Low NH$_{3}$/H$_{2}$O ratio in comet C/2020 F3 (NEOWISE) at 0.7 au from the Sun
Maria N. Drozdovskaya, Dominique Bockel\'ee-Morvan, Jacques Crovisier,, Brett A. McGuire, Nicolas Biver, Steven B. Charnley, Martin A. Cordiner,, Stefanie N. Milam, Cyrielle Opitom, and Anthony J. Remijan

TL;DR
This study measures the ammonia to water ratio in comet C/2020 F3 (NEOWISE) at 0.7 au, finding it significantly lower than in other comets, which suggests variability in nitrogen reservoirs and thermal processing effects in cometary comae.
Contribution
First measurement of the NH₃/H₂O ratio in comet C/2020 F3 (NEOWISE) at close heliocentric distance, revealing a lower abundance than in other comets and highlighting potential temporal and compositional variability.
Findings
NH₃/H₂O ratio is less than 0.29% at 0.7 au from the Sun.
Comet NEOWISE's NH₃ abundance is a few times lower than other comets at similar distances.
NH₃ abundance may vary with time due to dust heating and disintegration processes.
Abstract
A lower-than-solar elemental nitrogen content has been demonstrated for several comets, including 1P/Halley and 67P/C-G with independent in situ measurements of volatile and refractory budgets. The recently discovered semi-refractory ammonium salts in 67P/C-G are thought to be the missing nitrogen reservoir in comets. The thermal desorption of ammonium salts from cometary dust particles leads to their decomposition into ammonia and a corresponding acid. The NH/HO ratio is expected to increase with decreasing heliocentric distance with evidence for this in near-infrared observations. NH has been claimed to be more extended than expected for a nuclear source. Here, the aim is to constrain the NH/HO ratio in comet C/2020 F3 (NEOWISE) during its July 2020 passage. OH emission from comet C/2020 F3 (NEOWISE) was monitored for 2 months with NRT and observed from…
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