| Lecture
#8 |
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| CURMUDGEON
GENERAL'S WARNING. These "slides"
represent highlights from lecture and are neither
complete nor meant to replace lecture. It is
advised not to use
these as a reliable means to replace missed
lecture material. Do so at risk to healthy
academic performance in 09-105. |
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| Lecture Outline |
The Periodic Table (continued)
Electron configurations (exceptions)
Transition metal ions
Ionization energies
Second and third ionization energies
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| All the rules we've seen about the electron
configuration filling sequence apply to both atoms and
ions of the main group elements (s-block and p-block) and
to the transition metal atoms. For transition metal ions,
the sequence changes! |
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| To explain why the 4s-3d order shifts when
ionizing an element, we resort to a familiar example,
sodium, and look at its (excited) 4s and 3d excited
one-electron orbital energies. Zeff refers to
that for atomic Na in this illustration |
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| The states are graphed at their proper
energies, but we've indicated the effective nuclear
charges drived from these energies. If an inner electron
is removed completely from Na, we can estimate that the Zeff
for the outer valence electron osup by approximately 1. |
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| The other changes are similarly estimated and
-- lo and behold -- the 3d is now more stable than the 4s
orbital. When these are filled as in the transition metal
ions, the 3d is occupied while the 4s is empty. (Keep
in mind that the values shown are just the effective
nuclear charges, but the position of the energy level
corresponds to E as determined by n and Zeff.)
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| For this course, 09-105, at CMU, we will adopt the
general rule that notes a different configuration
decision about transition metal ions as
opposed to atoms and main group ions. |
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| The energy needed to remove the easiest-to-remove
electron from a neutral atom is called the first
ionization energy. |
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| First ionization energies for light elements. Using
this information, we can estimate the effective nuclear
charge, Zeff, for the electron being removed.
Helium as an example. |
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| Zeff for lithium |
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| Zeff for neon |
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| The detailed trend in ionization energies for the
light elements |
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| The n=1 shell filling |
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| The n=2 shell filling after which the n=3 shell
starts |
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| Starting the p-subshell causes a break in the smooth
trend across the row. |
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| Starting to pair up electrons after half the
p-subshell is filled causes a second break, which we
referred to as the mid-shell dip, in the smooth trend
across the row. |
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| First ionization energies across rows 1 through 3 of
the Periodic Table |
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| Overlapping the 2nd and 3rd row element ionization
energies to demonstrate the repeating pattern (determined
by valence electron configuration) |
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| Second ionization energies |
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| First, second, and third ionization energies for the
light elements |
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| First, second, and third ionization energies shifted
to show, again, that valence electron configuration is
the determining driver |
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| Electron affinity is the energy involved in
adding an electron to a neutral atom to form a negative
ion. It is numerically equal to minus the ionization
energy for that negative ion. As such, we should expect
that the electron affinities also depend on electron
configuration. |
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