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Ask Astro: How do stars make elements heavier than iron?

RELATED TOPICS: NEUTRON STARS | ELEMENTS
ASYSK1220_01
Two neutron stars merge in this illustration. As they combine, a fireball of the universe’s heaviest elements are thrown out into space. These elements become the basis of gas clouds that eventually form stars and planets.
NSF/LIGO/Sonoma State University/A. Simonnet
Q: Since the heaviest element produced by nuclear fusion is iron, how are elements like gold and uranium formed?
Brandon Chang 
Hong Kong 

A: The lightest elements in the universe — hydrogen, helium, and a little lithium — were born shortly after the Big Bang. The heavier elements, up to iron, were forged later, in the hearts of stars and in supernovae. However, looking at the periodic table, we see that that leaves two-thirds of the elements’ formation still unaccounted for.

So, how are they made?

Most of these “heavy elements” are created by atomic nuclei capturing neutrons. There are two forms of this neutron capture process: the rapid process (r-process) and the slow process (s-process). The s-process mostly produces lighter elements up to lead and bismuth on the periodic table, whereas the r-process typically produces elements as heavy as uranium. There is substantial overlap in the elements produced, but some elements are made purely by one process or the other; for example, gold, platinum, and uranium are only produced via the r-process.

By the early 1970s, scientists knew that the s-process happens in the envelopes of low-mass stars at the end of their lives. However, it is only recently that we could determine where the r-process takes place. Last year, we detected a freshly produced r-process element for the first time in the aftermath of two neutron stars merging. When neutron stars merge, they eject a few percent of their mass — about 10 million Earth masses — as neutron-rich matter. Within a fraction of a second, this ejected mass converts into a radioactive fireball of the heaviest elements through the r-process. These elements are scattered into interstellar space, seeding gas clouds and ultimately forming stars and planets with the elements in them.

The research in this area is ongoing — it seems likely, for example, that the r-process happens elsewhere in the universe as well, most likely in an unusual type of supernova. However, we believe that the bulk of the r-process elements were created by merging neutron stars. So, when you hold a piece of gold or platinum jewelry in your hands, you’re holding a fragment of what once was a neutron star.

Darach Watson 
Associate Professor, Niels Bohr Institute, University of Copenhagen, Denmark 
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