Showing posts with label ocean. Show all posts
Showing posts with label ocean. Show all posts

Sunday, 17 July 2011

Death of a Continent, Birth of an Ocean

access As Afar is pulled and jostled from below, fissures form across the landscape. Some areas are already below sea level.Lorraine Field/Univ. of Bristol

To those who live there, east Africa’s Afar region is “the place the devil plows.” One of the hottest and lowest areas on Earth, it is a landscape of baking desert and barren lava flows. To scientists, though, Afar means something more promising: geology in the raw.

There, on the edge of Africa, the continent is splitting apart. Pulled inexorably by the grind of tectonic plates, Afar is ripping asunder like a gateway to hell. Molten rock wells up from below, pouring onto the sweltering surface.

Yet for all the fire and brimstone, Afar is on its way to a watery end. A million years or so from now, the geological processes that rip the continent will give birth to a new seafloor. And Afar will lie at the bottom of Earth’s freshest ocean.

Until then, researchers have a front seat to an unparalleled physical spectacle. “It’s a really unique opportunity to understand how continents break apart,” says Tim Wright, a remote-sensing expert at the University of Leeds in England. Wright leads a large international consortium that began studying the region in 2005, when the splitting picked up pace.

Afar’s geological violence comes in many forms. Magma welling up from the depths sometimes erupts through existing volcanoes. Other times it pools underground, cooling to form giant vertical sheets called dikes. As it rises, the moving magma causes the ground to tremble in an earthquake drumroll. For the past couple of years scientists have listened to the landscape’s clamor, trying to discover what Afar has to say about the death of continents.

New findings reveal that the dikes stack up against each other — fresh ones pushing their way into places where the rock is least stressed, crackling with seismicity as the magma arrives. Other discoveries include the first-ever glimpse at how magma flows from storage reservoirs into such dikes along an intricate system of volcanic plumbing. For the first time, researchers have seen some of the planet’s most common geologic activity transpire nearly in real time, and on land where they can watch.

To its list of superlatives — hottest, lowest, least hospitable — Afar can now add the title of best-studied birth of an ocean.

access TENSION ON LANDAfar (shaded) sits where the East African Rift and two ocean-splitting centers meet, meaning the region is being pulled in many directions. Intense geologic activity results: In 2005, researchers detected a flurry of earthquakes and upwelling magma along the Dabbahu rift segment. Lava flows were also observed at the Erta Ale volcano (shown above) in 2010.Image: Lorraine Field/Univ. of Bristol; map: Graphi-Ogre, adapted by E. Feliciano

A violent story

A single earthquake, of magnitude 4.5, first alerted scientists to the tale unfolding in Afar. At Addis Ababa University in Ethiopia, in September 2005, seismologist Atalay Ayele saw the sign of an Afar quake pop up on his monitors. Then more quakes appeared, bigger ones, and then yet more. Something unusual, he realized, was going on.

“It was a surprise,” Ayele says. “We didn’t know at the beginning how big it was going to be. We just recorded all the quakes as we normally do.”

Ayele called Cynthia Ebinger, a geophysicist then at Royal Holloway College at the University of London, who arrived within days with extra seismometers to monitor the quaking ground. Ebinger in turn asked Wright to check for satellite imagery that, by bouncing radar waves off the ground and measuring their return, can reveal how much the ground is shifting, and where. If a big eruption were going on just under the surface, she reasoned, the satellites should have captured it.

“I kept bugging him and bugging him,” remembers Ebinger, now at the University of Rochester in New York. And then one day Wright called with striking news.

Because the Afar quakes hadn’t gotten much bigger than magnitude 5.5, Wright says, “we didn’t expect to see very much. But when we downloaded the data what we saw was astounding — the biggest signal we’d ever seen in terms of ground deformation. At that point it was immediately clear that something really unusual had happened.”

Whereas the ground might move a few centimeters during most volcanic eruptions or earthquakes, places in Afar had moved eight meters in just 10 days, a world record. By the time Ayele and colleagues arrived in the region to check what had happened, fresh fissures and steep cliff faces yawned across the landscape, created by the massively shifting ground. Brand-new lava glistened in the desert sun.

access HOW TO MAKE AN OCEANView larger image | Over time, the rift valley at Afar will become the world’s newest ocean. Ocean formation can take millions of years, but ongoing geologic activity offers researchers clues to the process.E. Feliciano

All this geological action traces to the fact that Afar sits at the intersection of three segments of Earth’s crust that are pulling apart, or rifting.

