Dust and Gas of Dying Stars tagged posts

Astronomers at the University of Arizona have developed a theory to explain the presence of the largest molecules known to exist in interstellar gas.

The team simulated the environment of dying stars and observed the formation of buckyballs (carbon atoms linked to three other carbon atoms by covalent bonds) and carbon nanotubes (rolled up sheets of single-layer carbon atoms). The findings indicate that buckyballs and carbon nanotubes can form when silicon carbide dust—known to be proximate to dying stars—releases carbon in reaction to intense heat, shockwaves and high energy particles.

“We know from infrared observations that buckyballs populate the interstellar medium,” said Jacob Bernal, who led the research...