ACCRETION

Accretion · Help

Click	capture the mouse and look around
W A S D	fly forward, left, back, right
E / Q	rise / descend
Scroll	adjust flight speed · Shift to boost
Esc	release the mouse to use panels and the timeline
Click a name	autopilot to that body (in a label or the Navigate list)
Arrival	after autopilot you ride along with the body as it orbits; fly far away to break off

Space	pause and resume
[ and ]	slow down, speed up time
Timeline	drag to jump to any moment in 4.6 billion years

Planet and Sun sizes, orbital distances, eccentricities and inclinations are true to scale (1 unit = 1000 km). Orbits use JPL approximate Keplerian elements.
Event chronology follows the standard model: first solids 4.567 billion years ago, gas disk gone within about 8 million years, the Moon forming impact about 4.51 billion years ago, heavy bombardment tailing off by 3.8 billion years ago.
The Moon really did form close to Earth and has been receding ever since; the simulation reproduces this.

Asteroids, planetesimals and the pre-solar cloud are enlarged and brightened, otherwise they would be invisible at true scale.
At high time speeds, orbital motion is smoothed rather than strobed; positions stay on the true orbits.
Planet formation locations are simplified: worlds grow near their present orbits, skipping early migration.

Planet textures: Solar System Scope, CC BY 4.0 · Orbits: JPL approximate ephemerides · Rendering: three.js