Like pieces in a moving jigsaw puzzle, the planet’s tectonic plates constantly elbow against one another, carrying continents great distances and allowing new oceans to be born and die. In large part, this plate jostling is driven by fresh magma that wells up from seams that run along the centers of oceans, like the underwater mountain chain that splits the Atlantic Ocean in two. Molten rock erupts onto the seafloor there, then cools and rifts away from the ridge on either side in a process known as seafloor spreading. Geologists can take a peek at this in Iceland, where the Atlantic’s mid-ocean ridge surfaces above the waves.

Plate tectonics can also pull continents apart. Instead of magma cleanly forming fresh ocean crust, continental rifts often have a wide, messy zone where parallel valleys form, accompanied by spasms of eruptions and earthquakes. Such is the case with the Great Rift Valley that runs down eastern Africa on dry land.

In Afar, that continental rift meets two ocean rifts, one bisecting the Red Sea and the other the Gulf of Aden. This tectonic “triple junction,” pulling at Afar from all directions, is the geologic equivalent of being drawn and quartered.

In eastern Africa, the current transition between continental and oceanic rift lies somewhere between Afar and the southern end of the Red Sea. As eastern Africa keeps stretching, though, its continental crust gets thinner and thinner. “Once there’s no continental plate left, once it’s completely thinned and gone, then that’s the end of continental breakup,” says Derek Keir, a former student of Ebinger now at the National Oceanography Centre in Southampton, England.

At that point, Afar will become a true seafloor spreading ridge. Magma welling up from below will be richer in heavy elements like iron, so that the newborn crust will be denser and sink lower in elevation compared with the rest of the African continent. Waters from the Red Sea will rush in, forming a new ocean.

Geologists have known the end is coming for Afar, and they got a preview beginning in 1978, in a part of the rift zone located in Djibouti. There, a small earthquake swarm popped up as magma intruded underground to form a dike. French scientists, who had seismometers and other ground-measuring instruments installed across Djibouti, watched the whole thing happen. “It really helped us understand the processes involved with rifting,” says Cécile Doubre, a tectonophysicist at the Institut de Physique du Globe in Strasbourg.

access ON THE MOVEIn 2005, the Envisat satellite captured how tectonic plates pulling apart in the Afar region caused the greatest ground deformation ever seen from space. At left, the rainbow pattern reveals which parts of the ground surrounding the Dabbahu rift segment moved between May and October of that year — due almost entirely to a September rifting event. Other analyses of ground motion (middle and right) reveal that movement was concentrated along a thin band in the rift zone.T.J. Wright et al/Nature 2006

The main Afar show, though, began in 2005. Geologists knew something was coming, and to some extent they knew pretty much what to expect. The next time magma welled up into the rift zone, Keir had predicted in his doctoral thesis, it would appear below a particular 60-kilometer-long segment of the rift zone with a volcano called Dabbahu at its northern end. But the sheer size of the September 2005 eruption astonished researchers. Over just a couple of days, some 2.5 cubic kilometers of molten rock squirted toward the surface.

Much of this magma had been lurking beneath the region for some time, Wright explains. The magma begins some 20 kilometers down, in the quasi-molten region known as the Earth’s mantle. From there, the magma can make its way toward the surface into shallow chambers, like temporary storage reservoirs, where it sits for some time. Eventually, pressure in these reservoirs gets too great, and the magma forces its way up again — either to erupt out as lava on the surface, or cool and solidify just underground.

In 2005, most of the magma cooled as a 70-kilometer-long dike without making it onto the surface. Since then, 13 other dikes have appeared beneath Afar, most of them much smaller, about 10 kilo­meters long. Scientists can track where the dikes appear and how big they are by monitoring patterns of earthquakes as well as by mapping changes in the ground’s electrical conductivity.

The dikes form one next to another, like a row of marching toy soldiers. In a paper published last year in Nature Geoscience, Wright, his student Ian Hamling and colleagues described how each new dike changes stress fields within the ground. Because magma likes to squirt into regions of lower stress, scientists could predict where the next dike in the sequence would appear.

Earthquakes rippling out from the central rift show how molten rock moves along natural underground pipes. A new study of five of the 14 dikes found that seismicity migrated away from the rift center for about 10 to 15 kilometers, just as it does at ocean spreading centers. Doubre and colleagues, led by Raphaël Grandin of the École Normale Supérieure in Paris, reported the finding in April in Geochemistry, Geophysics, Geosystems.

