Outgassing Behavior of C/2012 S1 (ISON) From September 2011 to June 2013
Karen J. Meech, Bin Yang, Jan Kleyna, Megan Ansdell, Hsin-Fang Chiang,, Olivier Hainaut, Jean-Baptiste Vincent, Hermann Boehnhardt, Alan Fitzsimmons,, Travis Rector, Timm Riesen, Jacqueline V. Keane, Bo Reipurth, Henry H. Hsieh,, Peter Michaud, Giannantonio Milani

TL;DR
This study tracks the outgassing behavior of comet C/2012 S1 (ISON) from 2011 to 2013, revealing a CO-driven activity with a long outburst likely caused by CO-induced ejection of water ice grains.
Contribution
It provides the first comprehensive multi-wavelength observational analysis of ISON's outgassing, including photometry and sub-mm data, and models the sublimation processes involved.
Findings
Outgassing was dominated by CO sublimation at large distances.
A long, slow outburst began in late 2011 and peaked in early 2013.
No gas was detected at the observed wavelengths, setting upper limits.
Abstract
We report photometric observations for comet C/2012 S1 (ISON) obtained during the time period immediately after discovery (r=6.28 AU) until it moved into solar conjunction in mid-2013 June using the UH2.2m, and Gemini North 8-m telescopes on Mauna Kea, the Lowell 1.8m in Flagstaff, the Calar Alto 1.2m telescope in Spain, the VYSOS-5 telescopes on Mauna Loa Hawaii and data from the CARA network. Additional pre-discovery data from the Pan STARRS1 survey extends the light curve back to 2011 September 30 (r=9.4 AU). The images showed a similar tail morphology due to small micron sized particles throughout 2013. Observations at sub-mm wavelengths using the JCMT on 15 nights between 2013 March 9 (r=4.52 AU) and June 16 (r=3.35 AU) were used to search for CO and HCN rotation lines. No gas was detected, with upper limits for CO ranging between (3.5-4.5)E27 molec/s. Combined with published water…
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
