Surface Composition of (99942) Apophis
Vishnu Reddy, Juan Sanchez, Roberto Furfaro, Richard Binzel, Thomas, Burbine, Lucille Le Corre, Paul Hardersen, William Bottke, Marina Brozovic

TL;DR
This study provides high-quality near-infrared spectral data of asteroid Apophis, analyzes its surface composition, and discusses implications for seismic activity during its 2029 close approach to Earth.
Contribution
It presents the most detailed pre-encounter spectral analysis of Apophis, using a naive Bayes classifier to estimate its composition and potential surface changes during the 2029 flyby.
Findings
Spectral data consistent with previous observations but with higher signal-to-noise ratio.
Likelihood of Apophis being an LL chondrite >99%.
Estimated source region in the inner main belt.
Abstract
On April 13, 2029, near-Earth asteroid (NEA) (99942) Apophis will pass at a distance of 6 Earth radii from Earth. This event will provide researchers with a unique opportunity to study the effects of tidal forces experienced by an asteroid during a close encounter with a terrestrial planet. Binzel et al. (2010) predicted that close flybys of terrestrial planets by NEAs would cause resurfacing of their regolith due to seismic shaking. In this work we present the best pre-encounter near-infrared spectra of Apophis obtained so far. These new data were obtained during the 2013 apparition using the NASA Infrared Telescope Facility (IRTF). We found that our spectral data is consistent with previous observations by Binzel et al. (2009) but with a much higher signal-to-noise ratio. Spectral band parameters were extracted from the spectra and were used to determine the composition of the…
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Taxonomy
Topicsthermodynamics and calorimetric analyses · Mass Spectrometry Techniques and Applications · Chemical Thermodynamics and Molecular Structure
