MESSENGER data reveals great valley on Mercury

American Geophysical Union

A full-colour composite image of Mercury taken during the first flyby of NASA's MESSENGER spacecraft on 14 January 2008. Mercury has a diameter of 3030 miles, or 38 percent that of the Earth. The planet rotates once in 58.6 days and its year is almost 88 days. With virtually no atmosphere, Mercury's heavily cratered surface endures wildly ranging temperatures from −173 °C at night to 427 °C during the day. Mercury's eccentric orbit means that its distance from the Sun varies between 28.6 million and 43.4 million miles. Image credit: NASA/Johns Hopkins University Applied Physics Laboratory/Carnegie Institution of Washington.
A full-colour composite image of Mercury taken during the first flyby of NASA’s MESSENGER spacecraft on 14 January 2008. Mercury has a diameter of 3030 miles, or 38 percent that of the Earth. With virtually no atmosphere, the inner planet’s heavily cratered surface endures wildly ranging temperatures from −173 °C at night to 427 °C during the day. A recent study reveals a new large valley on Mercury that may be the first evidence of buckling of the planet’s outer silicate shell in response to global contraction. Image credit: NASA/Johns Hopkins University Applied Physics Laboratory/Carnegie Institution of Washington – NASA/JPL.
Scientists have discovered a new large valley on Mercury that may be the first evidence of buckling of the planet’s outer silicate shell in response to global contraction. The researchers discovered the valley using a new high-resolution topographic map of part of Mercury’s southern hemisphere created by stereo images from NASA’s MESSENGER spacecraft. The findings were reported in a new study published in Geophysical Research Letters, a journal of the American Geophysical Union.

The most likely explanation for Mercury’s Great Valley is buckling of the planet’s lithosphere — its crust and upper mantle — in response to global contraction, according to the study’s authors. Earth’s lithosphere is broken up into many tectonic plates, but Mercury’s lithosphere consists of just one plate. Cooling of Mercury’s interior caused the planet’s single plate to contract and bend. Where contractional forces are greatest, crustal rocks are thrust upward while an emerging valley floor sags downward.

“There are examples of lithospheric buckling on Earth involving both oceanic and continental plates, but this may be the first evidence of lithospheric buckling on Mercury,” said Thomas R. Watters, senior scientist at the Center for Earth and Planetary Studies at the Smithsonian’s National Air and Space Museum in Washington, D.C., and lead author of the new study.

Using colourised topography, Mercury's 'great valley' (dark blue) and Rembrandt impact basin (purple, upper right) are revealed in this high-resolution digital elevation model merged with an image mosaic obtained by NASA's MESSENGER spacecraft. Image credit: NASA/JHUAPL/Carnegie Institution of Washington/DLR/Smithsonian Institution.
Using colourised topography, Mercury’s ‘great valley’ (dark blue) and Rembrandt impact basin (purple, upper right) are revealed in this high-resolution digital elevation model merged with an image mosaic obtained by NASA’s MESSENGER spacecraft. Image credit: NASA/JHUAPL/Carnegie Institution of Washington/DLR/Smithsonian Institution.
The valley is about 400 kilometres (250 miles) wide with its floor as much as 3 kilometres (2 miles) below the surrounding terrain. The valley is more than 1,000 kilometres (600 miles) long and extends into the Rembrandt basin, one of the largest and youngest impact basins on Mercury.

The valley is bound by two large fault scarps — steps on the planet’s surface where one side of a fault has moved vertically with respect to the other. Mercury’s contraction caused the fault scarps bounding the Great Valley to become so large they essentially became cliffs. The elevation of the valley floor is far below the terrain surrounding the mountainous faults scarps, which suggests the valley floor was lowered by the same mechanism that formed the scarps themselves, according to the study authors.

“Unlike Earth’s Great Rift Valley in East Africa, Mercury’s Great Valley is not caused by the pulling apart of lithospheric plates due to plate tectonics; it is the result of the global contraction of a shrinking one-plate planet,” Watters said. “Even though you might expect lithospheric buckling on a one-plate planet that is contracting, it is still a surprise when you find that it’s formed a great valley that includes the largest fault scarp and one of the largest impact basins on Mercury.”