What α=0 means: zero moles have broken apart, so every molecule is still whole. The mixture is pure A2, no free A atoms.
Which way it leans: entirely toward molecules (the left side). This is the picture at low temperature or very high pressure, where bonds survive.
Recall Solution
(a) Recombination — small pieces glue into a bigger molecule (releases heat).
(b) Dissociation — a molecule is torn into fragments (absorbs heat).
(c) Recombination — two atoms form one molecule (releases heat).
Rule of thumb: more molecules on the right = recombination; more fragments on the right = dissociation.
Step — energy diverted. Each dissociated mole eats ΔHd; the fraction dissociated is α, so per mole of product:
Elost=αΔHd=0.15×6.0=0.90MJ/mol.Step — as a percent of the intended heating:QElost=4.00.90=0.225=22.5%.Why it matters: nearly a quarter of the heat that should raise Tc is instead locked in broken bonds — a large hit to flame temperature if it is never recovered.
Recall Solution
Why this tool: the parent gives ve∝1/M at fixed Tc and γ, so the ratio of exhaust velocities is a ratio of 1/M.
ve,1ve,2=1/M11/M2=M2M1=1620=1.25≈1.118.Result: about a +11.8% increase in ve from lighter species alone — the "good side" of the tug-of-war.
Step — simplify the denominator. The two brackets (1−α)(1+α) are a difference of squares: multiplying out, the cross terms −α and +α cancel, leaving 1−α2. And (2α)2=4α2. So the expression collapses to
Kp=1−α24α2⋅p∘p.Step — put in p=p∘ (so p/p∘=1) and Kp=1: 1−α24α2=1.0.Step — clear the fraction:4α2=1−α2⇒5α2=1.Step — solve:α2=0.2⇒α=0.2≈0.447.Reading it: about 45% of the A2 has torn apart at this temperature and pressure — heavy dissociation. (We keep the positive root only; a negative α is physically meaningless.)
Recall Solution
Why Kp stays fixed:Kp depends only on temperature, through lnKp=−ΔG∘/(RuT) — where ΔG∘ is the reaction's standard Gibbs score and Ru the universal gas constant (both in the crib sheet). Change pressure, not temperature → Kp is untouched. What responds is α.
Step — general form with pressure back in:Kp=1−α24α2⋅p∘p.
With p/p∘=2 and Kp=1:
1=1−α24α2⋅2=1−α28α2.Step — solve:8α2=1−α2⇒9α2=1⇒α=91=31≈0.333.Reading it: dissociation dropped from 0.447 to 0.333 — Le Chatelier in numbers. Squeezing the gas pushes the equilibrium back toward whole molecules.
The figure below plots α against the pressure ratio p/p∘ for Kp=1: the curve falls as you move right, and the two black dots mark exactly the points we just computed (0.447 at p∘, 0.333 at 2p∘). Trace the red curve downhill — that downhill slope is Le Chatelier.
Baseline yardstick:ve∝Tc/M=3600/22. We compare each scenario as a ratio.
Equilibrium case (Tc=3600, M=18):
vebaseveeq=3600/223600/18=1822=1.222≈1.106.
→ +10.6%: energy came back andM is lighter → pure win.
Frozen case (Tc=3100, M=18):
vebasevefr=3600/223100/18=3600×183100×22=6480068200=1.0525≈1.026.
→ +2.6%: the lighter gas still wins, but the lost heat nearly cancels it.
The lesson: dissociation is not automatically bad. Even frozen, the M-benefit can edge out the Tc-loss. Equilibrium is clearly best. This is exactly the tug-of-war the parent warned about, now with numbers.
Recall Solution
Step — definition:Da=τflow/τchem=0.20/2.0=0.10.Step — interpret:Da=0.1≪1. The gas leaves the nozzle in one-tenth of the time a reaction needs, so recombination has no time to happen.
Conclusion:frozen flow — the bond energy stays locked up and is lost. To recover it you would need a longer nozzle (bigger τflow) or faster chemistry (smaller τchem), both pushing Da upward.
(a) Dissociation at each pressure. Using Kp=1−α24α2⋅p∘p=1:
At p=p∘: 4α2=1−α2⇒5α2=1⇒α=0.2≈0.447.
At p=3p∘: 12α2=1−α2⇒13α2=1⇒α=1/13≈0.277.
(b) Flame temperature (frozen, using the given linear cost).
At p∘: Tc=3600−500⋅(0.447/0.447)=3600−500=3100K.
At 3p∘: Tc=3600−500⋅(0.277/0.447)=3600−500⋅0.6197=3600−309.9≈3290K.
(c) Verdict. Tripling pressure cut α from 0.447 to 0.277 and raised Tc from 3100 K to about 3290 K. Higher pressure → less dissociation → hotter, more complete combustion, exactly as Le Chatelier predicts (fewer moles favoured under squeeze). This is why real engines run high chamber pressure.
The figure below shows both trends at once: the black curve is αfalling as pressure rises from p∘ to 3p∘, and the red curve is Tcrising over the same range — the two computed points are marked on each. Reading the two curves together makes the "less dissociation → hotter chamber" chain visible in one glance.
Recall Solution
Step — compute each Tc/M (proportional to ve):
p∘: 3100/18=172.22≈13.12.
3p∘: 3290/19.5=168.72≈12.99.
Step — ratio:ve(p∘)ve(3p∘)=13.1212.99≈0.990.
Reading it: here the higher-pressure case is about 1.0%lower in frozen ve! The Tc gain from suppressing dissociation was outweighed by the heavierM. Lesson: raising pressure is not a free lunch for ve in frozen flow — it trades a hotter chamber for a heavier gas. The real payoff of high pc comes through equilibrium recovery and higher mass flow, not this simple frozen ratio. Mastery means seeing that no single lever wins in isolation.