High resolution optical spectroscopy of 2I/Borisov: a surprising similarity to solar system comets
Authors: Opitom Cyrielle , Jehin Emmanuel , Hutsemékers Damien , Shinnaka Yoshiharu , Manfroid Jean , Rousselot Philippe , Raghuram Susarla , Kawakita Hideyo , Fitzsimmons Alan , Meech Karen , Micheli Marco , Snodgrass Colin , Yang Bin , Hainaut Olivier 
Published: July 2021

2I/Borisov - hereafter 2I - is the first visibly active interstellar comet observed in the solar system. It was discovered on August 20, 2019 and remained visible for several months, permitting observations with various telescopes around the world and in space. We observed 2I with UVES, the high-resolution optical spectrograph mounted on the UT2 telescope at Paranal observatory in Chile, with the objective to characterize its composition. We collected spectra at 12 different epochs between November 15, 2019, and March 16, 2020, covering a heliocentric distance range from 2.1 au pre-perihelion to 2.6 au post-perihelion.Our observations allowed us to make several key measurements, some being made for the first time in the coma of an interstellar comet. We detected emissions from the radicals OH, NH, CN, CH, C2, and NH2, the [OI]forbidden oxygen lines at 557.73, 630.03, and 636.37 nm, as well as several FeI and NiI lines. We derived the abundance of FeI and NiI in the coma using the model described in [1] and find log Q(NiI)=21.88&#177;0.07 molecules/s and Q(FeI)=21.67&#177;0.16&#160; molecules/s,&#160; corresponding to log(NiI/FeI)=0.21&#177;0.18. This ratio agrees with the value recently found in solar system comets [1], as shown in Fig. 1.NH2 ortho and para lines from the ro-vibronic (0,8,0) and (0,9,0) bands were measured and allowed us to derive a NH2 ortho-to-para ratio (OPR) of 3.21&#177;0.15, corresponding to an OPR and spin temperature of ammonia of 1.11&#177;0.08 and 31+10/-5 K, respectively. These values are consistent with measurements in solar system comets and likely reflect the physico-chemical conditions in the comet inner coma.We measured the three forbidden oxygen lines and determined the ratio between the intensity of the green [OI] line and the red doublet. We obtained a rather high value G/R=0.31&#177;0.05 close to perihelion, with possibly an increasing trend while the comet moved away from the Sun. This is consistent with the high CO abundance in the coma of 2I and the increase of the CO/H2O ratio with the heliocentric distance [2,3].Finally, from the OH (0-0) emission band around 309 nm we derived a water production rate of (2.2&#177;0.2) x 1026 molecules/s close to perihelion on December 24 and 26, 2019.In conclusion, high spectral resolution observations of 2I/Borisov and the associated measurements of the NH2OPR and the Ni/Fe abundance ratio are remarkably similar to solar system comets. The measured G/R ratio is unusually high but consistent with the high abundance ratio of CO/H2O found by other investigators [2,3] and potentially suggesting formation in a colder environment.&#160;Figure 1: Comparison between the log(Ni/Fe) ratio of 2I and the values measured by [1] for a sample of solar&#160; system&#160; comets&#160; (Jupiter&#160; Family&#160;Comets&#160; (JFC),&#160; Oort&#160; Cloud Comets (OC), and Halley Type Comets (HTC)). The horizontal line represents the average value for solar system comets from [1].&#160;&#160;References:[1] Manfroid, J., Hutsem&#233;kers, D., &amp; Jehin, E. 2021, Nature, 593, 372[2] Cordiner, M. A., Milam, S. N., Biver, N., et al. 2020, Nature Astronomy, 4, 861[3] Bodewits, D., Noonan, J. W., Feldman, P. D., et al. 2020, Nature Astronomy, 4,8