atomic number
He
He has a greater IE than H.
same shielding greater nuclear
charge
H
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Firs
t Ion
izat
ion
ener
gy
Atomic number
H
He
Li has lower IE than H
more shielding further away outweighs greater
nuclear charge
Li
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Firs
t Ion
izat
ion
ener
gy
Atomic number
H
He
Be has higher IE than Li
same shielding greater nuclear
charge
Li
Be
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Firs
t Ion
izat
ion
ener
gy
Atomic number
H
He B has lower IE than
Be same shielding greater nuclear
charge By removing an
electron we make s orbital half filled Li
Be
B
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Firs
t Ion
izat
ion
ener
gy
Atomic number
H
He
Li
Be
B
C
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Firs
t Ion
izat
ion
ener
gy
Atomic number
H
He
Li
Be
B
C
N
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Firs
t Ion
izat
ion
ener
gy
Atomic number
H
He
Li
Be
B
C
N
O
Breaks the pattern because removing an electron gets to 1/2 filled p orbital
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Firs
t Ion
izat
ion
ener
gy
Atomic number
H
He
Li
Be
B
C
N
O
F
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Firs
t Ion
izat
ion
ener
gy
Atomic number
H
He
Li
Be
B
C
N
O
F
Ne Ne has a lower
IE than He Both are full, Ne has more
shielding Greater distance
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Firs
t Ion
izat
ion
ener
gy
Atomic number
H
He
Li
Be
B
C
N
O
F
Ne Na has a lower
IE than Li Both are s1
Na has more shielding
Greater distance
Na
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Firs
t Ion
izat
ion
ener
gy
Atomic number
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Electron Affinity The energy change assciated with
adding an electron to a gaseous atom.
Easiest to add to group 7A. Gets them to full energy level. Increase from left to right atoms
become smaller, with greater nuclear charge.
Decrease as we go down a group.
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Ionic Size Cations form by losing electrons. Cations are smaller that the atom
they come from. Metals form cations. Cations of representative elements
have noble gas configuration.
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Ionic size Anions form by gaining electrons. Anions are bigger that the atom they
come from. Nonmetals form anions. Anions of representative elements
have noble gas configuration.
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Configuration of Ions Ions always have noble gas
configuration. Na is 1s12s22p63s1 Forms a +1 ion - 1s12s22p6 Same configuration as neon. Metals form ions with the
configuration of the noble gas before them - they lose electrons.
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Configuration of Ions Non-metals form ions by gaining
electrons to achieve noble gas configuration.
They end up with the configuration of the noble gas after them.
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Group trends Adding energy level Ions get bigger as
you go down.
Li+1
Na+1
K+1
Rb+1
Cs+1
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Periodic Trends Across the period nuclear charge
increases so they get smaller. Energy level changes between
anions and cations.
Li+1
Be+2
B+3
C+4
N-3O-2 F-1
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Size of Isoelectronic ions Iso - same Iso electronic ions have the same #
of electrons Al+3 Mg+2 Na+1 Ne F-1 O-2 and N-3 all have 10 electrons all have the configuration 1s12s22p6
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Size of Isoelectronic ions Positvie ions have more protons so
they are smaller.
Al+3
Mg+2
Na+1 Ne F-1 O-2 N-3
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Electronegativity
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Electronegativity The tendency for an atom to attract
electrons to itself when it is chemically combined with another element.
How fair it shares. Big electronegativity means it pulls
the electron toward it. Atoms with large negative electron
affinity have larger electronegativity.
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Group Trend The further down a group the farther
the electron is away and the more electrons an atom has.
More willing to share. Low electronegativity.
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Periodic Trend Metals are at the left end. They let their electrons go easily Low electronegativity At the right end are the nonmetals. They want more electrons. Try to take them away. High electronegativity.
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Ionization energy, electronegativity
Electron affinity INCREASE
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Atomic size increases, shielding constant
Ionic size increases