Brytalearn.How things workFind something
Back to the experimentTHE EVIDENCE BEHIND THE EXPERIENCE

What leaves changes what stays.: sources & model

Open a generic engine, follow what it carries and keep every bit of expelled mass in the story. Change who measures the motion, balance the thrust terms and discover what staging actually changes.

Scientific review · independent subject review pending

The source and model records are available for inspection. No external scientific reviewer has signed off yet.

rockets-1 · content 1 · setup format 1

What supports the explanation?

Onboard reactants and the two thrust terms

NASA Glenn Rocket Engine, Exit Pressure and Thrust Equation sections. Correct steady thrust equation; no surrounding-air requirement is inferred.

NASA Glenn · Rocket thrust equation

Closed-system momentum and effective exhaust speed

MIT 16.522 Lecture 2, pp. 1–4, Eqs. 1–11,14,17 and discussion below 19. This independently supports c=uₑ+(pₑ−pₐ)Aₑ/q; no lecture artwork is reproduced.

MIT · Space propulsion fundamentals

Changing-mass rocket equation

NASA final logarithmic derivation. Its current intermediate effective-speed expression is malformed; the lesson follows the correct thrust equation and MIT relation instead.

NASA Glenn · Ideal rocket equation

Impulse and specific impulse definitions

NASA total-impulse and final Isp relations. Specific impulse is not burn duration. The same intermediate algebra issue is handled with the independently checked equation.

NASA Glenn · Specific impulse

Conventional standard gravity

D.R. Tate, NBS Technical Note 491, 1969, §6, printed pp. 4–5/PDF pp. 10–11: standard g₀=9.80665 m/s². It differs from local g and universal G.

NBS/NIST · Standard gravity

Drag magnitude and reference-area choice

NASA coefficient and reference-area discussion. CdA values are prescribed teaching choices, not measured from the generic rocket shape.

NASA Glenn · Drag equation

Initial vertical lift-off condition

NASA rocket lift-off discussion: thrust must exceed total weight in the selected vertical setting. The lesson’s two fixed flows satisfy that condition and do not model pad contact.

NASA Glenn · Thrust to weight

Historical pressure-fed architecture and its limitations

Gibson and Wood, NASA TN D-7375, 1973, Design Phase/Block I/Engine Assembly, printed pp. 3–6. Apollo SPS used helium pressurization, separate feeds and a nonthrottleable engine. The lesson is not an SPS reconstruction or throttle simulator.

NASA · Apollo Service Propulsion System

Actual historical photograph and identity

NASA owner page: Apollo 11 Saturn V launch, 16 July 1969, Pad 39A, credit NASA. The unchanged 720×900 owner-served image derivative is educational context, not model output.

NASA · Apollo 11 launches into history

Educational/editorial photograph reuse and attribution

NASA media guidance permits factual educational/editorial use under its conditions. Source credit retained; no logos extracted, endorsement implied or blanket CC0 license invented.

