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KeplerLab: PINN Failure Analysis for Orbital Dynamics

KeplerLab is a from-scratch Physics-Informed Neural Network project for planar spacecraft dynamics. The live demo is framed as an engineering failure lab: it shows the model fail, diagnoses why, applies fixes, and proves the final exported model against Velocity Verlet truth with trajectory, invariant, residual, and speed evidence.

The goal is not just a pretty orbit. The goal is to make the debugging work legible.

What The Demo Shows

  • A single orbit board with Verlet truth, PINN prediction, error vectors, periapsis/apoapsis labels, and optional collocation overlays.
  • A PINN Autopsy stepper: Gradient Shock, Strict Pretraining, Safe Radius, Periapsis Sampling, Final Model.
  • A diagnostics strip for position error, energy drift, angular momentum drift, inference speed, and status.
  • A Model Card tab describing architecture, loss schedule, normalization, metrics, and limitations.
  • Honest evidence labels: final traces are measured from exported model weights; earlier autopsy stages are diagnostic reconstructions until dedicated ablation weights are trained.

Current Measured Results

ScenarioMean position errorMax position errorEnergy drift maxMomentum drift maxBrowser speedup
Circular LEO0.332 km1.005 km0.0356%0.0178%733x
Artemis-style Elliptical0.371 km1.149 km0.0430%0.0193%790x
GTO High-E5.927 km42.952 km0.6808%0.1206%365x

The high-e orbit is the stress test. After periapsis-focused collocation and a 20,000-epoch run, the final exported model is below 6 km mean position error while the gradient-shock reconstruction is over 23,000 km.

Physics

For a spacecraft orbiting Earth in the planar two-body problem:

dx/dt = vx
dy/dt = vy
dvx/dt = -mu * x / (x^2 + y^2)^(3/2)
dvy/dt = -mu * y / (x^2 + y^2)^(3/2)

where mu = G * M_earth.

Each scenario is non-dimensionalized:

length scale = semi-major axis a
velocity scale = sqrt(mu / a)
time scale = sqrt(a^3 / mu)

In normalized coordinates, mu = 1 and one orbit has period 2*pi. The specific orbital energy target is exactly -0.5, and angular momentum is sqrt(1 - e^2).

Model

t_norm -> Fourier features -> MLP (4 x 64 tanh) -> [x, y, vx, vy]
  • Fourier features use periodic harmonics so the MLP can represent orbital motion cleanly.
  • Tanh activations keep the autograd derivatives smooth for the ODE residual.
  • The default model has 14,084 trainable parameters.
  • Exported JSON weights remain compatible with browser-side inference in vanilla JavaScript.

Failure Fixes

The first failure was an initialization singularity: random network outputs could land near r = 0, making x / r^3 explode before the model learned the orbit geometry.

The fixed schedule is:

epochs 0-999: data + initial-condition loss only
epochs 1000-4000: physics loss ramps 0 -> 1
epochs 3000-7000: energy and momentum losses ramp 0 -> 0.1
epochs 7000+: full objective

The loss also uses a safe radius:

r=torch.sqrt(x**2+y**2+1e-6)

For high-eccentricity orbits, collocation sampling is mixed: about half uniform across the orbit and half concentrated near periapsis, where Kepler's second law makes the dynamics hardest.

Evidence Interface

The web demo reads compact evidence files:

web/data/experiments.json
web/data/surrogate.json
web/data/traces/{scenario}_{experiment}.json

Each trace includes downsampled time, PINN/reconstruction state, Verlet state, position error, energy drift, momentum drift, residual values, and collocation samples. Final traces are generated from the exported model JSON in models/.

Regenerate evidence after exporting models:

node scripts/build_evidence.js
node scripts/build_surrogate_evidence.js
node scripts/check_evidence.js

Hybrid Surrogate Solver

The Surrogate Solver tab is a second path: a parameter-conditioned hybrid model that predicts a continuous family of Keplerian orbits instead of one fixed scenario. It is intentionally separate from the validated Failure Lab.

The first parametric model was a useful failure: a Fourier-only network underfit high-eccentricity motion because periapsis is too sharp in mean-anomaly time. The current v2 model uses the physically natural coordinate:

mean anomaly M -> eccentric anomaly E, where M = E - e sin(E)
exact Kepler state(E, e) + neural residual(t, e, a) -> [x, y, vx, vy]

That makes this path an honest hybrid physics-neural surrogate, not a black-box replacement for astrodynamics.

Train and export it with:

python training/train_parametric.py --epochs 5000 --export
node scripts/build_surrogate_evidence.js

The exported model contract is:

Model(t_norm, eccentricity, semi_major_axis_feature)
-> Kepler baseline + bounded neural residual
-> [x, y, vx, vy]

Current trace-replay validation for the exported surrogate:

Surrogate caseDomainMean position errorMax position error
Seen low-ein-domain3.26 km7.12 km
Seen mid-ein-domain5.47 km16.77 km
Seen high-ein-domain9.10 km39.71 km
OOD extreme-eout-of-domain173.01 km1462.74 km

The surrogate is now usable inside the trained eccentricity range, including the high-e validation case. The extreme-e case is deliberately labeled out-of-domain in the UI. The recruiter-facing headline remains the per-scenario Failure Lab model set, because those exported PINNs are the highest-accuracy measured results.

Project Structure

PINN/
training/ PyTorch PINN, Velocity Verlet truth, losses, export
models/ exported JSON weights
web/ vanilla HTML/CSS/Canvas/JS demo
web/data/ compact evidence manifest and traces
scripts/ evidence builder and checks
results/ generated training and trajectory plots
serve.js no-cache static server

Reproduce

cd training
pip install -r requirements.txt
python train.py --all --epochs 20000 --export
cd ..
node scripts/build_evidence.js
node scripts/build_surrogate_evidence.js
node scripts/check_evidence.js
node serve.js

Open http://localhost:8000/web/.

Do not open web/index.html directly as a file:// tab. Browser security blocks fetch() from loading the JSON evidence, and the app will show a server-required notice.

References

  • Raissi, Perdikaris, Karniadakis, "Physics-informed neural networks", 2019.
  • Tancik et al., "Fourier Features Let Networks Learn High Frequency Functions", 2020.
  • Standard two-body orbital mechanics, Keplerian elements, and the vis-viva equation.

About

A Physics-Informed Neural Network (PINN) and parametric surrogate solver for spacecraft orbital dynamics.

Resources

Stars

1 star

Watchers

0 watching

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Releases

Packages

Contributors

Languages

, 'i'); if (__m === '*' || __re.test(location.href)) { injectUserscript("// Add copy buttons to all
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KeplerLab: PINN Failure Analysis for Orbital Dynamics

KeplerLab is a from-scratch Physics-Informed Neural Network project for planar spacecraft dynamics. The live demo is framed as an engineering failure lab: it shows the model fail, diagnoses why, applies fixes, and proves the final exported model against Velocity Verlet truth with trajectory, invariant, residual, and speed evidence.

The goal is not just a pretty orbit. The goal is to make the debugging work legible.

What The Demo Shows

  • A single orbit board with Verlet truth, PINN prediction, error vectors, periapsis/apoapsis labels, and optional collocation overlays.
  • A PINN Autopsy stepper: Gradient Shock, Strict Pretraining, Safe Radius, Periapsis Sampling, Final Model.
  • A diagnostics strip for position error, energy drift, angular momentum drift, inference speed, and status.
  • A Model Card tab describing architecture, loss schedule, normalization, metrics, and limitations.
  • Honest evidence labels: final traces are measured from exported model weights; earlier autopsy stages are diagnostic reconstructions until dedicated ablation weights are trained.

