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Chem Exam 2

TermDefinition
characteristics of waves wavelength, frequency, speed, electromagnetic radiation
electromagnetic radiation provides an important means of energy transfer; one of the ways energy travels through space
wavelength the distance between two consecutive peaks or troughs in a wave
frequency number of waves (cycles) per second that pass a given point in space; low wavelength = high frequency, high wavelength = low frequency
speed of light wavelength x frequency (unit is hertz, Hz)
Planck's constant energy can be gained or lost only in whole number multiples (deltaE = nhv; h = Planck's constant (6.626 x 10^-34 J/s), v = frequency of the radiation); a quantum is a packet of energy, this means radiation waves behave like distinct particles (photons)
photoelectric effect when light strikes a metal surface, electrons can be emitted from the surface; light must be of a certain minimal frequency
Einstein's theory of relativity energy has mass, allowing us to calculate the apparent mass of a photon: m = E/c^2 (m = mass, E = energy, c = speed of light)
electrons dual nature electrons behave as particles, but also as waves when they form a diffraction pattern (when light is scattered from a regular array of points or lines)
Bohr model the electron in a hydrogen atom moves around the nucleus only in certain allowed circular orbits; model gives hydrogen atom energy levels consistent with the hydrogen emission spectrum
points about Bohr's model (1) it correctly fits the quantized energy levels of the hydrogen atom and postulates only certain allowed circular orbits for the electron
points about Bohr's model (2) as the electron becomes more tightly bound, it's energy becomes more negative relative to the 0 energy reference state (corresponding to the electron being at infinite distance from the nucleus); as electron gets closer to nucleus, energy is released
limitations to Bohr's model cannot be applied to atoms other than hydrogen, it's fundamentally incorrect
development of orbitals Schrodinger's equation allows us to determine the wave functions of an atom in terms of the total energy (E) of the atom; each solution of the equation gives us a wave function or orbital that is characterized by a particular energy value
orbital specific wave function; 1s orbital - wave function corresponding to the lowest energy for the hydrogen atom; wave function provides no info about the detailed path of an electron; orbital is a 3D region where an electron is most likely to be found
probability distribution intensity of color is used to indicate the probability value near a given point in space; represents the square of a wave function
radial probability distribution plots the total probability of finding an electron in each spherical shell versus the distance from the nucleus
hydrogen 1s orbital maximum radial probability; this is most likely the place to find an electron but lots of time, an electron will be somewhere else; size of 1s orbital: radius of the sphere that encloses 90% of the total electron probability
principal quantum number n, has integral values (1, 2, 3, etc.); related to the size and energy of the orbital; as n increases = orbital becomes larger and the electron spends more time farther from the nucleus; increase in n = higher energy because electron is less tightly bound
angular momentum quantum number l, has integral values from 0 to n-1 for each value of n; related to shape of atomic orbitals; value of l for a particular orbital is commonly assigned a letter: l = 0 is s, l = 1 is p, l = 2 is d, l = 3 is f
magnetic quantum number ml, has integral values between l and -l, including 0; the value of ml is related to the orientation of the orbital in space relative to the other orbitals in the atom
shape of s orbitals one lobe/sphere
shape of p orbitals two lobes separated by a node at the nucleus; one lobe has a positive sign, other lobe has a negative sign; occur in 3 orientations (-1, 0, 1 magnetic quantum number - x, y, and z orientations)
shape of d orbitals first appear in n=3; off-axis lobes; lobes have different signs for mathematical function; occur in five orientations (-2, -1, 0, 1, 2 magnetic quantum number - rename to xz, yz, xy, x2-y2, and z2)
shape of f orbitals first appear in n=4; more complex shapes
orbital energies all orbitals with the same n value are degenerate (have the same energy)
nodes areas of high probability separated by areas of zero probability; number of nodes increases as n increases
electron spin quantum number ms, can be +1/2 or -1/2 to imply the electron can spin in two diff directions; in each orbital you can have two electrons and they must have opposite spins
Pauli exclusion principle in an atom, no two electrons can have the same set of four quantum numbers
polyelectronic atom atoms with more than one electron; forces- attraction to nucleus due to opposite charge, repulsion from other electrons due to same charge; since electron paths are unknown, the electron repulsions can't be calculated
orbitals in polyelectronic atoms hydrogen-like orbitals, similar shapes; diff sizes and energies due to added electron repulsion; electrons prefer to be in lowest energy orbital available (spend time closer to nucleus)
Aufbau principle as protons are added one by one to the nucleus to build up the elements, electrons are similarly added to hydrogen-like orbitals
Hund's rule lowest energy configuration for an atom is the one having the maximum number of unpaired electrons allowed by Pauli principle in a particular set of degenerate orbitals (unpaired electrons have parallel spins)