Researchers have found that the dikes all appear to feed off a main chamber in the center of the Dabbahu rift segment,  Keir says; there isn’t an elongated chamber underlying the entire segment. Similar volcanic plumbing has been observed beneath mid-ocean ridges.

Looking at lava

While the dikes usually don’t make it to the surface, at other places in Afar magma does break through in bona fide volcanic eruptions. Some 110 kilometers north of Dabbahu, for instance, sits the well-known volcano Erta Ale. Most of the time, this volcano doesn’t spit out lava dramatically. Instead, a lava lake constantly burbles around within its crater, like a heated pot of water that never quite boils over.

But during a field trip to Afar in November 2010, Keir and Lorraine Field, a volcanology student at the University of Bristol in England, decided to check out Erta Ale. They climbed up its side, looked down, and realized that the lava lake was higher than scientists had seen it in years — overflowing the side in places. “We had 48 hours of lava heaven,” says Field. “I watched my rocks being born.”

Erta Ale’s lava is thinner and less sticky than that at Dabbahu, suggesting that it is erupting directly from the mantle rather than sitting in reservoir chambers for a while, says Field. (Magma undergoes chemical changes when it sits in a reservoir, such as by melting the surrounding rocks and incorporating their minerals.) Erta Ale is also much closer to the Red Sea’s spreading center, so the ground there may more closely resemble ocean crust than the Dabbahu rift zone does at the moment. How the two areas of volcanic activity are related — and how they fit into the bigger tectonic triple junction picture — remains to be explored.

In some ways, Afar’s chronic volcanism has become an everyday part of life in the region. The Afar people have adapted to gather water for themselves and their goats from natural fumaroles, or steam vents. First, says Field, the locals hold a piece of obsidian glass up to a vent; if it turns cloudy, that signifies too many poisons are in the steam. But if the obsidian stays clear, the people lay reeds down into the vent, then use a can to collect the water that condenses on and drips off the reeds.

In other ways, modern life has not adapted so well to local geology. The newly built regional capital of Afar, Semera, and a nearby dam lie atop the many fault lines that crisscross the region. Both were planned long before the September 2005 eruption and are unlikely to be decommissioned in a place where starvation and disease are more pressing concerns than geologic hazards.

Still, Ayele says he and his colleagues spend a lot of time working to educate the local government and people about the earthquake risk.

In the long term, Afar may need to brace for volcanoes and earthquakes for quite a while. Scientists aren’t sure exactly how long Afar will remain highly active, but they do have one point of comparison: the Krafla eruptions in northern Iceland, which took place over nearly a decade in the 1970s and 1980s. Eruptions at Krafla poured out lava for several years, then quieted down, then burst out again with a lot of magma right at the end.

At Afar, “things have been suspiciously quiet since May 2010,” Wright says, with no dikes or eruptions along the Dabbahu segment. But if Krafla offers a comparison, Afar might yet expect a lot of magma to pour out in another couple of years. Afar also has more magma underlying it to start with than Krafla did.

“We’re not done yet,” says Ebinger.

Already, researchers have recorded a flurry of earthquakes to the east, about 100 kilometers offshore in the Gulf of Aden. That activity, in December 2010, could mean a dike was injected there below the seafloor, which may be related to the activity at Dabbahu. “It’s likely when stress is relieved at one point it can trigger another point that is critically close to failure,” Ayele says. But scientists can’t take a ship to study the region, because of the threat of Somali pirates.

For now, scientists must content themselves with the wealth of data they have gathered from a five-year push in Afar. The data have yielded surprise discoveries, like details on an eruption north of Erta Ale that happened in November 2008. There, for the first time, scientists found and watched magma flow from a very shallow chamber stretched out along the rift axis.

Such “axial magma chambers” are common on the seafloor but almost never studied, says Wright, because they have been so inaccessible — until now. “There’s a huge amount of ocean floor formed through magma in these chambers,” he says, “and now we can actually see how they behave.”

Other remaining questions include where exactly the magma resides lower down in the mantle, from which it pipes to feed storage reservoirs closer to the surface. By piecing together details of the underground plumbing, Ebinger says, scientists can better understand some of the most everyday volcanic processes on Earth.

All from a little bit of rumbling in a remote corner of Africa. “It was just such an exciting event,” says James Hammond, a consortium seismologist at the University of Bristol. “It was a once-in-a-lifetime scientific opportunity.”


