The Hydrophobic Effect and the Protein Core

Drop a spoonful of olive oil into a glass of water and shake hard. However furiously you stir, the oil droplets reassemble. They form a single lens-shaped puddle within seconds. Nothing pulls the oil molecules together. There is no strong attraction between them stronger than what water offers. Instead, water excludes them. The oil aggregates because doing so is the path of least resistance for the surrounding water. This same asocial partitioning is played out on the scale of a single polypeptide chain. It is the single largest force that turns an unstructured ribbon of amino acids into a compact, folded, catalytically competent protein. The hydrophobic effect is not a bond. It is also not really a "force." It is not an attraction between nonpolar groups reaching out to grab each other. It is a statement about water. When a nonpolar side chain — leucine's isobutyl group, phenylalanine's ring, valine's isopropyl group — is exposed to liquid water, the surrounding water molecules cannot form hydrogen bonds through the nonpolar surface. So they reorganize into a more ordered, cage-like arrangement around it. They sacrifice translational and orientational entropy to preserve their hydrogen-bond network. Burying that same nonpolar surface inside a folded protein, away from water altogether, releases the caged water back into the bulk. There, it recovers this entropy. The favorable free energy of folding is, to first approximation, an entropy bookkeeping problem for water. It is not an energy story for the protein. This matters enormously because it resolves an old puzzle. Why does a protein fold at all? After all, it loses a huge amount of conformational entropy on folding. Thousands of accessible backbone and side-chain conformations collapse to essentially one. The hydrophobic effect supplies the driving free energy that pays for this entropic cost. It also pays for burying charged and polar backbone groups. These must be compensated by hydrogen bonds. They are also compensated by the geometry of Noncovalent Forces That Stabilize Folded Proteins. Without a hydrophobic core, secondary structure elements would have nothing to pack against. The marginal 20–65 kJ/mol of net stability separates the folded state from the vast unfolded ensemble. That margin simply would not exist. This article builds the hydrophobic effect from water structure upward. It covers the thermodynamic signature (large positive ΔS, small ΔH, strongly temperature-dependent ΔCp). It covers the microscopic cavity/clathrate picture that explains that signature. It covers the scaling of transfer free energy with buried nonpolar surface area. It also covers the resulting architecture of the protein core. That core is close-packed, nearly crystalline in density. It is the primary determinant of the overall fold. It closes with worked calculations of transfer free energies, core packing densities, and stability contributions. This prepares the ground for Tertiary Structure and the Fold and Protein Folding Pathways and Thermodynamics.

Key takeaways
  • Nonpolar solutes order the surrounding water into a low-entropy hydration shell; burying them releases that water, increasing entropy overall — this is the hydrophobic effect.
  • The thermodynamic signature is diagnostic: transferring a nonpolar group from water to oil or into a folded protein core has small ΔH, large positive ΔS at 25 °C, and a large positive heat capacity change ΔCp.
  • Transfer free energy scales roughly linearly with buried nonpolar surface area, ΔG ≈ σ·ΔA, with σ ≈ 25 cal/(mol·Å²) for hydrocarbon transfer.
  • The protein core is packed at near-crystalline density (packing coefficient ≈ 0.72–0.75), comparable to close-packed spheres, not a loose oil droplet.
  • ΔCp > 0 is uniquely diagnostic of hydrophobic burial and lets calorimetrists dissect folding thermodynamics into hydrophobic and polar contributions.
  • Key idea: protein folding is driven mainly by the entropy gained by water when nonpolar surface is removed from solvent, not by an intrinsic attraction between hydrophobic groups.

Where this lives today

Modern protein engineering and drug design routinely exploit the hydrophobic effect as a quantitative design parameter, not just a qualitative concept. Structure-based drug design uses buried nonpolar surface area between a ligand and its target pocket as a first-pass estimate of binding affinity, because the same ΔG≈σΔA\Delta G\approx\sigma\Delta A scaling that describes protein core burial also governs protein–ligand and protein–protein binding interfaces; hydrophobic "hot spots" at binding interfaces are systematically the residues whose mutation to alanine most destabilizes binding (alanine-scanning mutagenesis directly measures the cavity-plus-transfer penalty described above). Protein stabilization engineering for industrial enzymes and therapeutic antibodies frequently targets core-packing defects — filling small cavities with slightly larger hydrophobic residues, or replacing surface-exposed hydrophobic patches that risk aggregation — using exactly the surface-area/packing-density logic developed here. Computational structure prediction and design tools (Rosetta, AlphaFold-adjacent scoring functions, molecular dynamics force fields) all encode an implicit or explicit hydrophobic solvation term, typically parameterized directly from the atomic solvation parameter σ and from experimentally measured ΔCp values, because getting the hydrophobic core right is the single largest determinant of whether a predicted or designed fold is physically stable. In membrane biology, the same principle runs in reverse: transmembrane helices bury their hydrophobic surface not in a protein core but in the lipid bilayer interior, and the same ΔGtr\Delta G_{tr} scaling with nonpolar surface area (this time favoring the lipid environment over water) underlies hydropathy-plot algorithms used to predict transmembrane segments from sequence alone. Finally, understanding of cold denaturation and pressure denaturation — both explained through the temperature and pressure dependence of hydrophobic hydration free energy — is central to formulating stable biologics and to understanding piezophilic (high-pressure-adapted) deep-sea organisms.

