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AP CHEMISTRY Atomic Structure and Electrons

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AP CHEMISTRY Atomic Structure and Electrons Ch. 7 sec 1-9 Chemists found Rutherford s nuclear model lacking because it did not begin to account for the differences ... – PowerPoint PPT presentation

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Title: AP CHEMISTRY Atomic Structure and Electrons


1
AP CHEMISTRYAtomic Structure and Electrons
  • Ch. 7 sec 1-9

2
Light and Quantized Energy
  • Chemists found Rutherfords nuclear model lacking
    because it did not begin to account for the
    differences in chemical behavior among the
    various elements.
  • In the early 1900s, scientists observed that
    certain elements emitted visible light when
    heated in a flame.

3
Light and Quantized Energy
  • Analysis of the emitted light revealed that an
    elements chemical behavior is related to the
    arrangement of the electrons in its atoms.
  • In order to better understand this relationship
    and the nature of atomic structure, it will be
    helpful to first understand the nature of light.

4
The Electromagnetic Spectrum
  • Electromagnetic radiation includes radio waves
    that carry broadcasts to your radio and TV,
    microwave radiation used to heat food in a
    microwave oven, radiant heat used to toast bread,
    and the most familiar form, visible light.
  • All of these forms of radiant energy are parts of
    a whole range of electromagnetic radiation called
    the electromagnetic spectrum.

5
The Electromagnetic Spectrum
6
Particle Nature of Light
  • While considering light as a wave does explain
    much of its everyday behavior, it fails to
    adequately describe important aspects of lights
    interactions with matter.

7
The Quantum Concept
  • In 1900, the German physicist Max Planck
    (18581947) began searching for an explanation as
    he studied the light emitted from heated objects.

8
The Quantum Concept
  • His study of the phenomenon led him to a
    startling conclusion matter can gain or lose
    energy only in small, specific amounts called
    quanta.
  • That is, a quantum is the minimum amount of
    energy that can be gained or lost by an atom.

9
The Quantum Concept
  • While a beam of light has many wavelike
    characteristics, it also can be thought of as a
    stream of tiny particles, or bundles of energy,
    called photons
  • Thus, a photon is a particle of electromagnetic
    radiation with no mass that carries a quantum of
    energy.

10
Atomic Emission Spectra
  • The atomic emission spectrum of an element is the
    set of frequencies of the electromagnetic waves
    emitted by atoms of the element.

11
Atomic Emission Spectra
  • Hydrogens atomic emission spectrum consists of
    several individual lines of color, not a
    continuous range of colors as seen in the visible
    spectrum.
  • Each elements atomic emission spectrum is unique
    and can be used to determine if that element is
    part of an unknown compound.

12
Atomic Emission Spectra
13
Atomic Emission Spectra
  • An atomic emission spectrum is characteristic of
    the element being examined and can be used to
    identify that element.
  • The fact that only certain colors appear in an
    elements atomic emission spectrum means that
    only certain specific frequencies of light are
    emitted.

14
Bohr Model of the Atom
  • Why are elements atomic emission spectra
    discontinuous rather than continuous?
  • Niels Bohr, a young Danish physicist working in
    Rutherfords laboratory in 1913, proposed a
    quantum model for the hydrogen atom that seemed
    to answer this question.
  • Impressively, Bohrs model also correctly
    predicted the frequencies of the lines in
    hydrogens atomic emission spectrum.

15
Energy States of Hydrogen
  • Building on Plancks and Einsteins concepts of
    quantized energy (quantized means that only
    certain values are allowed), Bohr proposed that
    the hydrogen atom has only certain allowable
    energy states.
  • The lowest allowable energy state of an atom is
    called its ground state.

16
Energy States of Hydrogen
  • When an atom gains energy, it is said to be in an
    excited state.
  • And although a hydrogen atom contains only a
    single electron, it is capable of having many
    different excited states.

A02220MV.mpg
17
Energy States of Hydrogen
  • Bohr went even further with his atomic model by
    relating the hydrogen atoms energy states to the
    motion of the electron within the atom.
  • Bohr suggested that the single electron in a
    hydrogen atom moves around the nucleus in only
    certain allowed circular orbits.

18
Energy States of Hydrogen
19
Hydrogens Line Spectrum
  • Bohr suggested that the hydrogen atom is in the
    ground state, also called the first energy level,
    when the electron is in the n 1 orbit.

20
Hydrogens Line Spectrum
  • When energy is added from an outside source, the
    electron moves to a higher-energy orbit such as
    the n 2 orbit shown.

21
Hydrogens Line Spectrum
  • Such an electron transition raises the atom to an
    excited state.
  • When the atom is in an excited state, the
    electron can drop from the higher-energy orbit to
    a lower-energy orbit.
  • As a result of this transition, the atom emits a
    photon corresponding to the difference between
    the energy levels associated with the two orbits.

22
Hydrogens Line Spectrum
  • The four electron transitions that account for
    visible lines in hydrogens atomic emission
    spectrum are shown.

23
The Heisenberg Uncertainty Principle
  • Heisenberg concluded that it is impossible to
    make any measurement on an object without
    disturbing the objectat least a little.
  • The act of observing the electron produces a
    significant, unavoidable uncertainty in the
    position and motion of the electron.

24
The Heisenberg Uncertainty Principle
  • Heisenbergs analysis of interactions such as
    those between photons and electrons led him to
    his historic conclusion.
  • The Heisenberg uncertainty principle states that
    it is fundamentally impossible to know precisely
    both the velocity and position of a particle at
    the same time.

25
Mathematic Equations
cln c speed of light (3.0 x 108m/s) l
wavelength (m) n frequency (s-1 or Hz)
Ehn Eenergy (J or kgm2/s2) hPlancks constant
(6.63x10-34 Js or kgm2/s) nfrequency (s-1)
Combining them Ehc/l
26
Mathematic Equations (contd)
deBroglie equation lh/mv lwavelength
(m) h6.63x10-34 kgm2/s mmass (kg) vvelocity
(m/s)
pmv pmomentum (kgm/s) mmass (kg) vvelocity
(m/s)
27
Energy levels, sublevels, orbitals
  • Energy levelsclouds or shells around nucleus
    (n1,2,3)
  • Sublevelsfound inside energy levels (s,p,d,f)
  • Atomic orbitalsfound within sublevels
  • s 1 orbital (sphere)
  • p 3 orbitals (dumbell)
  • d 5 orbitals (p. 313)
  • f 7 orbitals
  • 2 e- max per orbital

28
Rules Governing e- Configurations
  • Aufbau Principle e- fill orbitals with lowest
    energy first
  • Pauli Exclusion Principle e- in the same
    orbital have opposite spins ? no 2 e- in a single
    atom will have the same set of quantum numbers
  • Hunds Rule e- occupy one orbital in each
    sublevel before pairing up (p,d,f)

29
Electron Configurations
  • Use Periodic Table to find e- configurations

30
Electrons
  • Diamagnetism all of e- are paired not strongly
    affected by magnetic fields
  • Paramagnetism has unpaired e- strongly
    affected by magnetic fields
  • Valence e- e- in outermost energy level
  • For Representative Elements 1A-8A, groups
    numbernumber of valence e-
  • Period numberenergy level of valence e-

31
Quantum Numbers
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