Water Production Rates And Activity Of Interstellar Comet 2I/Borisov

We observed the interstellar comet 2I/Borisov using the Neil Gehrels-Swift Observatory’s Ultraviolet/Optical Telescope. We obtained images of the OH gas and dust surrounding the nucleus at four epochs spaced before and just after perihelion (-2.56 AU to 2.03 AU).
Water production rates increased steadily before perihelion from (7.0±1.5)×1026 molecules s−1 on Nov. 1, 2019 to (10.7±1.2)×1026 molecules s−1 on Dec. 1. This rate of increase in water production rate is slower than that of most Jupiter-family comets and quicker than most dynamically new comets. After perihelion, the water production rate decreased rapidly to (4.9±0.9)×1026 molecules s−1 on Dec. 21. Our sublimation model constrains the minimum radius of the nucleus to 0.37 km, and indicates an active fraction of at least 55% of the surface. A(0)fρ calculations show variation between 90 and 106 cm with a slight trend peaking before the perihelion, lower than previous and concurrent published values. The observations confirm that 2I/Borisov is carbon-chain depleted and enriched in NH2 relative to water.
Zexi Xing, Dennis Bodewits, John Noonan, Michele T. Bannister
(Submitted on 14 Jan 2020)
Comments: 11 pages, 3 figures, 2 tables, submitted to ApJL
Subjects: Earth and Planetary Astrophysics (astro-ph.EP)
Cite as: arXiv:2001.04865 [astro-ph.EP] (or arXiv:2001.04865v1 [astro-ph.EP] for this version)
Submission history
From: Zexi Xing
[v1] Tue, 14 Jan 2020 16:01:33 UTC (1,574 KB)
https://arxiv.org/abs/2001.04865
Astrobiology, Astrochemistry