Chapter 5 Flashcards

(38 cards)

1
Q

thermodynamics

A

the study of energy and its transformations

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2
Q

thermochemistry

A
  • the study of the relation between chemical reactions and changes in energy
    • chemical rxns: energy transferred as heat
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3
Q

heat(q)

A
  • the energy transferred between objects because of a difference in their temperatures
  • not a state function
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4
Q

thermal equilibrium

A

a condition in which temperature is the same throughout a material and no further energy transfer occurs

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5
Q

work(w)

A
  • the energy required to move(cause motion) an object through a given distance
  • work is a form of energy
    • work = Force x distance
  • not a state function
    • w = -PΔV
  • work done by the system leads to an increase in the system’s volume AND transfers energy to the surroundings
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6
Q

potential energy (PE)

A
  • the energy stored in an object because of its position
  • on a moecular level:
    • chemical bonds and differential electric charges cause interactions btwn particles that give rise to PE
    • temperature governs motion
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7
Q

state function

A
  • a property based solely on a current chemical and/or physical state
    • it is independent of the path followed to acquire PE
      • ΔH and ΔE are state functions (also T,V,etc)
    • depends only on difference btwn initial and final states
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8
Q

kinetic energy(KE)

A
  • KE depends on mass and velocity
    • velocity depends on temp too so KE depends on temp
  • the energy of an object in motion due to its mass and speed
    • KE = 1/2(m)(u)​2
    • u=speed
  • KE on a molcular level
    • as temp increases, avg. KE increases
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9
Q

thermal energy

A
  • the KE associated with the total random motion of molecules
  • thermal energy is proportional to temp
  • thermal energy depends on # of particles in a sample
    • more molcules = more themal energy if temp is constant
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10
Q

electrostatic potential energy (Eel)

A
  • the energy a particle has b/c of its electrostatic charge and its position w/ respect to another particle
  • Eel is proportional to (Q1 x Q2)/d
    • d = distance btwn two particles
    • Q1 and Q2 = charge of each particle
  • postive Eel = particles repel
  • negative Eel = particles attract
  • A lower electrostatic PE (a more negative Eel) indicates greater stability
  • total energy always = KE due to random motion of particles + PE due to particle arrangment
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11
Q

energy(E)

A
  • the ability to do work and/or transfer heat
  • the energy given off/absorbed during a rxn is equal to the difference in the energy of the reactants and the products
    • positive = absorbed?
    • negative = released?
  • energy ca be used to do work, transfer heat
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12
Q

system

A
  • the specific part of the universe we are studying
    • often a chemical rxn or physical process
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13
Q

surroundings

A
  • everything that is not part of the system
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14
Q

isolated system

A
  • a system that exchanges neither energy nor matter with the surroundings
    • a thermos of hot soup with the lid screwed on tightly
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15
Q

closed system

A
  • a system that exchanges energy, but NOT matter with the surroundings
    • a cup of hot soup with a lid
      • heat goes out
  • most real systems we deal with are closed b/c they are easier to model quantitatively
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16
Q

open system

A
  • a system that exchanges both energy and matter with the surrooundings
    • an open cup of hot soup
      • matter goes out as steam
      • matter goes in as crackers cheese and pepper
      • heat goes out
  • cells, organisms, and Earth are all open
17
Q

exothermic process

A
  • energy flows from system to surroundings
  • q is negative
18
Q

endothermic

A
  • energy flows from surroundings into system
  • q is positive
19
Q

internal energy(E)

A
  • E = KE of all components system + PE of system
    • not possible to determine exact values
  • ΔE= Efinal - Einitial
    • a state function b/c ΔE depends only on the initial and final states….how the change occurs in the system doesn’t matter
  • doing work on a system adds to its internal energy
  • total increase of the internal energy of a closed system
    • ΔE = q+w
20
Q

first law of thermodynamics

A
  • essentially the law of conservation of energy
  • The energy (ΔE=q+w) gained or lost by a system must equal the energy gained or lost by the surroundings
    • ΔEsys+ΔEsurr=0
  • when work is done by a system on its surroundings, internal energy of system decreases
  • pressure-volume work(P-V work):
    • the work associated with the expansion or compression of a gas
    • when the pressure on a system remains constant but the volume of the system changes
      • a hot air balloon- heating the balloon causes volume to increase even though atmospheric pressure remains constant
21
Q

calorie(cal)

