paper

Near-Infrared Polarimetric Study of Near-Earth Object 252P/LINEAR: An Implication of Scattered Light from the Evolved Dust Particles

arXiv:1907.03952 · doi:10.1051/0004-6361/201935542

Abstract

Aims. We aim to constrain the size and porosity of ejected dust particles from comet 252P/LINEAR and their evolution near the perihelion via near-infrared multiband polarimetry. A close approach of the comet to the Earth in March 2016 (~0.036 au) provided a rare opportunity for the sampling of the comet with a high spatial resolution. Methods. We made NIR JHKS bands polarimetric observations of the comet for 12 days near perihelion, interspersed between broadband optical imaging observations over four months. In addition, dynamical simulation of the comet was performed 1000 yr backward in time. Results. We detected two discontinuous brightness enhancements. Before the first enhancement, the NIR polarization degrees were far lower than those of ordinary comets at a given phase angle. Soon after the activation, however, they increased by ~13 % at most, showing unusual blue polarimetric color over the J and H bands (-2.55 % / um on average) and bluing of both J-H and H-Ks dust color. Throughout the event, the polarization vector was marginally aligned perpendicular to the scattering plane. The subsequent postperihelion reactivation of the comet lasted for approximately 1.5 months, with a factor of ~30 times pre-activation dust mass-loss rates in the Rc band. Conclusions. The marked increase in the polarization degree with blue NIR polarimetric color is reminiscent of the behaviors of a fragmenting comet D/1999 S4 (LINEAR). The most plausible scenario for the observed polarimetric properties of 252P/LINEAR would be an ejection of predominantly large, compact dust particles from the desiccated surface layer. We conjecture that the more intense solar heating that the comet has received in the near-Earth orbit would cause the paucity of small, fluffy dust particles around the nucleus of the comet.

arXiv comment16 pages, 10 figures, accepted for publication in Astronomy & Astrophysics

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