Negative polarization properties of regolith simulants -- Systematic experimental evaluation of composition effects

TL;DR

This study experimentally investigates how mineral composition and aggregate size influence the negative polarization of asteroid regolith simulants, revealing composition-dependent effects and invariance to aggregate size.

Contribution

It systematically evaluates the effects of mineral mixing and aggregate size on polarization phase curves of asteroid-like regolith simulants.

Findings

Mixing minerals significantly alters polarization behavior.

Negative polarization is unaffected by aggregate sizes up to centimeters.

Results help explain polarization features of certain asteroid classes.

Abstract

Polarization phase curves of asteroids and other small airless bodies are influenced by the compositional and physical properties of their regolith. The mixing of minerals composing the regolith influences the negative polarization at small phase angles because it changes the multiple scattering properties of the medium. This work aims to demonstrate experimentally how the mixing effect influences the polarization phase curve at small phase angles for different mineralogies relevant for asteroids, and to determine how different aggregate sizes affect the negative polarization. We prepared a set of binary and ternary mixtures with different common minerals on asteroids and one set of the same mixture with different aggregate sizes. We measured their reflected light at 530 nm with full Stokes polarimetry at phase angles ranging from 0.8{\deg} to 30{\deg}. The mixing effect of the mixtures with both bright and dark minerals significantly changes the behavior of the phase curves in terms of minimum polarization, phase angle of the minimum, and inversion angle with respect to the mineral components that are mixed together. The changes in phase curve could explain the polarization observation of particular classes of asteroids (F and L class) and other asteroids with peculiar polarization curves or photometric properties. Furthermore, we demonstrate that the negative polarization is invariant to the presence of dust aggregates up to centimeter sizes.