Water is essential for life on Earth and is one of our most precious natural resources. But considering how our planet formed, it is quite surprising how much water we still have. The Earth aggregated from a cloud of gas and dust – a protoplanetary disk – and was incandescently hot for the first few million years. Its surface was kept molten by impacts from comets and asteroids. Earth’s interior was also (and still is) kept liquid by a combination of gravitational heating and the decay of radioactive isotopes.
That means that if there were any initial water (and organic compounds) on the Earth, it should have boiled off quickly. So how come there’s plenty of water on our planet today – where did it actually come from? A surprising new study, published in Science Advances, suggests that a type of asteroid we didn’t think contained very much water could be responsible – simultaneously demonstrating that the solar system is probably a lot wetter than had previously been thought.
Scientists have long debated exactly where the Earth’s water comes from. One theory suggests that it might have been captured from the asteroids and comets that collided with it. Another argues that water was always present in the rocks of the Earth’s mantle and was gradually released to the surface through volcanoes.
Thanks to the Japanese Hayabusa mission we now have fresh evidence. The spacecraft brought back a precious cargo of grains retrieved from the surface of asteroid 25143 Itokawa in 2010. The researchers behind the new study were able to analyse the water content of two grains. They used a sophisticated piece of kit called an ion microprobe, which bombards a sample with a beam of ions (charged atoms) in order to probe the composition of its surface.
The experiment was not easy – the grains are tiny, less than 40 microns (one millionth of a metre) across, and each grain was made up of several different minerals. The ion microprobe had to be focused on one specific mineral within each grain so that the authors could gather the required data. The species of mineral that they analysed was an iron and magnesium-bearing silicate known as a pyroxene, which is almost entirely free of calcium.
This type of substance is not usually associated with water – indeed, it is regarded as a Nominally Anhydrous Mineral (NAM). The lattice of a pyroxene crystal does not contain vacant sites for water molecules in the same way that, for example, a clay mineral does – so its structure is not necessarily conducive to taking up water. However, the sensitivity of the technique that the authors used was such that they could detect and measure tiny quantities of water.
The results were surprising: the grains contained up to 1,000 parts per million of water. Knowing the composition of Itokawa, the researchers could then estimate the water content of the entire asteroid, which translated to between 160 and 510 parts per million of water. This is more than had been anticipated – remote measurements of two similar bodies (also S-type asteroids) found that one contained 30 and the other 300 parts per million water.