3.4.22 · D1Rocket Flight Mechanics

Foundations — Thermal protection systems — ablators (PICA, SLA), metallic tiles, RCC

2,440 words11 min readBack to topic

This page builds the toolbox. The parent note throws around symbols like , , , , and phrases like "stagnation point" and "". If any of those looked like magic runes, this page turns them into pictures. We go in order, so each idea leans on the one before.


1. Speed — how fast, in a straight line

The picture: an arrow along the flight path. The length of the arrow is the speed. A longer arrow means more distance covered each tick of the clock.

Why the topic needs it: every heating formula depends on — and dangerously so. As we build up to the convective heating law in section 6, we will see the heat scale as , meaning doubling the speed multiplies the heating eightfold.


2. Kinetic energy and specific energy

Why the and not just ? Because energy is what it takes to stop the motion, and stopping something twice as fast costs four times as much work — the captures that. Try it: pushing against a wall twice as hard over twice the distance is four times the effort.

The picture: imagine slicing the vehicle into 1-kg cubes. Each cube carries the same . This lets us talk about heating "per kg of shield" without knowing the total mass.

Worked number (matches the parent): at m/s, The prefix M (mega) means one million, so MJ J. That is the "terrifying" number: about four times the energy needed to boil away a kilogram of steel.

See Specific Impulse and Energy Budgets for where this "per kilogram" bookkeeping comes from.


3. Density — how much air is packed in

The picture: a box one metre on each side. Count the air molecules inside it and weigh them — that weight is . A crowded box = high density; a nearly empty box = low density.

Why the topic needs it: the heat the vehicle feels depends on how much hot gas is thrown at it each second, and that is set by . As we will see in section 6, the convective heating combines and into a product that peaks at a middle altitude — high up there is too little air ( small), low down the vehicle has already slowed ( small). We meet that product properly once its formula is on the table.


4. Nose radius — how "round" the front is

The picture: below, a fat rounded nose (large ) versus a pointy nose (small ), each with the biggest circle that fits.

Why the topic needs it: the stagnation-point heating scales as — a bigger, blunter nose lowers heating. We explain why in section 6, right after the convective-flux symbol is defined. This single fact explains why reentry capsules are round bowls, not arrows. Details live in Blunt Body Aerodynamics.


5. The bow shock and the stagnation point

The picture: a curved shock standing off the nose like a bow-wave in front of a boat. Between the shock and the wall is the glowing shock layer. The centreline hits the wall at the stagnation point.

More in Bow Shock and Stagnation Point and Reentry Aerothermodynamics.


6. Convective heat flux — heat carried into the wall

The picture: shine a heat lamp on a stamp-sized patch of the shield. is how brightly that patch is being cooked; is the share of that cooking done by hot gas scrubbing against the surface.


7. Temperature , radiative flux , and the exponent-four law

Why the fourth power and not just ? Because radiated power grows ferociously with temperature — this is measured, not chosen, and captured by the Stefan–Boltzmann law. It is the reason a glowing tile can dump enormous heat back out: doubling multiplies the radiated heat by .

The picture: the same tile at rising temperature glows dull red, orange, then white — and the arrows of escaping light thicken far faster than the temperature climbs.

The full story is in Radiative Heat Transfer and Stefan–Boltzmann Law.


8. The ablator symbols: , , ,

The picture: the char surface peeling back like a slowly melting candle; is the speed the surface retreats, is the mass of "smoke" it releases.


How the pieces feed the topic

speed v

specific kinetic energy e_k

convective heat flux q_conv

air density rho

nose radius R_n

bow shock and stagnation point

heat flux at the wall

temperature T

radiative heat flux q_rad

surface energy balance

heat of ablation Q star

mass loss rate m dot

Thermal Protection System choice

Every box carries a symbol you now own, spelled the same way as in the text: is "q_conv", is "q_rad", and is "m dot". The parent note's formulas are just these boxes wired together.


Equipment checklist

Cover the right side and answer each before revealing:

What does the dot in or mean?
"Per second" — it marks a rate.
What are the units of speed ?
metres per second (m/s).
Why is kinetic energy and not just ?
Stopping something twice as fast costs four times the work, so energy grows with .
What does "specific" mean in ?
Per kilogram (J/kg).
What is and its units?
Air density — kilograms of air per cubic metre (kg/m³).
Why does convective heating carry a factor ?
Each kg of gas dumps energy , and the mass rammed in per second is ; multiplied that gives .
Does a big nose radius raise or lower heating?
Lower it — a blunter nose grows a thicker boundary-layer cushion, so heating scales as .
Where is the stagnation point?
The dead-centre spot on the nose where oncoming air is brought fully to rest — the hottest point.
What are the units of heat flux ?
Watts per square metre (W/m²).
What distinguishes from ?
is heat carried by hot gas touching the wall; is heat arriving/leaving as glowing light.
Heat flux versus total heat load — the difference?
is a rate at one instant; total load is summed over the whole reentry (J/m²).
What does the Stefan–Boltzmann law say a hot surface radiates?
.
What is emissivity ?
A dial from 0 (mirror) to 1 (perfect radiator) for how well a surface glows heat away.
What does measure?
Joules of heat absorbed per kilogram of ablator that decomposes (J/kg).
How is recession rate related to mass loss ?
.