Following are a few things to note and the new output plot as well as a video I made to validate some aspects of the model.
Things to note:
- The torques and forces are in the body frame. To make it useful it needs to be put into the orbital frame (check the video).
- The average temperature reaches steady state as the number of faces increases and the asteroid becomes circular about the rotation axis (if the rotational and orbital angular momentum axes also align).
- The warmest time on the asteroids is in the afternoon (around 2-4).
For the video below, the yellow line is the direction of solar rays, the red line is the direction of the force due to solar radiation pressure and thermal emittance. The color of the asteroid is relative to it's temperature with the colormap [1 0 0] (red) being the total hottest temperature and [0 0 0] being absolute zero.
Asteroid Rotation Video viewed along the Z-axis
(Sorry about the resolution, uploading it requires compressing)
New output plot
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