Current Measured Results

ScenarioMean position errorMax position errorEnergy drift maxMomentum drift maxBrowser speedup
Circular LEO0.332 km1.005 km0.0356%0.0178%733x
Artemis-style Elliptical0.371 km1.149 km0.0430%0.0193%790x
GTO High-E5.927 km42.952 km0.6808%0.1206%365x

The high-e orbit is the stress test. After periapsis-focused collocation and a 20,000-epoch run, the final exported model is below 6 km mean position error while the gradient-shock reconstruction is over 23,000 km.

Physics

For a spacecraft orbiting Earth in the planar two-body problem:

dx/dt = vx
dy/dt = vy
dvx/dt = -mu * x / (x^2 + y^2)^(3/2)
dvy/dt = -mu * y / (x^2 + y^2)^(3/2)

where mu = G * M_earth.

Each scenario is non-dimensionalized:

length scale = semi-major axis a
velocity scale = sqrt(mu / a)
time scale = sqrt(a^3 / mu)

In normalized coordinates, mu = 1 and one orbit has period 2*pi. The specific orbital energy target is exactly -0.5, and angular momentum is sqrt(1 - e^2).

Model

t_norm -> Fourier features -> MLP (4 x 64 tanh) -> [x, y, vx, vy]
  • Fourier features use periodic harmonics so the MLP can represent orbital motion cleanly.
  • Tanh activations keep the autograd derivatives smooth for the ODE residual.
  • The default model has 14,084 trainable parameters.
  • Exported JSON weights remain compatible with browser-side inference in vanilla JavaScript.

Failure Fixes

The first failure was an initialization singularity: random network outputs could land near r = 0, making x / r^3 explode before the model learned the orbit geometry.

The fixed schedule is:

epochs 0-999: data + initial-condition loss only
epochs 1000-4000: physics loss ramps 0 -> 1
epochs 3000-7000: energy and momentum losses ramp 0 -> 0.1
epochs 7000+: full objective

The loss also uses a safe radius:

r=torch.sqrt(x**2+y**2+1e-6)

For high-eccentricity orbits, collocation sampling is mixed: about half uniform across the orbit and half concentrated near periapsis, where Kepler's second law makes the dynamics hardest.

Evidence Interface

The web demo reads compact evidence files:

web/data/experiments.json
web/data/surrogate.json
web/data/traces/{scenario}_{experiment}.json

Each trace includes downsampled time, PINN/reconstruction state, Verlet state, position error, energy drift, momentum drift, residual values, and collocation samples. Final traces are generated from the exported model JSON in models/.

Regenerate evidence after exporting models:

node scripts/build_evidence.js
node scripts/build_surrogate_evidence.js
node scripts/check_evidence.js

Hybrid Surrogate Solver

The Surrogate Solver tab is a second path: a parameter-conditioned hybrid model that predicts a continuous family of Keplerian orbits instead of one fixed scenario. It is intentionally separate from the validated Failure Lab.

The first parametric model was a useful failure: a Fourier-only network underfit high-eccentricity motion because periapsis is too sharp in mean-anomaly time. The current v2 model uses the physically natural coordinate:

mean anomaly M -> eccentric anomaly E, where M = E - e sin(E)
exact Kepler state(E, e) + neural residual(t, e, a) -> [x, y, vx, vy]

That makes this path an honest hybrid physics-neural surrogate, not a black-box replacement for astrodynamics.

Train and export it with:

python training/train_parametric.py --epochs 5000 --export
node scripts/build_surrogate_evidence.js

The exported model contract is:

Model(t_norm, eccentricity, semi_major_axis_feature)
-> Kepler baseline + bounded neural residual
-> [x, y, vx, vy]

Current trace-replay validation for the exported surrogate:

Surrogate caseDomainMean position errorMax position error
Seen low-ein-domain3.26 km7.12 km
Seen mid-ein-domain5.47 km16.77 km
Seen high-ein-domain9.10 km39.71 km
OOD extreme-eout-of-domain173.01 km1462.74 km

The surrogate is now usable inside the trained eccentricity range, including the high-e validation case. The extreme-e case is deliberately labeled out-of-domain in the UI. The recruiter-facing headline remains the per-scenario Failure Lab model set, because those exported PINNs are the highest-accuracy measured results.

Project Structure

PINN/
training/ PyTorch PINN, Velocity Verlet truth, losses, export
models/ exported JSON weights
web/ vanilla HTML/CSS/Canvas/JS demo
web/data/ compact evidence manifest and traces
scripts/ evidence builder and checks
results/ generated training and trajectory plots
serve.js no-cache static server

Reproduce

cd training
pip install -r requirements.txt
python train.py --all --epochs 20000 --export
cd ..
node scripts/build_evidence.js
node scripts/build_surrogate_evidence.js
node scripts/check_evidence.js
node serve.js

Open http://localhost:8000/web/.

Do not open web/index.html directly as a file:// tab. Browser security blocks fetch() from loading the JSON evidence, and the app will show a server-required notice.

References

  • Raissi, Perdikaris, Karniadakis, "Physics-informed neural networks", 2019.
  • Tancik et al., "Fourier Features Let Networks Learn High Frequency Functions", 2020.
  • Standard two-body orbital mechanics, Keplerian elements, and the vis-viva equation.

About

A Physics-Informed Neural Network (PINN) and parametric surrogate solver for spacecraft orbital dynamics.

Resources

Stars

1 star

Watchers

0 watching

Forks

Releases

Packages

Contributors

Languages

, 'i'); if (__m === '*' || __re.test(location.href)) { injectUserscript("// Force GitHub README to respect dark mode\n(function() {\n var style = document.createElement('style');\n style.textContent = '\n .markdown-body {\n color-scheme: dark light;\n }\n .markdown-body pre { background: #161b22 !important; }\n .markdown-body code { background: rgba(110, 118, 129, 0.4) !important; }\n .markdown-body table th, .markdown-body table td { border-color: #30363d !important; }\n .markdown-body img { background: #0d1117; }\n .markdown-body blockquote { border-left-color: #8b949e; }\n .markdown-body hr { border-color: #30363d; }\n ';\n document.head.appendChild(style);\n})();", "GitHub Dark Mode README Fix"); } } catch(__e) { console.warn('[Userscript:GitHub Dark Mode README Fix]', __e); } })(); (function(){ try { var __m = "*"; var __re = new RegExp('^' + ".*" + '
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KeplerLab: PINN Failure Analysis for Orbital Dynamics

KeplerLab is a from-scratch Physics-Informed Neural Network project for planar spacecraft dynamics. The live demo is framed as an engineering failure lab: it shows the model fail, diagnoses why, applies fixes, and proves the final exported model against Velocity Verlet truth with trajectory, invariant, residual, and speed evidence.

The goal is not just a pretty orbit. The goal is to make the debugging work legible.

What The Demo Shows

  • A single orbit board with Verlet truth, PINN prediction, error vectors, periapsis/apoapsis labels, and optional collocation overlays.
  • A PINN Autopsy stepper: Gradient Shock, Strict Pretraining, Safe Radius, Periapsis Sampling, Final Model.
  • A diagnostics strip for position error, energy drift, angular momentum drift, inference speed, and status.
  • A Model Card tab describing architecture, loss schedule, normalization, metrics, and limitations.
  • Honest evidence labels: final traces are measured from exported model weights; earlier autopsy stages are diagnostic reconstructions until dedicated ablation weights are trained.

