What Event Created the Atoms of Gold on Earth?

The gold atoms found in jewelry or technology are relics of a profound cosmic history. Gold, along with platinum and uranium, belongs to a class of elements that cannot be forged in the routine life cycle of a star. Gold’s presence on Earth is a direct signature of a rare and extraordinarily violent event that occurred billions of years ago. Understanding the origin of gold requires tracing the path of element creation, known as nucleosynthesis, from the universe’s earliest moments to the formation of our planet.

Stellar Nurseries: How Lighter Elements Are Forged

The universe began with elements established during Big Bang nucleosynthesis, which took place in the first few minutes after the universe cooled. The rapid expansion created a hot, dense environment where fundamental particles could combine. This initial cosmic event produced almost all the hydrogen and helium found today, along with trace amounts of lithium and beryllium. Everything heavier than these lightest elements required the birth and death of stars.

Stars function as natural nuclear fusion reactors, transforming lighter nuclei into heavier ones in a staged process. In a star like our Sun, hydrogen fuses into helium, releasing the energy that makes the star shine. As stars age and exhaust their hydrogen fuel, their cores contract and heat up, enabling the fusion of progressively heavier elements, such as carbon, oxygen, neon, and silicon. This stellar nucleosynthesis is responsible for creating all the elements on the periodic table up to iron.

Iron represents a stopping point for energy-releasing fusion. Fusing elements lighter than iron releases energy, which supports the star against gravity. However, iron’s nucleus possesses the highest binding energy per nucleon, meaning that fusing iron consumes energy rather than releasing it. This energy deficit causes the star’s core to collapse, setting the stage for more exotic element-creation processes. Even the slow neutron capture process (s-process), which occurs in low-to-intermediate-mass stars, cannot efficiently create gold. The s-process accounts for about half of the elements heavier than iron, but not the majority of Earth’s gold.

The Cosmic Foundry: Creating Elements Heavier Than Iron

To bypass the iron energy barrier and create elements as heavy as gold, a far more intense and explosive environment is required. These elements are created via the rapid neutron capture process, known as the r-process. This mechanism requires an extremely high density of free neutrons that bombard atomic nuclei much faster than the nuclei can undergo radioactive decay. The rapid succession of captures forces the nucleus to become highly neutron-rich, pushing it far from stability.

Once the neutron flux subsides, the newly formed, unstable nuclei undergo a series of beta decays, where a neutron converts into a proton. This process ultimately builds the nuclei of stable, heavy elements like gold, platinum, and uranium. For decades, scientists theorized about the exact cosmic event that could provide the necessary conditions for this rapid process. The environments must be neutron-rich, short-lived, and powerful.

The most compelling evidence now points to the merger of two super-dense stellar remnants—two neutron stars—an event known as a kilonova. When two of these ultra-dense objects spiral inward and violently collide, they eject a vast amount of neutron-rich debris. This ejected material is the perfect environment for the r-process to occur, creating gold and other heavy elements in a flash of cosmic alchemy.

The first direct observation of this process occurred in August 2017, when gravitational waves (GW170817) and a corresponding light signature (AT2017gfo) were detected from a binary neutron star merger. Analysis of the light from this kilonova confirmed the presence of freshly-synthesized heavy elements, including strontium, which validated the merger as a site for the r-process. Estimates suggest that a single kilonova event can generate an amount of gold equivalent to many times the mass of the Earth. While core-collapse supernovae may contribute a small fraction of r-process elements, binary neutron star mergers are now considered the primary source of gold and other heavy elements in the universe.

Delivery Mechanism: How Ancient Gold Atoms Reached Earth

Once forged in the kilonova, the newly created gold atoms were blasted into the interstellar medium. The debris mixed with the gas and dust clouds that permeate the galaxy. Over millions of years, these enriched clouds eventually condensed under gravity to form new star systems, including our Solar System approximately 4.6 billion years ago. The gold atoms were incorporated into the materials that accreted to form the planets.

As the early Earth formed, it was largely a molten sphere, and a process called planetary differentiation took place. Due to gold’s chemical nature as a highly siderophile, or “iron-loving,” element, the majority of the planet’s initial gold content bonded with iron. This heavy, metal-rich material sank deep into the core, stripping the mantle and crust of precious metals. If the planet’s formation had ended there, gold would be almost entirely inaccessible to us today.

The gold we find near the surface is accounted for by the “Late Veneer” hypothesis. This theory proposes that after Earth’s core had fully formed, a final, intense barrage of meteorites and planetesimals struck the planet. These late-arriving impactors, rich in heavy elements like gold, delivered a fresh layer of material to the planet’s surface. Because the core had already stabilized, this newly delivered material could no longer sink, leaving the highly siderophile elements scattered throughout the mantle and crust.