Rock and (Not) Roll: Study Eyes How To Keep A Mars Tumbleweed Rover Moving On Rocky Terrain

For Immediate Release

Matt Shipman | News Services | 919.515.6386

Release Date: 05.23.2012
Filed under Releases

New research from North Carolina State University shows that a wind-driven “tumbleweed” Mars rover would be capable of moving across rocky Martian terrain – findings that could also help the National Aeronautics and Space Administration (NASA) design the best possible vehicle.

Model of a tumbleweed rover

“There is quite a bit of interest within NASA to pursue the tumbleweed rover design, but one of the questions regarding the concept is how it might perform on the rocky surface of Mars,” says Dr. Andre Mazzoleni, an associate professor of mechanical and aerospace engineering (MAE) at NC State and co-author of a paper describing the research. “We set out to address that question.”

Mazzoleni and Dr. Alexander Hartl, an adjunct professor of MAE at NC State, developed a computer model to determine how varying the diameter and mass of a tumbleweed rover would affect its speed and ability to avoid getting stuck in Martian rock fields. Rock fields are common on the surface of Mars, which averages one rock per square meter.

“We found that, in general, the larger the diameter, and the lower the overall weight, the better the rover performs,” Mazzoleni says. In addition, the study found that a tumbleweed rover would need to have a diameter of at least six meters in order to achieve an acceptable level of performance – meaning the rover could move through rock fields without getting stuck.

Using the model, the researchers also found that tumbleweed rovers are more likely to bounce than roll across the surface, due to the spacing of the rocks and the size of the rovers.

The surface of Mars averages one rock per square meter.

“Computer simulations are crucial for designing Mars rovers because the only place where you find Martian conditions is on Mars,” says Mazzoleni. “Earth-based testing alone cannot establish whether a particular design will work on Mars.” Mars has approximately three-eighths of Earth’s gravity. And the atmospheric density on the surface of Mars is only duplicated around 100,000 feet above the Earth’s surface.

Tumbleweed rovers are attractive because they can cover much larger distances, and handle rougher terrain, than the rovers that have already been sent to Mars – such as Spirit and Opportunity. “This model is a tool NASA can use to assess the viability of different designs before devoting the time and expense necessary to build prototypes,” Mazzoleni says.

While tumbleweed rovers would lack the precise controls of the wheeled rovers, they would also not rely on a power supply for mobility – they would be literally blown across the Martian landscape by the wind.

The paper, “Terrain Modeling and Simulation of a Tumbleweed Rover Traversing Martian Rock Fields,” is published in the March/April issue of the Journal of Spacecraft and Rockets. Hartl is lead author. The research was supported in part by North Carolina Space Grant and NASA.

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Note to Editors: The study abstract follows.

“Terrain Modeling and Simulation of a Tumbleweed Rover Traversing Martian Rock Fields”

Authors: Alexandre E. Hartl, Andre P. Mazzoleni, North Carolina State University

Published: March/April issue of the Journal of Spacecraft and Rockets

Abstract: A tumbleweed rover is a spherical wind-driven vehicle designed to negotiate harsh Martian terrain while searching for areas of scientific interest. This paper models Martian rock fields and analyzes the rover’s dynamics on these terrains. Computational procedures are established for creating randomized Martian rock fields based on statistical models. Optimization techniques allow for terrain generation to coincide with the rover’s motion, reducing the computational cost of exploring broad regions. Efficient collision detection routines reduce the number of tests of potential collisions that must be performed between the rover and the terrain while establishing new contact constraints. Simulations demonstrate that bouncing is the rover’s dominant mode of travel through the rock fields, and Monte Carlo simulations illustrate how the rover’s downrange position depends on the rover design and atmospheric conditions. The rover’s capacity for long-distance travel over Martian rock fields is verified.

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