Amazing stuff! The charm of stardust! Or when stardust catches the eyes of scientists! 😊
"... Roughly 4.6 billion years ago, part of a giant molecular cloud collapsed, with most mass collecting to form what would one day become our Sun. The leftover matter flattened into a rotating protoplanetary disc, which ultimately gave rise to planets, moons, and other objects that make up the Solar System. As the disc cooled, some of its matter condensed to form tiny mineral structures known as calcium-aluminum-rich inclusions (CAIs). These materials, which are preserved inside meteorites, represent some of the Solar System’s oldest known rocks.
Scientists recently found that some of these CAIs contain large amounts of strontium-84, a relatively rare isotope found in certain kinds of stardust that existed before the Sun formed. The discovery came as a surprise, since it was previously assumed that the region where CAIs formed was hot enough to completely vaporize this dust. The team posits that grains of ancient stardust instead acted as nucleation seeds, drawing the Solar System’s earliest solids to condense around them—just as a particle of dust might accumulate water droplets that freeze to form a snowflake."
From the abstract:
"Recent reports of extreme strontium-84 excesses in primitive Solar System condensates, known as fine-grained calcium-aluminum–rich inclusions (fg-CAIs), suggest that presolar stardust may be preserved in refractory meteoritic components.
This is at odds with preconceptions that presolar grains were completely vaporized in the CAI-forming region.
Here, we reappraise the role of presolar materials in early condensation and overall disk heterogeneity by isolating strontium from primary fg-CAI phases.
We demonstrate that extreme strontium-84 anomalies are likely hosted in a subpopulation of CAI oxides. The anomalies of primitive noncarrier phases are shown to be attenuated but correlated with the abundance of presolar precursors, which suggests that carriers exert leverage on ensuing condensate compositions. We propose that this relationship between isotope anomalies in refractory CAI components stems from stardust acting as nucleation seeds for the earliest solids formed in the Solar System."


