Geochemistry Flashcards
The study of the nature and distribution of chemical elements in rock and minerals
Geochemistry
The application of basic chemistry to earth sciences
Geochemistry
It is used for dating rocks by using the radioactivity of elements
Geochronology or Isotope Geochemistry
Geochemistry was first coined by
Christian Friedrich Schonbein
Chemistry professor from University of Basel in Switzerland, in 1838
Christian Friedrich Schonbein
The first geochemist in the modern sense of the world of USGS in 1908
Frank W. Clarke
Book written by Frank Clarke
The Data of Geochemistry
He correlated the mineral formation and structure to its chemical composition
Victor M. Goldschmidt
Victor M. Goldschmidt studied at
University of Gottingen in Germany
He stated the rational explanation of isomorphous substitution in crystals based on the capability of the radii and charges of the ions
Victor M. Goldschmidt
Father of modern chemistry and crystal chemistry
Victor M. Goldschmidt
He proposed the classification of minerals according to preferred hosts
Victor M. Goldschmidt
it is a rock loving mineral
Lithophile
It is an iron loving mineral
Siderophile
It is an ore loving mineral
Chalcophile
It is a gas loving mineral
Atmophile
Goals of Geochemistry
- To know the distribution of the chemical element in the Earth and in the solar system
2 . To discover the causes for the observed chemical composition of terrestrial and extraterrestrial materials - To study the chemical reactions on the surface of the earth, in its interior and in the solar system around us
- To assemble this information into geochemical cycles and to learn how this cycle operated in the geologic past and how they maybe altered in the future
A model of the evolution of the universe that postulates its origin from a hot, dense mass that expanded rapidly and cooled
Big Bang Theory
In the Big Bang Theory the fundamental composition that eventually combined or nucleated to become organized into the nuclei of H and He
Quark Soup
Clues of “expanding Universe”
- The “red shift” of spectral light emitted by distant galaxies - the use of “doppler Effect” calculations
2.The “cosmic Microwave Radiation” which is the energy of radiation produced at a specific wavelength when the universe was at temperatures greater than about 3000oK
Hierarchy of Heavenly Bodies
> Cluster of Galaxies
Galaxies
Stars, Pulsars, and Black Holes
Planets
Satellites
Comets
Asteroids
Meteoroids
Dust Particles
Molecules
Atoms of H and He
basin unit in the hierarchy
Star
Produced by contraction of interstellar gases resulting in increase in temperature
Main Sequence Stars
Energy production by H fusion becomes possible and thus produces star
Main Sequence Stars
High Luminosity and High temperature stars
Blue Giants
Stars less massive than the sun
Red Dwarfs
Bigger than the sun and is formed by depletion of H in the core during the main phase; the energy production shifted from the core to the outer shell
Red Giants
How Red Giants are formed?
formed by depletion of H in the core during the main phase; the energy production shifted from the core to the outer shell
End stage of stellar evolution
Pulsars (neutron stars), White Dwarf and Black Holes
Contraction leads to the increase in core temperature and eventually explodes to form the supernova
Pulsars (neutron stars), White Dwarf and Black Holes
The star cycle begins again
Pulsars (neutron stars), White Dwarf and Black Holes
The theory that explains the complexation of material from the simple structure of H and deuterium (isotope of H)
Nucleosynthesis
First 4 statement in Nucleosynthesis
- H and He are the most abundant isotopes in the universe
- The abundances of the first 50 elements decreases exponentially
- The abundances of the elements having atomic numbers greater than 50 are very low and do not vary appreciably with increasing atomic number
- Elements with even atomic numbers are more abundant than immediate neighbors with odd atomic numbers
Last 4 statements in Nucleosynthesis
- The abundances of Li, Be, and B are anomalously low compared to other elements of low atomic number
- The abundance of Fe is notably higher than those of other elements with similar atomic numbers
- Tc and Pm do not occur in the solar system because all of their isotopes are unstable and decay rapidly
- The elements having atomic number greater than 83 (Bi) have no stable isotopes, but occur naturally at very low abundances because they are daughters of long - lived radioactive isotopes of U and Th
Diffuse mass of interstellar gas and dust
Solar Nebula
Condensates accreted to form larger bodies as a result of selective adhesion caused by electrostatic and magnetic forces
Planetisimals
High density, small planets
Terrestrial planets
Low Density, Large planets
Jovian Planets
Volatile rich planetisimals composed of water, ammonia, methane and other volatiles
Cometisimals
Diagram that shows the luminosity and temperature of the star
Hertzsprung-Russell Diagram
Chuck of rock from space that land on Earth
Meteorites
Kind of Meteorites
> Iron
Stones
Stony-irons
Predominantly Ni-Fe alloys Minor amounts of other minerals such as Troilite (FeS)
Iron Meterorites
Iron meteorites are classified according to ________________
% of Ni
Hexahedrite, Octahedrite and Ataxite are examples of what meteorite
Iron Meteorites
Chiefly Silicates, mostly ferromagnesian Up to 1/4 metallic
Stony Meteorites
Types of stone meteorites
- Chondrites
- Achondrites
Meteorites that contain chondrules
Chondrites
Meteorite composed chiefly of silicates such as olivine pyroxene, and plagioclase or glass important type
Carbonaceous Chondrite
High content of volatiles, including water and non biogenic carbon (will later show how determined to be non-biogenic)
Chondrites
Meteorite that have some composition as Sun’s atmosphere
Chondrites
Meteorite that has no chondrules
Achondrites
Meteorite that has the same composition as terrestrial mafic and ultramafic rocks
Achondrites
Most __________ are breccias
Achondrites
Equal amounts of silicates and Ni-Fe alloys
Stony-iron meteorites
Many are crystallized silicates which have been brecciated, then invaded by metallic and sulfide melts
Stony-iron meteorites
Stony- iron meteorites classified according to kind of silicates: Olivine
Pallasite
Stony- iron meteorites classified according to kind of silicates: Plagioclase, Pyroxene
Mesosiderite
Components of an atom
- A nucleus at the center, containing nearly all of the mass of their atom but accounting for only ten- thousandth of its diameter
- A family of electrons gathered around the nucleus, forming three dimensional clouds that makes up the volume of an atom
Protons are ___________X more massive than electron
1825X
Denotes any of the more than 1300 different atomic forms characterized by a distinct combination of protons and neutrons
Nuclide