Ask the tutor: How does the hydrophobic effect combine with backbone hydrogen bonding to determine which secondary structures form the protein's tertiary fold?

The physical picture

Water is a small, highly cohesive molecule that forms on average close to four hydrogen bonds per molecule in the bulk liquid, each roughly 1.9–2.1 Å (O···H) with bond enthalpies around 10–25 kJ/mol depending on geometry. This network is dynamic — bonds break and reform on picosecond timescales — but it is essentially unbroken in the bulk: every water molecule can find hydrogen-bonding partners in essentially any direction. When a nonpolar solute is introduced, water molecules at the interface cannot hydrogen-bond across the solute's surface. They compensate by reorienting to maximize hydrogen bonding among themselves, tangential to the solute surface, forming a partial cage — a "clathrate-like" shell reminiscent of the ordered hydrate crystals formed by methane and other small gases at low temperature. This reorientation is not free: it costs orientational and translational entropy, because the number of ways the shell waters can arrange while satisfying both their own hydrogen-bonding needs and the geometric constraint of the solute surface is much smaller than in the bulk. Crucially, the enthalpy of this hydration shell is often not unfavorable — shell waters can actually have as many or more hydrogen bonds as bulk water, just more constrained in orientation. This is why dissolving a small hydrocarbon like methane in water is enthalpically nearly neutral or even mildly exothermic at room temperature, yet strongly entropically unfavorable — the classic thermodynamic fingerprint of hydrophobic hydration. The free energy cost of solvation, ΔG = ΔH − TΔS, is dominated by the −TΔS term because ΔS is large and negative for the solute entering water (ordering the shell), which means ΔS is large and positive for the reverse process — the nonpolar group leaving water to be buried in a protein interior or an oil phase. The second essential feature is the heat capacity anomaly. Because ordered hydration-shell water has a different (lower) heat capacity contribution than bulk water, and because the degree of order in the shell itself is temperature-dependent, both ΔH and ΔS for hydrophobic hydration vary strongly and roughly linearly with temperature — producing a large, positive ΔCp for the process of dissolving a nonpolar group in water (and hence a large negative ΔCp for burial/folding, since burial is the reverse of solvation). This ΔCp is the single most reliable calorimetric signature that a given contribution to protein stability is hydrophobic in origin, because polar and electrostatic interactions contribute comparatively little to ΔCp.

Figure
Water ordering around a nonpolar solute, and its release upon burial
Hydration shell ordering and release CH₃–R ordered clathrate-like shell low entropy (S_shell small) burial CH₃–R Leu nonpolar core, no water water released → bulk (ΔS > 0)

The third piece of the picture is what the buried interior actually looks like once assembled. Protein cores are not oil droplets with residual liquid-like disorder; they are packed nearly as densely as a crystal of small organic molecules, with packing coefficients (fraction of volume actually occupied by atoms, using van der Waals radii) around 0.72–0.75, essentially indistinguishable from the packing density of crystalline amino acids and comparable to close-packed spheres (0.74 for face-centered cubic packing). This density is required for van der Waals contacts to contribute meaningfully to stability and explains why core mutations that change side-chain volume (e.g., Leu→Ala, creating a cavity) are often strongly destabilizing even though both residues are nonpolar — packing defects cost stability quite apart from any change in hydrophobicity per se.

Figure
Free energy of transfer: water → oil vs water → protein core
Transfer free energy scales with buried area buried nonpolar surface area, ΔA (Ų) ΔG_transfer (kcal/mol) ΔG ≈ −σ·ΔA, σ ≈ 25 cal/(mol·Å²) Ala side chain, ΔA≈40 Ų, ΔG≈−1.0 Leu side chain, ΔA≈140 Ų, ΔG≈−3.5 Phe side chain, ΔA≈200 Ų, ΔG≈−5.0 (kcal/mol, negative = favorable burial)

The core ideas

The free energy of transferring a nonpolar solute from water to a nonpolar (oil-like or protein-interior) environment is

ΔGtr=ΔHtr−TΔStr\Delta G_{tr} = \Delta H_{tr} - T\Delta S_{tr}

where:

