3D Laboratory // Experiment No. 01

The mesh of gravity

The graph paper of this notebook just gained a dimension. Drop masses, launch planets, and touch general relativity with your hands.

Calibrando instrumentos…

Field notes // Observations

What are you looking at?

OBS/01Gμν = 8πG/c⁴ · Tμν

Mass curves space

The mesh you see is spacetime. Einstein discovered that a mass does not "pull" on things: it deforms the geometry around it. Drag the sun and watch the grid sink beneath it.

OBS/02F = G·m₁m₂/r²

Orbits are falls

An orbiting planet is permanently falling toward the sun — but moving sideways so fast it never reaches it. Launch a planet at 100% orbital velocity and you get a perfect circle; lower it and it spirals in.

OBS/03v_esc = √2 · v_orb ≈ 141%

Escape velocity

Above 141% of orbital velocity (exactly √2), kinetic energy beats gravity and the planet escapes forever. Try it: push v₀ to the maximum and watch it leave the sheet.