  Aperture photometry was performed on images (from the SuperWASP instrument)
of the 19.2$^\circ$E geostationary Astras satellite constellation over 5 nights
to form light curves and predict model and movement parameters of the
satellites. The 1KR satellite is observed to have two peaks, 90$^\circ$ out of
phase indicating rotating wings, while satellite 1M is predicted to have
shadowing due to dips in its light curve or a single wing design due to a
single major peak. All satellites have peak magnitudes at the minimum sun phase
angle 28$^\circ$ as expected. The developed methods and results serve a
precursor to developing methods to address the ultimate goal of geostationary
debris profiling.
