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Electromagnetic Spectrum
All of the frequencies or wavelengths of electromagnetic radiation
Electromagnetic Spectrum Pneumonic Device
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Longest wavelength in EM
radio waves
lower energy state to higher energy state
photon absorption
higher energy state to lower energy state
photon emission
Bohr Equation
-2.18E-18(Z^2/n^2)
energy density
pictoral representation for a given energy sublevel of the probability of the electron lying within that region
radial proabability
energy density diagram as a plot
quantum mode of atoms
atoms only have certain allowed energy states
principal quantum number (n)
indiciates size and energy level
angular momentum quantum number (l)
from 0 to n-1, gives sublevels into which energy level is divided, also relates to shape of the orbital
magnetic quantum number (ml)
describes 3D orientation of the orbital in the space around the nucleus
what does the total number of ml values tell you
the number of orbitals in that energy level
spin quantum numbers (ms)
+1/2 or -1/2, corresponds to the two possible directions of the electrons magnetic field
p orbital shape
peanut
s orbital shape
sphere
d orbital shape
4 leaf clover
f orbital shape
flower
aufbau principle
An electron occupies the lowest-energy orbital that can receive it
pauli exclusion principle
An atomic orbital may describe at most two electrons, each with opposite spin direction, no 2 - can have the the same energy level
hunds rule
all orbitals will be singly occupied before any is doubly occupied
periodic table groups
vertical columns
periodic table periods
horizontal rows
alkali metals
group 1
alkali earth metals
group 2
transition metals
groups 3 - 12
metalloids
along the periodic table staircase
periodic table group 17
halogens
periodic table group 18
noble gas
inner electrons
noble gas and all completed energy levels
outer electrons
Electrons that occupy the highest energy level
valence electrons
dame as outer for main groups (ns) but ns and (n-1)d for transition elements
electron configuration of ions in the main group
lose ns/np
electron configuration of ions in the transition group
lose ns and (n-1)d
transition element stability rule
sometimes upgrade s block to fill more stable d5 or d10
paramagnetic
dimagnetic
all electrons are paired
lewis symbols dots
valence electrons
lewis symbol lone pairs
no bonds
lewis symbol bonded piars
shared electrons
atomic radius
size of an atom
ionic radius
Distance from the center of an ion's nucleus to its outermost electron
atomic radius trend
increases down and to the left
ionic radius trend
decreases across a period and increases down a group, anions are larger cations are smaller
groups 1 and 2
low IE small EA, lose e- readily strong reducing agents and become oxidized
groups 16 and 17
high IE high EA, gain e- strong oxidizing agents and become reduced
oxidation
electron loss
reduction
electron gain
ionization energy
The amount of energy required to remove an electron from an atom
ionization energy trend
increases up and to the right
electron affinity
the energy needed to remove an electron from a negative ion to form a neutral atom or molecule
electron affinity trend
increases up and to the right
main group metals (acid or basic)
transfer electrons to oxygen, so their oxides are ionic -> act as bases
nonmetals (acid or basic)
share electrons with oxygen, so nonmetal oxides are covalent -> they form acids
amphoteric
act as acids or bases, some metals and metalloids
more metallic (larger size, smaller IE)
oxides are more basic
less metallic (smaller size, higher IE)
oxides are more acidic
ionic bond
metal + nonmetal, transfer electrons, (+)(-) attraction, not molecules
covalent bond
both nonmetal, shared attraction, attraction between e- and nucleus, molecules
octet rule
8 is more stable, or 2 for H/Li
bond order
the number of shared electron pairs between two atoms
bond strength/energy
energy needed to break bond in 1 mol of gaseous molecule
bond length
distance between nuclei of two bonded atoms
relationship bond order, length, energy
as bond order increases energy increases and length decreases
lattice energy
the energy required to separate 1 mol of the ions of an ionic compound
enthalpy of reaction calculation
hess's law and bond energy of reactants - bond energy of prodcuts
compuitng lattice energy =
heat of formation = hess law - h lattice
lattice energy and ion size
Increases with the decreasing size of the ion
lattice energy and ion charge
- Lattice energy increases with the charge on the ions
lattice energy and electronegativity
lattice energy increases as lattice energy increases
molarity
moles solute / L solution
molality
moles solute / mass solvent
conversion between molarity and molality
using density
percent yield
(Actual yield / theoretical yield) * 100
percent error
( (actual - expected) / (expected) ) * 100
beer lambert law
Used to relate the concentration of colored solutions to the amount of visible light they absorb. A = e l c
beer lambert law A
absorbance
beer lambert law e
molar absorptivity constant: different for each compound and wavelength; units=L/mol*cm
beer lambert law l
path length: distance light passes through solution (typically 1 cm for spectroscopy)
beer lambert law c
solution concentration
photoelectric effect
light hits metal above threshold -> electrons ejected when struck by photons, happens almost instantly
what is polarity caused by
electronegativity difference
wavelength of max absorbance
optimal wavelength for spectrophotometric experiment
blank use in spectrophotometric experiment
used to ignore device walls and solvent
concentration and solution shade
higher concentration results in darker shade
spectrophotometry graph
absorbance vs concentration
E when looking at moles
E = Nhc / wavelength
isoelectronic
same electron configuration