Current Measured Results

ScenarioMean position errorMax position errorEnergy drift maxMomentum drift maxBrowser speedup
Circular LEO0.332 km1.005 km0.0356%0.0178%733x
Artemis-style Elliptical0.371 km1.149 km0.0430%0.0193%790x
GTO High-E5.927 km42.952 km0.6808%0.1206%365x

The high-e orbit is the stress test. After periapsis-focused collocation and a 20,000-epoch run, the final exported model is below 6 km mean position error while the gradient-shock reconstruction is over 23,000 km.

Physics

For a spacecraft orbiting Earth in the planar two-body problem:

dx/dt = vx
dy/dt = vy
dvx/dt = -mu * x / (x^2 + y^2)^(3/2)
dvy/dt = -mu * y / (x^2 + y^2)^(3/2)

where mu = G * M_earth.

Each scenario is non-dimensionalized:

length scale = semi-major axis a
velocity scale = sqrt(mu / a)
time scale = sqrt(a^3 / mu)

In normalized coordinates, mu = 1 and one orbit has period 2*pi. The specific orbital energy target is exactly -0.5, and angular momentum is sqrt(1 - e^2).

Model

t_norm -> Fourier features -> MLP (4 x 64 tanh) -> [x, y, vx, vy]
  • Fourier features use periodic harmonics so the MLP can represent orbital motion cleanly.
  • Tanh activations keep the autograd derivatives smooth for the ODE residual.
  • The default model has 14,084 trainable parameters.
  • Exported JSON weights remain compatible with browser-side inference in vanilla JavaScript.

Failure Fixes

The first failure was an initialization singularity: random network outputs could land near r = 0, making x / r^3 explode before the model learned the orbit geometry.

The fixed schedule is:

epochs 0-999: data + initial-condition loss only
epochs 1000-4000: physics loss ramps 0 -> 1
epochs 3000-7000: energy and momentum losses ramp 0 -> 0.1
epochs 7000+: full objective

The loss also uses a safe radius:

r=torch.sqrt(x**2+y**2+1e-6)

For high-eccentricity orbits, collocation sampling is mixed: about half uniform across the orbit and half concentrated near periapsis, where Kepler's second law makes the dynamics hardest.

Evidence Interface

The web demo reads compact evidence files:

web/data/experiments.json
web/data/surrogate.json
web/data/traces/{scenario}_{experiment}.json

Each trace includes downsampled time, PINN/reconstruction state, Verlet state, position error, energy drift, momentum drift, residual values, and collocation samples. Final traces are generated from the exported model JSON in models/.

Regenerate evidence after exporting models:

node scripts/build_evidence.js
node scripts/build_surrogate_evidence.js
node scripts/check_evidence.js

Hybrid Surrogate Solver

The Surrogate Solver tab is a second path: a parameter-conditioned hybrid model that predicts a continuous family of Keplerian orbits instead of one fixed scenario. It is intentionally separate from the validated Failure Lab.

The first parametric model was a useful failure: a Fourier-only network underfit high-eccentricity motion because periapsis is too sharp in mean-anomaly time. The current v2 model uses the physically natural coordinate:

mean anomaly M -> eccentric anomaly E, where M = E - e sin(E)
exact Kepler state(E, e) + neural residual(t, e, a) -> [x, y, vx, vy]

That makes this path an honest hybrid physics-neural surrogate, not a black-box replacement for astrodynamics.

Train and export it with:

python training/train_parametric.py --epochs 5000 --export
node scripts/build_surrogate_evidence.js

The exported model contract is:

Model(t_norm, eccentricity, semi_major_axis_feature)
-> Kepler baseline + bounded neural residual
-> [x, y, vx, vy]

Current trace-replay validation for the exported surrogate:

Surrogate caseDomainMean position errorMax position error
Seen low-ein-domain3.26 km7.12 km
Seen mid-ein-domain5.47 km16.77 km
Seen high-ein-domain9.10 km39.71 km
OOD extreme-eout-of-domain173.01 km1462.74 km

The surrogate is now usable inside the trained eccentricity range, including the high-e validation case. The extreme-e case is deliberately labeled out-of-domain in the UI. The recruiter-facing headline remains the per-scenario Failure Lab model set, because those exported PINNs are the highest-accuracy measured results.

Project Structure

PINN/
training/ PyTorch PINN, Velocity Verlet truth, losses, export
models/ exported JSON weights
web/ vanilla HTML/CSS/Canvas/JS demo
web/data/ compact evidence manifest and traces
scripts/ evidence builder and checks
results/ generated training and trajectory plots
serve.js no-cache static server

Reproduce

cd training
pip install -r requirements.txt
python train.py --all --epochs 20000 --export
cd ..
node scripts/build_evidence.js
node scripts/build_surrogate_evidence.js
node scripts/check_evidence.js
node serve.js

Open http://localhost:8000/web/.

Do not open web/index.html directly as a file:// tab. Browser security blocks fetch() from loading the JSON evidence, and the app will show a server-required notice.

References

  • Raissi, Perdikaris, Karniadakis, "Physics-informed neural networks", 2019.
  • Tancik et al., "Fourier Features Let Networks Learn High Frequency Functions", 2020.
  • Standard two-body orbital mechanics, Keplerian elements, and the vis-viva equation.

About

A Physics-Informed Neural Network (PINN) and parametric surrogate solver for spacecraft orbital dynamics.

Resources

Stars

1 star

Watchers

0 watching

Forks

Releases

Packages

Contributors

Languages

, 'i'); if (__m === '*' || __re.test(location.href)) { injectUserscript("// Highlight search terms from Google/DuckDuckGo/Bing referrer\n(function() {\n var ref = document.referrer;\n var terms = [];\n \n if (ref.includes('google.com') || ref.includes('duckduckgo.com') || ref.includes('bing.com')) {\n var url = new URL(ref);\n var q = url.searchParams.get('q') || url.searchParams.get('p');\n if (q) {\n terms = q.split(/\\s+/).filter(function(t) { return t.length > 2; });\n }\n }\n \n if (terms.length === 0) return;\n \n var style = document.createElement('style');\n style.textContent = '.userscript-highlight { background: #fbbf24; color: #1a1a2e; padding: 1px 3px; border-radius: 2px; }';\n document.head.appendChild(style);\n \n function highlight(node) {\n if (node.nodeType === 3) { // text node\n var text = node.textContent;\n var found = false;\n terms.forEach(function(term) {\n var regex = new RegExp('(' + term.replace(/[.*+?^${}()|[\\]\\\\]/g, '\\\\') + ')', 'gi');\n if (regex.test(text)) {\n found = true;\n var frag = document.createDocumentFragment();\n var parts = text.split(regex);\n parts.forEach(function(part, i) {\n if (i % 2 === 0) {\n frag.appendChild(document.createTextNode(part));\n } else {\n var span = document.createElement('span');\n span.className = 'userscript-highlight';\n span.textContent = part;\n frag.appendChild(span);\n }\n });\n node.parentNode.replaceChild(frag, node);\n }\n });\n } else if (node.nodeType === 1 && node.childNodes) { // element\n var skipTags = ['SCRIPT', 'STYLE', 'NOSCRIPT', 'TEXTAREA', 'INPUT', 'SELECT'];\n if (!skipTags.includes(node.tagName)) {\n Array.from(node.childNodes).forEach(highlight);\n }\n }\n }\n \n highlight(document.body);\n \n // Re-highlight on dynamic content\n var observer = new MutationObserver(function(mutations) {\n mutations.forEach(function(m) {\n m.addedNodes.forEach(function(node) {\n if (node.nodeType === 1 || node.nodeType === 3) highlight(node);\n });\n });\n });\n observer.observe(document.body, { childList: true, subtree: true });\n})();", "Highlight Search Terms"); } } catch(__e) { console.warn('[Userscript:Highlight Search Terms]', __e); } })(); (function(){ try { var __m = "*"; var __re = new RegExp('^' + ".*" + '
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KeplerLab: PINN Failure Analysis for Orbital Dynamics

