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The six most common elements in our galaxy are as follows:

  1. Hydrogen: 74%
  2. Helium: 24%
  3. Oxygen: 1.04%
  4. Carbon: 0.42%
  5. Neon: 0.13%
  6. Iron: 0.11%

These values, obtained by spectroscopy, will give accurate estimates for local regions of the universe.

The abundance of elements in more distant galaxies will have lower percentages of heavy elements (ie heavier than Helium) as they have had a shorter period of time to accumulate heavy elements from stellar nucleosynthesis.

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