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    Chapter 1

    Structure Determines Properties

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    1.1

    Atoms, Electrons, and Orbitals

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    Protons

    positively charged

    mass = 1.6726 X 10-27 kg

    Neutrons

    neutral

    mass = 1.6750 X 10-27 kg

    Electrons

    negatively charged

    mass = 9.1096 X 10-31 kg

    +

    Atoms are composed of

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    Atomic number (Z) = number of protons in nucleus(this must also equal the number of electrons

    in neutral atom)

    Mass number (A) = sum of number of protons

    + neutrons in nucleus

    X

    Z

    A

    Atomic Number and Mass Number

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    Schrdinger combined the idea that an electron

    has wave properties with classical equations

    of wave motion to give a wave equation for the

    energy of an electron in an atom.

    Wave equation (Schrdinger equation) gives a

    series of solutions called wave functions ( ).

    Schrdinger Equation

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    Only certain values of are allowed.

    Each corresponds to a certain energy.

    The probability of finding an electron at aparticular point with respect to the nucleus is

    given by 2.

    Each energy state corresponds to an orbital.

    Wave Functions

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    Figure 1.1 Probability distribution (2) for anelectron in a 1s orbital.

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    Figure 1.2 Boundary surfaces of a 1s orbitaland a 2s orbital.

    1s 2s

    A boundary surface encloses the region

    where the probability of finding an electron

    is high

    on the order of 90-95%

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    Each orbital is characterized by a unique

    set of quantum numbers.

    The principal quantum numbernis a wholenumber (integer) that specifies the shell and is

    related to the energy of the orbital.

    The angular momentum quantum numberisusually designated by a letter (s,p, d, f, etc)

    and describes the shape of the orbital.

    Quantum Numbers

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    s Orbitals are spherically symmetric.

    The energy of an s orbital increases with the

    number ofnodal surfaces it has.

    A nodal surface is a region where the probability

    of finding an electron is zero.

    A 1s orbital has no nodes; a 2s orbital has one;

    a 3s orbital has two, etc.

    s Orbitals

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    No two electrons in the same atom can have

    the same set of four quantum numbers.

    Two electrons can occupy the same orbitalonly when they have opposite spins.

    There is a maximum of two electrons per orbital.

    The Pauli Exclusion Principle

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    1s 2s 2p

    H

    He

    Principal quantum number (n) = 1

    Hydrogen Helium

    Z= 1 Z= 2

    1s 1 1s 2

    First Period

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    p Orbitals are shaped like dumbells.

    Are not possible forn = 1.

    Are possible forn = 2 and higher.

    p Orbitals

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    p Orbitals are shaped like dumbells.

    Are not possible forn = 1.

    Are possible forn = 2 and higher.

    There are three p orbitals for each value

    ofn (when n is greater than 1).

    p Orbitals

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    p Orbitals are shaped like dumbells.

    Are not possible forn = 1.

    Are possible forn = 2 and higher.

    There are three p orbitals for each value

    ofn (when n is greater than 1).

    p Orbitals

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    p Orbitals are shaped like dumbells.

    Are not possible forn = 1.

    Are possible forn = 2 and higher.

    There are three p orbitals for each value

    ofn (when n is greater than 1).

    p Orbitals

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    Principal quantum number (n) = 2

    1s 2s 2p

    Be 4

    B 5

    C 6

    Li 3

    Z

    Second Period

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    1s 2s 2p

    O 8

    F 9

    Ne 10

    N 7

    Z

    Second Period

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    1.2

    Ionic Bonds

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    An ionic bond is the force of electrostaticattraction between oppositely charged ions

    Cl

    (anion)

    Na+ (cation)

    Ionic Bonding

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    Ionic bonds are common in inorganic chemistry

    but rare in organic chemistry.

    Carbon shows less of a tendency to form cationsthan metals do, and less of a tendency to form

    anions than nonmetals.

    Ionic Bonding

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    In 1916 G. N. Lewis proposed that atoms

    combine in order to achieve a more stable

    electron configuration.

    Maximum stability results when an atom

    is isoelectronic with a noble gas.

    An electron pair that is shared betweentwo atoms constitutes a covalent bond.

    The Lewis Model of Chemical Bonding

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    Covalent Bonding in H2

    H . H.

    Two hydrogen atoms, each with 1 electron,

    can share those electrons in a covalent bond.

    H: H

    Sharing the electron pair gives each hydrogen

    an electron configuration analogous to helium.

