Abstract
The Near-Earth Object (NEO) Surveyor mission is a NASA Observatory designed to discover and characterize asteroids and comets. The mission’s primary objective is to find the majority of objects large enough to cause severe regional impact damage (>140 m in effective spherical diameter) within its 5 yr baseline survey. Operating at the Sun-Earth L1 Lagrange point, the mission will survey to within 45° of the Sun in an effort to find objects in the most Earth-like orbits. The survey cadence is optimized to provide observational arcs long enough to distinguish near-Earth objects from more distant small bodies that cannot pose an impact hazard reliably. Over the course of its survey, NEO Surveyor will discover ∼200,000-300,000 new NEOs down to sizes as small as ∼10 m and thousands of comets, significantly improving our understanding of the probability of an Earth impact over the next century.
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CITATION STYLE
Mainzer, A. K., Masiero, J. R., Abell, P. A., Bauer, J. M., Bottke, W., Buratti, B. J., … Zengilowski, G. R. (2023). The Near-Earth Object Surveyor Mission. Planetary Science Journal, 4(12). https://doi.org/10.3847/PSJ/ad0468
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