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PERIODICITY

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Title: PERIODICITY


1
PERIODICITY
2
History of the Periodic Table
  • 70 elements had been discovered by the
    mid-1800s, but until Dmitri Mendeleev, no one
    had a come with a way to organize the elements.
  • Mendeleev came up with the first working system
    of filing the elements.
  • He listed the elements in columns in order of
    increasing atomic mass, and then put columns
    together that were similar

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History of the Periodic Table
  • Mendeleev left gaps in the table since there were
    no current elements that seemed to fit those
    spots
  • Those elements were eventually discovered and
    they fit perfectly into an open spot.
  • The 1st scientist that set the table in order of
    atomic number was Henry Moseley

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History of the Periodic Table
  • The modern PT is arranged by increasing atomic
    number
  • Increases from left to right, and top to bottom
  • This establishes the periodic law
  • When the elements are arranged in order of
    increasing atomic , there is a periodic
    repetition of their phys chem properties

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PNICOGENS
CHALCOGENS
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Periodic Properties
  • An elements properties can go hand in hand with
    electron arrangement
  • We can use an elements location on the PT to
    predict many properties.
  • Atomic radius
  • Electron affinity
  • Electronegativity
  • Ionization energy
  • Ionic Size

10
Periodic Properties
  • The radius of an atom is defined by the edge of
    its last energy level.
  • However, this boundary is fuzzy
  • An atoms radius is the measured distance between
    the nuclei of 2 identical atoms chemically
    bonded together - divided by 2.

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Periodic Properties
  • As we examine atomic radius from left to right
    across the PT we see a grad-ual decrease in
    atomic size.
  • As e- are added to the s and p sublevels in the
    same energy level, they are gradually pulled
    closer to the highly positive nucleus
  • The more e-s in the atom the less dramatic this
    trend looks

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Periodic Properties
  • The change in atomic radii across the PT is due
    to e- shielding or to the effective nuclear
    charge
  • As we move across the
    PT we are adding e- into
    the same gen- eral vol.
    in which case they will
    shield or interact
    with each other
    (repulsion)

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Periodic Properties
  • We are also adding protons into the nucleus which
    increases the p-e- interaction (attraction)
  • So the nucleus gains strength while the e- arent
    gaining much distance, so the atom is drawn in
    closer and closer to the nucleus.
  • Decreasing the overall radius of the atom

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Periodic Properties
  • How does the size of an atom change when
    electrons are added or removed?

As an Atom loses 1 or more electrons (becomes
positive), it loses a layer therefore, its radius
decreases.
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Periodic Properties
  • How does the size of an atom change when
    electrons are added or removed?

As an Atom gains 1 or more electrons
(negative), it fills its valence layer,
therefore, its radius increases.
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Periodic Properties
  • Elements in a group tend to form ions of the same
    charge.
  • Modeled by electron configurations.

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Periodic Properties
He
O
He
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Periodic Trend of Ionic Charges
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The Transition Elements are almost unpredictable,
and sometimes have more than one possible charge
-- due to d orbitals --
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Tend to lose electrons to become positive
Tend to gain electrons to become negative
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Periodic Properties
  • Another periodic trend on the table is ionization
    energy (a.k.a. potential)
  • Which is the energy needed to remove one of an
    atoms e-s.
  • Or a measure of how strongly an atom holds onto
    its outermost e-s.
  • If the e-s are held strongly the atom will have a
    high ionization energy

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Periodic Properties
  • The ionization energy is generally measured for
    one electron at a time
  • You can also measure the amount of energy needed
    to reach in and pluck out additional electrons
    from atoms.
  • There is generally a large jump in energy
    necessary to remove additional electrons from the
    atom.

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the amount of energy required to remove a 2p e
(an e- in a full sublevel) from a Na ion is
almost 10 times greater than that required to
remove the sole 3s e-
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Periodic Properties
  • There is simply not enough energy available or
    released to produce an Na2 ion to make the
    compnd NaCl2
  • Similarly Mg3 and Al4 require too much energy
    to occur naturally.
  • Chemical formulas should always describe
    compounds that can exist naturally the most
    efficient way possible

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Periodic Properties
  • Another periodic trend dealing with an e- is
    electron affinity
  • Which is a measure of the ability of an atom to
    attract or gain an electron.
  • Atoms that tend to accept an e- are those that
    tend to give a neg. charge.
  • The closer to a full outer shell an atom has, the
    higher the affinity (more neg. the measurement)

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Periodic Properties
  • An atoms ability to lose an e- or gain an e- can
    be used to understand the Octet Rule
  • Octet Rule atoms tend to gain, lose, or share
    electrons in order to acquire a full set of
    valence electrons.
  • 2 e- in the outermost s sublevel 6 e in the
    outermost p sublevel a full valence shell

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Periodic Properties
  • Electronegativity is a key trend.
  • It reflects the ability of an atom to attract
    electrons in a chemical bond.
  • F is the most electronegative element and it
    decreases moving away from F.
  • Electronegativity correlates to an atoms
    ionization energy and electron affinity

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BOILING POINT MELTING POINT VS. ATOMIC NUMBER
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Elemental Origins
  • On the PT, only the elements through 92 are
    naturally occurring
  • Elements are created through a process that took
    place in stars before our solar system came into
    being
  • This process is called stellar nucleosynthesis.