  • ΔGtr\Delta G_{tr} — standard free energy of transfer (water → nonpolar phase), negative for favorable burial
  • ΔHtr\Delta H_{tr} — enthalpy of transfer, small in magnitude near room temperature
  • TT — absolute temperature (K)
  • ΔStr\Delta S_{tr} — entropy of transfer, large and positive near room temperature (water released from an ordered shell to the bulk)

Reading: at 25 °C, ΔGtr\Delta G_{tr} for small hydrocarbons is dominated by the −TΔStr-T\Delta S_{tr} term; ΔHtr\Delta H_{tr} is often close to zero or even positive (unfavorable), meaning the whole driving force for burial is entropic at this temperature. The temperature dependence of ΔHtr\Delta H_{tr} and ΔStr\Delta S_{tr} is governed by a large, essentially temperature-independent heat capacity change:

ΔCp,tr=(∂ΔHtr∂T)P=T(∂ΔStr∂T)P\Delta C_{p,tr} = \left(\frac{\partial \Delta H_{tr}}{\partial T}\right)_P = T\left(\frac{\partial \Delta S_{tr}}{\partial T}\right)_P

where:

  • ΔCp,tr\Delta C_{p,tr} — heat capacity change on transfer (large, positive, for water → oil; hence large negative for oil/protein-interior → water, i.e., for unfolding)
  • the near-constancy of ΔCp,tr\Delta C_{p,tr} over 0–100 °C is the empirical basis for integrating it to get ΔH(T)\Delta H(T) and ΔS(T)\Delta S(T)

Integrating from a reference temperature ThT_h (the temperature at which ΔHtr=0\Delta H_{tr}=0) gives:

ΔHtr(T)=ΔCp,tr (T−Th)\Delta H_{tr}(T) = \Delta C_{p,tr}\,(T - T_h)
ΔStr(T)=ΔCp,tr ln⁡ ⁣(TTs)\Delta S_{tr}(T) = \Delta C_{p,tr}\,\ln\!\left(\frac{T}{T_s}\right)

where:

  • ThT_h — temperature at which the transfer enthalpy vanishes (empirically near 22 °C for many hydrocarbons)
  • TsT_s — temperature at which the transfer entropy vanishes (empirically near 112–140 °C for many hydrocarbons, always higher than ThT_h)

Reading: because Ts≫ThT_s \gg T_h, there is a wide temperature window (around physiological temperature) in which ΔHtr\Delta H_{tr} is small but ΔStr\Delta S_{tr} is still large and positive — exactly the regime in which hydrophobic burial is entropy-driven. As T→TsT \to T_s, ΔStr→0\Delta S_{tr}\to 0 and the driving force becomes purely enthalpic; this is the microscopic reason protein hydrophobic stability itself is temperature-dependent and why proteins can undergo cold denaturation. Empirically, the transfer free energy for burying nonpolar surface correlates linearly with the buried accessible surface area (ASA):

ΔGtr=σ ΔAnp+b\Delta G_{tr} = \sigma \, \Delta A_{np} + b

where:

  • σ\sigma — atomic solvation parameter, empirically about −25-25 cal/(mol·Å²) (favorable, i.e., negative sign for burial) for aliphatic/aromatic carbon transferring from water to a nonpolar liquid or protein-like environment
  • ΔAnp\Delta A_{np} — nonpolar surface area removed from water contact upon folding/burial (Ų)
  • bb — small intercept, often taken as zero in first approximation

Reading: this linear relation is the working currency of the field — it lets you predict the stability contribution of burying a given side chain, or the destabilization from a core cavity-forming mutation, directly from a change in buried surface area.

Derivation AFrom clathrate ordering to a positive ΔCp: a two-state shell model

Goal. Show mechanistically why hydrating a nonpolar solute in water produces a large positive heat capacity change, and why this heat capacity is the microscopic origin of the entropy-driven character of hydrophobic burial near room temperature.

Step 1 — Partition water into bulk and shell populations. Model the water in contact with a nonpolar solute as nn "shell" molecules in local equilibrium with the surrounding bulk. Shell water can adopt an ordered, low-entropy, hydrogen-bond-satisfying arrangement (call it state OO) or a bulk-like, higher-entropy arrangement (state BB) that sacrifices some hydrogen-bonding to the solute interface. At low temperature, entropy is not at a premium (the −TS-TS penalty is small), so shell water can afford to sit in the low-enthalpy, highly ordered state OO, maximizing hydrogen bonds even at the cost of restricted geometry. As TT rises, the entropic penalty −TS-TS of staying ordered grows, and shell water increasingly samples state BB, sacrificing some hydrogen bonds for more accessible configurations, exactly as bulk water itself becomes progressively less structured with rising TT.

