3.3.36 · D4Rocket Propulsion

Exercises — Burn rate r = a·P^n — Vieille's law

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This page drills Vieille's law . Keep this near you:

Here is the linear burn rate (how fast the solid surface recedes, in mm/s), is the chamber pressure, the burn-rate coefficient, and the pressure exponent.


Level 1 — Recognition

Recall Solution L1.1

What: we plug in . Why: anything raised to a power, when the base is , is : . That's the whole point of defining "at ": is the burn rate at unit pressure. The exponent never gets a chance to act because to any power stays .

Recall Solution L1.2

(i) the exponent — it is the sensitivity; a bigger means pressure changes swing the rate harder. (ii) the coefficient — the rate when . (iii) itself — the speed the burning surface eats into the solid, not the exhaust speed.


Level 2 — Application

Recall Solution L2.1

What: direct substitution. Why the exponential appears: is easiest through — the log turns the power into a multiply, then undoes the log. Sense check: pressure went up but barely doubled — that's exactly what a small should do.

Recall Solution L2.2

What: solve for . Why: divide first to isolate the power, then undo the power by raising to . Because means "square root of ", to get twice the burn rate you need four times the pressure.

Recall Solution L2.3

Why the ratio trick: we don't know , but dividing the law at two pressures cancels it completely:


Level 3 — Analysis

Recall Solution L3.1

Step 1 (why divide): the ratio kills so we can isolate : Step 2 (why logs): logs pull down from the exponent: Step 3 — recover by putting back into one point: Sense check: → this propellant is stable. ✔

Figure — Burn rate r = a·P^n — Vieille's law
Recall Solution L3.2

Why a straight line at all: taking of gives — the equation of a line with slope and intercept . Slope (=): rise over run between the two marked points: Intercept (=): at (i.e. ), , so . This is exactly the extraction method engineers use on real strand-burner runs.


Level 4 — Synthesis

Recall Solution L4.1

Why compare exponents: at equilibrium generation = exhaust. Bump up a little; whichever term grows faster wins.

  • A (): exhaust () grows faster than generation (). Extra gas leaves faster than it is made → pressure falls back → stable, survives.
  • B (): generation () outpaces exhaust (). The bump feeds itself → runaway → explodes. ❌ The single dividing line is . This is the 80/20 fact of the whole topic.
Recall Solution L4.2

Why divide distance by rate: is the recession speed, so time = distance ÷ speed, exactly like walking distance over walking speed: Link: the web comes from the Solid Rocket Motor Grain Geometry; the value of comes from Vieille's law given the operating . This is where the burn-rate law meets the actual hardware.

Recall Solution L4.3

Why the ratio: percent change only needs the factor, and the factor drops : So rises by . Sense check: pressure rose but rate only — small softens the response, as it should.


Level 5 — Mastery

Recall Solution L5.1

Why moves with temperature: a warmer grain starts closer to its ignition temperature, so less heat is needed to burn the next layer → faster recession → larger . This is Temperature Sensitivity of Propellants in action. Since and are shared, the ratio is just : Consequence: the same rocket burns faster on a hot day — higher peak , shorter burn. This is why motors are temperature-conditioned before firing.

Recall Solution L5.2

Stability first: both have , so both are stable — that filter alone doesn't decide it. Doubling test: when , rate factor : Y () nearly doubles — it meets spec (ii). X gives only . The tension: Y is closer to the knife-edge, so it is stable but less forgiving; a real designer weighs "responsiveness" (large ) against "safety margin" (distance below ). Spec-matching alone points to Y here.

Recall Solution L5.3

Why check the ratios: if one power law fits, then each doubling of must give the same slope. Use the two ratios: The two slopes agree () → one law fits. From the first point : . Verify the middle point: ✔.


Recall One-paragraph recap

Every problem here is one law, , read in three directions: forward (plug in ), backward (solve for ), and sideways (ratios and logs to get without knowing ). Stability is the single inequality ; temperature lives inside ; the web-over-rate gives burn time. Master those four moves and D4 is done.