44
Elemental Origins
  • Stars form when clouds of dust and hydrogen gas
    condense
  • As this material condenses, pressure builds and
    temperatures reach millions of degrees
  • The energy that is produced help stars live for
    billions of years
  • The principle source of stellar energy is nuclear
    fusion

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Elemental Origins
  • Fusion occurs when the nuclei of 2 or more atoms
    join together, to form the nucleus of a larger
    atom
  • Typically 2 H nuclei combine to
    produce one
    He nucleus.

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Elemental Origins
  • This is a type of nuclear rxn
  • The mass of helium nucleus formed in the fusion
    process is slightly less than the mass of the
    four hydrogen nuclei that went into it.
  • This small amount of missing mass is converted
    to energy according to Einsteins eqn Emc2

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Elemental Origins
  • The mass of combining nuclei supplies the
    enormous energy that stars use to shine
  • Nuclear fusion is not only the princ-iple source
    of energy for stars, but also the process by
    which elements heavier than H are created.
  • The sun converts about 400 million tons of H into
    He every second

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Elemental Origins
  • Other fusion rxns occur, depending on the mass of
    the star, the temp. of the star, the stage of
    its developmnt
  • 2 He-4 atoms might combine to form Be-8 1 He-4
    1 Be-8 can fuse to form C-12
  • When a star uses up all of the ele-ments that
    fuel its fusion, the star is no longer stable,
    it dies in a last great explosion

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Elemental Origins
  • The elements that were formed within the star are
    flung into space
  • When planets condense from this material, they
    take up the rich array of elements in the debris.
  • Elements heavier than Fe were created by
    supernovas

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Elemental Origins
  • On earth, which is considered a closed system,
    most elements are found in biogeochemical cycles.
  • Elements are recycled through processes that
    keeps the amount of elements on earth constant.
  • The big six cycles important for life are
    carbon, water, oxygen, phosphorus, nitrogen,
    sulfur

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Carbon Cycle
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Nitrogen Cycle
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Phosphorus Cycle
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Sulfur Cycle
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Oxygen Cycle
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Water Cycle
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Homemade Elements
  • The first artificial isotope was created in 1919
  • ? particles were being used to produce elements
    in the lab
  • Scientists were taking a particles and colliding
    them with nitrogen atoms
  • This led to the fusion of nuclei to form a
    synthetic isotope of oxygen

64
Homemade Elements
  • This was the first incident in which one element
    was transformed into another in a lab.
  • Today, scientists change one element into another
    by bombarding nuclei with various small particles
  • Protons, neutrons, alpha particles, and beta
    particles (fast moving electrons)

65
Homemade Elements
  • These nuclear bullets react with the nuclei
    they are aimed at forming iso-topes of naturally
    occurring elements
  • Numerous synthetic elements are created with this
    method
  • All of the elements with atomic s greater than
    92 but less than 101 were created with this
    process

66
Homemade Elements
  • The particles must be moving at extremely fast
    speeds and with a huge amount of energy in order
    to actually fuse rather than simply bouncing off
    of one another
  • A device called a Particle Accelerator is used
    to accomplish this task

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Homemade Elements
  • Elements with atomic 101 greater have been
    created by a colliding whole atoms rather than
    particles.
  • To make the bigger atoms, special accelerators
    hurl entire atoms at one another
  • Nobelium was created by crashing together
    Ca and Pb

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Homemade Elements
  • The discovery of element 109 has been thoroughly
    verified and accepted
  • It is extremely unstable
  • Only 3 atoms of element 109 have ever been
    produced
  • They only existed for a short time (.0034 seconds)

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Homemade Elements
  • Scientists are hoping to discover other heavier
    atoms that might be more stable, because of the
    nature of their nuclei
  • The atom smashers they plan to use are
    technological marvels, and there are only a few
    in the world

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Homemade Elements
  • An accelerator is a linear or circular device
    that is used to increase the velocity of charged
    particles
  • When the particle has been given a very
    high velocity and thus a very
    high energy, it is aimed at a target
    material.

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Homemade Elements
  • The collision can help scientists discover new
    info. About the nucleus, sometimes create a
    heavier atom.

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Homemade Elements
  • A typical accelerator is circular in shape
  • Particles are accelerated by electric fields in
    several loca- tions around the ring.
  • The particles path is confined to the ring by
    huge magnets.

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Homemade Elements
  • The greater the energy of the collision between
    the accelerated particles with the target.
  • The more scientists can learn about the structure
    and the behavior of the nucleus

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Collison of 2 Gold atoms
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