Research on Composition and Evolution of the Late Stage Mare Basalts in Oceanus Procellarum

来源 :第二届北京月球与深空探测国际论坛 | 被引量 : 0次 | 上传用户：zhhaibin

【摘要】

：

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

【作者】

：

Zhang Xunyu Ouyang Ziyuan Xu Aoao Tang Zesheng Chen Yuan Tang Xiao Wu Yunzhao

【机构】

：

Space Science Institute, Macau University of Science and Technology, Macau, China

【出处】

：

第二届北京月球与深空探测国际论坛

【发表日期】

：

2015年3期

【关键词】

：

Late Stage Mare Basalts M3 Band Center Composition Evolution

下载到本地 , 更方便阅读

下载此文赞助VIP

声明 : 本文档内容版权归属内容提供方 , 如果您对本文有版权争议 , 可与客服联系进行内容授权或下架

论文部分内容阅读

　　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 the last stage.Although there were a lot of researches in the past, considering the limit of data performance, some basic scientific questions about the mare basalts have not been solved.Previous researches usually extracted spectra from the large craters (diameter about 1000 m) to analyze spectra features.

其他文献

The Deep Lunar Interior with a Low-Viscosity Zone: Revised Constraints from Recent Geodetic Paramete

We revisit the constraints from our earlier investigation on the deep lunar interior with a possible low-viscosity layer by describing the Moons tidal response.

会议

In-situ Optical Measurements of Chang'E-3 Landing Site in Mare Imbrium: Mineral Abundances and

The visible and near-infrared (VIS-NIR) imaging spectrometer onboard the Yutu Rover of the ChangE 3 mission measured the in-situ lunar surface reflectance at a close distance (~1 meter) and collected

会议

in-situ lunar optical measurementsplanetary spectroscopyphase curvelunar mine

Thermal Behavior of Regolith at Cold Traps of Lunar South Pole:Revealed by CE-2 Microwave Brightness

The long-term stability of buried water ice at cold traps depends on subsurface temperature and regolith thermal properties.Based on microwave brightness data obtained by microwave radiometer onboard

会议

Thermal behaviorCold trapsWater iceLoss rate

LUT: A Lunar-based Ultraviolet Telescope on aboard CE-3

The Lunar-based Ultraviolet Telescope (LUT), on aboard CE-3, is designed to continuously monitoring variable stars for as long as dozens of days and performing low Galactic latitude sky surveys.

会议

ultravioletspace-based ultraviolet telescopelunar probe

An Unusual Geology of Chang'E-3 Landing Site

At 13∶11∶18 UTC on December 14 2013, the ChangE-3 (CE-3) spacecraft landed in the Eratosthenian basalts in northern Mare Imbrium.The landing site is near the eastern boundary of the Eratosthenian basa

会议

Chang-E-3MoonLate stage volcanism

Simulation of the image of the Earth's plasmasphere observed BY the EUV imager in CE-3 from THE

The ChangE-3 (CE-3) had been successful launched in Dec 2, 2013, where the EUV imager onboard CE-3 had provided abundant Earths plasmasphere EUV images for studying the physical characteristic of the

会议

Three-dimensional Hall MHD simulation of lunar mini-magnetosphere:general characteristics and compar

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

会议

Estimates of Primary Ejecta and Local Material for the Orientale Basin: Implications for the Formati

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

会议

The Orientale basinPrimary ejectaLocal materialEjecta depositsTransient crat

Major Elements Abundances in Chang'E-3 Landing Site from Active Particle-induced X-ray Spectrom

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).

会议

Chang'E-3Young mare basaltElements abundancesX-ray spectrometer

CE-3 EUVC Observations of the Plasmaspheric Evolutions during Substorms

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

会议

EUVCPlasmasphereEvolutionSubstorm

Research on Composition and Evolution of the Late Stage Mare Basalts in Oceanus Procellarum

与本文相关的学术论文