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CHEM HL YEAR REVIEW

  • Elements: The most simple, cannot be broken down, the basis of matter.

  • Mixtures: 2+ substances physically bonded NOT in fixed ratio. They retain individual properties and can be physically separated.

  • Compounds: 2+ elements chemically bonded, fixed ratio. They have new properties, and can't be physically broken.

  • Kinetic Molecular Theory: Explains physical properties of matter & change of state. Uses symbols & good pics.

  • Temperature (T): Average kinetic energy of particles.

  • Kelvin (K): SI unit of temperature with same increments as Celsius (C).

    • K = C + 273

  • Atom: Negatively charged, dense nucleus; occupy space outside nucleus.

  • Subatomic particles: Protons (+), neutrons (neutral), electrons (-).

    • Relative masses/charges of subatomic particles should be known

  • Atomic Mass (A): Mass of electron negligible.

  • Atomic number (Z): Number of protons.

  • Isotopes: Atoms of same element with different number of neutrons -> same chemical properties, different physical properties.

  • Emission spectra: Produced when photons are emitted from atoms as electrons in excited states return to lower energy levels.

  • Line emission spectrum of hydrogen: Provides evidence for the existence of electrons in discrete energy levels.

  • Relationship between energy, wavelength, frequency: Which converge at higher energies.

  • Continuous spectrum vs. line spectrum: Energy across electromagnetic spectrum (EMS).

  • Emission spectrum of hydrogen atom: Lines & energy transitions to 1st, 2nd, 3rd energy levels.

  • Main energy level: Given integer number, n. Can hold maximum of 2n2 electrons.

  • Division of main energy level into s, p, d, f sublevels: Of successively higher energy.

  • Orbitals: Have defined energy, shape for e-'s, and orientation and chemical environment; can hold 2 e-'s of opposite spin.

  • Aufbau principle: e-'s occupy each energy level to reduce max e-, Hund's rule, Pauli exclusion principle to reduce e- configuration.

  • e- configuration: (long) for atoms and ions up to Z=36; (full e- configuration), condensed ([Ne]3s2).

  • Ionization Energy: Energy required to remove one mol e-'s from one mol of gaseous atoms (kJ mol-1).

    • Can be calculated from emission spectra.

    • X(g) -> X+(g) + e-

  • Exceptions: To the Aufbau principle, there are two exceptions.

    • Exception #1

      • Be -> B: new e- is easier to remove

      • Mg -> Al: must be at a higher energy

      • Evidence for sublevels -> p is higher energy than s

    • Exception #2: Hund's rule

  • 2nd IE: X+(g) -> e- + X2+(g)

  • The mole (mol): An SI unit for an amount of something.

    • 6.02 * 1023 "entities" (cations/molecules/ions/e's...).

  • Ar: Relative atomic mass = weighted average of isotope abundances.

  • Mr: Relative molecular mass = add Ar for each atom in compound.

    • Mr = relative molecular mass = the mass of "C"

  • Mr: Molar mass = # HRS units of 1 mol.

  • Empirical formula: Simplest whole # ratio of elements in a compound.

    • Steps for converting to empirical formula:

      1. Treat percentages like grams

      2. Convert g -> mol of atoms for each element

      3. Divide all by smallest mol amount

      4. Multiply all to get whole numbers

  • Molecular formula: Actual formula.

  • Molar concentration of solutions:

    • Concentration mol dm-3 = mol/ dm3 solvent

  • Ideal gases: Particles moving with elastic collisions

    • Breaks down @ low temps: intermolecular forces.

    • Breaks down @ low volume: negligible particle volume

  • For the same gas sample (constant n):

    • P1V1/T1 = P2V2/T2

  • Ionic Bonding: Typically a metal & nonmetal.

    • Charged ions arranged in a lattice

    • Lattice enthalpy: strength of ionic bond, and becomes stronger with 1) higher charges and 2) smaller ions.

  • Physical properties of ionic compounds:

    • Volatility: Low b/c strong bonding (can't move)

    • Electrical conductivity: NO as solid (ions can't move) yes molten/liquid (ions can move)

    • Solubility: Based on lattice enthalpy; more soluble in polar solvent

    • Brittle = solids fracture when force applied

  • Metallic Bonding: An electrostatic attraction between a metal lattice & a "sea" of delocalized e's.

