Near-Infrared Spectroscopy Of The Nucleus Of Low-Activity Comet P/2016 BA$_{14}$ During Its 2016 Close Approach
Theodore Kareta (1, 2), Vishnu Reddy (2), Juan A. Sanchez (3),, Walter M. Harris (2) ((1) Lowell Observatory, (2) Lunar, Planetary, Laboratory, University of Arizona, (3) Planetary Science Institute)

TL;DR
This study presents near-infrared observations and thermal modeling of comet P/2016 BA$_{14}$, revealing its nucleus properties and suggesting it is a typical dormant comet, aiding future spacecraft mission planning.
Contribution
First detailed near-infrared spectral and thermal analysis of P/2016 BA$_{14}$, providing insights into its surface properties and activity state.
Findings
BA$_{14}$ has a low geometric albedo of 0.01-0.03.
Its reflectance spectrum is red and linear in H and K bands.
Thermal modeling suggests typical NEO beaming parameters.
Abstract
The Near-Earth Comet P/2016 BA (PanSTARRS) is a slow-rotatating nearly-dormant object, a likely dynamical twin of 252P/LINEAR, and was recently shown to have a mid-infrared spectrum very dissimilar to other comets. BA also recently selected one of the back-up targets for the ESA's \textit{Comet Interceptor}, so a clearer understanding of BA's modern properties would not just improve our understanding of how comets go dormant, but could also aid planning for a potential spacecraft visit. We present observations of BA taken on two dates during its 2016 Earth close approach with the NASA Infrared Telescope Facility, both of which are consistent with direct observations of its nucleus. The reflectance spectrum of BA is similar to 67P/Churyumov-Gerasimenko, albeit highly phase-reddened. Thermal emission contaminates the reflectance spectrum at longer…
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Taxonomy
TopicsAstro and Planetary Science · Nuclear Physics and Applications · Astronomical and nuclear sciences
