Cosmic Dust That Formed Our Planets Traced to Giant Stars

The chemical composition of the dust grains reveals important clues about the nuclear processes inside stars that led to their formation, the team says. Until now, however, tracing the origin of the grains to AGB stars had proven difficult.

While AGB stars are known to produce vast amounts of dust, the composition of grains recovered from meteorites did not seem to match those expected from these stars, researchers say.

The study solves this puzzle by identifying in the make-up of some meteoritic dust grains the effect of the nuclear reactions that occur in AGB stars.

A team of nuclear physicists found that fusion reactions between protons and a form of oxygen that is heavier than the type we breathe – called 17O – occur twice as often as was previously thought.

The effect of these nuclear reactions is clearly observed in some stardust grains found in meteorites, resolving the mystery of their origin, the team says.

The Laboratory for Underground Nuclear Astrophysics – or LUNA – is located more than 1km beneath the Earth’s surface. The facility is hosted by the Italian Institute for Nuclear Physics Gran Sasso Laboratory.

The study is published in the journal Nature Astronomy. The LUNA Collaboration involves around 40 scientists from 14 institutions in Italy, Germany, Hungary and the UK.

Professor Marialuisa Aliotta, of the University of Edinburgh’s School of Physics and Astronomy, who led LUNA’s UK team, said: “It is a great satisfaction to know that we have helped to solve a long-standing puzzle on the origin of these key stardust grains. Our study proves once again the importance of precise and accurate measurements of the nuclear reactions that take place inside stars.”

Dr Maria Lugaro, of Konkoly Observatory, Hungary, who led the study, said: “The long-standing question of the missing dust was making us very uncomfortable: it undermined what we know about the origin and evolution of dust in the Galaxy. It is a relief to have finally identified this dust thanks to the renewed LUNA investigation of a crucial nuclear reaction.”