Star in the constellation Aquarius
BPS CS22892-0052 (Sneden's Star ) is an oldpopulation II star located at a distance of 4.7kiloparsecs (15,000light-years ) in theMilky Way 'sgalactic halo . It belongs to a class of ultra-metal-poor stars (metallicity [Fe/H]=-3.1), specifically the very rare subclass ofneutron-capture (r-process ) enhanced stars. It was discovered byTim C. Beers and collaborators with the CurtisSchmidt telescope at theCerro Tololo Inter-American Observatory inChile . Extended high-resolutionspectroscopic observations since around 1995 (withChris Sneden from theUniversity of Texas at Austin as the leading observer) allowed observers to determine the abundances of 53chemical elements in this star, as of December 2005 only second in number to the Sun.
Frombarium (Z=56) on, all elements show the pattern of the r-process contribution to theabundances of the elements in the Solar System . Comparing the observed abundances for astable element such aseuropium (Z=63) and the radioactive elementthorium (Z=90) to calculated abundances of an r-process in a type IIsupernova explosion (as from the universities atMainz andBasel groups ofKarl-Ludwig Kratz andFriedrich-Karl Thielemann ) have allowed observers to determine the age of this star to be about 14 billion years. Similar ages have been derived for other ultra-metal-poor stars (CS31082-001 ,BD+17°3248 andHE 1523-0901 ) from thorium-to-uranium ratios.[citation needed ]
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