American Institute of Physics
SEARCH AIP
home contact us sitemap
Physics News Update
Number 845, November 2 , 2007 by Phil Schewe

Martian Dunes Take Their Time.

They need 1000 years to travel a few meters. This is the conclusion of a new study that tries to simulate the observed structures of dunes on the red planet and to determine whether present conditions could have been responsible. On Earth, a sand dune is shaped by wind and water. On Mars, there doesn't seem to be any surface water movement (at least not any that would shape dunes), and as for wind, there isn't much of that either.

With an atmosphere only 1/100 the density of Earth's the wind speed on Mars would have to be considerable to move sand around. Eric Parteli of the Universitaet Stuttgart in Germany and his colleague Hans Herrmann of the Universidade Federal do Ceara in Brazil calculate that on Mars (where the gravity is only 1/3 the Earth strength) a dune at a height of 1 meter would require a wind velocity of 35 m/s (roughly 75 mph) to be moved appreciably.

This speed occurs only a few times a decade, hence the glacial pace of dunes on Mars. Their most surprising finding, Parteli said, comes from their study of bimodal sand dunes, those that bear evidence of being shaped by winds from two perpendicular directions. They deduce a wind oscillation period on Mars of 50,000 years (the time it takes for winds to shift around by 90 degrees), roughly the same as the period for the precession of Mars's axis. (Physical Review E, October 2007; parteli@icp.uni-stuttgart.de)

Granular Liquids with Zero Surface Tension.

New experiments with spherical glass beads show that liquid behavior can arise simply from rapid collisions among a sufficiently dense stream of particles. The experiment was undertaken by Xiang Cheng, Heinrich Jaeger and Sidney Nagel and their colleagues at the University of Chicago, experts on discovering novel effects with granular materials (see http://www.aip.org/pnu/2005/split/725-3.html and http://www.aip.org/pnu/2005/split/759-2.html).

If one or two beads are dropped from above on a horizontal surface, they will bounce back in the direction from which they came. If, however, many beads are dropped all at once---constituting a dense granular stream hitting a target---then something else happens: the grains deflect out laterally in the form of a very thin, symmetrical sheet or cone as if they were a liquid.

Indeed, the experiments using granular matter quantitatively reproduce results obtained with streams of water. However, with beads, the “liquid” is one in the limit of vanishing surface tension. (To ensure there was no cohesiveness between the beads, which range in size between 50 microns and 2 millimeter, they were baked in a vacuum oven beforehand, evaporating any lurking moisture.) During the short interval the beads inside the stream collide with each other in front of the target, liquid-like conditions are established whose observable consequence are the thin sheets.

This novel, zero-surface-tension liquid state, the experimenters believe, might be of interest to physicists at the Relativistic Heavy Ion Collider (RHIC), where heavy nuclei colliding at high energies (see http://www.aip.org/pnu/2005/split/728-1.html) form a plasma of quarks and gluons that also resembles a liquid. Intriguingly, the collision pattern produced by the completely classical, macroscopic granular liquid can match that produced by the quark-gluon plasma. (Cheng et al., Physical Review Letters, 2 November 200,http://www.nscl.msu.edu/magnesium40)

Back to Physics News Update