The scale size of the lunar mini-magnetosphere formed by the interaction between the solar wind and a local crustal field is often comparable to the ion inertia length, suggesting that the Hall effect
The youngest lunar multi-ring basin, Orientale, provides the best preserved structure for determining the primary ejecta thickness and the local material thickness.The primary ejecta thickness was oft
ChangE-3, Chinas first Moon lander and rover mission, was launched at 17:30 on 1st December 2013 (UTC) and successfully landed on Moon surface at 13:11 on 14th December 2013 (UTC).
The Moon-based Extreme Ultraviolet Camera (EUVC) aboard Chinas Change-3 (CE-3) lunar lander has successfully imaged the entire plasmasphere for the first time by detecting the resonantly scattered sun
The late stage magma activities of lunar mainly happened at the west mare (Oceanus Procellarum and Mare Imbrium).Meanwhile the high-Fe-Ti mare basalts are the key to understand lunar evolution during
Based on the Martian magnetic field model established by magnetophdrodynamics simulation, we simulate the solar wind electron movement and determine the possible precipitation areas of the solar wind
Titanium abundance on lunar surface has great significance to study the formation and evolution history of the Moon.There are global TiO2 data derived from the remote sensing by orbital UV-VIS-IR spec
The Lunar Penetrating Radar (LPR) carried by ChangE-3 has imaged the shallow subsurface of the landing site at the northern Mare Imbrium.The antenna B of the Channel-2 onboard the LPR (LPR Channel-2B)
W UMa contact binaries contain two late-type main-sequence stars where both components are filling the critical Roche lobe and sharing a common convective envelope (CCE).