Polyaromatic hydrocarbons (PAHs) are found throughout the universe. The ubiquity of
these organic molecules means that they are of considerable interest in the context of
cosmic dust, which typically travels at hypervelocities (>1 km s
–1
)
within our solar system. However, studying such fast-moving micrometer-sized particles
in laboratory-based experiments requires suitable synthetic mimics. Herein, we use
ball-milling to produce microparticles of anthracene, which is the simplest member of
the PAH family. Size control can be achieved by varying the milling time in the presence
of a suitable anionic commercial polymeric dispersant (Morwet D-425). These anthracene
microparticles are then coated with a thin overlayer of polypyrrole (PPy), which is an
air-stable organic conducting polymer. The uncoated and PPy-coated anthracene
microparticles are characterized in terms of their particle size, surface morphology,
and chemical structure using optical microscopy, scanning electron microscopy, laser
diffraction, aqueous electrophoresis, FT-IR spectroscopy, Raman microscopy, and X-ray
photoelectron spectroscopy (XPS). Moreover, such microparticles can be accelerated up to
hypervelocities using a light gas gun. Finally, studies of impact craters indicate
carbon debris, so they are expected to serve as the first synthetic mimic for PAH-based
cosmic dust.