资源环境科技发展态势分析平台

The Mercury Laser Altimeter (MLA) measured surface reflectance, r(s), at 1064 nm. On Mercury, most water-ice deposits have anomalously low r(s) values indicative of an insulating layer beneath which ice is buried. Previous detections of surface water ice (without an insulating layer) were limited to seven possible craters. Here we map r(s) in three additional permanently shadowed craters that host radar-bright deposits. Each crater has a mean r(s) value >0.3, suggesting that water ice is exposed at the surface without an overlying insulating layer. We also identify small-scale cold traps (<5 km in diameter) where r(s)>0.3 and permanent shadows have biannual maximum surface temperatures <100 K. We suggest that a substantial amount of Mercury's water ice is not confined to large craters but exists within microcold traps, within rough patches and intercrater terrain.