Mars may have a Porous Crust, with the same lunar density

NASA scientists are one step closer to understanding the evolution of Mars. New evidence derive from gravity map

New evidence shows that the Red Planet’s outer crust, which is about 30 miles (50 kilometers) thick, is porous and not as dense as previously thought.

“A lower density could have important implications about Mars’ formation”, Sander Goossens, a researcher at NASA’s Goddard Space Flight Center (GSFC) in Maryland and lead author of the new study, said in a statement from NASA.

GSFC’s Planetary Geodynamics Laboratory made its crust discoveries by looking at Mars’ gravity field, which was previously derived using satellite tracking data and advanced mathematical tools. Goossens and his team used the gravity field in a modified technique, which correlates the field with precise measurements of Mars’ topography, or surface features, to make findings of Mars’ crust density more accurate.

Gravity Maps

Gravity fields allow scientists to understand Mars on a deeper level, literally. Similar techniques have been used, for example,to investigate the moon’s subterranean composition and history. Researchers measure a planetary body’s gravity field by tracking tiny changes in satellites’ orbits as they pass over specific areas that have differing gravitational pulls.

According to NASA, the Martian crust was found to have an average density of 2,582 kilograms per meter cubed (about 161 lbs. per cubic foot), or about the same average density as the crust on Earth’s moon.

Moon test

Previous estimates of Martian crust density relied more heavily on looking at the composition of the soil and the rocks themselves. That’s because up until now, the data sets that would produce gravity maps had a low resolution, NASA said. By comparison, the gravity field for Earth is very detailed, because the data sets have a high resolution, according to NASA.

“As this story comes together, we’re coming to the conclusion that it’s not enough just to know the composition of the rocks,” Goddard planetary geologist Greg Neumann, co-author on the paper, said in the statement. “We also need to know how the rocks have been reworked over time.”

To get findings that were more precise, Goossens and his team developed a technique to make correlations between Mars’ topography— in particular, changes in elevation — and the planet’s gravity field. Once they tested their new technique on Earth’s moon, and found that the method successfully produced results that matched those found by NASA’s Gravity Recovery and Interior Laboratory (GRAIL), the team used its model to analyze Martian surface density.


“With this approach, we were able to squeeze out more information about the gravity field from the existing data sets”, Goddard geophysicist Terence Sabaka, also a study co-author, said in the statement.

NASA’s Interior Exploration using Seismic Investigations, Geodesy and Heat Transport (InSight) mission is expected to provide measurements that can verify Goossens’ findings, in much the same way that GRAIL verified the lunar-density testing, according to the statement. InSight is scheduled to launch in 2018 with the Discovery Program mission, and when it arrives on Mars, InSight can probe the interior of this rust-colored neighbor planet.

(Source: journal Geophysical Research Letters)

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