HE 1219-0312

HE 1219-0312 is an extremely metal-poor star in the constellation Virgo, The star is located at around 41,400 light years away from earth.

It is thought to be a second generation, Population II or metal-poor star ([Fe/H] = -2.96), The star was found in the sample of extremely metal-poor halo stars from the Hamburg/ESO Survey by W. Hayek and collaborators. The group's research was published in the July 2, 2009 issue of The Astrophysical Journal.

If the age of the star HE 1219-0312 was confirmed at 17.6 billion years, that this star will be the oldest star in the universe.

Elemental abundance
The abundance of two strongly r-process enhanced in two metal-poor stars, BPS CS29491-0069 and HE 1219-0312 was detected by HERES project, which there was ([Fe/H] = -2.51, [r/Fe] = +1.1) and ([Fe/H] = -2.96, [r/Fe] = +1.5).

the analysis based on high-quality VLT/UVES spectra and MARCS model atmosphere was detected these eighteen heavy elements in the spectrum of HE 1219–0312 with an case of Th II 4019A line.

Radioactive dating for HE 1219–0312 with the observed thorium and rare-earth elements abundance pairs results in an average age of 9.5 billion years, when based on solar r-process residuals, that Age of the star HE 1219-0312 was 17.6 billion years, so, we puts the age of HE 1219-0312 into 13.6 billion years to avoid to exceed the universe's age.