Where it all came together? (Image: Pete Turner/Getty)

Talk about making an impact. One of the meteorites that slammed into the planet early in its history could have kick-started life: the collision may have generated all four of the bases in RNA.

Life appeared on Earth around 4 billion years ago, about the same time that the planet was experiencing a beating from large meteorites – an event called the Late Heavy Bombardment. As far as Svatopluk Civiš at the Academy of Sciences of the Czech Republic in Prague and his colleagues are concerned, that’s no coincidence.

They simulated a meteorite impact on early Earth by firing a high-power laser at samples of formamide – a liquid that would have existed on our primordial planet. The sample temperatures soared to 4200 °C, generating X-rays and extreme ultraviolet radiation that reacted with the formamide to create chemical radicals. These radicals, in turn, reacted with hydrogen and the remaining formamide to generate 2,3-diaminomaleonitrile – DAMN for short – which is a chemical precursor to the nucleobases.


When Civiš and his colleagues examined the end products of their reaction, they found all four RNA bases: adenine, guanine, cytosine and uracil – three of which are also found in DNA.

The work “nicely correlates the Late Heavy Bombardment and the energy that it delivered to Earth with the formation of RNA and DNA nucleobases from formamide”, says Steven Benner at the Foundation For Applied Molecular Evolution in Gainesville, Florida.

What an impact

It was two Italian researchers – Raffaele Saladino at the University of Tuscia and Ernesto Di Mauro at the Sapienza University of Rome – who first suggested, in 2001, that formamide played an important role in the origin of life.

It forms when hydrogen cyanide, which was present in Earth’s early atmosphere, reacts with water. Although Saladino and Di Mauro have shown other ways that formamide can generate the four nucleobases, Di Mauro says “this is the first time that solid theoretical treatment and experimental data are presented together”.

He adds that even more biologically important molecules can be generated if these experiments consider the role that various minerals inside the meteorites might have played as catalysts – something his latest, still unpublished work has explored. “The obtained products are astonishingly rich and variegated,” Di Mauro says.

Saladino and Di Mauro suggested formamide would have concentrated in warm lagoons on our young planet – particularly because formamide has a higher boiling point than water, so would concentrate as water evaporated.

Donald Lowe, a geologist at Stanford University who studies the Late Heavy Bombardment, says such environments did exist on early Earth – despite the disruption caused by the impacts.

Living the dry life

“Although the impact frequency may have been 10s or 100s of times greater than it is today, your chance of experiencing a large impact at the height of the LHB would have been small,” says Lowe. “Lagoons or, in more general terms, shallow-water protected settings, are likely to have been well developed on the early Earth.”

The work still doesn’t quite answer the question of how the RNA bases came together with other complex molecules to form RNA, though. “This is what we are working on right now,” says Civiš. For instance, they hope to generate carbohydrates through similar laser experiments.

But if huge impact events were critical for the generation of life’s key molecules, water was apparently not.

Saladino and Di Mauro’s work on formamide suggested that the first, small RNA molecules were most likely to come together in a relatively water-free environment – like a formamide-rich lagoon.

Benner points out that some geologists think early Earth had too much water to allow these environments to exist, which last year led him to suggest that these formamide reactions may actually have occurred on the much drier early Mars, before life later rode through space on Martian meteorites to reach Earth.

The idea is compatible with Civiš and his colleagues’ work emphasising the role of impact events. “The current view is that all of the inner planets experienced the Late Heavy Bombardment,” says Benner.

Journal reference: PNAS, DOI: 10.1073/pnas.1412072111