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Stabilized impact flux on the Moon at 2.8 Ga constrained by Chang’e-6 low-Ti basalts
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作者 Fanglu Luo Zhiyong Xiao +1 位作者 Yichen Wang Yi-Gang Xu 《The Innovation》 2025年第7期7-8,共2页
CURRENT KNOWLEDGE OF LUNAR IMPACT FLUX Impact craters are themost ubiquitous landforms on terrestrial planetary surfaces,recording crucial information about planetary evolution.Due to its minimal weathering rates,theM... CURRENT KNOWLEDGE OF LUNAR IMPACT FLUX Impact craters are themost ubiquitous landforms on terrestrial planetary surfaces,recording crucial information about planetary evolution.Due to its minimal weathering rates,theMoon preserves themost complete impact record,serving as the primary reference for reconstructing the impact history in the solar system.1 Impact craters formed by extralunar impactors(i.e.,primaries)since the emplacement of a geological unit constitute the production population,and their size-frequency distribution(SFD)can be mathematically described by the production function(PF).1 In combination with crater spatial densities,the radiometric ages of samples returned from the Moon provide a baseline to construct the lunar impact flux,which is termed the crater chronology function(CF). 展开更多
关键词 crater chronology function impact craters production function terrestrial planetary surfacesrecording extralunar impactors ieprimaries lunar impact flux reconstructing impact history
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