The Impact of Space Debris on Optical Astronomy
Anthony Mallama, Sergey Karpov, Richard E. Cole
astro-ph.IM, astro-ph.EP
Submitted: 2026-07-06
Comments: Reviewed by the IAU Centre for the Protection of the Dark and Quiet Sky
License: http://creativecommons.org/licenses/by/4.0/
The gist: Photometric observations of space debris objects brighter than magnitudes 6.0, 7.0 and 8.0 are characterized.
Terminology
Abstract
Photometric observations of space debris objects brighter than magnitudes 6.0, 7.0 and 8.0 are characterized. Those magnitudes pertain to different levels of interference with astronomy as defined by the International Astronomical Union. The densities of debris objects per square degree of sky and brighter than the magnitudes listed above are only 6, 13 and 24 parts per million, respectively. Furthermore, only about 1.4%, 2.5% and 3.8% of the 12,173 debris objects cataloged by NORAD exceed those magnitudes for even a small fraction of the time. So, debris trails have a minor impact on astronomical images and visual sightings are few. Characteristics of debris resulting from selected spacecraft collisions and rocket explosions are also quantified. This study is based on 13 million observations recorded by the MMT9 observatory.
Sources
- Call to Protect the Dark and Quiet Sky from Harmful Interference by Satellite Constellations
- Large or bright satellite constellations: Effects on observations, including on the background sky brightness
- Starlink Satellite Brightness -- Characterized From 100,000 Visible Light Magnitudes
- Brightness Characterization and Modeling for Amazon Leo Satellites
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