  • Physical Properties of metallic bonding:

    • High melting & boiling points (smaller ions & higher charges = stronger)

    • Electrical conductivity: yes solid (delocalized e's can move) yes liquid

    • Thermal conductivity (good at it) -> delocalized e's can carry/transfer heat quickly

    • Malleability & ductility

      • Can be beaten into a wire -> b/c cations can slide past each other without breaking a bond

      • Can be hammered -> into a drawn

  • Covalent Bonding: (includes metalloids)

    • Typically 2 nonmetals

    • An electrostatic attraction between shared pair(s) of e-'s & positive nuclei on either side of the e-'s.

  • Coordinate bond: When one atom donates both shared e-'s.

  • Electronegativity: Relative attraction an atom has for a shared pair of e-'s; polarity of a bond is based on EN difference

  • VSEPR Shapes: Linear, trigonal planar, bent, tetrahedral, trigonal pyramidal, bent.

  • Molecular Polarity: Based on bond polarities & shape; larger molecules = stronger dispersion forces

  • Size & polarity determine volatility: -> polar = dipole-dipole = hydrogen bonding -> high melting/boiling points (solids); non-polar = dispersion forces -> generally low melting/boiling -> volatile.

  • Giant covalent structures:

    • No conductivity (except graphite)

    • Si, SiO2 -> sand

  • Allotropes of carbon:

    • Diamond, graphite, fullerenes

  • Sigma bonds (σ): Head-on, linear combination of orbitals.

    • e- density is on the bond axis (between nuclei)

    • Single bond is always sigma bond.

  • Pi bonds (π): Lateral combination of p-orbitals.

    • e- density on opposite sides of bond axis.

    • Always form as 2nd or 3rd bond.

  • Hybridization: Mixing different orbital types.

  • Resonance structures: When there is more than one position for a double bond.

  • Formal Charge: A man-made concept to "determine" which Lewis structure is "preferred".

    • FC = V - N - 1/2B

    • Calculate for each atom

    • Preferred structure is closer to all zeroes

  • Polymers: Made of many repeating units (monomers).

    • Join together chemically

    • Form macromolecules

  • Condensation Polymers: Form by removing H2O.

  • Addition Polymers: Form by breaking a double bond.

  • Transition Elements: Shows variable oxidation states with at least one having an incomplete d sublevel.

  • All can be +2, b/c they lose their 4s e's first (easiest to take); there is not a big difference in energy between 4s & 3d.

  • Have magnetic properties (ferro/para/diamagnetic).

  • Form colored compounds

    • Form complex ions with ligands

  • Colored Complexes: In a free ion, the five d-orbitals are degenerate (equal in energy).

    • A ligand approaches to form a coordination bond with the ion

    • As the ligand approaches, the d-orbitals split

    • Light passing through the compound is absorbed & promotes an electron to the higher d-orbital

    • The non-absorbed colors are transmitted; we see the color complementary to the light/was absorbed (color wheel).

      • Factors affecting color seen:

        1. Geometry of the complex ion formed (we know octahedral)

        2. Which transition metal

        3. Oxidation state of the metal

        4. The ligand (strengths given below color wheel)

  • Stereoisomers: Same connectivities & bond multiplicities -> different 3-D arrangement.

  • Cis/trans isomers: Alkenes & cycloalkanes

    • Have free rotation

  • Optical isomers: Can bend polarized light

    • Contain a chiral carbon (attached to 4 different groups)

    • Enantiomers = non-superimposable "mirrored" images

  • Mass spectroscopy: Used to find molecular mass and fragmentation patterns.

    • M+ = molecular ion

  • IR Spectroscopy: Makes their bonds vibrate

    • Greenhouse gases absorb IR wavelengths of light which stops the light/ heat from escaping back out into space

  • Proton nuclear magnetic resonance (1H NMR):

    • What H environments exist

    • How many H environments (number of peaks)

    • How many H's in each environment (integral trace)

    • How many H's are in the adjacent environment (splitting pattern)

  • Atomic Radius: 1/2 of distance between 2 nuclei.

  • First Ionization Energy: The energy required to remove 1 mol of e-'s from 1 mol gaseous atoms (kJ mol-1).

    • X -> X+ + e-

  • Electron affinity: Energy change to add 1 mole e- to 1 mol gaseous atoms.

    • X(g) + e- -> X-(g)

  • Oxidation States: Number to show e-'s "transferred" when forming a bond

    • *Elements always +1 (except in hydrides, H-)

    • *Oxygen always -2 (except -1 in peroxides, H2O2)

    • *Hydrogen always +1 (except -1 in hydrides e.g., LiH)

  • Chemical reactions: Involve the transfer of energy between the system and surroundings; no energy is destroyed.

  • Temperature: Average kinetic energy.

  • Heat: Total energy (kJ).

  • Exothermic: If energy is transferred to the surroundings, the surroundings will get warmer, the surroundings get colder.

