Sublimation-Driven Activity in Main-Belt Comet 313P/Gibbs
Henry H. Hsieh, Olivier Hainaut, Bojan Novakovic, Bryce Bolin, Larry, Denneau, Alan Fitzsimmons, Nader Haghighipour, Jan Kleyna, Rosita, Kokotanekova, Pedro Lacerda, Karen J. Meech, Marco Micheli, Nick Moskovitz,, Eva Schunova, Colin Snodgrass, Richard J. Wainscoat

TL;DR
This study confirms that main-belt comet 313P/Gibbs exhibits sublimation-driven activity over multiple years, supported by observations, dust modeling, and dynamical analysis, indicating a stable orbit within an asteroid family.
Contribution
First detailed observational and dynamical analysis of 313P/Gibbs, establishing sublimation as the activity mechanism and linking it to the Lixiaohua asteroid family.
Findings
Activity observed in 2003 and 2014, suggesting recurrent sublimation.
Dust emission persists for at least three months during active periods.
Orbit is chaotic but appears stable over >50 million years.
Abstract
We present an observational and dynamical study of newly discovered main-belt comet 313P/Gibbs. We find that the object is clearly active both in observations obtained in 2014 and in precovery observations obtained in 2003 by the Sloan Digital Sky Survey, strongly suggesting that its activity is sublimation-driven. This conclusion is supported by a photometric analysis showing an increase in the total brightness of the comet over the 2014 observing period, and dust modeling results showing that the dust emission persists over at least three months during both active periods, where we find start dates for emission no later than 2003 July 24+/-10 for the 2003 active period and 2014 July 28+/-10 for the 2014 active period. From serendipitous observations by the Subaru Telescope in 2004 when the object was apparently inactive, we estimate that the nucleus has an absolute R-band magnitude of…
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