In a paper published today in Nature Physics, a research team from Lawrence Livermore National Laboratory (LLNL), the University of California, Berkeley and the University of Rochester provides experimental evidence for superionic conduction in water ice
at planetary interior conditions, verifying the 30 - year - old prediction.
Not exact matches
«For the first time, we have used a geophysical method to determine the internal structure of Enceladus, and the data suggest that indeed there is a large, possibly regional ocean about 50 kilometers below the surface of the south pole,» says David Stevenson, the Marvin L. Goldberger Professor of
Planetary Science at Caltech and an expert in studies of the interior of planetar
Planetary Science
at Caltech and an expert in studies of the
interior of
planetaryplanetary bodies.
Swirling winds blustering
at more than 1,000 miles per hour, along with heat rising from the
planetary interior, create the gold and yellow atmospheric bands.
«The answer is neither,» says David Stevenson, a
planetary scientist
at the California Institute of Technology who leads the Juno team studying the planet's
interior.
Heat from the impact that made Occator probably allowed a mixture of ice, salts, and rock in Ceres's
interior to become more fluid and rise up to the surface, scientists reported today
at the Lunar and
Planetary Science Conference in The Woodlands, Texas.
In the simulation, the Earth's
interior was too hot and runny
at first to push around the giant chunks of crust, researchers report in the June Physics of the Earth and
Planetary Interiors.
«Magnetic fields provide crucial information about the
interiors and evolution of planets, so it is gratifying that our experiments can test — and in fact, support — the thin - dynamo idea that had been proposed for explaining the truly strange magnetic fields of Uranus and Neptune,» said Raymond Jeanloz, co-author on the paper and professor in Earth &
Planetary Physics and Astronomy
at the University of California, Berkeley.
But how such ice would be formed
at the temperatures found in
planetary interiors has remained mysterious.
All we can really say
at the moment is that the plateau rocks look different from elsewhere,» says Nils Müller
at the Joint
Planetary Interior Physics Research Group of the University Münster and DLR Berlin, who headed the mapping efforts.
He served as professor of environmental sciences
at the University of Virginia, Charlottesville, VA (1971 — 94); distinguished research professor
at the Institute for Space Science and Technology, Gainesville, FL (1989 — 94); chief scientist, U.S. Department of Transportation (1987 — 89); vice chairman of the National Advisory Committee for Oceans and Atmosphere (NACOA)(1981 — 86); deputy assistant administrator for policy, U.S. Environmental Protection Agency (1970 — 71); deputy assistant secretary for water quality and research, U.S. Department of the
Interior (1967 — 70); founding dean of the School of Environmental and
Planetary Sciences, University of Miami (1964 — 67); first director of the National Weather Satellite Service (1962 — 64); and director of the Center for Atmospheric and Space Physics, University of Maryland (1953 — 62).