Optical observations and dust modelling of comet 156P/Russell-LINEAR
K. Aravind, Prithish Halder, Shashikiran Ganesh, Devendra Sahu, Miquel, Serra-Ricart, Jos\'e J. Chamb\'o, Dorje Angchuk, Thirupathi Sivarani

TL;DR
This study combines spectroscopic, photometric, polarimetric observations and dust modelling to analyze the dust composition, activity, and jet features of comet 156P/Russell-LINEAR, revealing its typical cometary nature and similarities to comet 67P.
Contribution
It provides a comprehensive multi-method analysis of comet 156P/Russell-LINEAR, including dust composition, activity patterns, and polarization properties, which was not previously documented.
Findings
Presence of strong CN, C3, C2 emissions indicating typical comet composition.
Detection of jets and non-steady state dust outflow.
Dust dominated by large, low-porosity grains with high silicate content.
Abstract
Comet 156P/Russell-LINEAR is a short period Jupiter family comet with an orbital period of 6.44 years. The results from spectroscopic, photometric, polarimetric observations and dust modelling studies are presented here. From the spectroscopic study, strong emissions from , \AA), and can be observed during both the epochs of our observations. The Q()/Q(CN) ratio classifies the comet as a typical comet. The imaging data reveals the presence of jets. The dust emission from the comet is observed to have a non-steady state outflow due to the presence of these strong jets which subside in later epochs, resulting in a steady state outflow. Polarimetric study at two different phase angles reveals the degree of polarization to be comparable to Jupiter family comets at similar phase angles. Localized…
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