Step 2 — Heat capacity as a fluctuation/population-shift quantity. Whenever a system can populate two (or more) states of different enthalpy and the population ratio shifts continuously with temperature, the ensemble exhibits an apparent heat capacity contribution beyond that of either pure state, given by a Schottky-like two-state formula:

Cpshell=Cpbulk-like avg+nOnBn⋅(ΔHOB)2RT2C_p^{shell} = C_p^{bulk\text{-like avg}} + \frac{n_O n_B}{n}\cdot\frac{(\Delta H_{OB})^2}{RT^2}

where nO,nBn_O, n_B are populations in states OO and BB (nO+nB=nn_O+n_B=n) and ΔHOB\Delta H_{OB} is the enthalpy difference between the ordered and bulk-like shell states. This extra term is always positive (it is a variance), and it is largest when the two states are comparably populated — precisely the situation for hydrophobic hydration shells at physiological temperature, where ordered and bulk-like configurations are close in free energy and the population shifts continuously with TT.

Step 3 — Consequence for ΔH and ΔS of solvation. Because the shell has excess heat capacity relative to bulk water alone, dissolving a nonpolar solute (converting some bulk water into shell water) gives the solvation process itself an anomalously large, positive ΔCp,solv\Delta C_{p,solv}. Integrating d(ΔH)/dT=ΔCpd(\Delta H)/dT = \Delta C_p and d(ΔS)/dT=ΔCp/Td(\Delta S)/dT = \Delta C_p/T from a convenient reference point shows that ΔHsolv(T)\Delta H_{solv}(T) and ΔSsolv(T)\Delta S_{solv}(T) both increase monotonically with TT — climbing from negative or near-zero values at low TT toward large positive values at high TT. Because the two curves have different curvature intercepts (Th≠TsT_h \neq T_s), there exists a broad temperature range, bracketing 25–37 °C for typical hydrocarbons, in which ΔHsolv≈0\Delta H_{solv}\approx 0 (little penalty for dissolving) but ΔSsolv≫0\Delta S_{solv} \gg 0 (a large entropy cost has already been paid). Reversing sign for the burial process (protein folding removes the solute from water) recovers the experimental hydrophobic-effect signature directly: ΔHburial≈0\Delta H_{burial}\approx 0, ΔSburial≫0\Delta S_{burial}\gg 0 at room temperature, and ΔCp,burial<0\Delta C_{p,burial} < 0, all falling directly out of the two-state shell picture without invoking any attractive force between nonpolar groups.

Step 4 — Why this is entropy, not enthalpy, near 25–37 °C. Because ΔGtr=ΔHtr−TΔStr\Delta G_{tr} = \Delta H_{tr} - T\Delta S_{tr} and because at physiological temperature ∣ΔHtr∣≪T∣ΔStr∣|\Delta H_{tr}|\ll T|\Delta S_{tr}|, essentially all the favorable free energy of burial in this regime comes from the −TΔStr-T\Delta S_{tr} term. This is the rigorous justification for the everyday shorthand "hydrophobic burial is entropically driven" — it is a statement about the specific temperature window of biology, not a universal law independent of TT, and it inverts as T→TsT\to T_s.

Go deeper · Derivation B · 1 minPredicting ΔΔG_stability for a core cavity mutation from buried surface area
Derivation BPredicting ΔΔG_stability for a core cavity mutation from buried surface area

Goal. Derive, from the empirical atomic solvation parameter, the expected destabilization when a large buried core residue (e.g., Leu) is mutated to a smaller one (e.g., Ala), creating an internal cavity, and separate the hydrophobic contribution from the packing/van der Waals contribution.

Step 1 — Define the accessible surface areas involved. For a residue buried in the folded core, essentially all of its nonpolar side-chain surface is removed from water contact upon folding: ΔAnpfold≈Anpside chain\Delta A_{np}^{fold} \approx A_{np}^{side\ chain} (the surface area the side chain would expose if it were on the outside of an unfolded chain, fully solvent-exposed). Leucine's side chain has a solvent-accessible surface area of roughly 140 Ų when fully exposed; alanine's is about 67 Ų (values from tabulated Lee–Richards ASA calculations on Gly-X-Gly tripeptides).

Step 2 — Apply the solvation-parameter relation to each residue's folded contribution. Using ΔGtr=σΔAnp\Delta G_{tr} = \sigma\Delta A_{np} with σ≈−25\sigma \approx -25 cal/(mol·Å²):

ΔGtrLeu=(−25 cal mol−1A˚−2)(140 A˚2)=−3500 cal/mol=−3.5 kcal/mol\Delta G_{tr}^{Leu} = (-25\ \text{cal mol}^{-1}\text{Å}^{-2})(140\ \text{Å}^2) = -3500\ \text{cal/mol} = -3.5\ \text{kcal/mol}
ΔGtrAla=(−25 cal mol−1A˚−2)(67 A˚2)=−1675 cal/mol≈−1.7 kcal/mol\Delta G_{tr}^{Ala} = (-25\ \text{cal mol}^{-1}\text{Å}^{-2})(67\ \text{Å}^2) = -1675\ \text{cal/mol} \approx -1.7\ \text{kcal/mol}

