Visual walkthrough — Gibbs-Helmholtz equation
Everything on this page is a slow-motion replay of the result on the parent Gibbs–Helmholtz note.
Step 0 — The three characters, drawn
Before any algebra, meet the players. Each is just a number attached to a system at some temperature.

Look at the stacked bar. The blue bar is the full enthalpy . The orange slice, , is the "temperature tax" — entropy multiplied by temperature . Whatever is left, the green bar, is the Gibbs energy . That picture is the equation:
- — what's left over to actually "spend."
- — the total pile.
- — temperature; taller when hotter, so the orange tax grows with heat.
- — entropy; how big the tax is per degree.
Why start here? Because everything below is just this one equation, viewed from clever angles.
Step 1 — How does the budget change when we warm it up?
WHAT. We nudge the temperature by a tiny amount and watch respond, holding pressure fixed.
WHY. We want to catch , but is hidden inside . To dig it out we need to know how moves with . The rate of that movement is written — read aloud: "how fast changes as changes, keeping pressure constant."
PICTURE.

The blue curve is plotted against temperature . The red tangent line is its slope. A remarkable fact of thermodynamics is that this slope equals minus the entropy:
- Left side — the slope of the blue curve.
- — negative because : increasing makes the orange tax bigger, so slides downward. More entropy ⇒ steeper downhill slope.
Where did this come from? From the differential (derived on the parent note and part of the Maxwell relations family). At constant the term dies, leaving slope .
Step 2 — Trap using that slope
WHAT. Substitute the slope-fact into the definition to isolate .
WHY. In the unknowns are and . Step 1 gave us , purely in terms of . Swap it in and is gone — only remains unknown.
Rearranging for :
H \;=\; G \;-\; T\left(\frac{\partial G}{\partial T}\right)_P \tag{$\star$}
PICTURE.

Read the figure geometrically. At temperature :
- the green dot is ;
- the red tangent has slope ;
- extend that tangent back to . Its intercept on the vertical axis is exactly (the orange dot).
That is what says: is the "back-project the tangent to " recipe. It works, but it needs both the value and the slope. The next step makes it prettier.
- — the intercept of the tangent.
- — the height of the curve at .
- — how far the tangent climbs back as we walk from down to .
Step 3 — The magic division: differentiate , not
WHAT. Instead of studying , we study the ratio and take its slope.
WHY. Formula is clumsy. But notice the shape . That exact combination is what pops out of the quotient rule applied to . Nature is hinting: divide first.
Apply the quotient rule with , (so ):
- Numerator — this is just , which is by .
- Denominator — comes from the quotient rule's .
PICTURE.

The left panel plots (its tangent hides both and ). The right panel plots — and the annotation shows the entropy term collapsing to a constant that the derivative erases. Watch the orange "" tag get crossed out.
Step 4 — The result appears
WHAT. Combine the last two lines.
WHY. We just showed the numerator equals . Divide by :
- The slope of versus — measurable.
- — the enthalpy, cleanly, no entropy in sight.
The minus sign is honest: as rises, shrinks, and (for positive ) climbs. No entropy anywhere. Mission accomplished.
Step 5 — The friendlier form: plot against
WHAT. Change the horizontal axis from to , so we read off a straight-line slope.
WHY. That awkward disappears under a change of variable. Let . A tiny calculus fact: (because ). Substituting kills the and flips the minus:
PICTURE.

Now plotted against is (for constant ) a straight line whose slope is simply — the green triangle's rise-over-run. This is exactly the plot chemists use, and feeding into it produces the van 't Hoff equation.
- Horizontal axis — "inverse temperature," small when hot.
- Slope of the line — the enthalpy (or for a reaction).
- No minus sign — the reason we prefer this form.
Step 6 — Edge cases: don't get burned
Every scenario, so the reader never hits a surprise.
The one-picture summary

One frame compressing all six steps: start from the stacked bar (left), divide by to shed the entropy (middle), and read as the slope of versus (right). Follow the arrows and you have re-derived Gibbs–Helmholtz from nothing.
Recall Feynman: tell the whole walkthrough to a 12-year-old
Your spendable pocket money is your total savings minus a "heat tax" that gets bigger when the day is hotter — the tax is temperature times messiness . If you just watch your pocket money change as it warms up, you're mostly watching the tax wobble, so you can't see your real savings. Clever move: look at money-per-degree, . Dividing by the temperature cancels the temperature inside the tax, so the tax turns into a flat number that stops changing. Now when you watch how shifts as the day changes, the tax sits still and only your real savings show through. Plot against "one-over-temperature" and the steepness of that straight line hands you on a plate. That steepness-reading is the Gibbs–Helmholtz equation.
Recall Quick self-check
- Why does slope downward with ? ::: because slope , and entropy is positive.
- Which combination made the quotient rule useful? ::: .
- What is the slope of vs ? ::: the enthalpy .
- What happens at ? ::: the relation diverges; use the Third Law instead.
Connections
- Gibbs free energy — the budget we start from.
- Enthalpy — the prize the trick extracts.
- Entropy — the term that cancels under .
- Maxwell relations — source of the slope fact.
- van 't Hoff equation — the plot applied to .
- Kirchhoff's law (thermochemistry) — fixes drifting .
- Helmholtz free energy — the constant-volume twin.