A Blow to the Building Blocks of Life ✎ express

Original: "High-Pressure Torsion-Induced Transformation of Adenosine Monophosphate: Insights into Prebiotic Chemistry of RNA by Astronomical Impacts"
arXiv:2601.21378 · 2026-01-29 · CC BY-NC-ND 4.0 · independent analysis · 1 min
Scientists squeezed an RNA precursor molecule under 6 GPa of pressure and found no polymerization.

Cometary ice slams into the young Earth. The pressure at the impact point is like stacking six aircraft carriers on your thumbnail. In the lab, such conditions are reproduced by squeezing a tiny sample between two rotating anvils.

This time, adenosine monophosphate — one of the letters of future RNA — was placed under the anvils. A little water was added to mimic a moist environment, and then it was squeezed. After releasing the pressure, the molecule was studied in five different ways: probed with X-rays, observed how it scatters light, and even weighed its fragments.

A pressure of 6 GPa is like the Eiffel Tower standing on a single coin.

They expected the molecules to link into long chains — like beads on a string. But no chains formed. Instead, adenosine monophosphate partially broke apart into pieces: adenine, sugar fragments, dehydrated and oxidized forms. So the impact didn't build; it rather broke things down.

However, the fragments are still organic. This means comets and asteroids could not only deliver ready-made substances but also reshape them into new combinations. The building blocks remain building blocks, even if the house didn't come together.

A pressure of 6 GPa is about 60,000 times atmospheric pressure — the same as created by a layer of rock 200 kilometers thick.

Scientists
Albert EinsteinHans BetheLise MeitnerMargaret BurbidgeFred HoyleRalph Alpher
Concepts
atp prebiotic chemistry origin of life first stars nucleosynthesis high pressure photosynthesis hydrogen cyanide first stars primordial nucleosynthesis abiogenesis atmospheric chemistry photochemistry amino acid Ammonia RNA hydrogen atmosphere atmosphere