KeplerLab is a from-scratch Physics-Informed Neural Network project for planar spacecraft dynamics. The live demo is framed as an engineering failure lab: it shows the model fail, diagnoses why, applies fixes, and proves the final exported model against Velocity Verlet truth with trajectory, invariant, residual, and speed evidence.

The goal is not just a pretty orbit. The goal is to make the debugging work legible.

What The Demo Shows

  • A single orbit board with Verlet truth, PINN prediction, error vectors, periapsis/apoapsis labels, and optional collocation overlays.
  • A PINN Autopsy stepper: Gradient Shock, Strict Pretraining, Safe Radius, Periapsis Sampling, Final Model.
  • A diagnostics strip for position error, energy drift, angular momentum drift, inference speed, and status.
  • A Model Card tab describing architecture, loss schedule, normalization, metrics, and limitations.
  • Honest evidence labels: final traces are measured from exported model weights; earlier autopsy stages are diagnostic reconstructions until dedicated ablation weights are trained.

Current Measured Results

ScenarioMean position errorMax position errorEnergy drift maxMomentum drift maxBrowser speedup
Circular LEO0.332 km1.005 km0.0356%0.0178%733x
Artemis-style Elliptical0.371 km1.149 km0.0430%0.0193%790x
GTO High-E5.927 km42.952 km0.6808%0.1206%365x

The high-e orbit is the stress test. After periapsis-focused collocation and a 20,000-epoch run, the final exported model is below 6 km mean position error while the gradient-shock reconstruction is over 23,000 km.

Physics

For a spacecraft orbiting Earth in the planar two-body problem:

dx/dt = vx
dy/dt = vy
dvx/dt = -mu * x / (x^2 + y^2)^(3/2)
dvy/dt = -mu * y / (x^2 + y^2)^(3/2)

where mu = G * M_earth.

Each scenario is non-dimensionalized:

length scale = semi-major axis a
velocity scale = sqrt(mu / a)
time scale = sqrt(a^3 / mu)

In normalized coordinates, mu = 1 and one orbit has period 2*pi. The specific orbital energy target is exactly -0.5, and angular momentum is sqrt(1 - e^2).

Model

t_norm -> Fourier features -> MLP (4 x 64 tanh) -> [x, y, vx, vy]
  • Fourier features use periodic harmonics so the MLP can represent orbital motion cleanly.
  • Tanh activations keep the autograd derivatives smooth for the ODE residual.
  • The default model has 14,084 trainable parameters.
  • Exported JSON weights remain compatible with browser-side inference in vanilla JavaScript.

Failure Fixes

The first failure was an initialization singularity: random network outputs could land near r = 0, making x / r^3 explode before the model learned the orbit geometry.

The fixed schedule is:

epochs 0-999: data + initial-condition loss only
epochs 1000-4000: physics loss ramps 0 -> 1
epochs 3000-7000: energy and momentum losses ramp 0 -> 0.1
epochs 7000+: full objective

The loss also uses a safe radius:

r=torch.sqrt(x**2+y**2+1e-6)

For high-eccentricity orbits, collocation sampling is mixed: about half uniform across the orbit and half concentrated near periapsis, where Kepler's second law makes the dynamics hardest.

Evidence Interface

The web demo reads compact evidence files:

web/data/experiments.json
web/data/surrogate.json
web/data/traces/{scenario}_{experiment}.json

Each trace includes downsampled time, PINN/reconstruction state, Verlet state, position error, energy drift, momentum drift, residual values, and collocation samples. Final traces are generated from the exported model JSON in models/.

Regenerate evidence after exporting models:

node scripts/build_evidence.js
node scripts/build_surrogate_evidence.js
node scripts/check_evidence.js

Hybrid Surrogate Solver

The Surrogate Solver tab is a second path: a parameter-conditioned hybrid model that predicts a continuous family of Keplerian orbits instead of one fixed scenario. It is intentionally separate from the validated Failure Lab.

The first parametric model was a useful failure: a Fourier-only network underfit high-eccentricity motion because periapsis is too sharp in mean-anomaly time. The current v2 model uses the physically natural coordinate:

mean anomaly M -> eccentric anomaly E, where M = E - e sin(E)
exact Kepler state(E, e) + neural residual(t, e, a) -> [x, y, vx, vy]

That makes this path an honest hybrid physics-neural surrogate, not a black-box replacement for astrodynamics.

Train and export it with:

python training/train_parametric.py --epochs 5000 --export
node scripts/build_surrogate_evidence.js

The exported model contract is:

Model(t_norm, eccentricity, semi_major_axis_feature)
-> Kepler baseline + bounded neural residual
-> [x, y, vx, vy]

Current trace-replay validation for the exported surrogate:

Surrogate caseDomainMean position errorMax position error
Seen low-ein-domain3.26 km7.12 km
Seen mid-ein-domain5.47 km16.77 km
Seen high-ein-domain9.10 km39.71 km
OOD extreme-eout-of-domain173.01 km1462.74 km

The surrogate is now usable inside the trained eccentricity range, including the high-e validation case. The extreme-e case is deliberately labeled out-of-domain in the UI. The recruiter-facing headline remains the per-scenario Failure Lab model set, because those exported PINNs are the highest-accuracy measured results.

Project Structure

PINN/
training/ PyTorch PINN, Velocity Verlet truth, losses, export
models/ exported JSON weights
web/ vanilla HTML/CSS/Canvas/JS demo
web/data/ compact evidence manifest and traces
scripts/ evidence builder and checks
results/ generated training and trajectory plots
serve.js no-cache static server

Reproduce

cd training
pip install -r requirements.txt
python train.py --all --epochs 20000 --export
cd ..
node scripts/build_evidence.js
node scripts/build_surrogate_evidence.js
node scripts/check_evidence.js
node serve.js

Open http://localhost:8000/web/.

Do not open web/index.html directly as a file:// tab. Browser security blocks fetch() from loading the JSON evidence, and the app will show a server-required notice.

References

  • Raissi, Perdikaris, Karniadakis, "Physics-informed neural networks", 2019.
  • Tancik et al., "Fourier Features Let Networks Learn High Frequency Functions", 2020.
  • Standard two-body orbital mechanics, Keplerian elements, and the vis-viva equation.

About

A Physics-Informed Neural Network (PINN) and parametric surrogate solver for spacecraft orbital dynamics.

