NEOWISE Observations of the Potentially Hazardous Asteroid (99942) Apophis

Akash Satpathy, Amy Mainzer, Joseph R. Masiero, Tyler Linder, Roc M. Cutri, Edward L. Wright, Jana Pittichová, Tommy Grav, Emily Kramer

Research output: Contribution to journalArticlepeer-review

5 Scopus citations

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-½ K−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.

Original languageEnglish (US)
Article number124
JournalPlanetary Science Journal
Volume3
Issue number5
DOIs
StatePublished - May 1 2022

ASJC Scopus subject areas

  • Astronomy and Astrophysics
  • Geophysics
  • Earth and Planetary Sciences (miscellaneous)
  • Space and Planetary Science

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