Mars has a porous crust, says NASA study. Mars’s crust is not as dense as previously thought and a lower density likely means that at least part of the Red Planet’s crust is relatively porous, says a new NASA study.
The findings, published in the journal Geophysical Research Letters, provide researchers clue that could help them better understand the interior structure and evolution of Mars. “The crust is the end-result of everything that happened during a planet’s history, so a lower density could have important implications about Mars’s formation and evolution,” said study lead author Sander Goossens of NASA’s Goddard Space Flight Center in Greenbelt, Maryland. The researchers mapped the density of the Martian crust, estimating the average density is 2,582 kgs per metre cubed. That’s comparable to the average density of the lunar crust.
Typically, Mars’s crust has been considered at least as dense as Earth’s oceanic crust, which is about 2,900 kgs per metre cubed.
The new value is derived from Mars’s gravity field, a global model that can be extracted from satellite tracking data using sophisticated mathematical tools. Previous estimates relied more heavily on studies of the composition of Mars’s soil and rocks.
“As this story comes together, we’re coming to the conclusion that it’s not enough just to know the composition of the rocks,” study co-author Greg Neumann, a planetary geologist at Goddard, said.
“We also need to know how the rocks have been reworked over time,” Neumann said.
Goossens and colleagues started with the same data used for an existing gravity model but put a new twist on it by coming up with a different constraint and applying it to obtain the new solution.
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