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Formation of Earth's Oceans and Atmospheres

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Polar molecules containing H bonded to either F, O, or N exhibit LDF, DDF, and ... Force of attraction between H in one polar molecule and a lone pair of electrons ... – PowerPoint PPT presentation

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Title: Formation of Earth's Oceans and Atmospheres


1
Formation of Earth's Oceans and Atmospheres
  • Components are molecular covalent substances
    which can exist as a gas or liquid at low T

2
Molecular Covalent Substances
  • Covalent bonds holding atoms together in a single
    molecule (intramolecular force) are very strong
  • Force of attraction between molecules
    (intermolecular force) is weak
  • Molecules with low intermolecular forces became
    components of the atmosphere of primitive Earth

3
Continued...
  • The molecule with the strongest intermolecular
    force (water) became the component of the oceans
    (hydrosphere)
  • To understand atmospheres and oceans, need to
    understand the factors that determine the
    strengths of intermolecular forces

4
Electronegativities of Atoms
  • Ability of an atom to attract electrons in a bond
    is called the electronegativity (EN) of the
    element
  • EN of Main Group elements (A-families) generally
    increase in going upward in a family or across a
    period from left to right

5
http//wine1.sb.fsu.edu/chm1045/notes/Bonding/Pola
rity/Bond05.htm
6
Electronegativity and Bonding
  • Ionic bonding occurs between atoms having widely
    differing EN (metal/non-metal) ?EN 2
  • Metallic bonding occurs between atoms having low
    EN (metals) ?EN 0 to 0.4
  • Covalent bonding occurs between atoms having high
    EN (non-metals) ?EN 0 to 2

7
Types of Covalent Bonds Based on Electronegativity
  • Two kinds of covalent bonds possible depending on
    the differences in the EN of the bonding atoms
  • Non-polar bond difference in EN is less than 0.4
  • Polar bond difference in EN is between 0.4 and
    2.

8
Predicting Polarities of Covalent Bonds
If the difference in electronegativities between
the two bonded atoms is lt 0.4, the bond is
non-polar covalent
Bonding pair of electrons is equally shared by
two F atoms
http//wine1.sb.fsu.edu/chm1045/notes/Bonding/Pola
rity/Bond05.htm
9
If the difference in electronegativities between
the two bonded atoms is between 0.4 and 2.0, the
bond is polar covalent
Atom having higher EN has a small negative charge
while atom with lower EN, a small positive
charge
http//wine1.sb.fsu.edu/chm1045/notes/Bonding/Pola
rity/Bond05.htm
10
Polarities of Molecules
  • A molecule is non-polar if it contains no polar
    bonds or if it contains identical polar bonds in
    geometries that cancel their polarities (linear,
    trigonal planar or tetrahedral)
  • A molecule is polar if it contains non-identical
    polar bonds or identical polar bonds in
    geometries that do not cancel bond polarities
    (bent, trigonal pyramidal)

11
Geometries and Polarities of Molecules
  • Molecules having one central atom and two
    terminal atoms are linear if there are no lone
    pairs on central atom or bent if there are lone
    pair(s) on central atom

Polar
http//wine1.sb.fsu.edu/chm1045/notes/Geometry/VSE
PR/Geom02.htm
12
Molecules having one central atom and 3 terminal
atoms are trigonal planar if there are no lone
pairs on the central atom or trigonal pyramidal
if there is a lone pair on the central atom
Non-polar for AB3
Polar
http//wine1.sb.fsu.edu/chm1045/notes/Geometry/VSE
PR/Geom02.htm
13
  • Simple molecules having one central atom and four
    terminal atoms are tetrahedral

Non-polar for AB4
http//wine1.sb.fsu.edu/chm1045/notes/Geometry/VSE
PR/Geom02.htm
14
Polarity and Intermolecular Forces
  • Forces between molecules are called
    intermolecular forces
  • Intermolecular forces depend, in part, on the
    polarities of molecules
  • Three types of intermolecular forces
    Dipole-Dipole Force, London Dispersion Force, and
    Hydrogen Bonding

15
Dipole-Dipole Force
Force of attraction between opposite charges of
permanent dipoles of adjacent polar molecules
Most readily observed in properties of molecules
having same size (molecular wt.)
http//wine1.sb.fsu.edu/chm1045/notes/Forces/inter
mol/Forces02.htm
16
Dipole Forces
Masterton/Hurley, Chemistry, 3rd, Saunders, 1997.
240
17
London Dispersion Force (LDF)
  • Weakest cohesive force present between all
    molecules (polar and non-polar)
  • Results from the force of attraction between
    temporary fluctuating dipoles consisting of an
    instantaneous dipole and induced dipoles

18
London Dispersion Force (LDF)
Force of attraction between a temporary
instantaneous dipole and an induced dipole
http//wine1.sb.fsu.edu/chm1045/notes/Forces/inter
mol/Forces02.htm
19
London Dispersion Force (LDF)
LDF increases with increasing size (molecular
weight) for similar molecules
Tro, 295
20
Hydrogen Bonding
  • Polar molecules containing H bonded to either F,
    O, or N exhibit LDF, DDF, and an additional
    intermolecular force called H-bonding
  • Force of attraction between H in one polar
    molecule and a lone pair of electrons on O, N, or
    F in an adjacent molecule

21
Hydrogen Bonding
Each water molecule can form H-bonds with 4 other
water molecules
http//users.rcn.com/jkimball.ma.ultranet/BiologyP
ages/H/HydrogenBonds.html
22
Effect of H-Bonding
As size decreases, LDF decreases, and B.P.
decreases. However, the smallest molecule, water,
has the highest B.P. due to a strong additional
force H-bonding
Ebbing/Gammon, General Chemistry,6th,Houghton
Mifflin, 1999, 461
23
Effect of H-Bonding
HF and NH3 exhibit H-bonding while CH4 does not
Ebbing/Gammon, General Chemistry,6th,Houghton
Mifflin, 1999, 461
24
Primitive Atmospheres of Earth
  • Atmosphere-1, when Earth formed 4.5 billion years
    ago, was H2 and He. When solar fusion started
    these light gases escaped earths gravity
  • Atmosphere-2 came from outgassing, "Big Burp" and
    volcanoes N2, H2, H2O, NH3, and CH4 and from
    collisions with comets, which consist primarily
    of ice

25
Formation of Oceans
  • Of the molecules in the second atmosphere of
    primitive Earth, water was most abundant and had
    the strongest intermolecular forces (LDF, DDF,
    and H-bonding)
  • As Earth cooled, water was the first to liquify
    and it came down as rain which formed the
    hydrosphere - oceans, etc

26
Formation of Earth Related to Chemical Bonding
LDF London Dispersion Force DDF
Dipole-Dipole Force
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