Great Arc distance between two points on a unit sphere: s=rcos^− 1(cosθ 1 cosθ 2 + sinθ 1 sinθ 2 cos(φ1−φ2)).
For a point (r, q, j)
For a point (r, q, j) j Provides a linear translation of distance, measured in radians.
For a point (r, q, j) j Provides a linear translation of distance, measured in radians. j IS the distance!
Our goal : find a simple rotational transformation which can be applied efficiently to all points, such that an arbitrary point moves to the North Pole. If successful, we can order all objects by f coordinate, to determine visibility by distance.
For a point (r, q, j)
For a point (r, q, j) q Provides a linear translation of distance, measured in radians.
For a point (r, q, j) q Provides a linear translation of distance, measured in radians. q IS the distance from prime meridian!
Rodrigues' rotation formula:
Rodrigues' rotation formula: 0
The Point of all this: Some concepts we’ve already learned could be giving us new and important insights into the problems we’re solving.