Enclosed mass
The editable layers set the enclosed mass; exterior shells cancel in the force.
M071 · Spherical gravity
Edit three spherical density layers, move a radial field probe and release a particle through a diameter tunnel. Compare a hollow cavity with a uniform sphere, then weigh the source using acquired exterior acceleration.
Physics tutorial
BackgroundA radial force is determined by the source and its geometry.
Why it mattersConnect the scene, the trajectory and a separately acquired sensor record.
Start with the essentials
The editable layers set the enclosed mass; exterior shells cancel in the force.
Outer shells still contribute a constant potential inside their cavity. The central limit is evaluated without dividing by zero.
A rest release inside a uniform sphere is harmonic; crossing the centre does not create a singular force.
The tunnel follows a diameter and does not remove source mass in this idealization.
Fit the slope through the physical zero using exterior raw accelerations and calibrated radii. Source mass is never supplied to the fit.
Typical misconceptionAn ideal model automatically describes a real planet or relaxed star cluster.
Better mental modelThe source is prescribed, the particle has no back reaction, and omitted effects are stated.
Drag the blue handle from the centre to the exterior. Compare the solid field with the dashed exterior point-mass reference.
What to observe: Inside the cavity the acceleration is zero while the potential remains negative.Try Uniform sphere, Dense core and Rest inside a hollow shell; edit all three densities.
What to observe: Density boundaries affect the interior field, while all exterior points depend only on total mass.Compare the stationary cavity release with Cross the empty cavity. Scrub the gold time handle.
What to observe: A particle entering the zero-field cavity continues with its acquired velocity.Acquire the radial scan, add noise and export the raw CSV.
What to observe: The exterior fit and exact source mass are separate outputs.