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An Overview of Ground-Based Radar and Optical Measurements Utilized By the Nasa Orbital Debris Program OfficeFor over 30 years, the NASA Orbital Debris Program Office (ODPO) has led the characterization of orbital debris (OD) too small to be tracked by the U.S. Space Surveillance Network (SSN), yet which may pose the greatest threat to human spaceflight and robotic missions. Measurements from specialized sensors, including ground-based radars and telescopes capable of detecting smaller objects, provide the foundation for developing statistical models to describe the current state and future evolution of the OD environment from low Earth orbit (LEO) to geosynchronous Earth orbit (GEO). Since 1990, the ODPO has partnered with the U.S. Department of Defense and the Massachusetts Institute of Technology Lincoln Laboratory (MIT/LL) to collect data using the Haystack Ultrawideband Satellite Imaging Radar (HUSIR) – formerly Haystack – to characterize OD in LEO with a sensitivity of approximately 5 mm at 1000 km altitude. In addition, since 1993, the Goldstone Orbital Debris Radar, operated by NASA’s Jet Propulsion Laboratory, has provided data on OD as small as approximately 2-3 mm for altitudes below 1000 km, some of the most sensitive ground-based measurements achievable at these altitudes. Recently, collaborations with the 18th Space Control Squadron of the U.S. Space Force have also provided the ODPO with special datasets from the Space Fence to extend coverage below the historical SSN limit of 10 cm and to characterize individual breakup events in LEO. For GEO altitudes, the Eugene Stansbery Meter Class Autonomous Telescope (ES-MCAT), a joint NASA-Air Force Research Laboratory project that reached full operational capability in 2021, collects data on debris smaller than 1 m and provides coverage of debris in historically under-sampled high-altitude orbital regimes. This paper summarizes the radar and optical sensors utilized by the ODPO, their unique capabilities, and recent datasets and applications for statistical sampling of the dynamic OD environment.
Document ID
20230014530
Acquisition Source
Johnson Space Center
Document Type
Conference Paper
Authors
Alyssa Manis
(Johnson Space Center Houston, Texas, United States)
Jessica A. Arnold
(Jacobs (United States) Dallas, Texas, United States)
James Murray
(Tomorrow.io Boston, Massachusetts, United States)
Brent Buckalew
(Jacobs (United States) Dallas, Texas, United States)
Corbin Cruz
(Jacobs (United States) Dallas, Texas, United States)
Mark Matney
(Johnson Space Center Houston, Texas, United States)
Date Acquired
October 5, 2023
Subject Category
Optics
Space Communications, Spacecraft Communications, Command and Tracking
Meeting Information
Meeting: 2nd International Orbital Debris Conference (IOC II)
Location: Houston, TX
Country: US
Start Date: December 4, 2023
End Date: December 7, 2023
Sponsors: Lunar and Planetary Institute
Funding Number(s)
WBS: 817091.40.81.72
Distribution Limits
Public
Copyright
Portions of document may include copyright protected material.
Technical Review
NASA Technical Management
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