orbital diagrams depiction of quantum number assignments for electrons; where electrons are (boxes with arrows); electron configuration = 1s2 2s2, etc.
valence electrons the electrons in the outermost principal quantum level of an atom; involved in bonding; elements in the same group (vertical column) have the same valence electron configuration and show similar chemical behavior
noble gas electron configuration to avoid writing inner-level electrons, can write electron configuration starting from the previous noble gas (ex. for oxygen, original: 1s2 2s2 2p4; noble gas: [He] 2s2 2p4)
ionization energy energy required to remove an electron from a gaseous atom or ion; increases from left to right and decreases going down a group
electron affinity energy change associated with the addition of an electron to a gaseous atom; decreases from left to right and increases going down a group
atomic radius half the distance between the nuclei of atoms in a chemical compound; decreases from left to right and increases down a group
ionic bonds force of attraction between oppositely charged ions, usually between metal and nonmetal; usually balance opposing charges evenly to reach a neutral molecule (cation - positive; anion - negative)
covalent bond formed by sharing electrons between atoms
forces in ionic bonds attraction to the protons in the nucleus
bond energy the energy required to break a bond in a chemical compound
size of ions positive ions- decrease in radius because you're getting rid of an orbital negative ions- increase in radius because you're adding on or filling an orbital
isoelectronic ions ions containing the same number of electrons; size decreases as number of protons increases in a group of isoelectronic ions because electrons experience a greater attraction as the positive charge on the nucleus increases
forces in covalent bonds electron is attracted to protons in both nuclei, there is electron-electron repulsion for both atoms but less for one atom
bond length distance between the nuclei of two atoms in a bond; the position at which the energy associated with the compound is minimal
polar covalent bond unequal sharing of electrons between the two atoms forming the covalent bond (one atom has partial negative charge, one has partial positive)
electronegativity ability of an atom in a molecule to attract shared electrons to itself; differences in electronegativity affect the type of bond formed: no difference (<0.5) = pure covalent; small difference (<2) = polar covalent; large difference (>2) = ionic
electronegativity trend increases left to right, decreases going down a group
dipole moment molecules that have a center of positive charge and a center of negative charge are called dipolar; any diatomic molecule with a polar bond will have a dipole moment (arrow points to partial negative atom and end of arrow goes on partial positive atom)
lone pairs those pairs of electrons to be localized on an atom (not bonded to other atom)
bonding pairs those electrons found in the space between atoms
Lewis dot structure a way of depicting atoms and compounds that shows location of all valence electrons; helps visualize octet rule and appropriate bonding configurations
drawing lewis structures determine number of valence electrons, draw skeleton structure, draw a single bond between each set of atoms, fill in octets of the atoms, working from outside of the molecule in, until all remaining electrons are used up
formal charge number of valence electrons on free atom - number of valence electrons assigned to the atom in the molecule; atoms try to have formal charges as close to 0 as possible, any negative formal charges are expected to reside on the most electronegative atoms
resonance occurs when more than one valid Lewis structure can be written for a particular model; indicates that the resulting electron structure of the molecule is given by the average of the valid Lewis structures
VSEPR model valence shell electron-pair repulsion; molecular structure- 3D arrangement of molecules in an atom; predicts the molecular structure of molecules formed from nonmetals
VSEPR main postulate structure around a central atom is determined by minimizing electron-pair repulsion
location of lone pairs in VSEPR structures lone pairs take up more space than bonding pairs so orientation will minimize electron repulsion; often compresses angle of bonded pairs; two lone pairs will point away from each other
VSEPR problem solving draw lewis structure, determine number of lone pairs and bonds around central atom, number of lone pairs + bonds equals the electronic geometry, number of bonds determines molecular geometry
two bonded pairs linear; pairs are 180 degrees from each other on opposite sides of central atom
three bonded pairs trigonal planar; each pair is 120 degrees from each other
four bonded pairs tetrahedral; 109.5 degree bond angle
three bonded pairs and one lone pair trigonal pyramid; each pair is <120 degrees from each other
two bonded pairs, one/two lone pairs bent; <120 degree bond angles
five bonded pairs trigonal bipyramidal; 120 and 90 degree bond angles
six bonded pairs octahedral; 90 degree bond angles
no single central atom molecular structure can be predicted from the arrangement of pairs around multiple central atoms
four bonded pairs and one lone pair see-saw; 90, 120, and 180 degree bond angles
three bonded pairs and two lone pairs t-shaped; 90 and 180 degree bond angles
two bonded pairs and three lone pairs linear; 180 degree bond angles
four bonded pairs and two lone pairs square planar; 90 and 180 degree bond angles
five bonded pairs and one lone pair square pyramidal; 90 and 180 degree bond angles
Created by: jpawloski
 

 



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