Found in: Earth

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Wednesday, 8 June 2011

Melting icebergs fertilize ocean

access CASTING IRONIn iron-poor Antarctic waters, meltwater from icebergs is fertilizing the seas with the metal, fueling a proliferation of sea life — and removing carbon dioxide from the atmosphere.Debbie Nail Meyer © 2009 MBARI

Efforts to remove climate-warming carbon dioxide from Earth’s atmosphere appear to be getting a helping hand from a surprising source: the iron in meltwater from Antarctic icebergs.

Icebergs calving off of Antarctica are shedding substantial iron — the equivalent of a growth-boosting vitamin — into waters starved of the mineral, a new set of studies demonstrates. This iron is fertilizing the growth of microscopic plants and algae, transforming the waters adjacent to ice floes into teeming communities of everything from tiny shrimplike krill to fish, birds and sometimes mammals.

To grow, these plants and animals use carbon drawn into the water from carbon dioxide in the atmosphere. Some share of this carbon will eventually be excreted as wastes that fall to the ocean floor, essentially removing it as a near-term climate risk.

“Icebergs should be considered by climate modelers, because the more icebergs that develop [from the breakup of glaciers], the more carbon dioxide you’ll draw out of the atmosphere,” says Ken Smith of the Monterey Bay Aquarium Research Institute in Moss Landing, Calif.

Smith and colleagues first fingered icebergs as hotspots of biological and chemical activity in a 2007 study published in Science. New data from Antarctic cruises in 2008 and 2009 by Smith and other scientists from nine research institutions now appear as 20 papers in the June Deep Sea Research Part II. 

Researchers refer to icebergs’ carbon removal as an export. “And the amount of carbon being exported near icebergs is twice as high as in areas away from them,” Smith says.

Counterbalancing icebergs’ carbon removal: No one views the sea-level rise accompanying massive ice melting as a good thing. The rate of iceberg calving — and ice loss — in recent years has increased there, as elsewhere, in response to warming of Earth’s atmosphere.

Prior to the new studies, “we didn’t know the nature of the biological communities associated with icebergs and we certainly didn’t know their direct relationship to carbon exports,” says chemist Timothy Shaw of the University of South Carolina in Columbia, who coauthored several of the new reports.

One surprise: The proliferation of phytoplankton — tiny plants at the base of the marine food chain — that were witnessed in the waters around ice floes “could only account for about half of the increased carbon export we measured,” Shaw says. His team now attributes the other half to changes in the chemistry of iron and carbon use by phytoplankton living next to and under the icebergs.

Benjamin Twining of the Bigelow Laboratory for Ocean Sciences in West Boothbay Harbor, Maine, points to another big surprise: Icebergs’ iron enrichment of southern waters could vary by a factor of 100 from one iceberg to another, or even along walls of a given berg. This patchy enrichment reflects differences in chemical reactions triggered by various organisms and to the unexpectedly complicated turbulence associated with water melting from the floes.


Found in: Earth, Environment, Life and Molecules

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Sunday, 29 May 2011

NASA's Galileo reveals magma 'ocean' beneath surface of Jupiter's moon

ScienceDaily (May 12, 2011) — A new analysis of data from NASA's Galileo spacecraft has revealed that beneath the surface of Jupiter's volcanic moon Io is an "ocean" of molten or partially molten magma.

The finding, from a study published May 13 in the journal Science, is the first direct confirmation of such a magma layer on Io and explains why the moon is the most volcanic object known in the solar system. The research was conducted by scientists from UCLA, UC Santa Cruz and the University of Michigan-Ann Arbor.

"The hot magma in Io's ocean is millions of times better at conducting electricity than rocks typically found on the Earth's surface," said the study's lead author, Krishan Khurana, a former co-investigator on Galileo's magnetometer team and a research geophysicist with UCLA's Institute of Geophysics and Planetary Physics. "Just like the waves beamed from an airport metal detector bounce off metallic coins in your pocket, betraying their presence to the detector, Jupiter's rotating magnetic field continually bounces off the molten rocks in Io's interior. The bounced signal can be detected by a magnetometer on a passing spacecraft.

"Scientists are excited that we finally understand where Io's magma is coming from and have an explanation for some of the mysterious signatures we saw in some of Galileo's magnetic field data," Khurana added. "It turns out Io was continually giving off a 'sounding signal' in Jupiter's rotating magnetic field that matched what would be expected from molten or partially molten rocks deep beneath the surface."

