Negative polarization properties of regolith simulants -- Systematic experimental evaluation of composition effects
arXiv:2207.08767 · doi:10.1051/0004-6361/202243844
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° to 30°. 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.
References in corpus (4)
- Exploring the surface properties of Transneptunian Objects and Centaurs with polarimetric FORS1/VLT observations
- Retrieving Dust Grain Sizes from Photopolarimetry: An Experimental Approach
- Polarimetry of M-type asteroids in the context of their surface composition
- Directional aspects of vegetation linear and circular polarization biosignatures
Cited by in corpus (3)
- Reflection, emission, and polarization properties of surfaces made of hyperfine grains, and implications for the nature of primitive small bodies
- Optical spectropolarimetry of large C-complex asteroids: polarimetric evidence for heterogeneous surface compositions
- Quantitative grain size estimation on airless bodies from the negative polarization branch. I. Insights from experiments and lunar observations