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ATOMIC STRUCTURE AND THEORY

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Atoms of the same element are alike and differ from any other element. ... Dosimeter. Geiger counter. Nuclear Energy. Nuclear Fission ... – PowerPoint PPT presentation

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Title: ATOMIC STRUCTURE AND THEORY


1
ATOMIC STRUCTURE AND THEORYNUCLEAR CHEMISTRY
  • CHAPTERS 4 25

2
Early Models of the Atom
  • Democritus (450 BC) Matter is composed of tiny
    indivisible particles.
  • Daltons Atomic Theory (1803) Based on four
    statements.
  • Each element is composed of atoms.
  • Atoms of the same element are alike and differ
    from any other element.
  • Atoms can not be created nor destroyed by
    chemical reactions.
  • Atoms combine in simple whole number ratios.

3
  • Atom The smallest particle of an element that
    retains the chemical identity of that element.
  • Approximately 114 elements. The alphabet of
    chemistry.
  • The chemists goal is to understand the atoms
    that make up the world.

4
Discovering Atomic Structure
  • Magnetism The theory for the discovery of the
    electron and proton.
  • Electrostatics Opposite charges attract and
    likes repel.
  • Benjamin Franklin An object could have one of
    two charges (positive or negative).
  • Michael Faraday (1839) Drew the connection
    between the electrical current and the structure
    of the atom.

5
Equipment to Isolate Sub-Atomic Particles
  • Eugene Goldstein Designed the cathode ray tube
    and the canal ray tube.
  • Vacuum inside, current flows between cathode and
    the anode (blue), source of electrons or x-rays.

6
Discovery of the ElectronJ.J. Thompson
  • Defines the charge of the electron.
  • Designs the mass spectrometer.
  • Begins to define the mass of the electron.
  • Places bar magnets around the tube and creates a
    magnetic field in which the beam of blue light
    bends toward the positive pole of the magnet.

7
Defining the ElectronRobert Milikan
  • Defines a more accurate mass of the electron.
  • Oil Drop Experiment
  • Timed the rate at which the charged oil drop
    would rise and fall depending upon the strength
    of the electromagnetic field vs. the strength of
    gravity.

8
Discovery of the Proton
  • Eugene Goldstein Defined the charge of the
    proton.
  • J.J. Thompson Defined the mass of the proton to
    be 1837 times the mass of the electron.

9
The Nuclear AtomRutherford
  • Gold Foil Experiment
  • Concluded a nucleus existed.
  • Contained the positive charge as well as the
    majority of the mass.

10
Atomic Structure
  • Atoms are composed of protons, neutrons, and
    electrons.
  • Create chart on the board of sub-atomic particles
    for comparison.

11
Atomic Number and Mass
  • Atomic number Z of protons.
  • Atomic mass M of protons and neutrons.
  • An individual atom is electrically neutral.
  • Protons Electrons.
  • p Z, Charge p - e, and n M Z.

12
IONS
  • Created when an atom gains or loses one or more
    electrons.
  • It acquires a net electrical charge.
  • Charge of ion the number of protons the
    number of electrons.

13
Isotopes
  • Daltons postulate that all atoms of a given
    element are identical is not exactly true.
  • An isotope is an atom that has the same number of
    protons but a different number of neutrons.

14
Periodic TableDevelopment
  • Why?
  • Mendeleev
  • Based on increasing atomic mass.
  • Predictions.
  • Moseley
  • Based on increasing atomic number.
  • Why did Mendeleevs work?
  • Periodic Law When elements are arranged in
    order of increasing atomic number, their physical
    and chemical properties show a periodic pattern.

15
  • Metals Properties include luster or shine, good
    conductors of heat/electricity, malleable, and
    ductile.
  • Nonmetals Large variation in properties.
  • Metalloids or Semimetals The in between.

16
  • Family Names
  • Representative (1A 8A)
  • Transition (1B 8B)
  • Inner Transition
  • Alkali Metals
  • Alkaline Earth Metals
  • Boron family
  • Carbon family
  • Nitrogen family
  • Oxygen family
  • Halogens
  • Noble gases

17
Nuclear ChemistryThe Changing Nucleus
  • Strong Nuclear Force between extremely close
    subatomic particles.
  • Atomic s 1 thru 20 protons neutrons.
  • Past 20 Need more neutrons than protons to be
    stable.
  • Past 83 All are radioactive.
  • Too many or too few neutrons radioactivity.

18
RadioactivityAlpha, Beta, and Gamma
  • Distinguished by charge, mass, and penetrating
    power.
  • Radioactive decay when an atom emits one of
    these kinds of radiation.
  • Decay nucleus decays to form a new nucleus
    releasing radiation in the process.
  • Nuclear reactions change the composition of the
    atoms nucleus.

19
Types of Radiation
20
Nuclear Equations
  • Keep track of the reactions components.
  • The sum of the mass numbers and atomic numbers
    are the same before and after.
  • Sample problems.

21
Effects of Radiation
  • Harmful to living things
  • Effects depend on the amount and type.
  • Effects on living tissue
  • Ionizing radiation disrupts living cells.
  • Somatic damage direct.
  • Genetic damage reproduction.

22
Uses of Nuclear Chemistry
  • Radioactive dating.
  • Smoke detectors.
  • Imaging.
  • Radiotracers.
  • Cancer therapy.
  • Food preservation.
  • Energy.

23
Measuring Radiation
  • Equipment
  • Dosimeter.
  • Geiger counter.

24
Nuclear EnergyNuclear Fission
  • A large nucleus is split into two smaller nuclei
    of approximately the same mass.
  • The missing mass energy.
  • Nuclear chain reactions.
  • Nuclear reactors.
  • Three Mile Island (loss of coolant).
  • Chernobyl (failure of the moderator).
  • Waste disposal (fuel rods and burial).

25
Nuclear EnergyNuclear Fusion
  • Two small nuclei join to form a large nucleus.
  • Difficult to produce and control.
  • Electron cloud repulsion.
  • Nucleus repulsion.
  • Benefits
  • Uses hydrogen abundant.
  • No radioactive waste.
  • Problem
  • High temps required.

26
Half-life
  • The half-life of a radioactive isotope is the
    time it takes for one half of a sample of that
    isotope to decay.
  • Uranium-238 4.5 billion years (alpha decay).
  • Carbon-14 5,730 years (beta decay).
  • Sample problems.
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