Origin of Water on Earth
How did Earth get its water?
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Here’s the part we think we understand well: Just shy of a trillionth of a trillionth of a second after the Big Bang, the energy that sparked the outward swelling of space transmuted into a hot, uniform bath of particles. During the next three minutes, these primordial constituents bumped and jostled, combined and recombined, yielding the first atomic nuclei. One of the great triumphs of modern cosmology is its mathematical description of these processes, which gives accurate predictions for the cosmic abundances of the simplest nuclei—a lot of hydrogen, less helium and trace amounts of lithium. Producing copious hydrogen is a propitious start en route to water. That’s where stars, already plentiful about a billion years after the Big Bang, enter the picture. Deep within their blisteringly hot interiors, stars are nuclear furnaces that fuse the Big Bang’s simple nuclei into more complex elements, including carbon, nitrogen and, yes, oxygen. Later in their lives, when stars go supernova, the explosions spew these elements into space. Oxygen and hydrogen commingle to make H2O.
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