Io's volcanoes are the only known active magma volcanoes in the solar system other than those on Earth; Io produces about 100 times more lava each year than all of Earth's volcanoes. While those on Earth occur in localized hotspots like the "Ring of Fire" around the Pacific Ocean, Io's volcanoes are distributed all over its surface. A global magma ocean lying beneath about 20 to 30 miles (30 to 50 km) of Io's crust helps explain the moon's activity.

"It has been suggested that both the Earth and moon may have had similar magma oceans billions of years ago, at the time of their formation, but they have long since cooled," said Torrence Johnson, who was Galileo's project scientist, based at NASA's Jet Propulsion Laboratory in Pasadena, Calif., and who was not directly involved in the study. "Io's volcanism informs us how volcanoes work and provides a window in time to styles of volcanic activity that may have occurred on the Earth and moon during their earliest history."

Io's volcanoes were discovered by NASA's Voyager spacecraft in 1979. The energy for the volcanic activity comes from the squeezing and stretching of the moon by Jupiter's gravity as Io orbits the immense planet, the largest in the solar system.

Galileo was launched in 1989 and began orbiting Jupiter in 1995. After a successful mission, the spacecraft was intentionally sent into Jupiter's atmosphere in 2003. The unexplained signatures appeared in the magnetic-field data taken from Galileo fly-bys of Io in October 1999 and February 2000, during the final phase of the mission.

"But at the time, models of the interaction between Io and Jupiter's immense magnetic field, which bathes the moon in charged particles, were not yet sophisticated enough for us to understand what was going on in Io's interior," said study co-author Xianzhe Jia of the University of Michigan.

Recent work in mineral physics showed that a group of what are known as "ultramafic" rocks become capable of carrying substantial electrical current when melted. These rocks are igneous in origin -- that is, they are formed through the cooling of magma. On Earth, ultramafic rocks are believed to derive from the mantle. The finding led Khurana and colleagues to test the hypothesis that the strange signature was produced by an electrical current flowing in a molten or partially molten layer of this kind of rock.

Tests showed that the signatures detected by Galileo were consistent with a rock like lherzolite, an igneous rock rich in silicates of magnesium and iron found, for example, in Spitzbergen, Norway. The magma ocean layer on Io appears to be more than 30 miles (50 km) thick, making up at least 10 percent of the moon's mantle by volume. The blistering temperature of the magma ocean probably exceeds 2,200 degrees Fahrenheit (1,200 degrees Celsius).

Additional co-authors on the paper are Christopher T. Russell, professor of geophysics and space physics in UCLA's Department of Earth and Space Sciences; Margaret Kivelson, professor emeritus of space physics in UCLA's Department of Earth and Space Sciences; Gerald Schubert, professor of geophysics and planetary physics in UCLA's Department of Earth and Space Sciences; and Francis Nimmo, associate professor of Earth and planetary sciences at UC Santa Cruz.

The Galileo mission was managed by the Jet Propulsion Laboratory (JPL), a division of the California Institute of Technology in Pasadena, for NASA.

Story Source:

The above story is reprinted (with editorial adaptations by ScienceDaily staff) from materials provided by University of California - Los Angeles. The original article was written by Jia-Rui Cook.

Journal Reference:

Krishan K. Khurana, Xianzhe Jia, Margaret G. Kivelson, Francis Nimmo, Gerald Schubert, Christopher T. Russell. Evidence of a Global Magma Ocean in Io’s Interior. Science, 2011; DOI: 10.1126/science.1201425

Note: If no author is given, the source is cited instead.

Disclaimer: Views expressed in this article do not necessarily reflect those of ScienceDaily or its staff.


View the original article here

Monday, 16 May 2011

NASA's Galileo reveals magma 'ocean' beneath surface of Jupiter's moon

ScienceDaily (May 12, 2011) — A new analysis of data from NASA's Galileo spacecraft has revealed that beneath the surface of Jupiter's volcanic moon Io is an "ocean" of molten or partially molten magma.

The finding, from a study published May 13 in the journal Science, is the first direct confirmation of such a magma layer on Io and explains why the moon is the most volcanic object known in the solar system. The research was conducted by scientists from UCLA, UC Santa Cruz and the University of Michigan-Ann Arbor.

