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Prentice-Hall © 2002General Chemistry: Chapter 2Slide 1 of 25
Chapter 2: Atoms and the Atomic Theory
Philip DuttonUniversity of Windsor, Canada
Prentice-Hall © 2002
General ChemistryPrinciples and Modern Applications
Petrucci • Harwood • Herring
8th Edition
Prentice-Hall © 2002General Chemistry: Chapter 2Slide 2 of 25
Contents
• Early chemical discoveries • Electrons and the Nuclear Atom• Chemical Elements• Atomic Masses• The Mole
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Early Discoveries
Lavoisier 1774Law of conservation of mass
Proust 1799 Law of constant composition
Dalton 1803-1888 Atomic Theory
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Dalton’s Atomic Theory
Each element is composed of small particles called atoms.
Atoms are neither created nor destroyed in chemical reactions.
All atoms of a given element are identical
Compounds are formed when atoms of more than one element
combine
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Consequences of Dalton’s theory
In forming carbon monoxide, 1.33 g of oxygen combines with 1.0 g of carbon.
In the formation of carbon dioxide 2.66 g of oxygen combines with 1.0 g of carbon.
Law of Definite Proportions: combinations of elements are in ratios of small whole numbers.
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Behavior of charges
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Cathode ray tube
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Properties of cathode rays
Electron m/e = -5.6857 x 10-9 g coulomb-1
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Charge on the electron
From 1906-1914 Robert Millikan showed ionized oil drops can be balanced against the pull of gravity by an electric field.
The charge is an integral multiple of the electronic charge, e.
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Radioactivity
Radioactivity is the spontaneous emission of radiation from a substance.
X-rays and g-rays are high-energy light.
a-particles are a stream of helium nuclei, He2+.
b-particles are a stream of high speed electrons
that originate in the nucleus.
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The nuclear atom
Geiger and Rutherford1909
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The a-particle experiment
Most of the mass and all of the positive charge is concentrated in a small region called the nucleus .
There are as many electrons outside
the nucleus as there are units of positive charge on the nucleus
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The nuclear atom
Rutherfordprotons 1919
James Chadwickneutrons 1932
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Scale of Atoms
Useful units:
1 amu (atomic mass unit) = 1.66054 x 10-27 kg 1 pm (picometer) = 1 x 10-12 m 1 Å (Angstrom) = 1 x 10-10 m = 100 pm = 1 x 10-8 cm
The heaviest atom has a mass of only 4.8 x 10-22 g
and a diameter of only 5 x 10-10 m.
Biggest atom is 240 amu and is 50 Å across.
Typical C-C bond length 154 pm (1.54 Å)
Molecular models are 1 Å /inch or about 0.4 Å /cm
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Atomic Diameter 10-8 cm Nuclear diameter 10-13 cm
Nuclear Structure
Particle Mass Chargekg amu Coulombs (e)
Electron 9.109 x 10-31 0.000548 –1.602 x 10-19 –1Proton 1.673 x 10-27 1.0073 +1.602 x 10-19 +1Neutron 1.675 x 10-27 1.0087 0 0
1 Å
The nuclei of most atoms consist of protons and neutrons, which are called the nucleons.
Atomic number: the number of protons defines the type of the element.
The number of neutrons determines the isotope of an element.
The stability of the neutron
• In the stable nuclei the bound neutrons are stable.
• The free neutrons are unstable; they undergo beta decay with a half-life of just about 10.2 minutes (614 s). Quark structure: Feynmann diagram:
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Half life of the decaying free neutron
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0 10 20 30 40 50 600
25
50
75
100
t [min]
N
Half-life: t ½ = 10.2 min
2/1
21
)0()(t
t
NtN
n0 → p+ + e− + ūe
Free neutrons decay by emission of an electron and an electron antineutrino to become a proton, a process known as beta decay:
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Energy – mass conversion
Einstein (1905): E = mc2
• All energy changes are accompanied by mass changes (Δm)– In chemical reactions ΔE is too small to notice:
Δm < 0.0000001 u (negligible). – In nuclear reactions ΔE > 1.1 MeV/nucleon.
1 MeV = 1.6022x10-13 J
If ΔE =1.4924x10-10 J or 931.5 MeV then Δm = 1.0 u
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Nuclear Binding Energy
Total mass defect
Positive binding energy:
0.0304 x 931.5 = 28.4 MeV
Per nucleon:
28.4 / 4 = 7.1 MeV/nucleon
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Isotopes, atomic numbers and mass numbers
To represent a particular atom we use the symbolism:
A= mass number Z = atomic number
Isotopes of an element
• Isotopes are different types of atoms (nuclides) of the same chemical element, Z, each having a different atomic mass (A: mass number)
• Same number of protons, but different number of neutrons.