Step 3 — Compute the hydrophobic-burial component of the destabilization. The mutation Leu→Ala at a buried position removes (140−67)=73(140-67)=73 Ų of nonpolar surface from the buried inventory, so the loss in favorable transfer free energy is:

ΔΔGhydrophobic=ΔGtrAla−ΔGtrLeu=(−1.7)−(−3.5)=+1.8 kcal/mol\Delta\Delta G_{hydrophobic} = \Delta G_{tr}^{Ala} - \Delta G_{tr}^{Leu} = (-1.7) - (-3.5) = +1.8\ \text{kcal/mol}

(destabilizing, since folded Ala buries less nonpolar area than folded Leu would have).

Step 4 — Add the packing/cavity penalty. Experimentally, Leu→Ala core mutations in T4 lysozyme and similar model systems destabilize the protein by roughly 3–5 kcal/mol — substantially more than the ≈1.8 kcal/mol predicted from surface-area loss alone. The residual ≈1.5–3 kcal/mol arises because removing three methyl-sized groups leaves an unfilled cavity: the protein cannot fully collapse around the smaller side chain without breaking other packing contacts, so lost van der Waals contact energy and an entropically unfavorable void (or a compensating, often incomplete, local structural relaxation) contribute an additional destabilization on top of the pure hydrophobic-transfer term. This decomposition — ΔΔGtotal≈ΔΔGhydrophobic+ΔΔGpacking\Delta\Delta G_{total} \approx \Delta\Delta G_{hydrophobic} + \Delta\Delta G_{packing} — is the standard way mutagenesis data on core residues are interpreted, and it is precisely why cavity-creating mutations are systematically more destabilizing than the ASA-only prediction: burial free energy and packing density are separable but both matter.

Worked examples

Example 1 — Foundational: transfer free energy of a simple hydrocarbon, water → cyclohexane. Experimental data for the transfer of ethane from water to a nonpolar solvent (a classic model system for the hydrophobic effect, per Tanford and later calorimetric work) near 25 °C give approximately:

ΔHtr≈+2.0 kcal/mol,ΔStr≈+25 cal/(mol ⋅ K)\Delta H_{tr} \approx +2.0\ \text{kcal/mol}, \qquad \Delta S_{tr} \approx +25\ \text{cal/(mol}\,\cdot\,\text{K)}

Compute ΔGtr\Delta G_{tr} at T=298 KT = 298\ \text{K}:

ΔGtr=ΔHtr−TΔStr=2.0 kcal/mol−(298 K)(0.025 kcal/(mol ⋅ K))\Delta G_{tr} = \Delta H_{tr} - T\Delta S_{tr} = 2.0\ \text{kcal/mol} - (298\ \text{K})(0.025\ \text{kcal/(mol}\,\cdot\,\text{K)})
ΔGtr=2.0−7.45=−5.45 kcal/mol\Delta G_{tr} = 2.0 - 7.45 = -5.45\ \text{kcal/mol}

This is favorable overall (ΔGtr<0\Delta G_{tr}<0, ethane prefers the nonpolar phase) despite an unfavorable (positive) enthalpy — the entropy term alone, −TΔStr=−7.45-T\Delta S_{tr}=-7.45 kcal/mol, more than compensates. This is the textbook demonstration that hydrophobic partitioning can be enthalpically uphill and still occur, because it is entropically driven. Limiting-case check: if ΔStr\Delta S_{tr} were exactly zero (no water reorganization at all, e.g. an artificial solute that does not perturb water structure), ΔGtr\Delta G_{tr} would simply equal ΔHtr=+2.0\Delta H_{tr}=+2.0 kcal/mol — unfavorable, and ethane would prefer to stay in water. The favorable partitioning we actually observe is entirely a consequence of the nonzero, positive ΔStr\Delta S_{tr}, confirming the entropic origin of the effect in this system.

Example 2 — Applied: burial free energy of a phenylalanine side chain from ASA data. Phenylalanine's fully exposed side-chain ASA is about 200 Ų (aromatic ring plus CH₂ linker); in a typical folded protein core it becomes almost completely buried, losing contact with water. Using σ=−25\sigma = -25 cal/(mol·Å²):

ΔGtrPhe=σ⋅ΔAnp=(−25 cal mol−1A˚−2)(200 A˚2)\Delta G_{tr}^{Phe} = \sigma \cdot \Delta A_{np} = (-25\ \text{cal mol}^{-1}\text{Å}^{-2})(200\ \text{Å}^2)
ΔGtrPhe=−5000 cal/mol=−5.0 kcal/mol\Delta G_{tr}^{Phe} = -5000\ \text{cal/mol} = -5.0\ \text{kcal/mol}