"The hot magma in Io's ocean is millions of times better at conducting electricity than rocks typically found on the Earth's surface," said the study's lead author, Krishan Khurana, a former co-investigator on Galileo's magnetometer team and a research geophysicist with UCLA's Institute of Geophysics and Planetary Physics. "Just like the waves beamed from an airport metal detector bounce off metallic coins in your pocket, betraying their presence to the detector, Jupiter's rotating magnetic field continually bounces off the molten rocks in Io's interior. The bounced signal can be detected by a magnetometer on a passing spacecraft.

"Scientists are excited that we finally understand where Io's magma is coming from and have an explanation for some of the mysterious signatures we saw in some of Galileo's magnetic field data," Khurana added. "It turns out Io was continually giving off a 'sounding signal' in Jupiter's rotating magnetic field that matched what would be expected from molten or partially molten rocks deep beneath the surface."

Io's volcanoes are the only known active magma volcanoes in the solar system other than those on Earth; Io produces about 100 times more lava each year than all of Earth's volcanoes. While those on Earth occur in localized hotspots like the "Ring of Fire" around the Pacific Ocean, Io's volcanoes are distributed all over its surface. A global magma ocean lying beneath about 20 to 30 miles (30 to 50 km) of Io's crust helps explain the moon's activity.

"It has been suggested that both the Earth and moon may have had similar magma oceans billions of years ago, at the time of their formation, but they have long since cooled," said Torrence Johnson, who was Galileo's project scientist, based at NASA's Jet Propulsion Laboratory in Pasadena, Calif., and who was not directly involved in the study. "Io's volcanism informs us how volcanoes work and provides a window in time to styles of volcanic activity that may have occurred on the Earth and moon during their earliest history."

Io's volcanoes were discovered by NASA's Voyager spacecraft in 1979. The energy for the volcanic activity comes from the squeezing and stretching of the moon by Jupiter's gravity as Io orbits the immense planet, the largest in the solar system.

Galileo was launched in 1989 and began orbiting Jupiter in 1995. After a successful mission, the spacecraft was intentionally sent into Jupiter's atmosphere in 2003. The unexplained signatures appeared in the magnetic-field data taken from Galileo fly-bys of Io in October 1999 and February 2000, during the final phase of the mission.

"But at the time, models of the interaction between Io and Jupiter's immense magnetic field, which bathes the moon in charged particles, were not yet sophisticated enough for us to understand what was going on in Io's interior," said study co-author Xianzhe Jia of the University of Michigan.

Recent work in mineral physics showed that a group of what are known as "ultramafic" rocks become capable of carrying substantial electrical current when melted. These rocks are igneous in origin -- that is, they are formed through the cooling of magma. On Earth, ultramafic rocks are believed to derive from the mantle. The finding led Khurana and colleagues to test the hypothesis that the strange signature was produced by an electrical current flowing in a molten or partially molten layer of this kind of rock.

Tests showed that the signatures detected by Galileo were consistent with a rock like lherzolite, an igneous rock rich in silicates of magnesium and iron found, for example, in Spitzbergen, Norway. The magma ocean layer on Io appears to be more than 30 miles (50 km) thick, making up at least 10 percent of the moon's mantle by volume. The blistering temperature of the magma ocean probably exceeds 2,200 degrees Fahrenheit (1,200 degrees Celsius).

Additional co-authors on the paper are Christopher T. Russell, professor of geophysics and space physics in UCLA's Department of Earth and Space Sciences; Margaret Kivelson, professor emeritus of space physics in UCLA's Department of Earth and Space Sciences; Gerald Schubert, professor of geophysics and planetary physics in UCLA's Department of Earth and Space Sciences; and Francis Nimmo, associate professor of Earth and planetary sciences at UC Santa Cruz.

The Galileo mission was managed by the Jet Propulsion Laboratory (JPL), a division of the California Institute of Technology in Pasadena, for NASA.

Story Source:

The above story is reprinted (with editorial adaptations by ScienceDaily staff) from materials provided by University of California - Los Angeles. The original article was written by Jia-Rui Cook.

Journal Reference:

Krishan K. Khurana, Xianzhe Jia, Margaret G. Kivelson, Francis Nimmo, Gerald Schubert, Christopher T. Russell. Evidence of a Global Magma Ocean in Io’s Interior. Science, 2011; DOI: 10.1126/science.1201425

Note: If no author is given, the source is cited instead.

Disclaimer: Views expressed in this article do not necessarily reflect those of ScienceDaily or its staff.


View the original article here