• About 339 nuclides occur naturally on Earth, of which 256 (~75%) are stable. 3100 are known currently
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Az anyag22
The isotopes of the hydrogen2H=D1
3H=T1
1H=H1
(t1/2) : 12.33 years
Mass defect of the isotopes vs. energy
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Z A Atomic mass Mass defect MeV/nucleon
H 1 1 1.00783 [amu]D 1 2 2.01410 0.00239 1.11T 1 3 3.01605 0.00911 2.83He 2 3 3.01603 0.00829 2.57
2 4 4.00260 0.03038 7.07Li 3 6 6.01512 0.03435 5.33
3 7 7.01600 0.04213 5.61Be 4 9 9.01218 0.06244 6.46B 5 10 10.01294 0.06951 6.47
5 11 11.00931 0.08181 6.93C 6 12 12.00000 0.09894 7.68
6 13 13.00335 0.10425 7.476 14 14.00324 0.11303 7.52
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Average Binding Energy as a Function of Mass Number
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Neutron-to-Proton Ratio (Segré diagram)
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Measuring atomic masses
The relative atomic mass
• Unit: rest mass of carbon-12 is exactly12.• It is the mean of the atomic masses over all
the isotopes of the element weighted by isotopic abundance as found in a particular environment (standard: the earth crust).
• This number may be a fraction which is not close to a whole number, due to the averaging process.
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Isotopic abundance in the earth crust
Az anyagKészítette: Dr. Csonka Gábor egyetemi tanár, [email protected]
28
Z A Atomic mass abundance% t1/2
H 1 1 1.00783 99.9885D 1 2 2.01410 0.0115T 1 3 3.01605 12.33 yHe 2 3 3.01603
2 4 4.00260 99.9999Li 3 6 6.01512 7.59
3 7 7.01600 92.41Be 4 9 9.01218 100.0000B 5 10 10.01294 19.9
5 11 11.00931 80.1
Isotopic abundance in the earth crust (2)
Az anyagKészítette: Dr. Csonka Gábor egyetemi tanár, [email protected]
29
Z A Atomic mass abundance% t1/2
C 6 12 12.00000 98.93006 13 13.00335 1.07006 14 14.00324 5730 y
N 7 14 14.00307 99.63207 15 15.00011 0.3680
O 8 16 15.99491 99.75708 17 16.99913 0.03808 18 17.99916 0.2050
Cl 17 35 34.96885 75.780017 37 36.96590 24.2200
30
Boron (Z=5)
Isotope composition
19.8 % 10B m = 10.013 u
80.2 % 11B m = 11.009 u
(0.198 10.013 u) + (0.802 11.009 u) = 10.811 uThe last digit is uncertain due to the variable isotope compositionof boron in the earth crust (±0.007 u)
Definition:An element consists of the mixture of its isotopes in the earth crust
The relative atomic mass (atomic weight) of the boron element:
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The Periodic tableAlkali Metals
Alkaline Earths
Transition Metals
Halogens
Noble Gases
Lanthanides and Actinides
Main Group
Main Group
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The Periodic Table
• Read relative atomic masses.• Read the ions formed by main group elements.• Read the electron configuration.• Learn trends in physical and chemical properties.
We will discuss these in detail in Chapter 10.
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The Mole
• Physically counting atoms is impossible.• We must be able to relate measured mass to
numbers of atoms.– buying nails by the pound.– using atoms by the gram
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Avogadro’s number
The mole is an amount of substance that contains the same number of elementary entities as there are carbon-12 atoms in exactly 12 g of carbon-12.
NA = 6.02214199 x 1023 mol-1
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Molar Mass
• The molar mass, M, is the mass of one mole of a substance.
M (g/mol 12C) = A (g/atom 12C) x NA (atoms 12C /mol 12C)
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Combining Several Factors in a Calculation—Molar Mass, the Avogadro Constant, Percent Abundance.
Potassium-40 is one of the few naturally occurring radioactive isotopes of elements of low atomic number. Its percent natural abundance among K isotopes is 0.012%. How many 40K atoms do you ingest by drinking one cup of whole milk containing 371 mg of K?
Want atoms of 40K, need atoms of K,
Want atoms of K, need moles of K,
Want moles of K, need mass and M(K).
Example 2-9
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Convert strategy to plan
mK(mg) x (1g/1000mg) mK (g) x 1/MK (mol/g) nK(mol)
Convert mass of K(mg K) into moles of K (mol K)
Convert moles of K into atoms of 40K
nK(mol) x NA atoms K x 0.012% atoms 40K
nK = (371 mg K) x (10-3 g/mg) x (1 mol K) / (39.10 g K)
= 9.49 x 10-3 mol K
and plan into action
atoms 40K = (9.49 x 10-3 mol K) x (6.022 x 1023 atoms K/mol K)
x (1.2 x 10-4 40K/K)= 6.9 x 1017 40K atoms
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Chapter 2 Questions
3, 4, 11, 22, 33, 51, 55, 63, 83.