Presolar SiC Grain

8 µmdiameter

Updated

8.00µm
Visual creditKathryn Hynes / CC BY 2.0Source: Wikimedia Commons

Details

A presolar silicon carbide grain is literal stardust that formed before the Sun existed. Some grains like this wandered through the Galaxy for millions of years, survived the Solar System’s birth, and ended up locked inside meteorites on Earth.

Presolar silicon carbide condensed around stars that lived before the Sun. Some of those grains survived interstellar travel, the formation of the Solar System, and later processing inside an asteroid before being recovered from a meteorite on Earth.

Researchers recognize this material by isotope ratios that differ sharply from the Solar System average. Different SiC populations preserve signatures associated with stellar environments such as asymptotic giant branch stars and supernovae, allowing individual microscopic grains to be tested as samples of stellar nucleosynthesis.

Key facts

Category
Cosmic dust
Object class
Presolar silicon carbide grain
Composition
Silicon carbide
Scale fact
8 µmdiameter
Estimated age
Older than the Solar System
Embed

Size neighbors

Objects near Presolar SiC Grain on the scale

On the logarithmic size axis, Presolar SiC Grain falls between Dust Aggregate and Micrometeorite. The band uses nearby Cosmic dust records.

Shared physical scale
6.12µm

Sources

References for Presolar SiC Grain

Measurements and descriptive context are compiled by the Scale of Space team from the references below. If you find an error, please let us know.

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