http://www.news.cornell.edu/releases/Dec03/Mars.wheels.bpf.html

Spinning spokes: Cornell scientists develop method for using rover 
wheels to study Martian soil by digging holes

FOR RELEASE: Dec. 19, 2003

Contact:  Blaine P. Friedlander Jr.
Office:  607-255-3290
E-mail:  [EMAIL PROTECTED]


PASADENA, Calif. -- After the twin Mars Exploration Rovers bounce 
onto the red planet and begin touring the Martian terrain in January, 
onboard spectrometers and cameras will gather data and images --- and 
the rovers' wheels will dig holes.

Working together, a Cornell University planetary geologist and a 
civil engineer have found a way to use the wheels to study the 
Martian soil by digging the dirt with a spinning wheel. "It's nice to 
roll over geology, but every once in a while you have to pull out a 
shovel, dig a hole and find out what is really underneath your feet," 
says Robert Sullivan, senior research associate in space sciences and 
a planetary geology member of the Mars mission's science team. He 
devised the plan with Harry Stewart, Cornell associate professor of 
civil engineering, and engineers at the Jet Propulsion Laboratory 
(JPL) in Pasadena.

The researchers perfected a digging method to lock all but one of a 
rover's wheels on the Martian surface. The remaining wheel will spin, 
digging the surface soil down about 5 inches, creating a 
crater-shaped hole that will enable the remote study of the soil's 
stratigraphy and an analysis of whether water once existed. For 
controllers at JPL, the process will involve complicated maneuvers -- 
a "rover ballet," according to Sullivan -- before and after each hole 
is dug to coordinate and optimize science investigations of each hole 
and its tailings pile.

JPL, a division of the California Institute of Technology, manages 
the Mars Exploration Rover project for NASA's Office of Space 
Science, Washington, D.C. Cornell, in Ithaca, N.Y., is managing the 
science suite of instruments carried by the two rovers.

Each rover has a set of six wheels carved from aluminum blocks, and 
inside each wheel hub is a motor. To spin a wheel independently, JPL 
operators will simply switch off the other five wheel motors. 
Sullivan, Stewart and Cornell undergraduates Lindsey Brock and Craig 
Weinstein used Cornell's Takeo Mogami Geotechnical Laboratory to 
examine various soil strengths and characteristics. They also used 
Cornell's George Winter Civil Infrastructure Laboratory to test the 
interaction of a rover wheel with the soil. Each rover wheel has 
spokes arranged in a spiral pattern, with strong foam rubber between 
the spokes; these features will help the rover wheels function as 
shock absorbers while rolling over rough terrain on Mars.

In November, Sullivan used JPL's Martian terrain proving ground to 
collect data on how a rover wheel interacts with different soil types 
and loose sand. He used yellow, pink and green sand -- dyed with food 
coloring and baked by Brock. Sullivan used a stack of large picture 
frames to layer the different colored sands to observe how a wheel 
churned out sloping tailings piles and where the yellow, pink and 
green sand finally landed. "Locations where the deepest colors were 
concentrated on the surface suggest where analysis might be 
concentrated when the maneuver is repeated for real on Mars," he says.

Stewart notes similarities between these tests and those for the 
lunar-landing missions in the late-1960s, when engineers needed to 
know the physical characteristics of the moon's surface. Back then, 
geologists relied on visual observations from scouting missions to 
determine if the lunar lander would sink or kick up dust, or whether 
the lunar surface was dense or powdery.

  "Like the early lunar missions, we'll be doing the same thing, only 
this time examining the characteristics of the Martian soil," Stewart 
says. "We'll be exposing fresh material to learn the mineralogy and 
composition."

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