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    Covalent Bonding in F2

    Two fluorine atoms, each with 7 valence electrons,

    can share those electrons in a covalent bond.

    Sharing the electron pair gives each fluorine an

    electron configuration analogous to neon.

    ..

    ..F. F.: :

    ..

    ..

    F: F: :..

    ..

    ..

    ..

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    The Octet Rule

    The octet rule is the most useful in casesinvolving covalent bonds to C, N, O, and F.

    F: F: :..

    ..

    ..

    ..

    In forming compounds, atoms gain, lose, orshare electrons to give a stable electron

    configuration characterized by 8 valence

    electrons.

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    C .. .

    .F:..

    ...

    Combine carbon (4 valence electrons) and

    four fluorines (7 valence electrons each)

    to write a Lewis structure for CF4.

    : F:..

    ..

    C: F:....

    : F:

    ..

    ..: F:

    ..

    ..

    The octet rule is satisfied for carbon and

    each fluorine.

    Example

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    It is common practice to represent a covalent

    bond by a line. We can rewrite

    : F:..

    ..C

    : F:..

    ..

    : F:..

    ..: F:..

    ..

    ..

    CF

    F

    F

    F

    ..

    ......: :

    : :

    : :

    ..

    as

    Example

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    1.4

    Double Bonds and Triple Bonds

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    C: : :O..

    :O..

    : : C :O..

    O..

    :

    : : :N:C:H :NCH

    Carbon dioxide

    Hydrogen cyanide

    Inorganic Examples

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    Ethylene

    Acetylene: : :C:C:H H CCH H

    C: :C..

    H : :..

    H

    HH

    C C

    H H

    HH

    Organic Examples

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    An electronegative element attracts electrons.

    An electropositive element releases electrons.

    Electronegativity

    Electronegativity is a measure of the ability

    of an element to attract electrons toward

    itself when bonded to another element.

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    1.0

    Na

    0.9

    Li Be B C N O F

    1.5

    Mg

    1.2

    2.0

    Al

    1.5

    2.5

    Si

    1.8

    3.0

    P

    2.1

    3.5

    S

    2.5

    4.0

    Cl

    3.0

    Electronegativity increases from left to right

    in the periodic table.

    Electronegativity decreases going down a group.

    Pauling Electronegativity Scale

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    The greater the difference in electronegativity

    between two bonded atoms; the more polar the

    bond.

    Generalization

    nonpolar bonds connect atoms of

    the same electronegativity

    HH :N N:F:....F: ....

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    The greater the difference in electronegativity

    between two bonded atoms; the more polar the

    bond.

    Generalization

    polar bonds connect atoms ofdifferent electronegativity

    :O C

    F:..

    ..H

    O..

    ..H

    H O:.. ..

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    Electrostatic potential maps show the charge

    distribution within a molecule.

    Electrostatic Potential Maps

    Red is negative charge;

    blue is positive.

    F:

    ..

    ..H

    Solid

    surface

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    Electrostatic potential maps show the charge

    distribution within a molecule.

    Electrostatic Potential Maps

    Red is negative charge;

    blue is positive.

    F:

    ..

    ..H

    Transparent

    surface

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    Electrostatic potential maps show the charge

    distribution within a molecule.

    Electrostatic Potential Maps

    Red is negative charge;

    blue is positive.

    F:..

    ..

    H

    LiH

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    The order in which the atoms of a

    molecule are connected is called its

    constitution orconnectivity.

    The constitution of a molecule mustbe determined in order to write a

    Lewis structure.

    Constitution

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    Condensed structural formulas

    Lewis structures in which many (or all)

    covalent bonds and electron pairs are

    omitted.

    H

    O

    C C C

    H H H

    H

    HH : :

    H

    can be condensed to:

    CH3CHCH3

    OH

    (CH3)2CHOHor

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    Bond-line formulas

    CH3CH2CH2CH3 is shown as

    CH3CH2CH2CH2OHis shown as OH

    Omit atom symbols. Represent

    structure by showing bonds between

    carbons and atoms other thanhydrogen.

    Atoms other than carbon and hydrogen

    are called heteroatoms.

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    Bond-line formulas

    H Cl

    C

    C

    H2C

    H2C

    CH2

    CH2

    HH

    is shown as

    Cl

    Omit atom symbols. Represent

    structure by showing bonds between

    carbons and atoms other than

    hydrogen.

    Atoms other than carbon and hydrogen