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Origin of the Chemical Elements

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Galaxies and Stars. Gravity brought atoms of H and He together to form galaxies of protostars ... Galaxies. 1 billion yr. Stars (99% H, 1% He) 7 billion yr ... – PowerPoint PPT presentation

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Title: Origin of the Chemical Elements


1
Origin of the Chemical Elements
2
Formation of First Atoms
  • Following the Big Bang, nuclei of atoms and
    electrons existed as a gas (plasma), primarily
    H, He2, and e-
  • When Universe cooled sufficiently, 300000-500000
    years, e- became associated with nuclei to form
    atoms of H and He having electrons moving in
    circles about nucleus

3
Galaxies and Stars
  • Gravity brought atoms of H and He together to
    form galaxies of protostars
  • Gravity initiated nuclear reactions in stars
    which produced heavier nuclei
  • When resulting plasma cooled, the neutral atoms
    of the heavier elements were formed

4
Origin of the Chemical Elements
Galaxies
5
Stabilities of Nuclei
  • Particles making up the nucleus are called
    nucleons sum of the protons and neutrons Mass
    Number, A
  • Mass of nucleus lt total mass of nucleons making
    it up
  • Difference is called mass defect total mass of
    nucleons in nucleus - actual mass of nucleus

6
Nuclear Binding Energy
  • Mass defect is the mass which is converted to
    energy, E mc2
  • This energy holds nucleus together nuclear
    binding energy, NBE
  • NBE/A nuclear binding energy per nucleon
    serves to measure stability
  • The larger NBE/A the more stable the nucleus

7
http//www.courses.fas.harvard.edu/chem15/lecture
s/1_nuclear.pdf
8
http//www.courses.fas.harvard.edu/chem15/lecture
s/1_nuclear.pdf
9
http//www.courses.fas.harvard.edu/chem15/lecture
s/1_nuclear.pdf
10
Stability of nucleus is measured by NBE/A 2.37
x 10-11 J /19 nucleons 12 x 10-13 J/nucleon
http//www.courses.fas.harvard.edu/chem15/lecture
s/1_nuclear.pdf
11
Graph of Nuclear Binding Energy per Nucleon
http//www.courses.fas.harvard.edu/chem15/lecture
s/1_nuclear.pdf
12
Stabilty of Nuclei and Fusion Reactions
Stability Increasing
Jones, "Chemistry, Man and Society", Saunders,
1972, 623
13
Synthesis of the Chemical Elements in Stars
Olmstead, Chemistry, Mosby, St. Louis, MO,
1994, p. 960.
Olmstead, Chemistry, Mosby, St. Louis, MO,
1994, p. 960.
Olmstead, Chemistry, Mosby, St. Louis, MO,
1994, p. 960.
14
Birk, ChemistryHoughton Mifflin, Boston,
MA,1994,p 880.
15
Star Composition at Supernova
Cox, The Elements, Oxford, New York, NY, 1989,
p. 80
16
Collapse of Star and Supernova
As Fe builds in core, core temperature drops
since Fe does not undergo fusion. The unbalanced
gravitational force causes star to collapse.
http//wine1.sb.fsu.edu/chm1046/notes/Nucleo/Nucle
o.htm
17
Cosmic Dust
Coalescing
H-Burning
He-Burning
C-Burning
Silberberg, Chemistry Mosby,St. Louis, MO,
1996, p 965
Supernova
18
Formation of Nuclides Heavier Than Iron
  • Supernovas produce large amounts of neutrons
  • Neutrons can react with atoms one at a time and
    release electrons to produce elements heavier
    than iron
  • Many neutrons can also react with one atom and
    release electrons to produce elements heavier
    than iron

19
Reactions that Produce Nuclides Heavier than Iron
20
(No Transcript)
21
Abundances of the Chemical Elements in Universe
Heavier elements formed only in a supernova are
less abundant due to short time frame for
collisions with neutrons - only a small fraction
of lighter atoms converted in each supernova
Radel/Navidi, "Chemistry", West, NY,1990, 987
22
Debris from supernova is recycled in a new star
making it possible to form heavier and heavier
nuclei but in decreasing amounts
http//www.howstuffworks.com/star5.htm
23
Formation of Atoms of Heavier Elements
  • As the debris from a supernova cools, the nuclei
    will pick up electrons to form atoms
  • Electrons repel each other sufficiently to cause
    groups of electrons to occupy shells at
    ever-increasing distances from nucleus

24
Electron Structures of Atoms
  • Electrons move about the nucleus in spherical
    shells designated as K,L,M... or 1,2,3 starting
    nearest nucleus
  • Capacities of shells given by 2n2 where n shell
    number (2,8,18, 32 )
  • Order of filling of shells is in order of
    increasing n except outermost shell (valence
    shell) never exceeds 8e

25
Elements 1-18
26
Elements 19-20
When outermost shell reaches 8e, a new shell is
added which is occupied by the next two electrons
27
Elements 21-30
After valence shell acquires 2e, the next ten
electrons are added to the third shell until its
reaches capacity of 18e
28
Elements 31-36
Once 3rd shell is filled, the next electrons are
added to valence shell until it reaches 8e when
a new shell is added and pattern repeats
29
Valence Electrons
30
Periods and Families
31
Main Group Transition Elements
Electrons add to inner shell
32
Electron Structures of Atoms
33
Metals and Non-Metals
34
Relative Sizes of Atoms
35
Periodic Table
  • Periodic table provides the link between the real
    world and the imaginary world
  • Elements in same family are observed to have
    similar properties in real world
  • Explanation atoms of elements in the same family
    have the same valence shell electron structure in
    the imaginary world

36
Valence Electrons and Chemical Reactions
  • Valence shells of approaching atoms come in
    contact first
  • Atoms having same numbers of e in valence shell
    have similar reactions
  • Chemical reactions involve a rearrangement of
    valence electrons

37
A-Families of Periodic Table
1A 2A 3A 4A 5A 6A 7A 8A
1 2 3 4 5 6
7 8 Valence Electrons
http//www.chemicalelements.com/index.html
38
Reactions of Selected 1A Elements with Water
Real World all 1A elements react with water
Imaginary World all 1A elements have 1 valence e
Real World speeds of reactions of 1A elements
with water are different
Imaginary World The larger the 1A atom, the
faster the reaction
http//www.chemicalelements.com/index.html
39
Periodic Table(Symbolic World)
40
B-Families of Periodic Table
3B 4B 5B 6B 7B 8
8 8 1B 2B
For Chem 83, disregard irregularities and assume
all have 2e in their valence shells
http//www.chemicalelements.com/index.html
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