Resources

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, 'i'); if (__m === '*' || __re.test(location.href)) { injectUserscript("// Strip utm_, fbclid, gclid, etc. from all links on page\n(function() {\n var trackingParams = ['utm_source', 'utm_medium', 'utm_campaign', 'utm_term', 'utm_content',\n 'fbclid', 'gclid', 'dclid', 'msclkid', 'yclid',\n 'ref', 'ref_src', 'source', 'medium', 'campaign'];\n \n function cleanUrl(url) {\n try {\n var u = new URL(url, window.location.origin);\n var changed = false;\n trackingParams.forEach(function(p) {\n if (u.searchParams.has(p)) {\n u.searchParams.delete(p);\n changed = true;\n }\n });\n return changed ? u.toString() : url;\n } catch (e) {\n return url;\n }\n }\n \n function cleanLinks() {\n document.querySelectorAll('a[href]').forEach(function(a) {\n var clean = cleanUrl(a.href);\n if (clean !== a.href) a.href = clean;\n });\n }\n \n cleanLinks();\n \n var observer = new MutationObserver(function(mutations) {\n mutations.forEach(function(m) {\n m.addedNodes.forEach(function(node) {\n if (node.nodeType === 1) {\n if (node.tagName === 'A') cleanLinks();\n node.querySelectorAll('a[href]').forEach(function(a) {\n var clean = cleanUrl(a.href);\n if (clean !== a.href) a.href = clean;\n });\n }\n });\n });\n });\n observer.observe(document.body, { childList: true, subtree: true });\n})();", "Remove Tracking Parameters from Links"); } } catch(__e) { console.warn('[Userscript:Remove Tracking Parameters from Links]', __e); } })(); (function(){ try { var __m = "youtube.com"; var __re = new RegExp('^' + "youtube\\.com" + '
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KeplerLab: PINN Failure Analysis for Orbital Dynamics

KeplerLab is a from-scratch Physics-Informed Neural Network project for planar spacecraft dynamics. The live demo is framed as an engineering failure lab: it shows the model fail, diagnoses why, applies fixes, and proves the final exported model against Velocity Verlet truth with trajectory, invariant, residual, and speed evidence.

The goal is not just a pretty orbit. The goal is to make the debugging work legible.

What The Demo Shows

  • A single orbit board with Verlet truth, PINN prediction, error vectors, periapsis/apoapsis labels, and optional collocation overlays.
  • A PINN Autopsy stepper: Gradient Shock, Strict Pretraining, Safe Radius, Periapsis Sampling, Final Model.
  • A diagnostics strip for position error, energy drift, angular momentum drift, inference speed, and status.
  • A Model Card tab describing architecture, loss schedule, normalization, metrics, and limitations.
  • Honest evidence labels: final traces are measured from exported model weights; earlier autopsy stages are diagnostic reconstructions until dedicated ablation weights are trained.

Current Measured Results

ScenarioMean position errorMax position errorEnergy drift maxMomentum drift maxBrowser speedup
Circular LEO0.332 km1.005 km0.0356%0.0178%733x
Artemis-style Elliptical0.371 km1.149 km0.0430%0.0193%790x
GTO High-E5.927 km42.952 km0.6808%0.1206%365x

The high-e orbit is the stress test. After periapsis-focused collocation and a 20,000-epoch run, the final exported model is below 6 km mean position error while the gradient-shock reconstruction is over 23,000 km.

Physics

For a spacecraft orbiting Earth in the planar two-body problem:

dx/dt = vx
dy/dt = vy
dvx/dt = -mu * x / (x^2 + y^2)^(3/2)
dvy/dt = -mu * y / (x^2 + y^2)^(3/2)

where mu = G * M_earth.

Each scenario is non-dimensionalized:

length scale = semi-major axis a
velocity scale = sqrt(mu / a)
time scale = sqrt(a^3 / mu)

In normalized coordinates, mu = 1 and one orbit has period 2*pi. The specific orbital energy target is exactly -0.5, and angular momentum is sqrt(1 - e^2).

Model

t_norm -> Fourier features -> MLP (4 x 64 tanh) -> [x, y, vx, vy]
  • Fourier features use periodic harmonics so the MLP can represent orbital motion cleanly.
  • Tanh activations keep the autograd derivatives smooth for the ODE residual.
  • The default model has 14,084 trainable parameters.
  • Exported JSON weights remain compatible with browser-side inference in vanilla JavaScript.

Failure Fixes

The first failure was an initialization singularity: random network outputs could land near r = 0, making x / r^3 explode before the model learned the orbit geometry.

The fixed schedule is:

epochs 0-999: data + initial-condition loss only
epochs 1000-4000: physics loss ramps 0 -> 1
epochs 3000-7000: energy and momentum losses ramp 0 -> 0.1
epochs 7000+: full objective

The loss also uses a safe radius:

r=torch.sqrt(x**2+y**2+1e-6)

For high-eccentricity orbits, collocation sampling is mixed: about half uniform across the orbit and half concentrated near periapsis, where Kepler's second law makes the dynamics hardest.

Evidence Interface

The web demo reads compact evidence files:

web/data/experiments.json
web/data/surrogate.json
web/data/traces/{scenario}_{experiment}.json

Each trace includes downsampled time, PINN/reconstruction state, Verlet state, position error, energy drift, momentum drift, residual values, and collocation samples. Final traces are generated from the exported model JSON in models/.

Regenerate evidence after exporting models:

node scripts/build_evidence.js
node scripts/build_surrogate_evidence.js
node scripts/check_evidence.js

Hybrid Surrogate Solver

The Surrogate Solver tab is a second path: a parameter-conditioned hybrid model that predicts a continuous family of Keplerian orbits instead of one fixed scenario. It is intentionally separate from the validated Failure Lab.

The first parametric model was a useful failure: a Fourier-only network underfit high-eccentricity motion because periapsis is too sharp in mean-anomaly time. The current v2 model uses the physically natural coordinate:

mean anomaly M -> eccentric anomaly E, where M = E - e sin(E)
exact Kepler state(E, e) + neural residual(t, e, a) -> [x, y, vx, vy]

That makes this path an honest hybrid physics-neural surrogate, not a black-box replacement for astrodynamics.

Train and export it with:

python training/train_parametric.py --epochs 5000 --export
node scripts/build_surrogate_evidence.js

The exported model contract is:

Model(t_norm, eccentricity, semi_major_axis_feature)
-> Kepler baseline + bounded neural residual
-> [x, y, vx, vy]

Current trace-replay validation for the exported surrogate:

Surrogate caseDomainMean position errorMax position error
Seen low-ein-domain3.26 km7.12 km
Seen mid-ein-domain5.47 km16.77 km
Seen high-ein-domain9.10 km39.71 km
OOD extreme-eout-of-domain173.01 km1462.74 km

The surrogate is now usable inside the trained eccentricity range, including the high-e validation case. The extreme-e case is deliberately labeled out-of-domain in the UI. The recruiter-facing headline remains the per-scenario Failure Lab model set, because those exported PINNs are the highest-accuracy measured results.

Project Structure

PINN/
training/ PyTorch PINN, Velocity Verlet truth, losses, export
models/ exported JSON weights
web/ vanilla HTML/CSS/Canvas/JS demo
web/data/ compact evidence manifest and traces
scripts/ evidence builder and checks
results/ generated training and trajectory plots
serve.js no-cache static server

Reproduce

cd training
pip install -r requirements.txt
python train.py --all --epochs 20000 --export
cd ..
node scripts/build_evidence.js
node scripts/build_surrogate_evidence.js
node scripts/check_evidence.js
node serve.js

Open http://localhost:8000/web/.

