The oldest stars in the Galaxy almost certainly belong to globular
clusters. It is suspected that all globular clusters are about the
same age - around 10 or 11 billion years. By contrast the Sun
formed relatively recently - about 5 billion years ago.
There are several reasons for believing that globular clusters are
very old. First, their more massive stars are all in advanced
states of evolution, or have long since ended their lives as
supernovae. Second, they are distributed throughout the
spherical halo of the Galaxy, which suggests they are remnants
of the era before the Galaxy collapsed to its present disc shape.
Third, globular cluster stars contain very low proportions of
chemical elements heavier than hydrogen or helium. This is
because there were hardly any atoms of heavier elements in
existence when these stars formed. The heavier elements have
been created inside stars then recycled back into interstellar
clouds to be incorporated in stars forming later, such as the Sun.
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