1chemistry 2c lecture 6: april 12 th, 2006 lecture 6:transition metals corrosion- unwanted oxidation...
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1Chemistry 2C Lecture 6: April 12th, 2006
Lecture 6:Transition Metals
• Corrosion- unwanted oxidation of material (e.g. rust with Fe)
• Cathodic Protection (sacrificial metals)• Electrolysis (of water)
• Electroplating
I. MetallurgyII. Electronic Configuration
III. Transition Metal properties
2Chemistry 2C Lecture 6: April 12th, 2006
Metallurgy
In chapter 24, we will ignore metallurgy (24.2 & 24.3). Read it for fun as they deal with how metals are extracted from their natural
sources. But, let’s talk about occurrence of metal in a general sense.
Almost all metals are founded in combined form in nature. If not, we say they are in the “native form.” Au, Ag, and Pt are the main ones otherwise, the metals are found in minerals (usually oxides, sulfides
or silicates).
Hematite: Fe2O3 Galena: PbS Sphalerite: ZnS
http://mineral.galleries.com/minerals/
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Ores refer to concentrated deposits that have commercial value
Recovering metals from these ores is the science of metallurgy and involve several steps, specific to the metal that you are extracting, the purity of the product or whether an alloy is
produced
Manganese Ore Lead Ore Gold Ore
Metallurgy
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Alloys are metallic materials containing two or more metals
Alloys are usually designed to have properties that are more desirable than those of their components. For instance, steel is
stronger than iron, one of its main elements.
An amalgam is any alloy of mercury. Most metals are soluble in mercury, but some (such as iron) are not. Amalgams are commonly used in dental
fillings.
Dental fillings: Ag/Sn/Cu/Hg
14 Carat Gold: Cu/Au
24 Carat Gold: Pure Au, but too soft for rings and other jewelry
Metallurgy
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Transition Metals Facts
Many of the most important metals in modern society are the transition metals
In the periodic table, they comprise of more
than half of the elements.
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Transition Metals FactsWhere are they:
The s block elements - Groups 1 & 2 (1A-2A)The p block elements- Groups 13-18 (3A-
8A)The d block elements - Groups 3-12 (3B-1B)The f block elements
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Transition Metals Facts
Electronic configurations for noble gases
[He] 1s2
[Ne] 1s2 2s2 2p6
[Ar] 1s2 2s2 2p6 3s2 3p6
In multi-electron atoms (not Hydrogenic atoms), the orbital energies are like this
(qualitative)
1s
2s
2p 2p 2p
3s
3p 3p 3p
4s
3d 3d 3d
Energ
y
3d3d
4p 4p 4p
Each box is an orbital (can hold 2 e-)
Within each sub-shell, the orbitals are degenerate (same energy)
•The three p oribals are degenerate•The five d-orbiatal are degenerate
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Transition Metals Facts
n, l, ml, ms
n Principle quantum number
l angular momentum QNml magnetic QNms spin QN
Recall the Pauli exclusion principle:No two electrons in an atom can have the same set of four quantum
numbers
3d 3d 3d 3d3d
For the 3d orbitalsn=3l=2
ml= -2, -1, 0, 1, 2Ms= ½ or -½
Orbitals can hold a max of 2 electrons and they must be of opposite spin: So there are 2x5 elements for each row of
d-block Transition metals
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Electronic configurationAfter Ar, things get more interesting, complex, and even cool!
Can simplify the electronic configuration by using the configuration of the closest noble gas configuration (e.g. Ar)
[Ar]: 1s2 2s2 2p6 3s2 3p6
[K]: 1s2 2s2 2p6 3s2 3p6 4s1
[Ca]: 1s2 2s2 2p6 3s2 3p6 4s2
Now we start to fill in the d-orbitals
[Sc]: 1s2 2s2 2p6 3s2 3p6 4s2 3d1
d-oribitals
[Sc]: [Ar] 4s2 3d1
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Electronic configurationOrbitals are filled according to Hund’s rule – unpaired electrons first before
putting two electrons in a single orbital
[Mn]: [Ar] 4s2 3d5 ↑↓
↑ ↑ ↑ ↑↑
4s 3sAll five d electrons are unpaired and occupy separate orbitals
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Electronic configurationOrbitals are filled according to Hund’s rule – unpaired electrons first before
putting two electrons in a single orbital
[Co]: [Ar] 4s2 3d7 ↑↓
↑↓
↑ ↑ ↑↑↓
4s 3s
Now two d-oribtals are occupied with two electrons (ms= ½ and ms= -½)
12Chemistry 2C Lecture 6: April 12th, 2006
Electronic configurationAfter the d orbitals are filled, the 4p orbitsal will start to be filled starting
with Ga and continuing until Kr
[Kr]: [Ar] 4s2 3d10 4p6 ↑↓
↑↓
↑↓
↑↓
↑↓
↑↓
4s 3s
The same pattern occurs in the next row, so that the 5s is filled before 4d, which is
then filled before 5p
↑↓
↑↓
↑↓
4p
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Rare Earth Transition Metals
After the 6s, there is a break and the then start to fill the 4f orbitals
Lanthanide Elements
Actinide Elements
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Rare Earth Transition Metals
The 4f and the 5d energies are close, so there is some mixing with the d-block metals, but mostly the order is: 6s, 4f, 5d, 6p
[La]: [Xe] 6s2 5d1
[Ce]: [Xe] 6s2 4f2
Table D in the text book (pg. A17)
The first two lanthanides
Actinides: Rare and radioactive and will be discussed later
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Transition Metals
So, the transition elements” term refers to the d-block and also the f-block elements. The name also refers to their intermediate properties between
the very reactive s-block and less reactive p-block metals
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Transition Metals PropertiesTransition metals are all metals which means:1) Clean metallic surface has a characteristic luster
2) Conduct heat well (flow of thermal energy)3) Conduct electricity (flow of electrons)
4) Most are malleable (can be hammered)5) Most are ductile (can be drawn in a wire
Most TS have high melting points except Zn, Cd, Hg (weaker metallic bonding)
e.g. V, 1917◦Ce.g. Zn, 420◦C
Atomic radius (result from the combination of several factors)1) As nuclear charge ↑ and electrons ↑, the effective nuclear charge
exerts a greater pull on the valence electrons and they are pulled in close; thus atomic radii decrease in going from Left to Right in a row
2) However, electrons in the d-subshell tend to experience repulsive effects and expand the radius
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Transition Metals Radii
21 [Sc] [Ar] 4s2 3d1 161 pm
22 [Ti] [Ar] 4s2 3d2 145 pm23 [V] [Ar] 4s2 3d3 132 pm24 [Cr] [Ar] 4s1 3d5 125 pm25 [Mn] [Ar] 4s2 3d5 124 pm26 [Fe] [Ar] 4s2 3d6 124 pm27 [Co] [Ar] 4s2 3d7 125 pm28 [Ni] [Ar] 4s2 3d8 125 pm29 [Cu] [Ar] 4s1 3d10 128 pm30 [Zn] [Ar] 4s2 3d10 133 pm
Z (nuclear charge) Metals Electronic ConfigurationMetallic Radius
100 pm=1Å
Special stability of half filled shells results in extra energy required to
pair electrons