Thermophysical model for realistic surface layers on airless small bodies: applied to study the spin orientation and surface dust properties of (24) Themis from WISE/NEOWISE multi-epoch thermal lightcurves

TL;DR

This paper introduces a detailed thermophysical model (RSTPM) for airless small bodies, enabling precise interpretation of thermal lightcurves to determine physical properties like spin orientation and surface dust characteristics, demonstrated on asteroid (24) Themis.

Contribution

The paper presents a comprehensive thermophysical model that accounts for realistic surface and orbital factors, improving the interpretation of multi-epoch thermal lightcurves for small bodies.

Findings

Derived Themis's spin orientation as (137°, 59°) in ecliptic coordinates.

Estimated dust grain size on Themis surface to be around 140 μm.

Inferred surface thermal inertia varies seasonally from 3 to 60 Jm^{-2}s^{-0.5}K^{-1}.

Abstract

This work proposes a thermophysical model for realistic surface layers on airless small bodies (RSTPM), for the use of interpreting their multi-epoch thermal lightcurves (e.g WISE/NEOWISE). RSTPM considers real orbital cycle, rotation cycle, rough surface, temperature dependent thermal parameters, as well as contributions of sunlight reflection to observations, hence being able to produce precise temperature distribution and thermal emission of airless small bodies regarding the variations in orbital time scales. Details of the physics, mathematics and numerical algorithms of RSTPM are presented. When used to interpret multi-epoch thermal lightcurves by WISE/NEOWISE, RSTPM can give constraints on the spin orientation and surface physical properties, like mean thermal inertia or mean size of dust grains, roughness fraction, albedo and so on via radiometric procedure. As an application example, we apply this model to the main-belt object (24) Themis, the largest object of the Themis family, which is believed to be the source region of many main-belt comets. We find multi-epoch (2010, 2014-2018) observations of Themis by WISE/NEOWISE, yielding 18 thermal lightcurves. By fitting these data with RSTPM, best-fit spin orientation of Themis is derived to be ($\lambda=137^\circ$, $\beta=59^\circ$) in ecliptic coordinates, the mean radius of dust grains on the surface is estimated to be $\tilde{b}=140^{+500}_{-114}(6\sim640)~\mu$m, indicating the surface thermal inertia to vary from $\sim3\rm~Jm^{-2}s^{-0.5}K^{-1}$ to $\sim60\rm~Jm^{-2}s^{-0.5}K^{-1}$ due to seasonal temperature variation. Further analysis found that thermal light curves of Themis show a weak rotation-phase dependent feature, indicative of heterogeneous thermal properties or imperfections of lightcurve inversion shape model.