Chemical element - Cosmic Abundances, Elements, Periodic Table

chemical element

Table of Contents

Introduction
General observations
Historical development of the concept of element
The atomic nature of the elements
- The structure of atoms
- The existence of isotopes
Origin of the elements
- Cosmic abundances of the elements
  - Stars and gas clouds
  - Cosmic rays
  - Solar system
  - Summary of observations
- Processes producing heavier elements
  - Reaction stages reflecting increasing temperature
    - Hydrogen burning
    - Helium burning
    - Carbon and oxygen burning
    - Silicon burning
    - Reversible nuclear reaction equilibrium
  - Neutron capture
- Regions of element synthesis
  - Element production in the universe as a whole
  - Element production in stars
  - Element production in massive objects
- Radioactive chronologies
Geochemical distribution of the elements
- Terrestrial distribution
  - The Earth’s core
  - The Earth’s mantle
  - The Earth’s crust
    - Igneous rocks
      Major components
      Elements of minor and trace abundance
    - Sedimentary rocks
    - Metamorphic rocks
    - Ore deposits
    - Mineral fuels
    - Soils
  - The hydrosphere
    - Composition of seawater
    - Circulation of water through the hydrosphere
    - Geochemical balance of seawater over time
  - The atmosphere
    - Composition
    - Geochemical history
- The geochemical cycle
  - Early history of the Earth
  - Results of magmatism, sedimentation, and metamorphism

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The relative numbers of atoms of the various elements are usually described as the abundances of the elements. The chief sources of data from which information is gained about present-day abundances of the elements are observations of the chemical composition of stars and gas clouds in the Galaxy, which contains the solar system and part of which is visible to the naked eye as the Milky Way; of neighbouring galaxies; of the Earth, Moon, and meteorites; and of the cosmic rays. Atoms absorb and emit light, and the atoms of each element do so at specific and characteristic wavelengths. A ...(100 of 18829 words)

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