AGU Planet Earth Committee Report Part II Interior and Crust
نویسندگان
چکیده
T h e Ear th ' s man t l e , core , a n d crus t com prise 9 9 . 9 8 % of its mass . T h e man t l e , m a k i n g u p t he bulk of t he mass at 70% a n d com posed of h i g h e r densi ty rocks (rich in m a g n e sium silicates, p lus some i ron silicates), ex t ends an average of 1 5 2 9 0 0 km d e e p . T h e core is the cen te r of t he Ea r th , 2 9 0 0 6 3 7 0 km d e e p , c o m p o s e d mainly of mo l t en i ron . T h e crus t is t he o u t e r m o s t layer of t he solid Ea r th , c o m p o s e d of lower densi ty rocks (rich in silica a n d a l u m i n u m a n d calcium silicates) 6 4 0 km thick. T h e Ear th ' s ocean a n d a t m o s p h e r e out gassed f rom the in te r io r very long ago , a n d economic minera l depos i t s also f o r m e d far back in the past . T o d a y , however , i m p o r t a n t processes still s h a p e t he Ea r th , such as the con t inuous recycling of volat i les—water a n d ca rbon d i o x i d e — t h r o u g h the in ter ior , as well as the chemical a n d mechanica l b r e a k d o w n of rocky mater ia l essential to soil on t he land a n d to sed imen t s in the ocean . W i t h o u t these processes, the b io sphe re could no t exist. Most of this base of t he solid Ea r th , essential to life, has been fu rn i shed on t ime scales of mil lions of years, m u c h longer t h a n those of cir culat ion a n d renewal in the ocean , a t m o s p h e r e , and b iosphe re . But , by t he s ame to ken, those pa r t s of the e n v i r o n m e n t tha t d e p e n d on solid Ea r th processes , such as soil a n d p e t r o l e u m , canno t be r ep l en i shed in hu m a n t ime if exploi ted o r des t royed . A n d the solid Ea r th can also have drast ic impacts on h u m a n beings in a very shor t t ime, such as t h r o u g h e a r t h q u a k e s a n d volcanic e r u p t i o n s . U n d e r s t a n d i n g this complex system requ i r e s go ing very d e e p in to t he Ea r th a n d very far back in t ime.
منابع مشابه
Chapter 11
aving considered the Earth’s formation in the last chapter, let’s now use the tools of geochemistry we acquired in the first eight chapters to consider how the Earth works. The Earth, unlike many of its neighbors, has evolved over its long history and it remains geologically active. Four and a half billion years later, it is very different place than it was first formed. Certainly one of the ma...
متن کاملThe Mercurian magma ocean , first crust , and implications for planetary formation mechanisms by Stephanie
The size of the Mercurian core and the low ferrous iron bearing silicate content of its crust offer constraints on formation models for the planet. Here we consider a bulk composition that allows endogenous formation of the planet's large core, and by processing the mantle through a magma ocean, would produce a low-iron crust. More Earth-like bulk compositions require silicate removal, perhaps ...
متن کاملAb initio theory of phase transitions and thermoelasticity of minerals
Accurate quantum-mechanical simulations have significantly extended the current picture of the Earth and hold a great promise for the future of the Earth and planetary sciences. Studies of phase transitions, equations of state, elasticity and thermoelastic properties of the Earth-forming minerals are essential to geophysics. This chapter gives a basic background of the physics of the deep Earth...
متن کاملExploring the hidden interior of the Earth with directional neutrino measurements
Roughly 40% of the Earth's total heat flow is powered by radioactive decays in the crust and mantle. Geo-neutrinos produced by these decays provide important clues about the origin, formation and thermal evolution of our planet, as well as the composition of its interior. Previous measurements of geo-neutrinos have all relied on the detection of inverse beta decay reactions, which are insensiti...
متن کاملPristine Noachian crust and key geologic transitions in the lower walls of Valles Marineris: Insights into early igneous processes on Mars
Valles Marineris is a unique vertical section through the uppermost kilometers of the martian crust. Its location, east of the Tharsis bulge, and its water-related history, fuel a great diversity of rock types in this area (Carr, M.H., Head, J.W. [2010]. Earth Planet. Sci. Lett. 294, 185–203). HiRISE and CRISM data available over the walls of the canyon were analyzed to infer the importance of ...
متن کاملTheoretical Equations of State
Monogr. 13, edited by P. J. Hart, pp. 225-230, AGU, Washington, D.C., 1969. Talwani, M., and X. Le Pichon, Gravity field over the Atlantic Ocean, in The Earth's Crust and Upper Mantle, Geophys. Monogr. 13, edited by P. J. Hart, pp. 341-351, AGU, Washington, D.C., 1969. Tarr, A. C., New maps of polar seismicity, Bull. Seismol. Soc. Amer., 60, 1745-1747,1970. Toksoz, M. N., M. A. Chinnery, and D....
متن کامل