NEOWISE Observations of the Potentially Hazardous Asteroid (99942) Apophis
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Satpathy_2022_Planet._Sci._J._ ...
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Satpathy, A.Mainzer, A.
Masiero, J.R.
Linder, T.
Cutri, R.M.
Wright, E.L.
Pittichová, J.
Grav, T.
Kramer, E.
Affiliation
Lunar and Planetary Laboratory, University of ArizonaIssue Date
2022
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Institute of PhysicsCitation
Satpathy, A., Mainzer, A., Masiero, J. R., Linder, T., Cutri, R. M., Wright, E. L., Pittichová, J., Grav, T., & Kramer, E. (2022). NEOWISE Observations of the Potentially Hazardous Asteroid (99942) Apophis. Planetary Science Journal, 3(5).Journal
Planetary Science JournalRights
Copyright © 2022. 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
Large potentially hazardous asteroids (PHAs) are capable of causing a global catastrophe in the event of a planetary collision. Thus, rapid assessment of such an object’s physical characteristics is crucial for determining its potential risk scale. We treated the near-Earth asteroid (99942) Apophis as a newly discovered object during its 2020–2021 close approach as part of a mock planetary defense exercise. The object was detected by the Near-Earth Object Wide-field Infrared Survey Explorer (NEOWISE), and data collected by the two active bands (3.4 and 4.6 μm) were analyzed using thermal and thermophysical modeling. Our results indicate that Apophis is an elongated object with an effective spherical diameter Deff = 340 ± 70 m, a geometric visual albedo pV = 0.31 ± 0.09, and a thermal inertia Γ ∼ 150–2850 J m−2 s-½ K−1 with a best-fit value of 550 J m−2 s-½K−1. NEOWISE “discovery” observations reveal that (99942) Apophis is a PHA that would likely cause damage at a regional level and not a global one. © 2022. The Author(s). Published by the American Astronomical Society.Note
Open access journalISSN
2632-3338Version
Final published versionae974a485f413a2113503eed53cd6c53
10.3847/PSJ/ac66d1
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Except where otherwise noted, this item's license is described as Copyright © 2022. 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.