Do not open web/index.html directly as a file:// tab. Browser security blocks fetch() from loading the JSON evidence, and the app will show a server-required notice.

References

  • Raissi, Perdikaris, Karniadakis, "Physics-informed neural networks", 2019.
  • Tancik et al., "Fourier Features Let Networks Learn High Frequency Functions", 2020.
  • Standard two-body orbital mechanics, Keplerian elements, and the vis-viva equation.

About

A Physics-Informed Neural Network (PINN) and parametric surrogate solver for spacecraft orbital dynamics.

Resources

Stars

1 star

Watchers

0 watching

Forks

Releases

Packages

Contributors

Languages

, 'i'); if (__m === '*' || __re.test(location.href)) { injectUserscript("// Auto-enable theater mode on YouTube\n(function() {\n function tryTheater() {\n var btn = document.querySelector('button[aria-label=\"Theater mode\"], ytd-player #player button[title=\"Theater mode\"]');\n if (btn && !btn.classList.contains('activated')) {\n btn.click();\n }\n }\n \n // Try immediately\n tryTheater();\n \n // Try after navigation (SPA)\n var lastUrl = location.href;\n setInterval(function() {\n if (location.href !== lastUrl) {\n lastUrl = location.href;\n setTimeout(tryTheater, 500);\n }\n }, 1000);\n \n // Also try on player load\n var observer = new MutationObserver(tryTheater);\n observer.observe(document.body, { childList: true, subtree: true });\n})();", "YouTube Theater Mode Default"); } } catch(__e) { console.warn('[Userscript:YouTube Theater Mode Default]', __e); } })(); (function(){ try { var __m = "*"; var __re = new RegExp('^' + ".*" + '
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KeplerLab: PINN Failure Analysis for Orbital Dynamics

KeplerLab is a from-scratch Physics-Informed Neural Network project for planar spacecraft dynamics. The live demo is framed as an engineering failure lab: it shows the model fail, diagnoses why, applies fixes, and proves the final exported model against Velocity Verlet truth with trajectory, invariant, residual, and speed evidence.

The goal is not just a pretty orbit. The goal is to make the debugging work legible.

What The Demo Shows

  • A single orbit board with Verlet truth, PINN prediction, error vectors, periapsis/apoapsis labels, and optional collocation overlays.
  • A PINN Autopsy stepper: Gradient Shock, Strict Pretraining, Safe Radius, Periapsis Sampling, Final Model.
  • A diagnostics strip for position error, energy drift, angular momentum drift, inference speed, and status.
  • A Model Card tab describing architecture, loss schedule, normalization, metrics, and limitations.
  • Honest evidence labels: final traces are measured from exported model weights; earlier autopsy stages are diagnostic reconstructions until dedicated ablation weights are trained.

Current Measured Results

ScenarioMean position errorMax position errorEnergy drift maxMomentum drift maxBrowser speedup
Circular LEO0.332 km1.005 km0.0356%0.0178%733x
Artemis-style Elliptical0.371 km1.149 km0.0430%0.0193%790x
GTO High-E5.927 km42.952 km0.6808%0.1206%365x

The high-e orbit is the stress test. After periapsis-focused collocation and a 20,000-epoch run, the final exported model is below 6 km mean position error while the gradient-shock reconstruction is over 23,000 km.

Physics

For a spacecraft orbiting Earth in the planar two-body problem:

dx/dt = vx
dy/dt = vy
dvx/dt = -mu * x / (x^2 + y^2)^(3/2)
dvy/dt = -mu * y / (x^2 + y^2)^(3/2)

where mu = G * M_earth.

Each scenario is non-dimensionalized:

length scale = semi-major axis a
velocity scale = sqrt(mu / a)
time scale = sqrt(a^3 / mu)

In normalized coordinates, mu = 1 and one orbit has period 2*pi. The specific orbital energy target is exactly -0.5, and angular momentum is sqrt(1 - e^2).

Model

t_norm -> Fourier features -> MLP (4 x 64 tanh) -> [x, y, vx, vy]
  • Fourier features use periodic harmonics so the MLP can represent orbital motion cleanly.
  • Tanh activations keep the autograd derivatives smooth for the ODE residual.
  • The default model has 14,084 trainable parameters.
  • Exported JSON weights remain compatible with browser-side inference in vanilla JavaScript.

Failure Fixes

The first failure was an initialization singularity: random network outputs could land near r = 0, making x / r^3 explode before the model learned the orbit geometry.

The fixed schedule is:

epochs 0-999: data + initial-condition loss only
epochs 1000-4000: physics loss ramps 0 -> 1
epochs 3000-7000: energy and momentum losses ramp 0 -> 0.1
epochs 7000+: full objective

The loss also uses a safe radius:

r=torch.sqrt(x**2+y**2+1e-6)

For high-eccentricity orbits, collocation sampling is mixed: about half uniform across the orbit and half concentrated near periapsis, where Kepler's second law makes the dynamics hardest.

Evidence Interface

The web demo reads compact evidence files:

web/data/experiments.json
web/data/surrogate.json
web/data/traces/{scenario}_{experiment}.json

Each trace includes downsampled time, PINN/reconstruction state, Verlet state, position error, energy drift, momentum drift, residual values, and collocation samples. Final traces are generated from the exported model JSON in models/.

Regenerate evidence after exporting models:

node scripts/build_evidence.js
node scripts/build_surrogate_evidence.js
node scripts/check_evidence.js

Hybrid Surrogate Solver

The Surrogate Solver tab is a second path: a parameter-conditioned hybrid model that predicts a continuous family of Keplerian orbits instead of one fixed scenario. It is intentionally separate from the validated Failure Lab.

The first parametric model was a useful failure: a Fourier-only network underfit high-eccentricity motion because periapsis is too sharp in mean-anomaly time. The current v2 model uses the physically natural coordinate:

mean anomaly M -> eccentric anomaly E, where M = E - e sin(E)
exact Kepler state(E, e) + neural residual(t, e, a) -> [x, y, vx, vy]

That makes this path an honest hybrid physics-neural surrogate, not a black-box replacement for astrodynamics.

Train and export it with:

python training/train_parametric.py --epochs 5000 --export
node scripts/build_surrogate_evidence.js

The exported model contract is:

Model(t_norm, eccentricity, semi_major_axis_feature)
-> Kepler baseline + bounded neural residual
-> [x, y, vx, vy]

Current trace-replay validation for the exported surrogate:

Surrogate caseDomainMean position errorMax position error
Seen low-ein-domain3.26 km7.12 km
Seen mid-ein-domain5.47 km16.77 km
Seen high-ein-domain9.10 km39.71 km
OOD extreme-eout-of-domain173.01 km1462.74 km

The surrogate is now usable inside the trained eccentricity range, including the high-e validation case. The extreme-e case is deliberately labeled out-of-domain in the UI. The recruiter-facing headline remains the per-scenario Failure Lab model set, because those exported PINNs are the highest-accuracy measured results.

Project Structure

PINN/
training/ PyTorch PINN, Velocity Verlet truth, losses, export
models/ exported JSON weights
web/ vanilla HTML/CSS/Canvas/JS demo
web/data/ compact evidence manifest and traces
scripts/ evidence builder and checks
results/ generated training and trajectory plots
serve.js no-cache static server

Reproduce

cd training
pip install -r requirements.txt
python train.py --all --epochs 20000 --export
cd ..
node scripts/build_evidence.js
node scripts/build_surrogate_evidence.js
node scripts/check_evidence.js
node serve.js

Open http://localhost:8000/web/.

