2023/01/24 by Nathan Golovich, Golovich, Nathan
Engineering · Physics and Astronomy · #Advanced Semiconductor Detectors and Materials #Earth and Planetary Astrophysics (astro-ph.EP) #FOS: Physical sciences #Infrared Target Detection Methodologies #Instrumentation and Methods for Astrophysics (astro-ph.IM) #Space exploration and regulation
paper · pdf · doi:10.48550/arxiv.2301.10348
openalex publication_date 2023/01/24 · openalex created_date 2025/10/10 · openalex updated_date 2026/07/29
In 2005, the United States Congress passed a bill mandating the detection, tracking, cataloguing and characterization of 90% of the 140 meter and larger near-Earth objects (NEOs) by 2020. At the deadline ∼35% were detected, tracked and catalogued, but only a small fraction were characterized. At the present rate, it will take 40 years to meet the detection mandate, and there are insufficient global facilities dedicated to NEO characterization to come close to the characterization threshold. The major surveys focus mainly on detection and initial orbit determination, which must be refined in order to fully be tracked and catalogued. Characterization requires observations spanning multiple wavelengths, cadences, and instruments, so it is challenging for observers to acquire the requisite data in a timely manner for planetary defense. Two upcoming surveys will easily meet the 90% threshold for detection, but each will require separate facilities to tip and queue to refine orbits and characterize new discoveries, and they will provide too many discoveries for ground and space-based assets to keep up with. Here, I argue for a constellation of proliferating small satellites carrying visible and infrared sensors that would offer the needed coverage and flexibility to follow up detections from current and upcoming surveys in a timely manner. Such a constellation would enable NASA to move beyond the detection focused investments and fully meet the 2005 Congressional mandate.