Space-Based Thermal Infrared Studies of Asteroids

TL;DR

Space-based infrared surveys have greatly advanced our understanding of asteroid physical properties by providing high-resolution data, enabling the derivation of diameters, albedos, and thermal inertia for numerous minor planets.

Contribution

This paper reviews recent developments in space-based thermal infrared observations of asteroids, highlighting the improvements in detector technology and the resulting increase in observed asteroid data.

Findings

Significant increase in asteroid diameter and albedo data from space missions.

Enhanced spatial resolution improves physical property estimations.

Large datasets enable better understanding of asteroid populations.

Abstract

Large-area surveys operating at mid-infrared wavelengths have proven to be a valuable means of discovering and characterizing minor planets. Through the use of radiometric models, it is possible to derive physical properties such as diameters, albedos, and thermal inertia for large numbers of objects. Modern detector array technology has resulted in a significant improvement in spatial resolution and sensitivity compared with previous generations of space-based infrared telescopes, giving rise to a commensurate increase in the number of objects that have been observed at these wavelengths. Space-based infrared surveys of asteroids therefore offer an effective means of rapidly gathering information about small body populations' orbital and physical properties. The AKARI, WISE/NEOWISE, Spitzer, and Herschel missions have significantly increased the number of minor planets with well-determined diameters and albedos.