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DellaGiustina, D.N.Nolan, M.C.
Polit, A.T.
Moreau, M.C.
Golish, D.R.
Simon, A.A.
Adam, C.D.
Antreasian, P.G.
Ballouz, R.-L.
Barnouin, O.S.
Becker, K.J.
Bennett, C.A.
Binzel, R.P.
Bos, B.J.
Burns, R.
Castro, N.
Chesley, S.R.
Christensen, P.R.
Crombie, M.K.
Daly, M.G.
Daly, R.T.
Enos, H.L.
Farnocchia, D.
Freund, Kasper, S.
Garcia, R.
Getzandanner, K.M.
Guzewich, S.D.
Haberle, C.W.
Haltigin, T.
Hamilton, V.E.
Harshman, K.
Hatten, N.
Hughes, K.M.
Jawin, E.R.
Kaplan, H.H.
Lauretta, D.S.
Leonard, J.M.
Levine, A.H.
Liounis, A.J.
May, C.W.
Mayorga, L.C.
Nguyen, L.
Quick, L.C.
Reuter, D.C.
Rivera-Valentín, E.
Rizk, B.
Roper, H.L.
Ryan, A.J.
Sutter, B.
Westermann, M.M.
Wibben, D.R.
Williams, B.G.
Williams, K.
Wolner, C.W.V.
Affiliation
Lunar & Planetary Laboratory, University of ArizonaSchool of Earth and Space Exploration, Arizona State University
Indigo Information Services, Tucson, AZ, United States
Department of Astronomy & Planetary Science, Northern Arizona University
Issue Date
2023-10-31
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Institute of PhysicsCitation
Daniella N. DellaGiustina et al 2023 Planet. Sci. J. 4 198Journal
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 Origins, Spectral Interpretation, Resource Identification, and Security-Regolith Explorer (OSIRIS-REx) spacecraft mission characterized and collected a sample from asteroid (101955) Bennu. After the OSIRIS-REx Sample Return Capsule released to Earth’s surface in 2023 September, the spacecraft diverted into a new orbit that encounters asteroid (99942) Apophis in 2029, enabling a second mission with the same unique capabilities: OSIRIS-Apophis Explorer (APEX). On 2029 April 13, the 340 m diameter Apophis will draw within ∼32,000 km of Earth’s surface, less than 1/10 the lunar distance. Apophis will be the largest object to approach Earth this closely in recorded history. This rare planetary encounter will alter Apophis’s orbit, will subject it to tidal forces that change its spin state, and may seismically disturb its surface. APEX will distantly observe Apophis during the Earth encounter and capture its evolution in real time, revealing the consequences of an asteroid undergoing tidal disturbance by a major planet. Beginning in 2029 July, the spacecraft’s instrument suite will begin providing high-resolution data of this “stony” asteroid—advancing knowledge of these objects and their connection to meteorites. Near the mission’s end, APEX will use its thrusters to excavate regolith, a technique demonstrated at Bennu. Observations before, during, and after excavation will provide insight into the subsurface and material properties of stony asteroids. Furthermore, Apophis’s material and structure have critical implications for planetary defense. © 2023. The Author(s). Published by the American Astronomical Society.Note
Open access journalISSN
2632-3338Version
Final published Versionae974a485f413a2113503eed53cd6c53
10.3847/PSJ/acf75e
Scopus Count
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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.

