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The Moon was once thought to be depleted in volatile elements. Analyses of the carbon contents of lunar volcanic glasses reveal that carbon monoxide degassing could have produced the fire-fountain eruptions from which these glasses were formed.
Evidence for a Neoproterozoic Snowball Earth in the sedimentary record has been controversial. A weathered horizon preserved in sedimentary rocks from Svalbard may provide a rare signature of prolonged global glaciation.
Braided channels are rare on ocean floors, but abundant on land. Experiments and theory suggest that deeper flows and rapid overbank deposition restrict braiding in underwater rivers relative to their terrestrial counterparts.
Saturn's F ring is chaperoned on both sides by the tiny moons Prometheus and Pandora. Numerical simulations show that this celestial ballet can result from the collision of two aggregates that evolved out of Saturn's main rings.
Tropospheric ozone is generated from precursor pollutants, but can be blown far afield. Satellite observations show rising ozone levels over China — and almost stable levels over western North America despite stricter regulations.
On 25 April 2015 northern Nepal shifted up to 7 m southward and Kathmandu was raised by 1 m. The causal earthquake failed to fully rupture the main fault beneath the Himalaya and hence a large earthquake appears to be inevitable in Nepal's future.
Antarctic Ice Sheet change during the last glacial cycle is unclear. The timing of moraine development in the Ross basin suggests that the ice sheet reached maximum thickness under the warming temperatures of the last termination.
Anthropogenic climate change alters the risk of some extreme weather events. High-resolution computer simulations suggest that Black Sea warming made the devastating 2012 Krymsk flood possible — a virtually impossible event just 30 years ago.
The ocean is an important source of the potent greenhouse gas N2O. Measurements in the tropical South Pacific have revealed a massive efflux of N2O from the coastal upwelling zone.
Earth's crust was thought to deform uniformly over most of the seismic cycle. Analysis of two centuries of nautical surveys from Chile reveals temporal variability that complicates our view of time-dependent seismic hazards.
The continents are archives of Earth's evolution. Analysis of the isotopic signature of continental crust globally suggests that buoyant, silicic continents began to form 3 billion years ago, possibly linked to the onset of plate tectonics.
Saturn's poles exhibit giant swirling cyclones, whereas Jupiter's poles may not. Simulations of giant planet atmospheres suggest that just the right balance of convective storm energy and poleward drift of cyclones may explain Saturn's vortices.
The Earth's long-term silica cycle is intimately linked to weathering rates and biogenic uptake. Changes in weathering rates and the retention of silica on land have altered silica availability in the oceans for hundreds of millions of years.
Global surface warming has slowed since the start of the twenty-first century, while Pacific heat uptake was enhanced. Analyses of ocean heat content suggest that the warm water was transferred to the Indian Ocean, through the Indonesian straits.
An ancient carbon release resulted in widespread dissolution of carbonates at the sea floor. Numerical simulations suggest that the pattern of dissolution can be explained by a top-down invasion of corrosive bottom waters from the North Atlantic.
It is intuitive, but evidence that high levels of precipitation increase erosion rates has been elusive. The ages of exposed porphyry copper deposits reveal that rocks emplaced at depth travel to the surface faster where precipitation rates are high.
The Indian Plate moved north unusually quickly during the late Cretaceous. Numerical simulations suggest that this rapid migration was caused by the pull of two coupled, narrowing subduction zones.