Disintegration of Comet C/2012 S1 (ISON) Shortly Before Perihelion: Evidence from Independent Data Sets
Zdenek Sekanina, Rainer Kracht

TL;DR
This study analyzes the disintegration process of comet C/2012 S1 (ISON) before perihelion using independent data sets, revealing early activity, explosive fragmentation, and the comet's complete disintegration shortly before closest approach to the Sun.
Contribution
It provides a detailed, multi-data set analysis of the comet's disintegration process, highlighting the sequence of activity and fragmentation events leading to its complete disintegration.
Findings
Early gravel production at ~100 AU from the Sun.
Rapid explosions causing nucleus fragmentation.
Complete disintegration 3.5 hours before perihelion.
Abstract
As an Oort Cloud object with a record small perihelion distance of 2.7 Rsun and discovered more than a year before its encounter with the Sun, comet C/2012 S1 is a subject of considerable scientific interest. Its activity along the orbit's inbound leg evolved through a series of cycles. Two remarkable events preserved in SOHO's and/or STEREO's near-perihelion images of its tail were an early massive production of gravel at heliocentric distances of up to ~100 AU, evidently by the annealing of amorphous water ice on and near the nucleus' surface; and, about a week before perihelion, a rapid series of powerful explosions, from the comet's interior, of water with dust at extremely high rates, causing precipitous fragmentation of the nucleus, shattering it into a vast number of sublimating boulders, and ending up, a few days later, with a major, sudden drop in gas emission. The…
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Taxonomy
TopicsAstro and Planetary Science · Solar and Space Plasma Dynamics · Stellar, planetary, and galactic studies
