The Periodic Table
Jan 25, 2016
The Periodic Table
Periodic Table
Dmitri Mendeleev (1834-1907)
"We could live at the present day without a Plato, but a double number of Newtons is required to discover the secrets of nature, and to bring life into harmony with the laws of nature."
Modern Periodic Table
s- and p-orbitals
‘Aufbau’ Principle: filling orbitals
1s 2s 2p
n = 1l = 0
ml = 0
n = 2l = 0
ml = 0
n = 2l = 0
ml = 0 ml = 1ml = -1
H: 1s1
s- and p-orbitals
‘Aufbau’ Principle: filling orbitals
1s 2s 2p
n = 1l = 0
ml = 0
n = 2l = 0
ml = 0
n = 2l = 0
ml = 0 ml = 1ml = -1
He: 1s2
s- and p-orbitals
‘Aufbau’ Principle: filling orbitals
1s 2s 2p
n = 1l = 0
ml = 0
n = 2l = 0
ml = 0
n = 2l = 0
ml = 0 ml = 1ml = -1
Li: 1s2 2s1
s- and p-orbitals
‘Aufbau’ Principle: filling orbitals
1s 2s 2p
n = 1l = 0
ml = 0
n = 2l = 0
ml = 0
n = 2l = 0
ml = 0 ml = 1ml = -1
Be: 1s2 2s2
s- and p-orbitals
‘Aufbau’ Principle: filling orbitals
1s 2s 2p
B: 1s2 2s22p1
‘core’closed shell open shell: valence electrons
s- and p-orbitals
‘Aufbau’ Principle: filling orbitals
Hund’s rule: maximum number of unpaired electrons is the lowest energy arrangement.
1s 2s 2p
C: 1s2 2s22p2
s- and p-orbitals
‘Aufbau’ Principle: filling orbitals
1s 2s 2p
N: 1s2 2s22p3
O: 1s2 2s22p4
s- and p-orbitals
‘Aufbau’ Principle: filling orbitals
1s 2s 2p
F: 1s2 2s22p5
Ne: 1s2 2s22p6
s- and p-orbitals
‘Aufbau’ Principle: filling orbitals
Na: 1s22s22p63s1 or [Ne]3s1
Mg: 1s22s22p63s2 or [Ne]3s2
P: [Ne]3s23p3
Ar: [Ne]3s23p6
d-orbitals
E
1s
2s
3s
4s
2p
3p
3d
Due to deeper penetration of s-orbitals, 4s lies lower in energy than 3d
d-orbitals
K: 1s22s22p63s23p64s1 or [Ar]4s1
Ca: [Ar]4s2
Sc: [Ar]4s23d1
V: [Ar]4s23d3
Cr: [Ar]4s13d5
Co: [Ar]4s23d7
Cu: [Ar]4s13d10
Zn: [Ar]4s23d10
Ga: [Ar]4s23d104p1
Kr: [Ar]4s23d104p6
Beyond the d-orbitals
lanthanides
actinides
‘s’-groups ‘p’-groups
d-transition elements
f-transition elements
Aufbau rules
1. Within a shell (n) the filling order is s>p>d>f
2. Within a subshell (l), lowest energy arrangement has the highest number of unpaired spin (Hund’s rule)
3. The (n+1)s orbitals always fill before the nd orbitals
4. After lanthanum ([Xe]6s25d1), the 4f orbitals are filled
5. After actinium ([Rn]7s26d1), the 5f orbitals are filled
Filled subshells accommodate:
s: 2 electronsp: 6 electrons
d: 10 electronsf: 14 electrons
Electron configuration
Give the electron configuration of Zirconium and Tellurium.
Identify the period and the group of the element
Zirconium is in period 5 and is the 2nd element in the d-transition element group.
Zr: 1s22s22p63s23p64s23d104p65s24d2 or [Kr]5s24d2
Tellurium is in period 5 and is the 4th element in the ‘p’- group.
Te: 1s22s22p63s23p64s23d104p65s24d105p4 or [Kr]5s24d105p4
Exotic elementsElements with atomic numbers higher than 92 (Uranium) typically don’t exist in nature and have to be made by nuclear synthesis
The first synthesized elements were named after the planets:
uraniumneptunium
plutonium
Ur92
Np93
Pu94
Exotic elements
Md
101Mendelevium
Es
99Einsteinium
Bh
107BohriumLives for only 10 ms!
Uun
110
No name yet! Barbarium?
Atomic Radius
The atomic radius r is usually determined from the distances between atoms in covalent bonds.
How big is an atom?
Atomic radius decreases across a period from left to right due to increased effective nuclear charge
Atomic radius increases down a group because of the larger sizes of the orbitals with higher quantum numbers.
Atomic Radius
Atomic Radius
Atomic Radius
Covalent radius is much smaller than the anionic radius.
Atomic RadiusArrange the following sets of atoms in order of increasing size:
Sr, Se, Ne :
Fe, P, O :
Ne(10) < Se(34) < Sr(38)
O(8) < P(15) < Fe(26)
Li+(3) < Na+(11) < Rb+(37)
Arrange the following sets of ions in order of increasing size:
Na+, Rb+, Li+ :
Cl-, F-, I- : F-(9) < Cl-(17) < I-(53)
Ionization Energy
Ionization energy is the energy required to remove an electron from a gaseous atom or ion :
e-
+
X(g) X+(g) + e-
S(g) S+(g) + e- I1 = 999.6 kJ/mol 1st ionization energy
S+(g) S2+(g) + e- I2 = 2251 kJ/mol 2nd ionization energy
S2+(g) S3+(g) + e- I3 = 3361 kJ/mol 3rd ionization energy
Ionization EnergyS(g) S+(g) + e- I1 = 999.6 kJ/mol 1st ionization energy
S+(g) S2+(g) + e- I2 = 2251 kJ/mol 2nd ionization energy
S2+(g) S3+(g) + e- I3 = 3361 kJ/mol 3rd ionization energy
S: 1s22s22p63s23p4
Which electrons are removed in successive ionizations?
Electrons in the outer subshells take the least amount of energy to remove (valence electrons)
It takes about 1•103 kJ/mol to remove successive electrons from the 3p shell of sulfur.
Ionization EnergyIonization energies of aluminum:
Al(g) Al+(g) + e- I1 = 580 kJ/mol 1st ionization energy
Al+(g) Al2+(g) + e- I2 = 1815 kJ/mol 2nd ionization energy
Al2+(g) Al3+(g) + e- I3 = 2750 kJ/mol 3rd ionization energy
Al3+(g) Al4+(g) + e- I4 = 11,600 kJ/mol 4th ionization energy
Al: 1s22s22p63s23p1
1st electron: 3p valence electron
2nd electron: 3s valence electron
3rd electron: 3s valence electron
4th electron: 2p core electron!core electrons take much more energy to remove
Ionization Energy
Ionization EnergyFirst ionization energies
Ionization energy increases across the period from left to right.
Ionization energy decreases going down a group
General trends:
Ionization EnergyA closer look…..
B: 1s22s22p1
O: 1s22s22p4
New subshell, electron is easier to remove.
First paired electron in 2p orbital: repulsion.
Understanding a groupAtoms in a group have the same valence electron configuration and share many similarities in their chemistry.
Group 1A: Alkali metals
KNaLi
Cs
Understanding a group
Trends down the group reflect periodic changes in mass, volume and charge.
Group 1A: Alkali metals
Periodic Table in Brief
Periodic Table Redux
Periodic Table Redux