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abundance of the elements

chemistry
Also known as: elemental abundance

Quick Summary

The abundance of elements refers to the relative number of atoms of different elements in the universe. Hydrogen and helium are by far the most common elements, with all others being much less abundant. This pattern generally shows a decline in abundance with increasing atomic mass, though there are exceptions and peaks, notably around iron.123

The origin of these elements is primarily attributed to nuclear fusion reactions within stars. The process begins with the fusion of hydrogen into helium, which releases significant energy. In more massive stars, helium can fuse into heavier elements up to iron. Elements heavier than iron require an input of energy to be produced and are formed through processes like supernovae explosions.123

Observations of stars, gas clouds, Earth, and meteorites provide the data for understanding these cosmic abundances. The chemical composition of stars changes over time due to these nuclear reactions, and some transmuted matter is released into interstellar space, influencing the composition of newly forming stars.124

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