Space Weathering on Near-Earth Objects investigated by neutral-particle detection
C. Plainaki, A. Milillo, S. Orsini, A. Mura, E. De Angelis, A. M. Di, Lellis, E. Dotto, S. Livi, V. Mangano, S. Massetti, M. E. Palumbo

TL;DR
This paper investigates space weathering effects on Near-Earth Objects by analyzing neutral particles, especially high-energy atoms, to understand surface erosion processes and proposes a new model and instrument for such measurements.
Contribution
It introduces the SPAWN model for space weathering on NEOs and proposes a specialized neutral-particle analyzer for detecting SHEA.
Findings
Identification of SHEA as key indicators of ion-sputtering.
Proposal of a new instrument for neutral particle detection.
Insights into surface loss and evolution of NEOs.
Abstract
The ion-sputtering (IS) process is active in many planetary environments in the Solar System where plasma precipitates directly on the surface (for instance, Mercury, Moon, Europa). In particular, solar-wind sputtering is one of the most important agents for the surface erosion of a Near-Earth Object (NEO), acting together with other surface release processes, such as Photon Stimulated Desorption (PSD), Thermal Desorption (TD) and Micrometeoroid Impact Vaporization (MIV). The energy distribution of the IS-released neutrals peaks at a few eVs and extends up to hundreds of eVs. Since all other release processes produce particles of lower energies, the presence of neutral atoms in the energy range above 10 eV and below a few keVs (Sputtered High-Energy Atoms - SHEA) identifies the IS process. SHEA easily escape from the NEO, due to NEO's extremely weak gravity. Detection and analysis of…
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Taxonomy
TopicsSpace exploration and regulation · Astro and Planetary Science · Planetary Science and Exploration
