Experiment with gravity models by modifying parameters and seeing real-time results. This interactive terminal lets you explore how different values affect galaxy rotation curves.
This code calculates how galaxies rotate under standard Newtonian gravity (white) and under Erik Verlinde's Emergent Gravity theory (pink). Modify the mass, radii, or a0
parameter to see how they affect the predicted rotation curves.
M_galaxy
), the acceleration scale (a0
), or the radius range to see how they affect the rotation curves.