turbowarp.org/1364116950/?turbo&hqpen Made from changes to my Kerr version: https://scratch.mit.edu/projects/1241362825/ Change the sliders to change the render. Press 1 and hold space to shoot a light ray from the camera (note that rays trace backwards in time, so it is actually what ray hit the camera and where it came from) press r to render image right click screen to save image
*Note: this is not 100% accurate. I used a method that goes against general relativity, it shows the correct Schwarzschild solution in the limiting case of just one black hole, but I combined the metrics in a way general relativity does not allow (It also does not simulate gravitational waves). This was just a test of a Newtonian case limit that I found linking the potential, Φ=-GM/r, to the metric, ds^2=guv*dxu*dxv #General #Relativity #Math Hole
