Title: PERIODICITY
1PERIODICITY
2History 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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4History 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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6History 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
7PNICOGENS
CHALCOGENS
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9Periodic 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
10Periodic 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.
11Periodic 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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13Periodic 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)
14Periodic 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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17Periodic 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.
18Periodic 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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20Periodic Properties
- Elements in a group tend to form ions of the same
charge. - Modeled by electron configurations.
21Periodic Properties
He
O
He
22Periodic Trend of Ionic Charges
23The Transition Elements are almost unpredictable,
and sometimes have more than one possible charge
-- due to d orbitals --
24Tend to lose electrons to become positive
Tend to gain electrons to become negative
25Periodic 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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28Periodic 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.
29the 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-
30Periodic 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
31Periodic 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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34Periodic 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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37Periodic 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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40BOILING POINT MELTING POINT VS. ATOMIC NUMBER
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43Elemental 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.
44Elemental 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
45Elemental 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.
46Elemental 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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48Elemental 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
49Elemental 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
50Elemental 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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52Elemental 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
53Carbon Cycle
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55Nitrogen Cycle
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57Phosphorus Cycle
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59Sulfur Cycle
60Oxygen Cycle
61Water Cycle
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63Homemade 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
64Homemade 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)
65Homemade 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
66Homemade 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
67Homemade 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
68Homemade 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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70Homemade 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
71Homemade 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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73Homemade Elements
- The collision can help scientists discover new
info. About the nucleus, sometimes create a
heavier atom.
74Homemade 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.
75Homemade 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
76Collison of 2 Gold atoms
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