Compare this to the total net stability of a typical small globular protein, ΔGfold≈−8\Delta G_{fold}\approx -8 to −12-12 kcal/mol below the unfolded state. A single buried phenylalanine can in principle contribute nearly half the entire net folding stability — which is exactly why single core mutations (Phe→Ala, Phe→Gly) at buried positions are so often severely destabilizing or fold-disrupting, and why aromatic and branched aliphatic residues are so strongly conserved at core positions across evolutionarily related folds. Limiting-case check: if the same Phe residue were instead placed at a fully solvent-exposed surface position in the folded state (as many are), ΔAnp→0\Delta A_{np}\to 0 and ΔGtr→0\Delta G_{tr}\to 0 — surface aromatic residues contribute essentially nothing to hydrophobic stabilization, consistent with the empirical observation that surface hydrophobic patches (unless involved in specific binding interfaces) do not correlate with increased protein stability.

Example 3 — Exam/competition level: dissecting a calorimetric unfolding curve into hydrophobic and polar contributions. A differential scanning calorimetry (DSC) experiment on a small globular protein (100 residues) gives, at the melting temperature Tm=333 KT_m = 333\ \text{K} (60 °C):

ΔHunfold(Tm)=90 kcal/mol,ΔCp,unfold=1.2 kcal/(mol ⋅ K)\Delta H_{unfold}(T_m) = 90\ \text{kcal/mol}, \qquad \Delta C_{p,unfold} = 1.2\ \text{kcal/(mol}\,\cdot\,\text{K)}

(a) Estimate ΔHunfold\Delta H_{unfold} at physiological temperature, 310 K (37 °C), using the Kirchhoff relation:

ΔHunfold(310 K)=ΔHunfold(Tm)+ΔCp,unfold (310−333)\Delta H_{unfold}(310\ \text{K}) = \Delta H_{unfold}(T_m) + \Delta C_{p,unfold}\,(310 - 333)
ΔHunfold(310 K)=90+(1.2)(−23)=90−27.6=62.4 kcal/mol\Delta H_{unfold}(310\ \text{K}) = 90 + (1.2)(-23) = 90 - 27.6 = 62.4\ \text{kcal/mol}

(b) Estimate ΔSunfold\Delta S_{unfold} at 310 K. At TmT_m, by definition ΔGunfold(Tm)=0\Delta G_{unfold}(T_m)=0, so ΔSunfold(Tm)=ΔHunfold(Tm)/Tm=90/333=0.270\Delta S_{unfold}(T_m) = \Delta H_{unfold}(T_m)/T_m = 90/333 = 0.270 kcal/(mol·K). Extrapolate using the heat capacity integral:

ΔSunfold(310)=ΔSunfold(Tm)+ΔCp,unfold ln⁡ ⁣(310333)\Delta S_{unfold}(310) = \Delta S_{unfold}(T_m) + \Delta C_{p,unfold}\,\ln\!\left(\frac{310}{333}\right)
ln⁡(310/333)=ln⁡(0.9309)=−0.0716\ln(310/333) = \ln(0.9309) = -0.0716
ΔSunfold(310)=0.270+(1.2)(−0.0716)=0.270−0.0859=0.184 kcal/(mol ⋅ K)\Delta S_{unfold}(310) = 0.270 + (1.2)(-0.0716) = 0.270 - 0.0859 = 0.184\ \text{kcal/(mol}\,\cdot\,\text{K)}

(c) Compute ΔGunfold\Delta G_{unfold} at 310 K:

ΔGunfold(310)=ΔHunfold(310)−TΔSunfold(310)=62.4−(310)(0.184)\Delta G_{unfold}(310) = \Delta H_{unfold}(310) - T\Delta S_{unfold}(310) = 62.4 - (310)(0.184)
ΔGunfold(310)=62.4−57.0=5.4 kcal/mol\Delta G_{unfold}(310) = 62.4 - 57.0 = 5.4\ \text{kcal/mol}

Since unfolding is unfavorable by +5.4 kcal/mol at 37 °C, folding is favorable by ΔGfold=−5.4\Delta G_{fold}=-5.4 kcal/mol at physiological temperature — a modest but entirely typical net stability for a small globular protein, arising as a small difference between a large favorable hydrophobic entropy term and large unfavorable conformational-entropy and polar-desolvation terms buried inside ΔHunfold\Delta H_{unfold} and ΔSunfold\Delta S_{unfold}. Limiting-case check: note that the large positive ΔCp,unfold=1.2\Delta C_{p,unfold}=1.2 kcal/(mol·K) is itself diagnostic — a value this large (typical experimental range 0.5–2 kcal/(mol·K) for globular proteins of this size) could not arise from polar or electrostatic interactions alone, whose heat capacity contributions are an order of magnitude smaller; it is essentially entirely attributable to exposure of the hydrophobic core upon unfolding, directly linking the calorimetric number to the physical picture of clathrate-shell formation developed above.

