Magnus Andersson
magnus.andersson@scilifelab.se
Theoretical & Computational Biophysics
Protein folds, fold classifjcations & structure stability
Protein Physics 2016 Lecture 9, Tuesday Feb 23
Protein folds, fold classi fj cations & structure stability - - PowerPoint PPT Presentation
Protein Physics 2016 Lecture 9, Tuesday Feb 23 Protein folds, fold classi fj cations & structure stability Magnus Andersson magnus.andersson@scilifelab.se Theoretical & Computational Biophysics Recap Globular proteins ,
magnus.andersson@scilifelab.se
Theoretical & Computational Biophysics
Protein Physics 2016 Lecture 9, Tuesday Feb 23
hydrophobic environment
Protein physics book: Chapters 15 & 16
relatively small number of folds? 1500
Evolutionary Divergence Functional Convergence Limited number
Simple permutations
Stable local patterns (lots of h-bonds) Hydrophobic patterns Contiguous sheets
Class Architecture Topology Homology
Orengo & Thornton
Murzin, Brenner, Chotia ASTRAL, SUPERFAMILY, etc.
pony/horse hemoglobin
complex than prokaryotic ones?
domains, and they can be larger
KcsA (bacterial) Kv1.2 (eukaryotic)
must face water
must be separate
divided into subdomains for stability!
sequences - that’s why they are common
special amino acids (e.g. Cys bridges) for stabilization, and can only accomodate a few sequences
It is not a coincidence that we see this pattern both on vases and in proteins - can you think of why? (Richardson, Nature 1977)
Globular Membrane Fibrous
5-10 kcal/mol?
fmexibility can only accommodate few sequences
conformations can accommodate more sequences in low energy states
question is why many sequences fjt it!
Defective patterns are not impossible, just quite rare!
proteins
hydrophobic/hydrophilic residues (DNA)
and secondary structures we see? i, i+2 i, i+3 OR i, i+4
in the sequence
groups we will fjnd in a stretch?
hri = ∑r2[W(r)r] ∑r2W(r) = ∑r2rpr ∑r2 pr
n
r=1
pr = p(1− pn) 1− p
about 3 for p=0.5!
hri = 3+ 1 2p2
~1kcal important for stability?
a Boltzmann distribution?
residue distribution in structures obey it reasonably well too!?
(by kT) than for all other states
Z −∆ε
−∞ P(∆F)d(∆F)
Z −∆ε
−∞ P(∆F)d(∆F) ≈
⇡ Cexp
σ2/h∆Fi
Increasing Δε reduces the number of stabilizing sequences exponentially
dependent on the size of the protein!
rather than the entire protein energy!
Most sequences do not fold into stable structures!
freedom can accommodate more sequences
means they will be more likely to appear in stable folds
energy distribution before!
interior, sheets or helices?
hydrophobic
place two small blocks inside!
C
Probability of observing structural elements in randomly created stable globules depends on the amount of sequences that stabilize the fold: This is not because of the Boltzmann distribution (no equilibrium), but it has the same shape and a typical temperature.
kcal/mol, regardless of size