The study focuses on the linear polarization of light from distant comets C/2010 S1, C/2010 R1, C/2011 KP36, C/2012 J1, C/2013 V4, and C/2014 A4, observed from 2011 to 2016 using a 6-m telescope in Russia.
The negative polarization measured was found to be significantly higher than that of comets near the Sun, indicating distinct dust properties in these distant comets.
Computer simulations using different model particle types demonstrated good agreement with the observed data, suggesting that the dust composition likely includes mixtures of water-ice and silicate or organic particles.