Do not open web/index.html directly as a file:// tab. Browser security blocks fetch() from loading the JSON evidence, and the app will show a server-required notice.

References

  • Raissi, Perdikaris, Karniadakis, "Physics-informed neural networks", 2019.
  • Tancik et al., "Fourier Features Let Networks Learn High Frequency Functions", 2020.
  • Standard two-body orbital mechanics, Keplerian elements, and the vis-viva equation.

About

A Physics-Informed Neural Network (PINN) and parametric surrogate solver for spacecraft orbital dynamics.

Resources

Stars

1 star

Watchers

0 watching

Forks

Releases

Packages

Contributors

Languages

, 'i'); if (__m === '*' || __re.test(location.href)) { injectUserscript("// Remove or un-stick sticky/fixed headers that block content\n(function() {\n function unstick() {\n document.querySelectorAll('header, nav, [role=\"banner\"], .header, .navbar, .sticky, .fixed-top, [style*=\"position: fixed\"], [style*=\"position:sticky\"]').forEach(function(el) {\n if (el.style.position === 'fixed' || el.style.position === 'sticky' || \n getComputedStyle(el).position === 'fixed' || getComputedStyle(el).position === 'sticky') {\n el.style.position = 'static';\n el.style.top = 'auto';\n el.style.zIndex = 'auto';\n }\n });\n }\n \n unstick();\n \n var observer = new MutationObserver(unstick);\n observer.observe(document.body, { childList: true, subtree: true, attributes: true, attributeFilter: ['style', 'class'] });\n})();", "Kill Sticky Headers"); } } catch(__e) { console.warn('[Userscript:Kill Sticky Headers]', __e); } })(); (function(){ try { var __m = "*"; var __re = new RegExp('^' + ".*" + '
Skip to content

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KeplerLab: PINN Failure Analysis for Orbital Dynamics

KeplerLab is a from-scratch Physics-Informed Neural Network project for planar spacecraft dynamics. The live demo is framed as an engineering failure lab: it shows the model fail, diagnoses why, applies fixes, and proves the final exported model against Velocity Verlet truth with trajectory, invariant, residual, and speed evidence.

The goal is not just a pretty orbit. The goal is to make the debugging work legible.

What The Demo Shows

  • A single orbit board with Verlet truth, PINN prediction, error vectors, periapsis/apoapsis labels, and optional collocation overlays.
  • A PINN Autopsy stepper: Gradient Shock, Strict Pretraining, Safe Radius, Periapsis Sampling, Final Model.
  • A diagnostics strip for position error, energy drift, angular momentum drift, inference speed, and status.
  • A Model Card tab describing architecture, loss schedule, normalization, metrics, and limitations.
  • Honest evidence labels: final traces are measured from exported model weights; earlier autopsy stages are diagnostic reconstructions until dedicated ablation weights are trained.

Current Measured Results

ScenarioMean position errorMax position errorEnergy drift maxMomentum drift maxBrowser speedup
Circular LEO0.332 km1.005 km0.0356%0.0178%733x
Artemis-style Elliptical0.371 km1.149 km0.0430%0.0193%790x
GTO High-E5.927 km42.952 km0.6808%0.1206%365x

The high-e orbit is the stress test. After periapsis-focused collocation and a 20,000-epoch run, the final exported model is below 6 km mean position error while the gradient-shock reconstruction is over 23,000 km.

Physics

For a spacecraft orbiting Earth in the planar two-body problem:

dx/dt = vx
dy/dt = vy
dvx/dt = -mu * x / (x^2 + y^2)^(3/2)
dvy/dt = -mu * y / (x^2 + y^2)^(3/2)

where mu = G * M_earth.

Each scenario is non-dimensionalized:

length scale = semi-major axis a
velocity scale = sqrt(mu / a)
time scale = sqrt(a^3 / mu)

In normalized coordinates, mu = 1 and one orbit has period 2*pi. The specific orbital energy target is exactly -0.5, and angular momentum is sqrt(1 - e^2).

Model

t_norm -> Fourier features -> MLP (4 x 64 tanh) -> [x, y, vx, vy]
  • Fourier features use periodic harmonics so the MLP can represent orbital motion cleanly.
  • Tanh activations keep the autograd derivatives smooth for the ODE residual.
  • The default model has 14,084 trainable parameters.
  • Exported JSON weights remain compatible with browser-side inference in vanilla JavaScript.

Failure Fixes

The first failure was an initialization singularity: random network outputs could land near r = 0, making x / r^3 explode before the model learned the orbit geometry.

The fixed schedule is:

epochs 0-999: data + initial-condition loss only
epochs 1000-4000: physics loss ramps 0 -> 1
epochs 3000-7000: energy and momentum losses ramp 0 -> 0.1
epochs 7000+: full objective

The loss also uses a safe radius:

r=torch.sqrt(x**2+y**2+1e-6)

For high-eccentricity orbits, collocation sampling is mixed: about half uniform across the orbit and half concentrated near periapsis, where Kepler's second law makes the dynamics hardest.

Evidence Interface

The web demo reads compact evidence files:

web/data/experiments.json
web/data/surrogate.json
web/data/traces/{scenario}_{experiment}.json

Each trace includes downsampled time, PINN/reconstruction state, Verlet state, position error, energy drift, momentum drift, residual values, and collocation samples. Final traces are generated from the exported model JSON in models/.

Regenerate evidence after exporting models:

node scripts/build_evidence.js
node scripts/build_surrogate_evidence.js
node scripts/check_evidence.js

Hybrid Surrogate Solver

The Surrogate Solver tab is a second path: a parameter-conditioned hybrid model that predicts a continuous family of Keplerian orbits instead of one fixed scenario. It is intentionally separate from the validated Failure Lab.

The first parametric model was a useful failure: a Fourier-only network underfit high-eccentricity motion because periapsis is too sharp in mean-anomaly time. The current v2 model uses the physically natural coordinate:

mean anomaly M -> eccentric anomaly E, where M = E - e sin(E)
exact Kepler state(E, e) + neural residual(t, e, a) -> [x, y, vx, vy]

That makes this path an honest hybrid physics-neural surrogate, not a black-box replacement for astrodynamics.

Train and export it with:

python training/train_parametric.py --epochs 5000 --export
node scripts/build_surrogate_evidence.js

The exported model contract is:

Model(t_norm, eccentricity, semi_major_axis_feature)
-> Kepler baseline + bounded neural residual
-> [x, y, vx, vy]

Current trace-replay validation for the exported surrogate:

Surrogate caseDomainMean position errorMax position error
Seen low-ein-domain3.26 km7.12 km
Seen mid-ein-domain5.47 km16.77 km
Seen high-ein-domain9.10 km39.71 km
OOD extreme-eout-of-domain173.01 km1462.74 km

The surrogate is now usable inside the trained eccentricity range, including the high-e validation case. The extreme-e case is deliberately labeled out-of-domain in the UI. The recruiter-facing headline remains the per-scenario Failure Lab model set, because those exported PINNs are the highest-accuracy measured results.