  • Endothermic: If the surroundings transfer energy to the reaction, the surroundings get colder.

  • Activation energy: Energy needed to break ionic lattice.

  • Reaction coordinate:

  • Bond Enthalpies: ΔH = energy within a bond in a gaseous molecule.

    • It's an average value

  • Covalent bond enthalpy: Energy within a bond of a gaseous molecules.

    • Form/from gaseous atoms.

  • Atomization energy: Energy needed to form 1 mol gaseous atoms from a standard state element; always endothermic.

  • Ionization energy: Energy needed to remove 1 mole e- from 1 mol gaseous atoms; always endothermic.

  • Lattice enthalpy: Forming/breaking an ionic lattice from/into gaseous ions.

    • Forming bonds = very exothermic

    • Breaking bonds = endothermic

    • Magnitude is based on ionic bond strengths: stronger when smaller & has higher charge

  • Combustion: Reactive metals, nonmetals, hydrocarbons in excess O2 to form oxides.

    • ΔHcΘ is the enthalpy change when 1 mol of substance completely combusts at standard conditions.

      • -kJ mol-1

  • Incomplete combustion: In limited O2, form some amounts of CO/C.

    • And/or soot & less energy is released

  • Fossil fuels: Variety compounds formed through decomposition of biological materials.

    • Reduction of biological complexes.

      • Contain C, H, O, N, S & metals

  • Petroleum: Mostly hydrocarbons

  • Natural gas: Mostly CH4, small sulfur compounds.

  • Coal: Mostly C, small hydrocarbons, sulfur compounds & metals.

  • Biofuels: Made from plant/animal matter; derived directly/ indirectly from sunlight.

  • Fuel Cells: Electrochemical energy comes from chemical reaction.

    • Combustion where oxidation is occurring - the anode

  • Greenhouse gases: The greenhouse effect occurs when CO2, CH4 or nitrogen oxides absorb IR radiation emitted from Earth's surface after they've been heated by the sun's rays.

    • Greenhouse gases emit IR radiation in all directions so net effect is higher solar energy trapped in atmosphere; global temp becomes higher

    • Why greenhouse gases absorb infrared radiation: Molecules can vibrate as the bonds in them stretch & bend. The energy used here is infrared energy. If the stretching & bending involves a change in dipole moment, the vibrations are IR active.

CHEM HL YEAR REVIEW

  • Elements: The most simple, cannot be broken down, the basis of matter.

  • Mixtures: 2+ substances physically bonded NOT in fixed ratio. They retain individual properties and can be physically separated.

  • Compounds: 2+ elements chemically bonded, fixed ratio. They have new properties, and can't be physically broken.

  • Kinetic Molecular Theory: Explains physical properties of matter & change of state. Uses symbols & good pics.

  • Temperature (T): Average kinetic energy of particles.

  • Kelvin (K): SI unit of temperature with same increments as Celsius (C).

    • K = C + 273

  • Atom: Negatively charged, dense nucleus; occupy space outside nucleus.

  • Subatomic particles: Protons (+), neutrons (neutral), electrons (-).

    • Relative masses/charges of subatomic particles should be known

  • Atomic Mass (A): Mass of electron negligible.

  • Atomic number (Z): Number of protons.

  • Isotopes: Atoms of same element with different number of neutrons -> same chemical properties, different physical properties.

  • Emission spectra: Produced when photons are emitted from atoms as electrons in excited states return to lower energy levels.

  • Line emission spectrum of hydrogen: Provides evidence for the existence of electrons in discrete energy levels.

  • Relationship between energy, wavelength, frequency: Which converge at higher energies.

  • Continuous spectrum vs. line spectrum: Energy across electromagnetic spectrum (EMS).

  • Emission spectrum of hydrogen atom: Lines & energy transitions to 1st, 2nd, 3rd energy levels.

  • Main energy level: Given integer number, n. Can hold maximum of 2n2 electrons.

  • Division of main energy level into s, p, d, f sublevels: Of successively higher energy.

  • Orbitals: Have defined energy, shape for e-'s, and orientation and chemical environment; can hold 2 e-'s of opposite spin.

  • Aufbau principle: e-'s occupy each energy level to reduce max e-, Hund's rule, Pauli exclusion principle to reduce e- configuration.

  • e- configuration: (long) for atoms and ions up to Z=36; (full e- configuration), condensed ([Ne]3s2).

  • Ionization Energy: Energy required to remove one mol e-'s from one mol of gaseous atoms (kJ mol-1).

    • Can be calculated from emission spectra.

    • X(g) -> X+(g) + e-

  • Exceptions: To the Aufbau principle, there are two exceptions.

