In a certain type of supernova, the detonation starts with a flame ball buried deep inside a white dwarf. The flame ball is much lighter than its surroundings, so it rises rapidly making a plume topped with an accelerating smoke ring.

"We created a smaller version of this process by triggering a special chemical reaction in a closed container that generates similar plumes and vortex rings," says Stephen Morris, a University of Toronto physics professor.

Autocatalytic chemical reactions release heat and change the composition of a solution, which can create buoyancy forces that can stir the liquid, leading to more reaction and a runaway explosive process. "A supernova is a dramatic example of this kind of self-sustaining explosion in which gravity and buoyancy forces are important effects. We wanted to see what the liquid motion would look like in such a self-stirred chemical reaction," says Michael Rogers, who led the experiment as part of his PhD research, under the supervision of Morris.

"It is extremely difficult to observe the inside of a real exploding star light years away so this experiment is an important window into the complex fluid motions that accompany such an event," Morris explains. "The study of such explosions in stars is crucial to understanding the size and evolution of the universe."

The research will appear in Physics Review E in the next few weeks. In addition to Morris and Rogers, the research team included Abdelfattah Zebib from Rutgers. The work was funded by the Natural Sciences and Engineering Research Council of Canada.

Note: If no author is given, the source is cited instead.

• Astrophysics
• Stars
• Astronomy

• Inorganic Chemistry
• Chemistry
• Physics

• Blue supergiant star
• List of phases of matter
• Supergiant
• Stellar evolution
• Red supergiant star
• Autocatalysis