Low NH/HO ratio in comet C/2020 F3 (NEOWISE) at 0.7 au from the Sun
arXiv:2307.11486 · doi:10.1051/0004-6361/202346402
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 GBT on 24 July and 11 August 2020. Contemporaneously with the 24 July 2020 OH observations, the NH hyperfine lines were targeted with GBT. The concurrent GBT and NRT observations allowed the OH quenching radius to be determined at km on 24 July 2020, which is important for accurately deriving . C/2020 F3 (NEOWISE) was a highly active comet with molec s one day before perihelion. The upper limit for is at au from the Sun. The obtained NH/HO ratio is a factor of a few lower than measurements for other comets at such heliocentric distances. The abundance of NH may vary strongly with time depending on the amount of water-poor dust in the coma. Lifted dust can be heated, fragmented, and super-heated; whereby, ammonium salts, if present, can rapidly thermally disintegrate and modify the NH/HO ratio.
Accepted for publication in A&A; 18 pages, 8 figures, 6 tables
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