New Research Shows How Stars Turn to Gold

    A study of the nearby dwarf galaxy Reticulum II hints at an exotic origin of the heaviest elements on Earth—through the merger of neutron stars. 

    Astrophysics has managed to paint a pretty accurate picture of how the elements were formed. Hydrogen and helium were created in those first staggering moments after the Big Bang; “metals” (all heavier elements) were later created through nuclear fusion in the central furnaces of super-massive stars.

    The problem is, once iron and nickel are formed, the fusion process requires more energy than it releases, which has predictable results—the star collapses. So how do heavier elements such as gold, lead, copper, and platinum form?

    The explanation is “neutron capture,” in which existing heavy elements accrete neutrons one at a time; subsequently, these neutrons beta decay into protons and voilà—you have a ready-made new element. Neutron capture may happen slowly, over long periods in stellar cores, or all at once, through a catastrophic neutron bombardment.

   Ultimately, astronomers are undecided about how such elements are formed—in supernova explosions, which are relatively common, or in something rare and exotic, such as the merger of neutron stars.

    Surprisingly, a new study of the dwarf galaxy Reticulum II hints that it is the latter.

The new research shows that of Reticulum II’s nine brightest stars, seven have a greater amount of heavy elements formed from rapid neutron capture than other dwarf galaxies; this fact, coupled with the excessive amounts of neutron capture-derived elements in the galaxy, seems to prove that a rarer mechanism than supernovae.

    Ancient stars in the Milky Way betray the same signatures of neutron capture, suggesting that an identical process obtains in larger galaxies as in the dwarfs—and that even Earth’s heavy elements were similarly formed. Which means the gold in that piece of jewelry you’re wearing may have been born inside colliding neutron stars.