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This Discovery Program mission, scheduled for launch in 2018, will place a geophysical lander on Mars to study its deep interior.
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The data sets for Mars don't have as much resolution, so it's more difficult to pin down the density of the crust from current gravity maps, which is why previous estimates relied more heavily on studies of the composition of Mars' 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,' said Goddard planetary geologist Dr Greg Neumann, a co-author on the paper.
Evidence of water on Mars dates back to the Mariner 9 mission, which arrived in 1971.
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'With this approach, we were able to squeeze out more information about the gravity field from the existing data sets,' said Goddard geophysicist Dr Terence Sabaka, the second author on the paper.
Before trying Mars, the researchers tested their approach by applying it to the gravity field that was in use before the GRAIL mission.
The new findings could help researchers understand the Red Planet's interior structure and evolution.
A new map of the thickness of Mars’ crust shows less variation between thicker regions (red) and thinner regions (blue), compared to earlier maps. The NASA team found that globally Mars’ crust is less dense, on average, than previously thought, which implies smaller variations in crustal thickness'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’ formation and evolution,' said Dr Sander Goossens of NASA’s Goddard Space Flight Center in Greenbelt, Maryland, and the lead author of a Geophysical Research Letters paper describing the work.
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There are many facets that require research beyond these questions, because the relationship between colour and shape is a puzzle with many solutions.