New observations from a spacecraft orbiting Mercury have revealed that the tiny, pockmarked planet harbors a highly unusual interior and the crafts glimpse of Mercurys surface topography suggests the planet has had a very dynamic history.
The observations were taken by a probe called MESSENGER (short for Mercury Surface, Space Environment, Geochemistry and Ranging), the first ever to enter orbit around Mercury. MESSENGER reached Mercurys orbit in March 2011, and has since circled the planet twice a day, collecting nearly 100,000 images and more than four million measurements of Mercurys surface.
A team of scientists from institutions including MIT, the Carnegie Institution of Washington, Johns Hopkins Universitys Applied Physics Laboratory and NASAs Goddard Space Flight Center have analyzed the data and precisely mapped the planets topography and gravitational fields. From the gravity estimates, the team found that Mercury likely has a highly unusual interior structure an exceptionally large iron core overlain by a solid layer of iron sulfide and a thin outer shell of silicate mantle and crust. From topographic measurements, the team mapped out a large number of craters on the planets surface, making a surprising finding: Many of these have tilted over time, suggesting that processes within the planet have deformed the terrain after the craters formed.
The researchers detail their findings in two papers published this week in the journal Science.
Prior to MESSENGERs comprehensive observations, many scientists believed that Mercury was much like the moon that it cooled off very early in solar system history, and has been a dead planet throughout most of its evolution, says co-author Maria Zuber, the E.A. Griswold Professor of Geophysics at MIT. Now were finding compelling evidence for unusual dynamics within the planet, indicating that Mercury was apparently active for a long time.
Getting into orbit about Mercury was no easy feat, mostly because of its proximity to the sun. Any spacecraft heading toward the planet speeds up, drawn in by the suns powerful gravitational field. To counteract the suns pull and slow MESSENGER down, the MESSENGER team programmed the probe to fly by Venus twice, and Mercury three times, before slowing down enough to be captured in Mercurys orbit with the help of a main engine burn.
After entering Mercurys orbit, the spacecraft began measuring the planets surface elevations via laser altimetry. Through radio tracking, the probe estimated the planets gravity field. Throughout the one-year mission, the MESSENGER spacecraft battled tides from the sun, which tugged the probe out of its optimal orbit, as well as what Zuber calls sunlight pressure photons or packets of light from the sun that exerted pressure on the spacecraft. The team periodically adjusted the probes orbit and made precise corrections to its measurements to account for the suns effects, mapping out the gravity field as well as the elevation of the surface of Mercurys northern hemisphere.
Inside and out
The teams measurements revealed surprising findings both in the planets interior and on its surface. From the probes gravity estimates, the group inferred that Mercury likely has a huge iron core comprising approximately 85 percent of the planets radius. (Earths core, by comparison, is about half the planets radius in size.) This means that Mercurys mantle and crust occupy only the outer 15 percent or so of the planets radius about as thin as the peel on an orange, Zuber says.
The researchers also reasoned, given Mercurys gravity field, that just above the outer molten layer of the planets core may be a solid layer of iron and sulfur a type of layered structure not known to exist on any other planet.
If the iron and sulfur model is correct, it would have implications for how the dynamo inside Mercury produces the planet's magnetic field, says Gerald Schubert, professor of earth and space sciences at the University of California at Los Angeles, who did not participate in the research. The dynamo generation process might work differently in Mercury compared with Earth.
Co-author Dave Smith, a research scientist in MITs Department of Earth, Atmospheric and Planetary Sciences, says the scientific process that led to the teams results was a journey in itself.
We had an idea of the internal structure of Mercury, [but] the initial observations did not fit the theory so we doubted the observations, Smith says. We did more work and concluded the observations were correct, and then reworked the theory for the interior of Mercury that fit the observations. This is how science is supposed to work, and its a nice result.
Through laser measurements of the planets surface, researchers mapped out multiple geologic features in Mercurys northern hemisphere, finding the range of elevations to be smaller than that of Mars or the moon. They also observed something unexpected in Mercurys Caloris basin, the largest impact feature on Mercury: Portions of the floor of the crater actually stand higher than its rim, suggesting that forces within the interior pushed the crater up after the initial impact that created it.
Zuber and her team also identified an area of lowlands approximately centered on Mercurys north pole that could conceivably have migrated there over the course of the planets evolution. Zuber explains that a process called polar wander can cause geological features to shift around on a planets surface due to the redistribution of mass on or within a planet by geodynamical processes.
One such process of transporting mass in a planets interior is convection within the mantle. Viscous material within the mantle circulates and can push fragments of crust up and out, shifting terrain around the globe. Given Mercurys extremely thin mantle, as revealed by MESSENGER, Zuber says its challenging to understand how convection operated to raise broad expanses of terrain to the elevations observed.
Its interesting to think what might be causing the observed deformation, Zuber says. It appears there are some very unusual dynamics going on inside Mercury.
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More information: www.sciencemag.org/content/early/2012/03/20/science.1218805