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

Precursor Photometric Study of Astras Satellite Cluster 19.2$^\circ$ E for Geostationary Debris Profiling