Limiting cases, scope & common traps

Regime / claimWhat actually holdsCommon error
Low temperature (≈0–10 °C)ΔHtr\Delta H_{tr} for solvation becomes negative (favorable); hydrophobic driving force weakens; can cause cold denaturationAssuming the hydrophobic effect is always maximal at low T — it is actually weakest there
Physiological range (25–40 °C)Entropy-dominated: ΔHtr≈0\Delta H_{tr}\approx 0, −TΔStr-T\Delta S_{tr} supplies nearly all the favorable ΔGtr\Delta G_{tr}Calling hydrophobic bonds "strong attractive forces" — there is no direct attraction, only water reorganization
High temperature (>100 °C, or T→TsT\to T_s)Entropy term vanishes; driving force becomes enthalpic; proteins can be unusually stable in thermophiles via enthalpically reinforced hydrophobic packingExtrapolating room-temperature entropy-driven language to all temperatures
Small nonpolar solute (methane, ethane)Classic clathrate/cage picture applies cleanly; convex, weakly curved surfaceUsing small-molecule ΔCp values directly for large buried protein surfaces without area-scaling
Large buried surface, protein coreScaling with ASA holds approximately; packing density (~0.74) adds a separate van der Waals/packing termTreating ΔG_tr from ASA alone as the entire stability contribution, ignoring packing defects
Charged/polar group burialCostly unless compensated by salt bridges or H-bonds; not part of "the hydrophobic effect" properLumping all core stabilization, including buried ion pairs, under "hydrophobic effect"

The chemist behind it

Walter Kauzmann (1916–2009) is the figure most closely associated with formalizing the hydrophobic effect as the dominant force in protein folding. Trained as a physical chemist at Princeton, Kauzmann worked in the 1950s at a moment when the physical basis of protein stability was almost entirely unknown — the double helix had just been solved, but nobody had a convincing account of why a linear chain of amino acids would spontaneously and reproducibly collapse into a unique three-dimensional structure. Kauzmann's landmark 1959 review, drawing on earlier solubility work by Kauzmann's contemporaries and on the classic thermodynamic studies of hydrocarbon solubility by researchers including Henry S. Frank and Marjorie Evans (whose 1945 "iceberg" model of water structuring around nonpolar solutes anticipated the modern clathrate picture), argued forcefully that burying nonpolar side chains away from water — not hydrogen bonding, which he showed could be satisfied about equally well in unfolded and folded states — was the dominant thermodynamic driving force for folding. This was a genuinely counterintuitive claim at the time, since hydrogen bonds are visually salient in structural models (Pauling's α-helix and β-sheet had just been proposed) and it was natural to assume they were also energetically dominant. Kauzmann's insight — that the entropy of water, not any direct bond within the protein, supplies most of the folding free energy — reoriented the entire field toward thinking about solvent thermodynamics as central to macromolecular structure, a viewpoint later reinforced quantitatively by Charles Tanford's systematic measurements of amino acid side-chain transfer free energies (the hydrophobicity scales still used today) and by decades of high-precision calorimetry establishing the ΔCp signature discussed above.

Origins · 1 minWalter Kauzmann and how this was discovered
WK
Walter Kauzmann
1916–2009 · Physical chemist, Princeton University; formalized the hydrophobic effect as the dominant driving force in protein folding (1959)

History
- 1945 — Frank and Evans propose the "iceberg" model of ordered water structuring around dissolved nonpolar gases, the conceptual root of the clathrate/hydration-shell picture.
- 1959 — Walter Kauzmann publishes his review arguing that hydrophobic burial, not hydrogen bonding, is the dominant force stabilizing folded proteins.
- 1960s — Charles Tanford develops systematic hydrophobicity scales from amino acid side-chain solubility and transfer free energy measurements.
- 1970s–1980s — High-precision differential scanning calorimetry (Privalov and others) establishes the characteristic large positive ΔCp of protein unfolding, quantitatively confirming the hydrophobic-hydration model.
- 1990s–2000s — Systematic core mutagenesis (e.g., T4 lysozyme cavity mutants, Matthews and coworkers) decomposes stability changes into hydrophobic transfer and packing/cavity contributions.
Is the hydrophobic effect the same thing as van der Waals attraction between side chains?

