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7 results for “Lunar basalt”
The Variability of Lunar Mare Basalt Properties from Surface Rock Abundance
<p>Derived data from Elder et al. (2022) The Variability of Lunar Mare Basalt Properties from Surface Rock Abundance, submitted.</p>
Unraveling silicate liquid immiscibility and apatite saturation in the mesostasis pocket of mare basalt: Evidences from Chang'E-5 lunar samples
<p><strong>Figure S1 </strong>Back scatter electron (BSE) images of Chang’E-5 breccia 136GP (top) and 143 GP (bottom)</p> <p><strong>Figure S2</strong> Chemical composition of silicate minerals in CE-5 136GP and 143 GP breccias and comparison with CE-5 mare basalts. A) Quadrilateral diagram of pyroxene in the Chang’E-5 mare basalt. B) Ternary diagram of feldspar from the Chang’E-5 mare basalts. C) Chemical compositions of olivine. The gray background areas represent the composition range of silicate minerals in Chang'e-5 basalts reported by previous studies (Che et al., 2021; He et al., 2022; Hu et al., 2021; Jiang et al., 2022; Tian et al., 2021).</p> <p><strong>Figure S3</strong> Element mapping of one representative mesostasis fragment in CE-5 136GP. a)-j) indicate the abundance maps of Si, Al, Mg, Na, K, Ca, Fe, Mn, Ti, and P within this lithic clast. All of them are in the same scale and the scale bar could be found in J. On each element map, the red or yellow color represents the relative elevated abundance of one specific element; the blue or black indicate its low abundance. k) is the BSE image of this clast and the yellow box outlines the mapping area.</p> <p><strong>Figure S4</strong> Predicted value of P<sub>2</sub>O<sub>5</sub> concentration (wt%) required for phosphate saturation in the Si-rich melts. The calculation is based on the equation built by Tollar et al. (2006). a) and b) represents the function of SiO<sub>2</sub> and CaO concentrations (wt%) respectively. The melt temperature is fixed at 1010 °C. The black circles indicate the data of Si-rich portion within the CE-5 mesostasis fragments investigated in the present study. These plots indicate that apatite crystallized in some of the Si-rich melts.</p> <p><strong>Table S1 Representative mineral EPMA analyses of major compositions (wt%) in the CE-5 mesostasis fragments.</strong></p> <p><strong>Table S2 Representative Raman spectra of minerals in the CE-5 mesostasis fragments.</strong></p>
Data sharing of: Sulfur inventory of the young lunar mantle constrained by experimental sulfide saturation of Chang'e-5 mare basalts and a new sulfur solubility model for silicate melts in equilibrium with sulfides of variable metal–sulfur ratio
<p>Data sharing of: Sulfur inventory of the young lunar mantle constrained by experimental sulfide saturation of Chang’e-5 mare basalts and a new sulfur solubility model for silicate melts in equilibrium with sulfides of variable metal–sulfur ratio</p>
Lunar dichotomy: Chang'e-6 2.83 Ga farside mare basalts reveal most depleted mantle to date
<p>The uploaded files contain the data and code used for plotting lunar crater chronology funtions. The Excel spreadsheet provides the N(1) values and sample ages for calibration points, along with the corresponding references.</p>
Repository: Lunar farside volcanism 2.8 billion years ago from Chang'e-6 basalts
<p>This repository contains all geochemical data (Supplementary Tables 1-5) generated in the paper "Lunar farside volcanism 2.8 billion years ago from Chang’e-6 basalts".</p> <p><strong>Supplementary Tables</strong></p> <p>Table 1. Pb-Pb isochron data for the Chang'e-6 basalts.</p> <p>Table 2. EMPA data of plagioclase and clinopyroxene in the 4.2 Ga high-Al basalt clast.</p> <p>Table 3. EPMA condition applied for mineral composition measurement.</p> <p>Table 4. Data of glass standard NIST610 of SIMS Pb isotope analyses.</p> <p>Table 5. Background measurements for electronic multiplier (EM) collectors.</p>
Repository: A dry lunar mantle reservoir for young mare basalts of Chang'E-5
<p>This repository contains all geochemical data (Extended Data Tables 1-5 and Supplementary Tables S1-S5) generated in the paper "A dry lunar mantle reservoir for young mare basalts of Chang'E-5".</p> <p><strong>Extended Data Tables:</strong></p> <p>Extended Data Table 1 | The Chang’E-5 basalt clasts</p> <p>Extended Data Table 2 | Water abundance and hydrogen isotopes of CE5 apatite</p> <p>Extended Data Table 3 | Water abundance and hydrogen isotopes of CE5 ilmenite-hosted melt inclusions</p> <p>Extended Data Table 4 | H/O ratios of CE5 clinopyroxene and reference San Carlos olivine measured by NanoSIMS 50L</p> <p>Extended Data Table 5 | Summary of the water abundances estimated for the lunar mantle source regions of basaltic products formed between ca. 4-2 Ga.</p> <p><strong>Supplementary Tables.</strong></p> <p>Table S1. Modal abundance of apatite in the CE5 basalt clasts.</p> <p>Table S2. EPMA analytical results of CE5 basalt clasts.</p> <p>Table S3. NanoSIMS analytical results of the standards and silicates of CE5 basalt clasts.</p> <p>Table S4. Water abundances and hydrogen isotope compositions of ilmenite-hosted melt inclusions with correction for spallation effects.</p> <p>Table S5. Summary of water abundances and hydrogen isotope compositions of apatite and melt inclusions from Apollo samples in the literature.</p>
Anatomy of a Mare Basalt-filled Lunar Silicic Construct: The Wolf Crater Complex on Mare Nubium and implications for early silicic magmatism on the Moon
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