  Jupiter's fast rotation - one rotation over 10 hours - creates strong jet
streams, smearing its clouds into linear bands of dark and light zonal belts
that circle the planet on lines of almost constant latitude. Such a high degree
of axisymmetry is absent in our own atmosphere. Moreover, Jupiter has the
largest and longest-living known atmospheric vortex, the Great Red Spot (GRS).
Such vortices abound in nature, but GRS's size, long-term persistence, and
temporal longitudinal oscillations make it unique. Here, we uncover, for the
first time, unsteady material structures that form the cores of zonal jets and
the boundary of the GRS in Jupiter's atmosphere. We perform our analysis on a
velocity field extracted from a video footage acquired by the NASA Cassini
spacecraft.
