Title: CCD polarimetry of distant comets C/2010 S1 (LINEAR) and C/2010 R1 (LINEAR) at the 6-m telescope of the SAO RAS Author: Oleksandra V. Ivanova, Janna M. Dlugach, Viktor L. Afanasiev, Volodymyr M. Reshetnyk, Pavlo P. Korsun
We present first measurements of the degree of linear polarisation of distant comets C/2010 S1 (LINEAR) and C/2010 R1 (LINEAR) at heliocentric distances r= 5.9 - 7.0 AU. Observations were carried out with the SCORPIO-2 focal reducer at the 6-m telescope of the SAO RAS. Both comets showed considerable level of activity beyond a zone where water ice sublimation is negligible (up to 5 AU). Significant spatial variations both in the intensity and polarisation are found in both comets. The slope of radial profiles of intensity changes gradually with the distance from the photocenter: from - 0.7 near the nucleus up to about - 1.3 for larger distances (up to 100000 km). The variation in polarisation profiles indicates the non uniformity in the polarisation distribution over the coma. The polarisation degree over the coma gradually increases (in absolute value) with increasing the photocentric distance from of about - 1.9% up to - 3% for comet C/2010 S1 (LINEAR), and from of about - 2.5% up to - 3.5% for comet C/2010 R1 (LINEAR). These polarisation values are significantly higher than typical value of the whole coma polarisation (-1.5%) for comets at heliocentric distances less than 5 AU. The obtained photometric and polarimetric data are compared with those derived early for other comets at smaller heliocentric distances. Numerical modelling of light scattering characteristics was performed for media composed of particles with different refractive index, shape, and size. The computations were made by using the superposition T-matrix method. We obtained that for comet C/2010 S1 (LINEAR), the dust in the form of aggregates of overall radius R ~ 1.3 µm composed of N = 1000 spherical monomers with radius a = 0.1 µm, refractive index m = 1.65 + i 0.05, allows to obtain a satisfactory agreement between the results of polarimetric observations of comet C/2010 S1 and computations.
Comet C/2010 S1 (LINEAR) was discovered by LINEAR survry telescope. The orbital elements of the comet indicate a perihelion passage on the 19th May, 2013, at a distance of 5.9 AU from the Sun.