No. Van der Waals (London dispersion) attractions between packed nonpolar side chains are real and do contribute to core stability, but they are comparatively weak per contact and not unique to water as a solvent — the same dispersion forces exist between nonpolar groups in any medium. The hydrophobic effect proper refers specifically to the solvent thermodynamics: the entropically costly ordering of water around exposed nonpolar surface, and the entropy gain when that surface is removed from water. In a well-packed protein core, both effects operate together — favorable van der Waals packing contacts plus favorable hydrophobic burial free energy — but they are conceptually and thermodynamically distinct contributions, which is why cavity-forming mutations (which reduce packing contacts without necessarily changing buried surface area proportionally) can be destabilizing beyond what surface-area scaling predicts.

Why does ΔCp for protein unfolding matter so much experimentally?

ΔCp is the cleanest experimental handle for isolating the hydrophobic contribution to stability because polar and electrostatic interactions have comparatively small, sometimes even opposite-signed, heat capacity signatures, while nonpolar hydration has an unusually large, robustly positive ΔCp (for the solvation direction). By measuring ΔCp calorimetrically (via DSC) and combining it with ΔH and ΔS at the melting temperature, one can extrapolate the full temperature dependence of protein stability, predict cold denaturation temperatures, and estimate what fraction of total stability is attributable to burial of nonpolar surface versus other contributions. It is essentially a spectroscopic fingerprint for "how much hydrophobic surface got buried" during folding.

Does the hydrophobic effect explain secondary structure formation (α-helices, β-sheets) directly?

Not directly — Noncovalent Forces That Stabilize Folded Proteins such as backbone hydrogen bonding are the immediate local determinant of helix and sheet geometry. The hydrophobic effect instead drives the overall collapse of the chain and dictates which secondary structure elements end up buried against each other to form a compact core, indirectly favoring secondary structure formation because burying backbone amide/carbonyl groups without satisfying their hydrogen-bonding potential is highly unfavorable — so the collapse essentially forces backbone hydrogen bonds to be satisfied internally (as helices or sheets) once the chain compacts. The interplay between these two forces is the subject of Tertiary Structure and the Fold.

Why do some proteins undergo cold denaturation at low temperature?

Because the entropic driving force for hydrophobic burial, −TΔStr-T\Delta S_{tr}, shrinks as TT decreases (since ΔStr\Delta S_{tr} itself decreases toward zero and can even go negative at very low TT, following the ΔCpln⁡T\Delta C_p \ln T dependence), while the entropic cost of chain ordering upon folding is comparatively insensitive to temperature. At sufficiently low temperature the hydrophobic driving force becomes too weak to compensate the conformational entropy loss of folding, and the protein unfolds even though it is thermally "cold" — a phenomenon predicted directly from the temperature dependence built into the ΔCp-based free energy equations above, and experimentally observed for many proteins typically below 0–10 °C (often requiring pressure or concentrated solution conditions to observe before ice formation intervenes).

How is the hydrophobic effect measured experimentally, independent of whole-protein folding?

Historically through solubility and partition measurements: dissolving small hydrocarbons or amino acid analogs in water versus a nonpolar reference solvent (e.g., octanol, cyclohexane, or the vapor phase) and measuring the equilibrium partition coefficient, which gives ΔGtr\Delta G_{tr} directly via ΔGtr=−RTln⁡Kpartition\Delta G_{tr}=-RT\ln K_{partition}. Temperature-dependent solubility measurements give ΔHtr\Delta H_{tr}, ΔStr\Delta S_{tr}, and ΔCp,tr\Delta C_{p,tr} from van't Hoff analysis. These small-molecule transfer free energies, tabulated by Tanford, Nozaki, and others, are the empirical basis for the atomic solvation parameter σ used throughout structural biology and remain the gold-standard reference data against which whole-protein calorimetry is interpreted.

Is the hydrophobic effect the largest single contributor to protein stability?

It is generally considered the largest favorable contributor to the free energy of folding, but net protein stability (typically only 20–65 kJ/mol, or roughly 5–15 kcal/mol) is a small difference between much larger favorable and unfavorable terms: favorable hydrophobic burial and van der Waals packing, versus unfavorable loss of backbone and side-chain conformational entropy upon folding, plus the cost of burying any polar/charged groups not fully compensated by internal hydrogen bonds or salt bridges. The hydrophobic effect is best understood as the dominant term that makes folding possible at all, even though the final observed stability is a much smaller residual after near-total cancellation of large opposing terms.

Does the hydrophobic effect apply the same way to RNA and lipid assembly?

The same underlying water-reorganization physics applies to any amphiphilic self-assembly process, including lipid bilayer formation and micelle formation, which is why lipid tail burial in a bilayer interior shows the same entropy-dominated, positive-ΔCp thermodynamic signature as protein core formation. RNA tertiary folding is more dominated by electrostatic and Mg²⁺-mediated interactions because of its dense anionic phosphate backbone, but stacking interactions between nucleobases (which have a substantial nonpolar/aromatic character) do carry a hydrophobic-like solvation component, so the effect is present but usually secondary to backbone electrostatics in nucleic acid folding.

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