Epic volcanic activity flooded Mercury's north polar region

September 29, 2011, Brown University
A View Looking Down on the North Pole of Mercury (Center)

(PhysOrg.com) -- Ever since the Mariner 10 mission in 1974 snapped the first pictures of Mercury, planetary scientists have been intrigued by smooth plains covering parts of the surface. Some suspected past volcanic activity, but there were no telltale signs like protruding volcanoes. Also, Mercury's northern plains are the same brightness as its cratered highlands, yet different from volcanic deposits on the Moon, which are darker than the highlands.

"For more than 35 years we have been uncertain about the role of on Mercury," said James W, Head III, professor of geological sciences at Brown University.

In a paper published in Science, Head and more than two dozen colleagues from Brown and other institutions used data from the orbiting MESSENGER spacecraft to examine Mercury's largely unseen northern high latitudes. They report that the smooth plains there are the result of volcanic activity. Early in the planet's history -- some 3.5 to 4 billion years ago, the scientists say -- huge volumes of poured out from cracks in Mercury's surface, flooding the surrounding, low-lying plains "like a bathtub," Head said. The lava flows, the scientists write, fill craters more than a mile deep and cover 6 percent of Mercury's surface, an area that would cover nearly 60 percent of the continental United States. The volume would have been enough to bury the state of Texas more than four miles deep.

Lava flows on Mercury more than 3.5 billion years ago -- a mile deep in places -- would have covered nearly 60 percent of the continental United States. Credit: Image courtesy of James Head research group, Brown University

The lava flows, "don't build a volcano like we see on Hawaii; rather, they cover up the place where the lava is coming out, and they're very difficult to understand in the context of the current Earth eruption conditions," said Head, who has studied volcanism on planets and moons for more than four decades.

"But one thing is clear," added Jennifer Whitten, a graduate student in Head's research group and a contributing author on the paper. "So much lava comes out so rapidly, that it's an entirely different type of volcanism than we see at Hawaii. This gives us big clues about what's going on in the interior of Mercury."

An Example of a Large Crater (Tyagaraja, 97 km in Diameter) with a Floor Partially Covered by Large Numbers of Coalesced Hollows

Head explained that the lava flows give scientists insights into how planets are born, how they evolved and whether they're still active. "For example, on the Moon, we see very little evidence of activity of volcanic processes over the last 2 to 3 billion years," he added.

To confirm the plains were caused by very rapid volcanism, the researchers looked at a feature about 125 miles outside the volcanic zone. There, they saw evidence of a fissure vent, with wide river-like channels emanating from the crack. "These features are similar to and very fluid flows that erode much of the surrounding terrain," said Debra Hurwitz, also a graduate student with Head, who studies similar features on the Moon and Mars and is a contributing author on the paper.

Schematic Illustration of the Operation of MESSENGER's Gamma-Ray Spectrometer (GRS)

The team believes this is similar to what happened in the smooth plains, but the clues have been largely erased by the sheer volume of lava that poured out.

"When trying to understand the origin of the smooth plains, it is helpful to look at the margin of the plains and its surroundings," said Caleb Fassett, a postdoctoral researcher at Brown now teaching at Mount Holyoke College, and a contributing author on the paper. "Where the plains thin and meet surrounding terrain, the differences between the plains and pre-existing terrain can help give us insight into how the plains were formed."

The MESSENGER spacecraft is currently in orbit around planet Mercury. The Fast Imaging Plasma Spectrometer (FIPS) on board is taking the first global measurements of the charged particles in Mercury's space environment. FIPS found that at the magnetic cusps near the planet's poles, the solar wind is able to bear down on Mercury enough to blast particles from its surface into its wispy atmosphere. Shannon Kohlitz, Media Academica, LLC

The has been orbiting Mercury since March. The same spacecraft executed three flybys of Mercury in previous years, which gave the scientists their first look at the smooth plains. The team hopes that other instruments on MESSENGER will allow them to better understand the minerals and chemical composition in the northern , as well as to compare the volcanic activity there with other regions that experienced volcanism.

"This one deposit is so huge," Head said, "volcanism has got to be important elsewhere."

Explore further: Researchers use multispectral images to reveal origin and evolution of Mercury

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3 / 5 (2) Sep 29, 2011
"The volume would have been enough to bury the state of Texas more than four miles deep."

Because that is so much easier to visualize. How about "enough to cover the island of Manhattan in 31,841 miles of lava" or "enough lava to fill 1.79x10^12 Olympic-size swimming pools"?

Hat tip to the Discovery Channel for every show they've ever had about big stuff.
1 / 5 (4) Sep 29, 2011
That is a very strange story!

The picture, "Schematic Illustration of the Operation of MESSENGER's Gamma-Ray Spectrometer (GRS)" seems totally out of place.

Could we ask Professor James W. Head, III to explain if his finding confirms or denies earlier reports that the terrestrial planets accreted heterogeneously [1,2] ?

1. "Inhomogeneous accumulation of the earth from the primitive solar nebula," Earth Planet. Sci. Lett. 6, 346-348 (1969).

2. "The noble gas record of the terrestrial planets", Geochem. J. 15, 247-267 (1981)


With kind regards,
Oliver K. Manuel

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