PPT-Mineral reservoirs and behaviors of hydrogen in Earth’s lower mantle

Tsingtao quarantine lodging 2020 EGU May 4 th 2020 Speaker Qingyang Hu 北京高压科学研究中心 HPSTAR Center for High Pressure Science and Technology Advanced Research. Richard Carlson. CIDER, July 2012. Molecular Cloud, M16. NASA/ESA. Protoplanetary Disk,. Hubble Telescope. When did planetary chemical differentiation begin?. Before there were planets!. Not Everything was Volatilized!. Things to Know. What do the layers of the Earth look like?. Check the following terms and definitions to see if they are in your journal.. Layers of the Earth. Inner core. – the solid inner core of the Earth. Pressure makes the iron found there a solid mass. . or . What we . (think we) know . about the . composition and evolution . of the Earth and how we know it.. William M. White. Cornell University. Outline. Meteorites, Chondrites and Chondritic . Abundances. Oceanic Intraplate Volcanism. GLY 4310 - Spring, 2016. 2. Hot Spots, Trails, and . Aseismic Ridges. Figure 14.1. . Map of relatively well-established hotspots and selected hotspot trails (island chains or aseismic ridges). Hotspots and trails from Crough (1983) with selected more recent hotspots from Anderson and Schramm (2005). Also shown are the geoid anomaly contours of Crough and Jurdy (1980, in meters). Note the preponderance of hotspots in the two major geoid highs (superswells).. An Introduction to Ch 11&12. Regions of the Earth. The Earth is made up predominantly of two major regions:. A predominantly molten, central core. A mostly solid outer mantle and crust. Hydrosphere and Crust . -I started CIDER as student participant in 2006, when my thesis advisor (Hart) encouraged me to participate. CIDER was the most powerful experience of my graduate education. . -Several publications emerged from interactions that I had at the CIDER workshop. One example: Raj and I were both students when we met at CIDER in 2006, and we have written 3 papers together.. Layers of the Earth. 1. 2. / . 24. 3. / . 24. Plate Tectonics. Earth’s lithosphere is broken up into plates. Hot, weak asthenosphere allows for plates to move. Plates are in motion and continually changing in shape and size. Inner planets are small and dense . Outer planets are large and have low density . Satellites of the outer planets are made mostly of ices . Cratered surfaces are everywhere in the Solar System . Saturn has such a low density that it can't be solid anywhere . Objectives. Describe the layers found within the earth.. Discuss the forces that change the earth’s surface.. Earth’s Layers. Inside our Earth. 3 layers: Crust, Mantle, and Core.. Core can be split up . https://. www.youtube.com/watch?v=rQx2wLyagk4. . Essential Question:. How are layers of the Earth different from one another?. Standard:. S6E5a. Compare and contrast the Earth’s crust, mantle, and core including temperature, density, and composition.. https://. www.youtube.com/watch?v=rQx2wLyagk4. . Essential Question:. How are layers of the Earth different from one another?. Standard:. S6E5a. Compare and contrast the Earth’s crust, mantle, and core including temperature, density, and composition.. What is Geology. Geo. - Earth. Ology. is the study of. This activity will help us study the earth by learning what it is made of and how it can be changed. 4 layers of the Earth. Crust. Mantle. Inner core. Richard Carlson. CIDER, July 2012. Molecular Cloud, M16. NASA/ESA. Protoplanetary Disk,. Hubble Telescope. When did planetary chemical differentiation begin?. Before there were planets!. Not Everything was Volatilized!. p. otential hotspot. p. otential hotspot. Based on illustration by . Lidunka. . Vočadlo. , University College London. We propose this scenario: . Layered Mantle Convection. Location of the boundary can be adjusted to suit different needs..