Earth is the only planet we know of with continents, the giant landmasses that provide homes to humankind and most of Earth’s biomass. We still don’t have firm answers to some basic questions about continents: how did they come to be, and why did they form where they did?
One theory is that they were formed by giant meteorites crashing into Earth’s crust long ago.
In new research published in Nature, we studied ancient minerals from Western Australia and found tantalizing clues suggesting the giant impact hypothesis might be right.
The continents form part of the lithosphere, the rigid rocky outer shell of Earth made up of ocean floors and the continents, of which the uppermost layer is the crust. The crust beneath the oceans is thin and made of dark, dense basaltic rock which contains only a little silica.
By contrast, the continental crust is thick and mostly consists of granite, a less dense, pale-coloured, silica-rich rock that makes the continents “Float.” Beneath the lithosphere sits a thick, slowly flowing mass of almost-molten rock, which sits near the top of the mantle, the layer of Earth between the crust and the core.
Impacts from giant meteorites-rocks from space tens or hundreds of kilometres across-are an extremely efficient way of doing exactly that. Giant impacts blast out huge volumes of material almost instantaneously. Rocks near the surface will melt for hundreds of kilometres or more around the impact site. Research shows these oceanic plateaus could have evolved to form the continents through a process known as crustal differentiation.
The thick oceanic plateau formed from the impact can get hot enough at its base that it also melts, producing the kind of granitic rock that forms buoyant continental crust. The thick crusts beneath Hawaii and Iceland formed not through giant impacts but “Mantle plumes,” streams of hot material rising up from the edge of Earth’s metallic core, a bit like in a lava lamp.
As this ascending plume reaches the lithosphere it triggers massive mantle melting to form an oceanic plateau.
So could plumes have created the continents? Based on the studies, and the balance of different oxygen isotopes in tiny grains of the mineral zircon, which is commonly found in tiny quantities in rocks from the continental crust, we don’t think so. We can also determine quite precisely when it was formed, based on the decay of the radioactive uranium it contains.
What’s more, we can find out about the environment in which zircon formed by measuring the relative proportion of isotopes of oxygen it contains.
Researchers looked at zircon grains from one of the oldest surviving pieces of continental crust in the world, the Pilbara Craton in Western Australia, which started forming more than three billion years ago. Many of the oldest grains of zircon contained more light oxygen isotopes, which indicate shallow melting, but younger grains contain a more mantle-like balance of isotopes, indicating much deeper melting.
This “Top-down” pattern of oxygen isotopes is what you might expect following a giant meteorite impact. Yes, there is! The zircons from the Pilbara Craton appear to have been formed in a handful of distinct periods, rather than continuously over time.
Spherule beds are deposits of droplets of material “Splashed out” by meteorite impacts. The fact the zircons have the same age suggests they may have been formed by the same events.
Further, the “Top-down” pattern of isotopes can be recognized in other areas of ancient continental crust, such as in Canada and Greenland. The next step of the research is to reanalyse these ancient rocks from elsewhere to confirm what we suspect-that the continents grew at the sites of giant meteorite impacts.