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Friday, March 23, 2012

Images from spacecraft reveal Mercury's secrets

Images from spacecraft reveal Mercury’s secrets

Above: Mercury, as taken from the spacecraft MESSENGER. The spacecraft captured nearly 100,000 images as it orbited the planet. (Courtesy: UC Santa Barbara)

UC SANTA BARBARA (US) — Scientists now have a good picture of Mercury, the solar system’s innermost planet, thanks to the MESSENGER spacecraft.

On March 17, MESSENGER (MErcury Surface, Space Environment, GEochemistry, and Ranging) completed its one-year primary mission, orbiting Mercury, capturing nearly 100,000 images, and recording data that reveals new information about the planet’s core, topography, and the mysterious radar bright material in the permanently shadowed areas near the poles.

The findings are presented in two papers published online in Science Express (paper #1 and paper #2).

“Mercury is the last unexplored planet,” says Stanton Peale, a physics professor emeritus at the University of California, Santa Barbara.

Peale devised the procedure used for detecting whether or not Mercury had a liquid core. The way Mercury was formed, he says, may show some constraints on the formation of the solar system.

Straight from the Source

Read the original study

DOI: 10.1126/science.1218809

For one thing, Mercury’s core is larger than expected—almost 85 percent of the planetary radius. The Earth’s core, in contrast, is just over half of the planet’s radius. Additionally, Mercury appears to have a more complex core than Earth’s—a solid iron sulfide layer that is now part of the mantle, which encases a liquid core, which may float on a solid inner core.

The scientists, led by MIT researchers David E. Smith and Maria T. Zuber, also found that Mercury’s solid outer core and liquid inner core contain more iron than Earth, relative to the whole planet, which influences the way Mercury’s magnetic field was generated. However, Peale noted that the surface is comprised of lighter elements.

“We didn’t expect so much sulfur,” he says, adding that there was almost no iron found on the surface of the planet. With no iron, the volcanic surface rocks are too light to have come from a mantle with the large average density derived for the internal structure. This led to the concept of a two-layer mantle—with a light upper silicate layer, which could provide the low-density surface material — over a dense iron sulfide layer.

In the larger picture, the presence of inordinately large amounts of sulfur on the surface indicates that Mercury’s formation was not as orderly as some scientists had previously assumed, according to Peale. “Mercury is composed of material that had condensed over a wide range from the Sun,” he says.

Other findings include a precise topographic model of the planet’s northern hemisphere, which reveals a smaller spread in elevations compared to those of Mars or the Moon.

Additionally, radar-bright features at the poles located in areas of permanent shadow have been found to be consistent with a water-ice hypothesis; however the notion has yet to be tested further with MESSENGER’s neutron spectrometer.

MESSENGER is already on the next phase of its investigations: an extended year-long mission that includes more comprehensive and more targeted measurements.

More news from UC Santa Barbara: www.ucsb.edu/news-topics

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