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.
Elemental abundance The elemental abundances of two strongly r-process enhanced metal-poor stars, BPS CS29491−0069 and HE 1219−0312, were measured by the HERES project, resulting in a value of [Fe/H] = –2.96 and [r/Fe] = +1.5 for HE 1219−0312. 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 a 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 age of 9.5 ± 6.0 billion years. When based on solar r-process residuals, an age of 17.6 ± 6.8 billion years is obtained. This roughly matches the typical age range for previously discovered metal-poor halo stars of 11–12 billion years.
See also HD 140283 HE 0107−5240 HE 1523−0901
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