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Entropy

Entropy. 1 st Law of Thermodynamics. Energy is neither created nor destroyed The energy of the universe is constant Energy just changes from one form to another This law lets us know the energy of the system, but does not give us any information about the direction of the energy flow.

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Entropy

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  1. Entropy

  2. 1st Law of Thermodynamics • Energy is neither created nor destroyed • The energy of the universe is constant • Energy just changes from one form to another • This law lets us know the energy of the system, but does not give us any information about the direction of the energy flow

  3. Spontaneity • Spontaneous process – a process that occurs without intervention • Spontaneous processes can be fast or slow • Spontaneity tells us the direction of the energy flow • It tells us NOTHING about the speed of the reaction

  4. For example… • A ball spontaneously rolls down a hill • It does not spontaneously roll up • If iron is exposed to air, it spontaneously rusts • The rust does not spontaneously turn back into air & iron

  5. Entropy • Entropy (s) – the measure of molecular randomness or disorder • Think of entropy as the amount of chaos • The driving force for a spontaneous process is an increase in entropy

  6. Entropy • The natural progression of things is from order to disorder • Or from lower entropy to higher entropy • Think of a deck of cards…when you drop one it goes from order to disorder • Think of your room… it goes from order to disorder • Think if entropy as a probability…not a certainty • Nature spontaneously proceeds toward that states that have the highest probability of existing

  7. Entropy • Predict which has the highest entropy • CO2 (s) or CO2 (g) CO2 (g) • 1 mol of N2 at 1 atm or 1 mol of N2 at 0.001 atm 1 mol of N2 at 0.001 atm

  8. Entropy • Predict the sign of the entropy change for the following… • Sugar is added to water to form a solution + • Iodine vapor condenses on a cold surface to produce a liquid -

  9. 2nd Law of Thermodynamics • 2nd Law of Thermodynamics – In any spontaneous process there is always an increase in entropy of the universe • Energy is conserved…entropy is NOT conserved! • The entropy of the universe is always increasing • S univ = + = spontaneous • S univ = - = not spontaneous (would be spontaneous in the opposite direction) • S univ = 0 = no tendency to occur (system is at equilibrium) • S univ = S sys + S surr

  10. Temperature & Spontaneity Ssurr = _ H T T must be in Kelvin • H is usually given in KJ/mol • S will be in KJ/K, but is usually changed to J/K

  11. Example Sb2S3 (s) + 3Fe (s)  2Sb (s) + 3FeS (s) H = -125 kJ Calculate Ssurr for this reaction at 25C and 1 atm S = - (H/T) S = - (-125KJ/298K) S = 0.419 KJ/K S = 419 J/K

  12. Example Sb4O6 (s) + 6C (s)  4Sb (s) + 6CO (g) H = 778 kJ Calculate Ssurr for this reaction at 25C and 1 atm S = - (H/T) S = - (778KJ/298K) S = -2.61 KJ/K S = -2610 J/K

  13. 3rd Law of Thermodynamics • The entropy of a perfect crystal at 0K is zero

  14. Free Energy • Free energy (G) – a thermodynamic function equal to the enthalpy minus the product of the entropy and the Kelvin temperature • G = H – TS • A process is only spontaneous in the direction where G is negative

  15. Example • At what temperatures is the following process spontaneous at 1 atm? • Br2(l)  Br2(g) • H = 31.0 KJ/mol  31000 J/mol • S = 93.0 J/ K mol • G = H – TS • 0 = 31000 – T(93.0) • T = 333K • Above 333K the reaction is spontaneous

  16. Dependence of H & S on Spontaneity G = H-TS Spontaneous at all temperatures Spontaneous at high temperatures Spontaneous at low temperatures Not spontaneous at any temperature

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