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Chapter 4: Electrolytes: Electrolytes conduct electricity when dissolved because they produce ions in aqueous solutions Strong Electrolytes: lots of ions Weak Electrolytes: few ions Non-electrolytes: molecular substance Non-ionic. Covalently bonded molecular substance Non-metals Acids: Strong acid = strong electrolyte Ion that acids make is H+ (protons) Weak acids = weak electrolyte Mostly stay together as molecules Few H+ ions produced Precipitation reactions Double Displacement Reactions leading to insoluble product. Start using states of matter in equations (aq) dissolved, (s) solid, (l) liquid, (g) gas Memorize or at least very familiar with solubility rules. Displacement Reactions DDR's often Redox reactions AB + CD ==> AD + CB SDR's always Redox reactions A + BC ==> AC + B if metal A + BC ==> AB + C if non-metal Net Ionic Equations This is a big change from Reg Chem. All equations that can be put in Net Ionic format MUST be put in Net Ionic format. Write complete balanced equation, with states of matter Rewrite Equation Ionize, dissociate anything soluble Cancel spectator ions. Write net ionic equation Acid/Base Reactions Learn Strong Acids: If not strong must be weak Learn Strong Bases: Group I and Soluble Group II hydroxides Weak base: ammonium hydroxide, amines. Neutralization: Acid + Base ==> Salt + Water Net ionic equation is always H+(aq) + OH-(aq)==> H2O(l) Exception: if base is insoluble it is not present as ions so can't cancel spectators Redox (Review your notes from Reg. Chem.)
Chapter 5 Thermodynamics Energy and work and heat are equivalent First Law of Thermodynamics Energy is conserved Exothermic reactions release stored heat to environment Delta H system is - Delta H environment is + Enthalpy is state function (stored heat) Enthalpies of Reaction (both physical changes and chemical changes) kJ or kJ/mol Check to see if the reaction produces many moles or just 1 A reaction that burns 4 moles of propane will produce more energy than one that burns 2 moles. CH4 (g) + 2 O2 (g) --> CO2 (g) + 2 H2O (g) deltaH = -802 kJ ( per mole of CH4 implied) 2CH4 (g) + 4 O2 (g) --> 2CO2 (g) + 4 H2O (g) deltaH = -1604 kJ ( per 2mole of CH4 implied) Example: How many joules are released by the burning of 28.0 grams methane in air, given that delta Hcombustion methane is -802 kJ/mol Balance equation: CH4 (g) + 2 O2 (g) --> CO2 (g) + 2 H2O (g) deltaH = -802 Kj/mol Factor label style:
= 1298.3 kJ Hess' Law. Since Enthalpy is a state function it is independent of path. So we can add subtract or multiply intermediate reactions and if we can get them to add up to the equation of interest we can calculate the overall enthalpy change by doing the same algebraic step to the enthalpies of reaction. Flip the sign if the equation is reversed, multiply by 3 if reaction tripled etc. Example: Calculate the enthalpy of reaction for: 2S (s) + 3O2 (g) --> 2 SO3 (g) Given:1.) S (s) + O2 (g) --> SO2(g) deltaH= -296.9kJ 2.) 2SO3(g) --> 2SO2(g) + O2(g) + 196.6 kJ Want 2S as a reactant, multiply reaction #1 by 2 remember multiply enthalpy also
2S (s) + 2O2 (g) -->
2S (s) + 3O2 (g) --> 2 SO3 (g) -790.4 kJ Enthalpies of formation Enthalpy required to make 1 mole of production from its constituent elements in their stable form at 25 °C and 1 atm. Units are kJ (per 1 mole is implied by definition) Enthalpy of formation of any element in its stable form at 25 ºC and 1 atm is 0 kJ.
Calorimetry Key concept: Heat lost by the hot object's cooling will be gained by the cool object's warming. Heat capacity: J/gºC how much energy is required to raise the temperature of a substance. Calorimeter constant J/°C how many Joules it takes to change a calorimeter's temperature 1°C (Must keep the calorimeter parameters constant: use exact same mass of water each trial. Heat capacity of water 4.184 J/gºC Heat of fusion of water 333.5 J/g energy required to melt (+) or liberated when freezing water. Heat of vaporization of water 2257 J/g (+) vaporizing, (-) condensing. Key relationship deltaH = m Cp delta T Example easy:
25.0 grams of water at 0 c is added to a calorimeter at 22.5 C if the ending temperature is 16 C What is the calorimeter constant. Heat gained by cold object is lost by warm object or reaction Heat gained by cold 25.0 grams x 4.184 J/g ºC x (16 ºC - 0 ºC) = + 1673.6 J. Calorimeter constant is Energy per degree of temp change -1673.6J/ -6.5 Cº = 257.5 J/ºC Now running a reaction in the exact same calorimeter, If the calorimeter is seen to rise 21.0 ºC how many calories are released by the chemical reaction? 257.5 J/ºC x 21 ºC = 5407.5 J since gain by calorimeter = loss by chemicals of reaction - 5407.5 J. Example- more thorough and complicated Modern Concept of the Atom/Atomic Structure (Chapter 6 Brown, LeMay and Others) Chapter 6: Atomic Structure and periodicity: Electromagnetic radiation: Is light a particle or a wave? Is matter energy? The smaller a bit of matter, the more wave-like it becomes.
Nature of matter:
n is quantum integer 1, 2, 3 etc. h is Planck’s constant 6.626 x –34 J∙s v =frequency of light. Photoelectric effect
Light below threshold frequency cannot remove electrons no matter what the intensity of the light For light above the threshold frequency increasing intensity does increase numbers of electrons.
hv0 is the energy required to remove the electron from the metal. Somewhat related
So m = E/c2 but we say that photons have no rest mass. Dual nature of Light Creates interference patterns, reflects, refracts just like waves Photoelectric effect best explained as particles Which is it? Both ???!!!!! DeBroglie equation
Electron diffraction by NaCl crystals have verified DeBroglie’s eqn. Hydrogen Spectra and the Bohr Model.
Bohr eqn: En= -2.178 x 10-18 J (1/n2) ΔE = E end level – E start level
c is speed of light: 2.9979 x 108 m/s λ = hc/ ΔE Quantum model of atom
The electrons travel in orbitals and have discrete quantized momenta, and therefore quantized energies. That is, not every orbit is possible but only certain specific ones, at certain specific distances from the nucleus. The electrons will not slowly lose energy as they travel, and hence will remain in stable, non-decaying orbits. Other points are: When an electron makes a jump from one orbit to another, the energy difference is carried away (or supplied) by a single quantum of light (called a photon)which has an energy equal to the energy difference between the two orbits (given by evaluating Bohr's equation) The allowed orbits depend on quantized (discrete) values of orbital angular momentum The lowest value of n is 1. This corresponds to a smallest possible radius of 0.0529 nm. This is known as the Bohr radius and an electron may get no closer to the proton. These quantized wave forms define electron orbitals that have a probability of being occupied by an electron p=0.9 4 Quantum numbers are needed to describe each electron in a many electron atom (i.e. more complex than H) n : Principal quantum number n= 1 to 7. Has a real world connotation of size. 2's bigger than 3's etc. l: angular quantum number l= 1 to 3. Has a real world connotation of shape. l= 1's are similar in shape m: magnetic quantum number m = -7 to + 7 Has a real world connotation of orientation in space. s: quantum spin s= +1/2 or - 1/2 Electrons must be spin paired in order to share an orbital.
Period Trends: You must get this under your belt. It allows you to predict outcomes that otherwise are simply a guess.
Electron affinity Ionization energy |