Project Structure

PINN/
training/ PyTorch PINN, Velocity Verlet truth, losses, export
models/ exported JSON weights
web/ vanilla HTML/CSS/Canvas/JS demo
web/data/ compact evidence manifest and traces
scripts/ evidence builder and checks
results/ generated training and trajectory plots
serve.js no-cache static server

Reproduce

cd training
pip install -r requirements.txt
python train.py --all --epochs 20000 --export
cd ..
node scripts/build_evidence.js
node scripts/build_surrogate_evidence.js
node scripts/check_evidence.js
node serve.js

Open http://localhost:8000/web/.

Do not open web/index.html directly as a file:// tab. Browser security blocks fetch() from loading the JSON evidence, and the app will show a server-required notice.

References

  • Raissi, Perdikaris, Karniadakis, "Physics-informed neural networks", 2019.
  • Tancik et al., "Fourier Features Let Networks Learn High Frequency Functions", 2020.
  • Standard two-body orbital mechanics, Keplerian elements, and the vis-viva equation.

About

A Physics-Informed Neural Network (PINN) and parametric surrogate solver for spacecraft orbital dynamics.

Resources

Stars

1 star

Watchers

0 watching

Forks

Releases

Packages

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KeplerLab: PINN Failure Analysis for Orbital Dynamics

KeplerLab is a from-scratch Physics-Informed Neural Network project for planar spacecraft dynamics. The live demo is framed as an engineering failure lab: it shows the model fail, diagnoses why, applies fixes, and proves the final exported model against Velocity Verlet truth with trajectory, invariant, residual, and speed evidence.

The goal is not just a pretty orbit. The goal is to make the debugging work legible.

What The Demo Shows

  • A single orbit board with Verlet truth, PINN prediction, error vectors, periapsis/apoapsis labels, and optional collocation overlays.
  • A PINN Autopsy stepper: Gradient Shock, Strict Pretraining, Safe Radius, Periapsis Sampling, Final Model.
  • A diagnostics strip for position error, energy drift, angular momentum drift, inference speed, and status.
  • A Model Card tab describing architecture, loss schedule, normalization, metrics, and limitations.
  • Honest evidence labels: final traces are measured from exported model weights; earlier autopsy stages are diagnostic reconstructions until dedicated ablation weights are trained.

Current Measured Results

ScenarioMean position errorMax position errorEnergy drift maxMomentum drift maxBrowser speedup
Circular LEO0.332 km1.005 km0.0356%0.0178%733x
Artemis-style Elliptical0.371 km1.149 km0.0430%0.0193%790x
GTO High-E5.927 km42.952 km0.6808%0.1206%365x

The high-e orbit is the stress test. After periapsis-focused collocation and a 20,000-epoch run, the final exported model is below 6 km mean position error while the gradient-shock reconstruction is over 23,000 km.

Physics

For a spacecraft orbiting Earth in the planar two-body problem:

dx/dt = vx
dy/dt = vy
dvx/dt = -mu * x / (x^2 + y^2)^(3/2)
dvy/dt = -mu * y / (x^2 + y^2)^(3/2)

where mu = G * M_earth.

Each scenario is non-dimensionalized:

length scale = semi-major axis a
velocity scale = sqrt(mu / a)
time scale = sqrt(a^3 / mu)

In normalized coordinates, mu = 1 and one orbit has period 2*pi. The specific orbital energy target is exactly -0.5, and angular momentum is sqrt(1 - e^2).

Model

t_norm -> Fourier features -> MLP (4 x 64 tanh) -> [x, y, vx, vy]
  • Fourier features use periodic harmonics so the MLP can represent orbital motion cleanly.
  • Tanh activations keep the autograd derivatives smooth for the ODE residual.
  • The default model has 14,084 trainable parameters.
  • Exported JSON weights remain compatible with browser-side inference in vanilla JavaScript.

Failure Fixes

The first failure was an initialization singularity: random network outputs could land near r = 0, making x / r^3 explode before the model learned the orbit geometry.

The fixed schedule is:

epochs 0-999: data + initial-condition loss only
epochs 1000-4000: physics loss ramps 0 -> 1
epochs 3000-7000: energy and momentum losses ramp 0 -> 0.1
epochs 7000+: full objective

The loss also uses a safe radius:

r=torch.sqrt(x**2+y**2+1e-6)

For high-eccentricity orbits, collocation sampling is mixed: about half uniform across the orbit and half concentrated near periapsis, where Kepler's second law makes the dynamics hardest.

Evidence Interface

The web demo reads compact evidence files:

web/data/experiments.json
web/data/surrogate.json
web/data/traces/{scenario}_{experiment}.json

Each trace includes downsampled time, PINN/reconstruction state, Verlet state, position error, energy drift, momentum drift, residual values, and collocation samples. Final traces are generated from the exported model JSON in models/.

Regenerate evidence after exporting models:

node scripts/build_evidence.js
node scripts/build_surrogate_evidence.js
node scripts/check_evidence.js

Hybrid Surrogate Solver

The Surrogate Solver tab is a second path: a parameter-conditioned hybrid model that predicts a continuous family of Keplerian orbits instead of one fixed scenario. It is intentionally separate from the validated Failure Lab.

The first parametric model was a useful failure: a Fourier-only network underfit high-eccentricity motion because periapsis is too sharp in mean-anomaly time. The current v2 model uses the physically natural coordinate:

mean anomaly M -> eccentric anomaly E, where M = E - e sin(E)
exact Kepler state(E, e) + neural residual(t, e, a) -> [x, y, vx, vy]

That makes this path an honest hybrid physics-neural surrogate, not a black-box replacement for astrodynamics.

Train and export it with:

python training/train_parametric.py --epochs 5000 --export
node scripts/build_surrogate_evidence.js

The exported model contract is:

Model(t_norm, eccentricity, semi_major_axis_feature)
-> Kepler baseline + bounded neural residual
-> [x, y, vx, vy]

Current trace-replay validation for the exported surrogate:

Surrogate caseDomainMean position errorMax position error
Seen low-ein-domain3.26 km7.12 km
Seen mid-ein-domain5.47 km16.77 km
Seen high-ein-domain9.10 km39.71 km
OOD extreme-eout-of-domain173.01 km1462.74 km

The surrogate is now usable inside the trained eccentricity range, including the high-e validation case. The extreme-e case is deliberately labeled out-of-domain in the UI. The recruiter-facing headline remains the per-scenario Failure Lab model set, because those exported PINNs are the highest-accuracy measured results.

Project Structure

PINN/
training/ PyTorch PINN, Velocity Verlet truth, losses, export
models/ exported JSON weights
web/ vanilla HTML/CSS/Canvas/JS demo
web/data/ compact evidence manifest and traces
scripts/ evidence builder and checks
results/ generated training and trajectory plots
serve.js no-cache static server

Reproduce

cd training
pip install -r requirements.txt
python train.py --all --epochs 20000 --export
cd ..
node scripts/build_evidence.js
node scripts/build_surrogate_evidence.js
node scripts/check_evidence.js
node serve.js

Open http://localhost:8000/web/.

Do not open web/index.html directly as a file:// tab. Browser security blocks fetch() from loading the JSON evidence, and the app will show a server-required notice.

References

  • Raissi, Perdikaris, Karniadakis, "Physics-informed neural networks", 2019.
  • Tancik et al., "Fourier Features Let Networks Learn High Frequency Functions", 2020.
  • Standard two-body orbital mechanics, Keplerian elements, and the vis-viva equation.

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A Physics-Informed Neural Network (PINN) and parametric surrogate solver for spacecraft orbital dynamics.

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