    • Exception #1

      • Be -> B: new e- is easier to remove

      • Mg -> Al: must be at a higher energy

      • Evidence for sublevels -> p is higher energy than s

    • Exception #2: Hund's rule

  • 2nd IE: X+(g) -> e- + X2+(g)

  • The mole (mol): An SI unit for an amount of something.

    • 6.02 * 1023 "entities" (cations/molecules/ions/e's...).

  • Ar: Relative atomic mass = weighted average of isotope abundances.

  • Mr: Relative molecular mass = add Ar for each atom in compound.

    • Mr = relative molecular mass = the mass of "C"

  • Mr: Molar mass = # HRS units of 1 mol.

  • Empirical formula: Simplest whole # ratio of elements in a compound.

    • Steps for converting to empirical formula:

      1. Treat percentages like grams

      2. Convert g -> mol of atoms for each element

      3. Divide all by smallest mol amount

      4. Multiply all to get whole numbers

  • Molecular formula: Actual formula.

  • Molar concentration of solutions:

    • Concentration mol dm-3 = mol/ dm3 solvent

  • Ideal gases: Particles moving with elastic collisions

    • Breaks down @ low temps: intermolecular forces.

    • Breaks down @ low volume: negligible particle volume

  • For the same gas sample (constant n):

    • P1V1/T1 = P2V2/T2

  • Ionic Bonding: Typically a metal & nonmetal.

    • Charged ions arranged in a lattice

    • Lattice enthalpy: strength of ionic bond, and becomes stronger with 1) higher charges and 2) smaller ions.

  • Physical properties of ionic compounds:

    • Volatility: Low b/c strong bonding (can't move)

    • Electrical conductivity: NO as solid (ions can't move) yes molten/liquid (ions can move)

    • Solubility: Based on lattice enthalpy; more soluble in polar solvent

    • Brittle = solids fracture when force applied

  • Metallic Bonding: An electrostatic attraction between a metal lattice & a "sea" of delocalized e's.

  • Physical Properties of metallic bonding:

    • High melting & boiling points (smaller ions & higher charges = stronger)

    • Electrical conductivity: yes solid (delocalized e's can move) yes liquid

    • Thermal conductivity (good at it) -> delocalized e's can carry/transfer heat quickly

    • Malleability & ductility

      • Can be beaten into a wire -> b/c cations can slide past each other without breaking a bond

      • Can be hammered -> into a drawn

  • Covalent Bonding: (includes metalloids)

    • Typically 2 nonmetals

    • An electrostatic attraction between shared pair(s) of e-'s & positive nuclei on either side of the e-'s.

  • Coordinate bond: When one atom donates both shared e-'s.

  • Electronegativity: Relative attraction an atom has for a shared pair of e-'s; polarity of a bond is based on EN difference

  • VSEPR Shapes: Linear, trigonal planar, bent, tetrahedral, trigonal pyramidal, bent.

  • Molecular Polarity: Based on bond polarities & shape; larger molecules = stronger dispersion forces

  • Size & polarity determine volatility: -> polar = dipole-dipole = hydrogen bonding -> high melting/boiling points (solids); non-polar = dispersion forces -> generally low melting/boiling -> volatile.

  • Giant covalent structures:

    • No conductivity (except graphite)

    • Si, SiO2 -> sand

  • Allotropes of carbon:

    • Diamond, graphite, fullerenes

  • Sigma bonds (σ): Head-on, linear combination of orbitals.

    • e- density is on the bond axis (between nuclei)

    • Single bond is always sigma bond.

  • Pi bonds (π): Lateral combination of p-orbitals.

    • e- density on opposite sides of bond axis.

    • Always form as 2nd or 3rd bond.

  • Hybridization: Mixing different orbital types.

  • Resonance structures: When there is more than one position for a double bond.

  • Formal Charge: A man-made concept to "determine" which Lewis structure is "preferred".

    • FC = V - N - 1/2B

    • Calculate for each atom

    • Preferred structure is closer to all zeroes

  • Polymers: Made of many repeating units (monomers).

    • Join together chemically

    • Form macromolecules

  • Condensation Polymers: Form by removing H2O.

  • Addition Polymers: Form by breaking a double bond.

  • Transition Elements: Shows variable oxidation states with at least one having an incomplete d sublevel.

  • All can be +2, b/c they lose their 4s e's first (easiest to take); there is not a big difference in energy between 4s & 3d.

  • Have magnetic properties (ferro/para/diamagnetic).

  • Form colored compounds

    • Form complex ions with ligands

  • Colored Complexes: In a free ion, the five d-orbitals are degenerate (equal in energy).