NASA · Images and media guidance

What this model assumes

  1. All performance parameters are fictional teaching inputs. The generic pressure-fed geometry supplies topology, not a measured engine, operating specification or construction plan.
  2. The ideal burn is one-dimensional, nonrelativistic and free of external forces. Its literal exhaust trajectories use a declared ideal collimated relative-speed model.
  3. The pressure comparison freezes its exit conditions. It does not solve nozzle flow, separation, atmospheric variation or engine transients.
  4. Every emission group is a mass-weighted interval. Its marker size is illustrative, and its centroid does not supply total exhaust kinetic energy or a measured molecular trajectory.
  5. The observer has constant velocity. Auto-fitting a camera is only a display operation, and positions/velocities are labeled in the selected frame.
  6. The short vertical model has uniform gravity, density and prescribed CdA. It terminates at cutoff, with no guidance, curvature, rotation, variable atmosphere, heating or apogee calculation.
  7. Staging positions are an event inventory, not a separation trajectory. The no-impulse event does not grant the expelled hardware an unmodeled kick.
  8. The source photograph is historical NASA evidence, separate from the fictional model. It does not imply NASA review, endorsement or measured performance for the lesson.
  9. Paper movement is bookkeeping, not physical momentum measurement. The activity is untrialed and uses no propelled object, pressurized container, propellant or launch apparatus.
  10. Generic architecture, distinct physical experiments: The engine geometry is an original representative pressure-fed arrangement. Tank fills encode normalized usable-propellant fractions, not equal liquid volumes or a mixture. Feed pressure, propellant formulation, ignition, construction dimensions and detailed thermal/fluid behavior are not supplied. The ideal burn, pressure comparison, vertical burn and staging inventory use separately stated assumptions.
  11. Thrust from momentum and pressure: For steady axial flow, F=q uₑ+(pₑ−pₐ)Aₑ. q is positive expelled mass flow; uₑ is physical exit speed relative to the engine; pₑ and pₐ are absolute pressures; Aₑ is exit area. Both terms have force units. The pressure contribution can be negative while total thrust remains positive.
  12. Effective speed and specific impulse: For q>0, effective speed is c=F/q=uₑ+(pₑ−pₐ)Aₑ/q. Specific impulse is Isp=c/g₀, with conventional g₀=9.80665 m/s². Isp has units of seconds but is not burn duration. The off-state has no operating F/q result; the display avoids division by zero. Two introductory NASA pages contain a malformed intermediate effective-speed expression; the correct formula here follows the thrust equation, dimensions and MIT derivation.
  13. The isolated changing-mass model: This one-dimensional, nonrelativistic model prescribes constant c and q with no external force. It uses an ideal collimated exhaust whose relative speed equals c. This is a pressure-matched idealization for literal mass trajectories; the separate pressure lab’s effective c is not silently substituted for its physical exit speed. Vacuum alone does not remove gravity.
  14. Mass endpoints and the logarithm: During a burn, m(t)=mᵢ−qt and v(t)=v₀+c ln[mᵢ/m(t)]. Ideal delta-v is c ln(mᵢ/mf). Initial and final masses are total retained vehicle masses, including structure, engine, tanks, payload and any retained pressurant. Final mass is not just empty structure if payload remains.
  15. Position, cutoff and coast: The exact isolated position is x=x₀+v₀t+(c/q)[mᵢ−m−m ln(mᵢ/m)] during the burn. A stable small-time series avoids subtracting nearly equal numbers. At cutoff, mass and velocity are continuous, thrust becomes zero and subsequent isolated motion is x=xb+vb(t−tb). Zero flow or zero propellant has a deliberate no-burn coast state.
  16. The default quantitative example: For 1000→ 500 kg, c=2000 m/s and q=25 kg/s, the burn lasts 20 s. Thrust while burning is 50 kN. Final speed gain is 1386.294361 m/s and position at cutoff is 12274.112778 m from a stationary origin. Isp is 203.943243 s. These are fictional inputs and calculations, not measured engine performance.
  17. Open and closed momentum accounts: The default thrust impulse is 1,000,000 N·s, while rocket-only momentum at cutoff is 693147.180560 kg·m/s. They need not be equal because material crosses the rocket boundary. In the complete isolated system, all exhaust momentum is the opposite amount when starting at rest. The display sums actual recorded groups and reports its numerical residual.
  18. Exact emission groups: Material emitted at time τ has inertial speed w(τ)=v(τ)−c and later position x(τ)+w(τ)(T−τ). For a fixed interval, its marker uses the mass-weighted integral of this position. Cumulative exhaust momentum EP(t)=mᵢv₀−m(t)v(t); cumulative first spatial moment EX(t)=mᵢ(x₀+v₀t)−m(t)x(t). Differences of those functions plus subsequent uniform motion give each interval’s exact momentum and centroid. Completed groups do not gain later material.
  19. Changing inertial observers: For a constant observer velocity U, every part transforms as v′=v−U and x′=x−UT. The closed sums are Σm=mᵢ, Σmv′=mᵢ(v₀−U) and Σmx′=mᵢ[x₀+(v₀−U)T]. An automatically fitted camera is not an accelerating physical frame. The kinetic energy of a whole group is not obtained by pretending all its material shares the mean velocity.
  20. A conditional nozzle-pressure comparison: The separate example freezes q=20 kg/s, uₑ=2000 m/s, pₑ=80 kPa and Aₑ=0.1 m². Ambient pressure 0/50/100 kPa gives momentum thrust 40 kN and pressure contributions +8/+3/−2 kN, totaling 48/43/38 kN. Effective speed is 2400/2150/1900 m/s, while prescribed physical exit speed stays 2000 m/s. Real nozzle flow, separation and changing exit conditions are not solved.
  21. A short vertical burn with external forces: This fixed example starts at rest with 1000 kg, burns 100 kg, and uses c=2000 m/s, uniform g=9.80665 m/s², still-air density 1.2 kg/m³ and a chosen constant CdA. The equation is v′=cq/m−g−(ρCdA/2m)v|v|. The two flow choices initially exceed weight. The record stops at its own cutoff; it does not calculate an apogee, orbit or pad-contact failure.
  22. The vertical speed budget: For q=10 kg/s and CdA=.5 m², ideal delta-v 210.721031 m/s minus gravity loss 98.0665 m/s minus drag loss 11.468978 m/s gives cutoff speed 101.185553 m/s. Height at its 10 s cutoff is 516.190975 m. The q=20 kg/s comparison cuts off after 5 s with greater speed but less height at that earlier time. Integration uses fixed 2 ms RK4 steps, with interpolation for display positions.
  23. Why staging helps later: The fixed inventory is 600 kg first-stage propellant, 100 kg first-stage dry mass, 200 kg second-stage propellant and 100 kg final retained mass. With c=2000 m/s in both isolated burns: 1000→400 kg adds 1832.581464 m/s; 400→300 kg no-impulse separation adds zero; 300→100 kg adds 2197.224577 m/s. Total is 4029.806041 m/s. Keeping the empty stage yields 3218.875825 m/s. All discarded and expelled parts remain in the signed momentum ledger.
  24. Finite paper packets are a different update rule: For a packet Δm with relative speed u measured against the post-ejection rocket, conservation gives vnew=v+uΔm/M, with packet velocity w=vnew−u. Five 1 kg packets from a 10 kg start with 5 kg retained and u=10 m/s give final speed 1627/252≈6.456349 m/s. Smaller packets approach the continuous 10 ln 2≈6.931472 m/s limit. Five large packets are not claimed to equal continuous flow.

What has been checked

Analytical reference cases, conservation or transition invariants, finite drawing commands, bounded setup parsing, discovery and route integrity are checked automatically. These checks do not establish anatomical fidelity, learner outcomes or browser/device compatibility. Independent subject review, learner trials, comprehensive accessibility review and browser video encoding checks remain pending.

Each source supports the associated claim. Sources do not certify this implementation or its visuals.

About the cover illustration

Original offline rendering of the lesson’s generic pressure-fed engine architecture. Authored geometry and fictional parameters; not a manufacturer model, Saturn V reconstruction or launch forecast. The source NASA photograph and its rights are separately credited in the lesson.

Our review process