Astrophysicist Explores Our Turbulent Universe

space, astrophysics, nsf, national science foundation, sciencelives, sl, Blakesley Burkhart, astrophysics, magnetized fluid dynamics, turbulence in interstellar space, interstellar medium, universe dynamics, solar radiation, solar wind, disturbance from s
A simulation of a turbulent supersonic cloud. Structures seen in the cloud, such as wisps, filaments, and clumps, are very similar to structures seen in real interstellar clouds.
(Image credit: Blakesley Burkhart and Alex Lazarian, UW Madison Astronomy Department)

This ScienceLives article was provided to LiveScience in partnership with the National Science Foundation.

Blakesley Burkhart is a National Science Foundation Graduate Research Fellow in astronomy at the University of Wisconsin-Madison. She received her master's degree in astronomy and in physics from the University of Wisconsin-Madison in 2010 and her bachelor's in physics and mathematics from the University of Louisville, in Kentucky, in 2008.

University of Wisconsin Madison