A

the amount of energy necessary to raise the temp of 1 gram of water by 1˚C

22
Q

joule(J)

A
  • the SI unit of energy
  • 4.184 J = 1 cal
23
Q

enthalpy change (ΔH)

A
  • the heat absorbed by an endothermic process or given off by an exothermic process occurring at constant pressure
    • ΔH = qp = ΔE + PΔV
      • qp = enthalpy change at constant pressure
  • ΔH<0 when energy flows out of a system and q<0
  • ΔH>0 when energy flows into a system and q>0
24
Q

enthalpy(H)

A
  • ΔH is defined as heat transferred at constant pressure
    • ΔH>0 = endothermic
    • ΔH<0 = exothermic
  • the sum of the internal energy and the pressure-volume product
    • H = E + PV
      • difficult to calculate so we use ΔH
  • unit is J or J/g or J/mol
  • ΔH and ΔE represent changes in a state function of a system
25
difference between ΔE and ΔH
* ΔE includes *all* the energy(heat and work) exchanged the sys with the surr * ΔE = q + w * ΔH is *only* q, the heat, exchanged at constant pressure * ΔH = qp * ΔE and ΔH are very similar with constant volumes
26
molar heat capacity (cp)
* the quantity of energy required to raise the temp of 1 mole of a substance by 1˚C at constant pressure * q = ncpΔT * ΔT is in Celsius * units = J/mol˚C
27
specific heat(cs)
* the quantity of energy required to raise the temp of 1 gram of a substane by 1˚C at constant pressure * units = J/g˚C
28
molar enthalpy of fusion(ΔHfus)
* the energy required to convert 1 mole of a solid substance at its melting point into the liquid state * Ex: the energy absorved as snow melts * q = nΔHfus
29
molar enthalpy of vaporization (ΔHvap)
* the energy required to convert 1 mole of a liquid substance at its boiling point to the gas/vapor state * q = nΔHvap
30
calorimetry
* the measurement of the quantity of energy transferred during a physical change or chemical process * **calorimeter:** device used to measure absorption or release of energy by a physical change/chem process * assume a **closed system** * heat from sys = heat to surr * qsys + qcal =0
31
enthalpy of reaction(ΔHrxn)
* used to quantify the (heat) energy absorbed or given off by a chemical reaction under constant pressure * * aka heat of reaction * ΔHrxn\<0 when exothermic aka heat is released * exiting system and going into surroundings * ΔHrxn\>0 when endothermic aka heat is absorbed * entering system from the surroundings
32
thermochemical equation
the chemical equation of a reaction that includes the change in enthalpy that accompanies that reaction
33
heat capacity(Cp)
* the quantity of energy needed to raise the temperature of an object by 1˚C at constant pressure * referred to as a calorimeter constant (Ccal) * this value is unique to every calorimeter so units are NEVER J/g˚C or J/mol˚C * units=J/˚C * qcalorimeter=CcalorimeterΔT * we can then use qcal to calculate quantities of energy produced * qcal = -ΔHrxn
34
Hess's law
* the principle that the enthalpy or reaction(ΔHrxn) for a reaction that is the sum of two or more reactions is equal to the sum of the ΔHrxn values of the constituent reactions * ΔH is a state function, so we can... * 1) multiply the coefficients by a common factor * 2) reverse the rxn if we flip the sign of ΔH * Hess's law works b/c enthalpy is a state function * for a particular set of reactants and products, the enthalpy change is the same regardless of how many steps the rxn took
35
standard enthalpy of formation(ΔH˚f)
* the enthalphy change of a **formation rxn** * **​formation rxn:** when 1 mole of a substance is formed from its constituent elemtns in their standard states * aka [standard] heat of formation * formation reaction DOES NOT EQUAL real life synthesis
36
standard conditions+states
* indicated by the ˚ in ΔH˚f, **standard** **conditions** are 1 atm, usually 25˚C, and 1M concentration * **standard states:** the most stable form of a substance under standard conditions * a pure element in its most stable form under standard conditions has ΔH˚f = 0
37
standard enthalpy of reaction(ΔH˚rxn)
* the energy associated with a rxn that takes place under standard conditions * aka standard heat of rxn
38
phase changes