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Pat Seitzer conducts optical studies of orbital debris for NASA. Using U-M’s 0.6-meter Curtis-Schmidt telescope at Cerro Tololo in Chile, he works to assess the total amount of debris at the geosynchronous orbit (GEO) -- where most communications satellites are located -- then follows up with spectroscopy at Magellan to characterize his targets by material. The data his team gathers is fed into NASA’s public software that models the risk to functional satellites from debris such as defunct satellites and spacecraft parts.
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Paolo Marzioli,Lorenzo Frezza,Federico Curianò,Andrea Gianfermo, Niccolò Picci, Diego Amadio, Emanuele Bedetti,Maria Giulia Pancalli,Eleonora Vestito,Simone Pirrotta,Fábio Santoni,Patrick Seitzer,
8th European Conference on Space Debris (2021)
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