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Most stars are made of hydrogen and helium, but when cooled they are revealed to contain small amounts of iron and silicate.
A nearby host star is observed to contain the same proportion of hydrogen and helium as that of the Sun.
Evidence emerges that the amount of iron in some rocky planets is considerably higher than the amount in their host star.
The method for determining the composition of rocky planets is discovered to be less effective when used to analyze other kinds of planets.