HE 1523-0901

HE 1523-0901 is a star of magnitude 11 located in the Balance which was studied in 2007 by Anna Frebel and its team.

It is a star Géante red of class G (comparable) which presents a Métallicité = -1,95. On the other hand, elements created during the Process R (" R" for rapid, it is about a process of capture of Neutron S by dense Nucléon S radioactive carried at high temperature) are superabundant with a report/ratio = 1,8.

It is also one of the oldest stars of the Galaxy: 13,2 billion years. According to Anna Frebel it is a star of 2nd or 3rd generation.

External bonds

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