Название | Geochemistry |
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Автор произведения | William M. White |
Жанр | Физика |
Серия | |
Издательство | Физика |
Год выпуска | 0 |
isbn | 9781119438113 |
10 Chapter 10Figure 10.1 The Hertzsprung–Russell diagram of the relationship between lumi...Figure 10.2 Solar system abundance of the elements relative to silicon as a ...Figure 10.3 Compositional evolution during cosmological nucleosynthesis. 7Be...Figure 10.4 Evolutionary path of the core of star of 25 solar masses (after ...Figure 10.5 Schematic diagram of stellar structure at the onset of the super...Figure 10.6 Rings of glowing gas surrounding the site of the supernova explo...Figure 10.7 Diagram of the r-process path on a Z versus N diagram. The r-pro...Figure 10.8 Z versus N diagram showing production of isotopes by the r-, s- ...Figure 10.9 Comparison of relative abundances in cosmic rays and the solar s...Figure 10.10 View of part of the chart of the nuclides. Mass numbers of stab...Figure 10.11 Relative abundance of major types of meteorite falls. The small...Figure 10.12 NWA869, a brecciated L-4 ordinary chondrite. Both chondrules an...Figure 10.13 Ratio of reduced and oxidized iron to Si in chondrites. Carbona...Figure 10.14 Abundances of the elements in CI carbonaceous chondrites versus...Figure 10.15 Silicon- and CI-normalized abundances of key elements in the ma...Figure 10.16 Variation in Fe/Mn and Fe/Mg ratios in achondrites and lunar ba...Figure 10.17 Phase diagram for iron–nickel alloy. After Wasson (1974).Figure 10.18 Co–Au and Ga–Au plots illustrating the compositional distinctio...Figure 10.19 Summary of high-precision Pb ages of Allende CAIs, ordinary cho...Figure 10.20 Correlation of the 53 Cr/ 52 Cr ratio with 55 Mn/ 52 Cr ratio in incl...Figure 10.21 Comparison of Al-Mg isotope systematics for two different meteo...Figure 10.22 Time scale of events in the early solar system based on calibra...Figure 10.23 Cosmic ray exposure ages of ordinary chondrites and SNC achondr...Figure 10.24 Comparison of the laboratory-determined reflectance spectrum of...Figure 10.25 Photograph of the asteroid 4 Vesta taken by the NASA DAWN space...Figure 10.26 Ceres as photographed by NASA's DAWN spacecraft. Bright spots h...Figure 10.27 Neon isotopic compositions in a step-heating experiment on Orgu...Figure 10.28 The isotopic composition of Kr and Xe of the Xe-HL component in...Figure 10.29 Isotopic composition of C and N in SiC from Murchison (CM2) met...Figure 10.30 Variation of O isotope ratios in meteorites: CO, CK, etc., carb...Figure 10.31 Isotopic variations in meteorites. ε 50 Ti, ε54Cr and ε50Ca are t...Figure 10.32 Heavy element isotopic variations in meteorites. ε92Mo and ε100Figure 10.33 The Great Nebula in Orion, shown in a Hubble Space Telescope ph...Figure 10.34 Cartoon illustrating the X-wind model. As a result of interacti...Figure 10.35 Two Hubble Space Telescope views of the T-Tauri star DG Tau B. ...Figure 10.36 Condensation sequence of a gas with solar composition. Fast coo...Figure 10.37 Simplified mineralogical condensation sequence. After McSween (...Figure 10.38 Total alkalis and FeO/MgO ratios as a function of SiO2 in Marti...Figure 10.39 The processes involved in the formation of chondrites and their...Figure 10.40 The Grand Tack model. Jupiter, Saturn, Uranus and Neptune are r...Figure 10.41 Rare earth patterns of representative lunar rocks. Based on Tay...Figure 10.42 Highlights of lunar chronology.Figure 10.43 Difference between εW of Earth and Moon (Δ) versus the age of t...
11 Chapter 11Figure 11.1 The PREM model of seismic velocities and density variation throu...Figure 11.2 Ternary diagram illustrating ultramafic rock nomenclature based ...Figure 11.3 Modal mineralogy of peridotite xenoliths in the Deep Lithosphere...Figure 11.4 Upper mantle phase diagram.Figure 11.5 Mineral assemblages in the upper 1000 km of the mantle. After Ri...Figure 11.6 The structure of bridgmanite (MgSiO3). The structure consists of...Figure 11.7 Structure of the post-perovskite phase in the lowermost mantle. ...Figure 11.8 Cross-section of the Earth illustrating the two LLSVPs at the ba...Figure 11.9 Variation of Mg/Si as a function of Al/Si in terrestrial mantle ...Figure 11.10 Correlation of SiO2, Al2O3, and CaO with MgO in peridotites fro...Figure 11.11 Abundances of the elements in the bulk silicate Earth (Table 11...Figure 11.12 Dependence of experimentally determined liquid metal–liquid sil...Figure 11.13 Rare earth patterns of mid-ocean ridge basalts and oceanic isla...Figure 11.14 εNd versus 87Sr/87Sr in MORB and selected OIB from the PetDB an...Figure 11.15 εNd versus 206Pb/204Pb in mid-ocean ridge basalts (MORB) and se...Figure 11.16 Mass fraction of the depleted mantle (DMM) calculated from eqn....Figure 11.17 “Spider diagram” displaying concentrations of trace elements no...Figure 11.18 Cartoon illustrating the oceanic crustal recycling model of Hof...Figure 11.19 Mass independently fractionated sulfur isotopes diamonds from t...Figure 11.20 3He/4He vs. 87Sr/86Sr in MORB and OIB. High 3He/4He in many OIB...Figure 11.21 129Xe/130Xe vs. 136Xe/130Xe in MORB and oceanic island basalts....Figure 11.22 Correlation between tungsten isotopic anomalies (μ182W) ...Figure 11.23 Olivine Mg#s in peridotite xenoliths from the Kaapvaal and Slav...Figure 11.24 Probability functions for Re−Os model rhenium depletion ages me...Figure 11.25 REE patterns in garnets from a lherzolite xenolith (solid black...Figure