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enthalpy

Amelia Claire Chemistry 100 Inglés 13 fichas

enthalpy

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  1. 1Conservation of Energy 1st Law of ThermodynamicsEnergy can neither be created nor destroyed - it can only change form
    The total Energy of the universe is constant
    = 1st Law of Thermodynamics
  2. 2SystemSystem = part of universe under study (e.g. - chemicals in a flask)
  3. 3SurroundingsSurroundings = the rest of the universe (or as much as needed (e.g. - the flask)
  4. 4UniverseUniverse = System + Surrounds
  5. 5Internal EnergyInternal Energy depends on:
    Temperature
    Type of material (mass and particles)
    Amount of material (number of particles)
  6. 6Calculating Thermodynamic ChangesEnergy change of a final system =
    ΔE = E final - E initial
  7. 7—ΔE positive : internal energy increasesΔE positive : internal energy increases
  8. 8—ΔE negative : internal energy decreasesΔE negative : internal energy decreases
  9. 9Heat CapacityHeat capacity = E required to raise the T(temperature) of an object by 1°C
    Specific Heat Capacity = E required to heat 1 gram of substance by 1°C
    Molar Heat Capacity = E required to heat 1 mole of substance by 1°C
  10. 10Specific HeatEnergy required to change Temp of an object is:
    Heat required =
    mass x specific heat x ΔTq = m c ΔT
    or…
    Heat required = moles x molar heat capacity x ΔT
    q = n cm ΔT
  11. 11When heat is ADDED to a systemq (heat) is positive
    the change is endothermic
    temperature decreases
    (liquid water boils to become gaseous water)
  12. 12When heat is REMOVED from a systemq (heat) is negative
    the change is exothermic
    temperature increases
    (gaseous water condenses to become liquid water)
  13. 13—

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enthalpy notes
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Amelia Claire
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