Researchers at ETH Zurich, led by Professor Maria Schönbächler, have published a chemical analysis of material from asteroid Bennu in Science Advances that identifies a distinctive isotopic fingerprint in iron, titanium, and chromium. The analysis shows that Bennu, the asteroid Ryugu, and a rare group of primitive meteorites called CI meteorites share strikingly similar isotopic patterns, indicating they formed from the same reservoir of ancient cosmic dust.
Contrary to earlier theories that primitive asteroids like Bennu originated in the outer Solar System, the new findings propose that Bennu's parent material accumulated near the water-ice line, a boundary in the young Sun's disk where water vapor could freeze into ice. Dust from both inner and outer regions mixed at this boundary, with water ice helping particles stick together to form larger bodies. "Bennu is a hybrid: the material does not clearly match either the inner or the outer Solar System," Schönbächler said.
The study also suggests that Jupiter played a crucial role in this process. Forming within about one million years of the Sun's birth, the gas giant's rapid growth and immense gravity are thought to have acted as a barrier that prevented larger particles from crossing its orbital path while allowing fine dust to circulate freely and mix near the water-ice line. This mixing produced material that retains a chemical composition close to that of the Sun.
Bennu's water-bearing minerals and organic compounds make it valuable for understanding how Earth obtained the ingredients necessary for life. "Bennu may offer our best glimpse of the original mix of chemical elements from which the terrestrial planets were ultimately built," Schönbächler said.
NASA's OSIRIS-REx mission delivered approximately 120 grams of asteroid material to Earth on September 23, 2023, when a capsule landed in the Utah desert. The ETH Zurich laboratory received half a gram for analysis.
