Name:
Mainzer_2023_Planet._Sci._J._4 ...
Size:
2.207Mb
Format:
PDF
Description:
Final Published Version
Author
Mainzer, A.K.Masiero, J.R.
Abell, P.A.
Bauer, J.M.
Bottke, W.
Buratti, B.J.
Carey, S.J.
Cotto-Figueroa, D.
Cutri, R.M.
Dahlen, D.
Eisenhardt, P.R.M.
Fernandez, Y.R.
Furfaro, R.
Grav, T.
Hoffman, T.L.
Kelley, M.S.
Kim, Y.
Kirkpatrick, J.D.
Lawler, C.R.
Lilly, E.
Liu, X.
Marocco, F.
Marsh, K.A.
Masci, F.J.
McMurtry, C.W.
Pourrahmani, M.
Reinhart, L.
Ressler, M.E.
Satpathy, A.
Schambeau, C.A.
Sonnett, S.
Spahr, T.B.
Surace, J.A.
Vaquero, M.
Wright, E.L.
Zengilowski, G.R.
Affiliation
University of ArizonaUniversity of Arizona,Planetary Science Institute
Issue Date
2023-12-01
Metadata
Show full item recordPublisher
Institute of PhysicsCitation
A. K. Mainzer et al 2023 Planet. Sci. J. 4 224Journal
Planetary Science JournalRights
© 2023. The Author(s). Published by the American Astronomical Society. Original content from this work may be used under the terms of the Creative Commons Attribution 4.0 licence.Collection Information
This item from the UA Faculty Publications collection is made available by the University of Arizona with support from the University of Arizona Libraries. If you have questions, please contact us at repository@u.library.arizona.edu.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. © 2023. The Author(s). Published by the American Astronomical Society.Note
Open access journalISSN
2632-3338Version
Final published Versionae974a485f413a2113503eed53cd6c53
10.3847/PSJ/ad0468
Scopus Count
Collections
Except where otherwise noted, this item's license is described as © 2023. The Author(s). Published by the American Astronomical Society. Original content from this work may be used under the terms of the Creative Commons Attribution 4.0 licence.

