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Lecture 01: Chemistry of Life
: )
Most Abundant Elements in Humans
CHNOPS
Carbon
4 ve-
4 covalent bonds per atom
109.5 degree bond angles
can form single/double/triple bonds
bond to many atoms, common to HNOPS
Polymers and Monomers
POLY: Protein (polypeptide) / Nucleic acid (polynucleotide) / Polysaccharide (complex carbohydrate)
MONO: Amino acid / Nucleotide / Monosaccharide (simple carbohydrate)
Cellular Compartmentalization
way to make molecules for specific purposes
prevents other molecules in the environment from interacting
allows for increased concentrations locally
increase in conc. = increase in rxn
increased efficiency
compartment conditions might benefit reaction (pH, available ions, etc.)
costs energy, time, and substrates to make compartments
Lecture 02: Thermodynamics
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Thermodynamics
study of the rlx among various forms of energy and how energy affects matter
more macroscopic, thus deals with amounts of matter large enough that avg. properties (temp, pressure) are well defined
Application of Thermodynamics
used in native folding comformation of proteins
metabolic pathway design
why molecules cross mebranes
how muscles generate mechanical force
would like to know if given conditions, will the process be spontaneous?
System
what we’re interested in (organism/rxn vessel)
Surroundings
everything else (rest of universe)
Matter/Energy vs System Chart
Exchange with Surroundings + Type of System
Open:
matter: YES
energy: YES
Closed:
matter: NO
energy: YES
Isolated
matter: NO
energy: NO

Living Organisms
open systems
1. take in nutrients
2. release waste
3. generate work/heat
Thermo Units & Constants
Energy:
1 J = 1Nm = 1CV
W (work) = F (force) * d (distance) = kgm²/s²
1 cal = 4.184 J
1 Cal = 1000 cal = 4184 J
Avogadro’s Number = 6.022e23 molecules/mol
Temperature = 273.15 K = 0 degrees C
Boltzmann Constant = kB = 1.3807e-23 J/K
Gas Constant = R = NAkB , R = 1.9872 cal/Kmol = 8.3145 J/Kmol
First Law of Thermodynamics
Energy can’t be created nor destroyed
ΔE = Ef - Ei
ΔE = q + w
q = heat absorbed by the system from surroundings
w = work done on the system from surroundings
System & Heat
Exothermic = system releases heat = -q
Endothermic = system gains heat = +q
Work done on the system = +w
Work done by the system = -w
Enthalpy
heat released or taken in at constant pressure
Work can be divided into 2 categories
-PΔV = pressure-volume work (expansion)
w’ = all other work
w = -PΔV + w’
ΔE = Ef - Ei = q+w
ΔH = ΔE + PΔV
ΔH = q + w + PΔV
ΔH = qp + (-PΔV + w’) + PΔV
ΔH = qp + w’ (w’ = 0)
ΔH = qp
Hess’s Law
regardless of the multiple stages or steps of a rxn, ΔH = sum off all changes
enthalpy = state function; depends only upon state of system and NOT the way in which the system acquired the state
Second Law of Thermodynamics
spontaneous processes occur in directions that increase disorder of the universe
entropy = measure of the number of specific ways in which a thermodynamic system can be arranged (disorder)
S = kB lnW
kB = Boltzmann’s constant
W = # ways to arrange system
Entropy
for any constant processes (ΔE = 0), a spontaneous process is characterized by ΔS > 0
any spontaneous process MUST cause the entropy of. the universe to increase
ΔSsystem + ΔSsurroundings = ΔSuniverse > 0
ΔS >= qp/T
entropy change of a reversible process at a constant temperature can be determined straightfowardly from the measurements of heat transferred (and temperature maintained)
Gibbs Free Energy
the change in energy for a process that combines enthalpy, entropy, and temperature (assuming constant pressure)
ΔG < 0 spontaneous (exergonic)
ΔG = 0 at equilibrium
ΔG > 0 not spontaneous (endergonic)
Enthalpy & Entropy Table
[image]
![<p>[image]</p>](https://assets.knowt.com/user-attachments/753f05ce-2170-4fe1-909e-fb86550a05ae.png)
Entropy (cont)
Entropy is a function of concentration
free energy change of chem rxn depends on the concentrations of both its reacting substances (reactants) and its reaction products
thus, the concentrations of reactants and products are important; oftentimes the availability of reactants dictates rxn direction