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The vortex, or spin center, in this work brings to mind satellite images of the whirling vortex in a major hurricane.  In “Cyclone” tiny bubbles suspended in a fluid are sucked in at the top, swirled down through the vortex, and released at the bottom.

Hurricane on Earth
Photo Credit: NASA

A Hurricane on Earth

In a hurricane, air flows toward the low pressure at the center and is deflected into a spin by Coriolis force.  Coriolis force describes the effect of the Earth’s rotation on the motion of moving objects.

This phenomenon can be seen on all the planets in our Solar System that possess atmospheres, because all of these planets spin.  Cyclones on Mars look much like their Earthly counterparts. 

Cyclone Near Mars' Polar Ice Cap, Photo Credit: NASA
Photo Credit: NASA

A Cyclone on the Planet Mars

In cyclones and hurricanes, airflow gains momentum as it approaches the center of the spin, exhibiting a central principle of astronomical motion called conservation of angular momentum.  Conservation of angular momentum (the natural law stating that the product of a spinning object’s speed and its distance from the center of its spin must stay constant unless acted upon by an outside force) is what accelerates the airflow in atmospheres, just as it causes spinning figure skaters to move faster as they bring their arms in.  In hurricanes, as in figure skating, if an object moves closer to its center of revolution, its speed must increase to keep the product of speed and distance from changing.

The movement exhibited in “Cyclone” is the same motion that led to the formation of the planets. The spinning primordial interstellar cloud that contained the material from which the Sun and its planets were formed was huge, and more spherical than the Solar System today.  As the material collapsed toward the center of its spin, that spin accelerated in order to keep its angular momentum constant.  Eventually the material’s spin grew to rates sufficient to place the material into more or less stable orbit around the sun forming at the center.  The various components of the spinning material drew ever closer together, eventually coalescing into planets.

This same process is observable today throughout the universe: in newly forming stars, in spinning disks of matter being drawn into stellar black holes, at the hearts of quasars (which possess galactic black holes), and even in the flattened spiral form of our own Milky Way and other spiral galaxies.