A question was raised elsewhere regarding the possibility of plotting planetary motion using the RC2014 using the various floating point libraries available through z88dk.
The question was intriguing, not because it is a unique application, but because it is a real test of the performance of the APU Module. And, the application can relatively easily be parallelised to effectively use multiple (up to 4x) APU Modules.

So over the past few days I've been building some new tools to make effective use of multiple APU Modules from C (rather than from assembly), and also getting my head around the planetary motion equations.
The program is very rough, and doesn't account for perturbations of Jupiter, Saturn, etc, but it is sufficiently accurate to use
compare with real life at CosineKitty.
solar day 7855.501000
Geocentric Coordinates
Sun x -0.207707 y 0.995251 z 0.000000
Moon x 0.002348 y 0.001304 z -0.000156
Mercury x 0.133501 y 0.801797 z -0.047167
Venus x -0.903895 y 1.170886 z 0.042585
Mars x -1.682168 y 1.768174 z 0.052462
Jupiter x -4.230069 y 4.028960 z 0.077058
Saturn x 6.109470 y -6.722128 z -0.115441
Uranus x 14.586440 y 14.054760 z -0.143821
Neptune x -29.764930 y 5.489574 z 0.584961
The initial results have
one APU Module being about twice as fast as using the math32 soft floating point library.
Over the next while I'll do the parallelisation, and post the results and code.
This is lots of fun.
P.