Did space deliver the essential building blocks for life on Earth?

Ingredients for Life: On Earth and in Space (Suomalainen) · 31:23 · Video: European Space Agency, ESA · Watch at the source

In short: To survive in space, humans must recreate Earth's vital environmental support systems. But where did our own ingredients come from? New research suggests the materials necessary for life may have been delivered to our primordial planet by meteorites from the early solar system.

The origins of Earth's 'volatiles'—elements or compounds that change into vapor at low temperatures—are central to understanding how life began. Recent studies suggest these materials, which include six common chemicals vital for living things, were delivered by meteorites from planetesimals. These small, rocky bodies formed approximately 4.6 billion years ago from dust and gas orbiting the infant sun. These meteorites were likely the broken remnants of early, unmelted asteroids. This process helped distribute the necessary chemical elements across the developing solar system.

By tracking the chemical element zinc, researchers from the University of Cambridge and Imperial College London discovered that Earth's volatiles arrived from two distinct regions. About half originated from the inner solar system, near Earth and other rocky worlds close to the sun. The other half appears to have come from beyond Jupiter, the fifth planet. This distribution is measurable because planetesimals were not uniform in composition. They were exposed to intense radiation from the young sun during their formation.

Identifying these ingredients is crucial for the search for extraterrestrial life. Scientists look for a specific set of circumstances: water, an energy source, and a suitable temperature. While water acts as a vital solvent for chemical reactions, carbon serves as a fundamental building block, capable of forming complex 3D structures like rings and branching trees. As we engineer life-support systems for the International Space Station, understanding these terrestrial requirements helps us hunt for life on distant worlds, such as Jupiter's icy moon Europa or Earth-like exoplanets like Kepler 186-f. Beyond liquid water and energy, scientists must also ensure that lethal radiation is not present. Additionally, the presence of carbon is vital, as it forms organic compounds like proteins and fats.

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