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Airborne Observation of the CYGNUS NG-20 Re-Entry

David Leiser1,Clemens Müller1,Stefan Loehle1,Martin Eberhart2,Fabian Zander3,Byrenn Birch3,Ranjith Ravichandran3,Gerard Armstrong3,Andrew Lock3,Savio Poovathingal4,Alexandre Martin5
HEFDiG, IRS, University of Stuttgart1HEFDiG, IRS, University of Stuttgartt2University of Southern Queensland3university of Kentucky4University of Kentucky5

Document details

Publishing year2025 PublisherESA Space Debris Office Publishing typeConference Name of conference9th European Conference on Space Debris
Pagesn/a Volume
9
Issue
1
Editors
S. Lemmens, T. Flohrer, F. Schmitz

Abstract

On the 13th of July 2024 the ISS resupply capsule CYGNUS NG-20 entered the Earth’s atmosphere above the south pacific for a controlled destructive re-entry, marking the end of the mission. The capsule was equipped with 5 re-entry experiments (KRUPS) from the University of Kentucky. The re-entry of CYGNUS was observed from an aircraft equipped with four instrument platforms capturing imaging, spectroscopic, and polarization data which were time synchronized using a GPS signal.
While the initial goal of the mission was to observe the KRUPS capsules after their release from the spacecraft, a delay in in-space operation shifted the trajectory downrange complicating this objective. Finally, the altitude region of 90km to 75km was successfully observed giving insight into the early entry phase before the main break-up and significant fragmentation occurs.
HEFDiG deployed a new transmission grating based spectroscopic camera system. This paper will show the experimental setup, its features and methodology of data acquisition and calibration. The captured wavelength region of 450 to 700 nm, will be the focus of the analysis. Recent findings from this novel system are presented and discussed in the final paper.

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