    • A ligand approaches to form a coordination bond with the ion

    • As the ligand approaches, the d-orbitals split

    • Light passing through the compound is absorbed & promotes an electron to the higher d-orbital

    • The non-absorbed colors are transmitted; we see the color complementary to the light/was absorbed (color wheel).

      • Factors affecting color seen:

        1. Geometry of the complex ion formed (we know octahedral)

        2. Which transition metal

        3. Oxidation state of the metal

        4. The ligand (strengths given below color wheel)

  • Stereoisomers: Same connectivities & bond multiplicities -> different 3-D arrangement.

  • Cis/trans isomers: Alkenes & cycloalkanes

    • Have free rotation

  • Optical isomers: Can bend polarized light

    • Contain a chiral carbon (attached to 4 different groups)

    • Enantiomers = non-superimposable "mirrored" images

  • Mass spectroscopy: Used to find molecular mass and fragmentation patterns.

    • M+ = molecular ion

  • IR Spectroscopy: Makes their bonds vibrate

    • Greenhouse gases absorb IR wavelengths of light which stops the light/ heat from escaping back out into space

  • Proton nuclear magnetic resonance (1H NMR):

    • What H environments exist

    • How many H environments (number of peaks)

    • How many H's in each environment (integral trace)

    • How many H's are in the adjacent environment (splitting pattern)

  • Atomic Radius: 1/2 of distance between 2 nuclei.

  • First Ionization Energy: The energy required to remove 1 mol of e-'s from 1 mol gaseous atoms (kJ mol-1).

    • X -> X+ + e-

  • Electron affinity: Energy change to add 1 mole e- to 1 mol gaseous atoms.

    • X(g) + e- -> X-(g)

  • Oxidation States: Number to show e-'s "transferred" when forming a bond

    • *Elements always +1 (except in hydrides, H-)

    • *Oxygen always -2 (except -1 in peroxides, H2O2)

    • *Hydrogen always +1 (except -1 in hydrides e.g., LiH)

  • Chemical reactions: Involve the transfer of energy between the system and surroundings; no energy is destroyed.

  • Temperature: Average kinetic energy.

  • Heat: Total energy (kJ).

  • Exothermic: If energy is transferred to the surroundings, the surroundings will get warmer, the surroundings get colder.

  • Endothermic: If the surroundings transfer energy to the reaction, the surroundings get colder.

  • Activation energy: Energy needed to break ionic lattice.

  • Reaction coordinate:

  • Bond Enthalpies: ΔH = energy within a bond in a gaseous molecule.

    • It's an average value

  • Covalent bond enthalpy: Energy within a bond of a gaseous molecules.

    • Form/from gaseous atoms.

  • Atomization energy: Energy needed to form 1 mol gaseous atoms from a standard state element; always endothermic.

  • Ionization energy: Energy needed to remove 1 mole e- from 1 mol gaseous atoms; always endothermic.

  • Lattice enthalpy: Forming/breaking an ionic lattice from/into gaseous ions.

    • Forming bonds = very exothermic

    • Breaking bonds = endothermic

    • Magnitude is based on ionic bond strengths: stronger when smaller & has higher charge

  • Combustion: Reactive metals, nonmetals, hydrocarbons in excess O2 to form oxides.

    • ΔHcΘ is the enthalpy change when 1 mol of substance completely combusts at standard conditions.

      • -kJ mol-1

  • Incomplete combustion: In limited O2, form some amounts of CO/C.

    • And/or soot & less energy is released

  • Fossil fuels: Variety compounds formed through decomposition of biological materials.

    • Reduction of biological complexes.

      • Contain C, H, O, N, S & metals

  • Petroleum: Mostly hydrocarbons

  • Natural gas: Mostly CH4, small sulfur compounds.

  • Coal: Mostly C, small hydrocarbons, sulfur compounds & metals.

  • Biofuels: Made from plant/animal matter; derived directly/ indirectly from sunlight.

  • Fuel Cells: Electrochemical energy comes from chemical reaction.

    • Combustion where oxidation is occurring - the anode

  • Greenhouse gases: The greenhouse effect occurs when CO2, CH4 or nitrogen oxides absorb IR radiation emitted from Earth's surface after they've been heated by the sun's rays.

    • Greenhouse gases emit IR radiation in all directions so net effect is higher solar energy trapped in atmosphere; global temp becomes higher

    • Why greenhouse gases absorb infrared radiation: Molecules can vibrate as the bonds in them stretch & bend. The energy used here is infrared energy. If the stretching & bending involves a change in dipole moment, the vibrations are IR active.

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