Wednesday, January 4, 2017

Nature Geoscience contents: January 2017 Volume 10 Number 1 pp1-68

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TABLE OF CONTENTS

January 2017 Volume 10, Issue 1

Editorial
News and Views
Articles
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Editorial

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More space for space   p1
doi:10.1038/ngeo2874
Born from astronomy, the study of planets is becoming increasingly geoscience. As divisions between disciplines continue to blur in Solar System studies, at Nature Geoscience we are looking forward to exciting joint projects with Nature Astronomy.

News and Views

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Carbon cycle: New pathways in the sand   pp3 - 4
Alexandra Rao
doi:10.1038/ngeo2855
Organic carbon decomposition in anoxic marine sediments was thought to be dominated by bacteria, but experimental data and microbial culture studies now show that microalgae buried in coastal sands may also play an important role in carbon turnover.
See also: Article by Bourke et al.

Plate tectonics: A supercontinental boost   pp4 - 5
Adrian Lenardic
doi:10.1038/ngeo2862
180 million years ago Earth's continents were amalgamated into one supercontinent called Pangaea. Analysis of oceanic crust formed since that time suggests that the cooling rate of Earth was enhanced in the wake of Pangaea's dispersal.
See also: Article by Van Avendonk et al.

Mark pagani: Carbon and ancient climates   p6
Jessica E. Tierney & Katherine H. Freeman
doi:10.1038/ngeo2867

Palaeoclimate: Climate's playground   pp7 - 8
Nerilie J. Abram
doi:10.1038/ngeo2856
Abrupt climate changes in the glacial North Atlantic altered the position of wind systems in the Northern Hemisphere and tropics. Ice-core data show that this disruption also reached the southern westerlies.
See also: Article by Markle et al.

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Articles

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Silicate mineralogy at the surface of Mercury   pp9 - 13
Olivier Namur & Bernard Charlier
doi:10.1038/ngeo2860
The MESSENGER spacecraft has revealed geochemical diversity across Mercury's surface. Magma crystallization experiments suggest a crustal mineralogy consistent with a transition towards shallower and cooler mantle melting conditions.

Evidence for an early wet Moon from experimental crystallization of the lunar magma ocean   pp14 - 18
Yanhao Lin, Elodie J. Tronche, Edgar S. Steenstra & Wim van Westrenen
doi:10.1038/ngeo2845
The Moon is thought to have initially had a magma ocean that gradually solidified. Crystallization experiments find that the resulting crustal thickness depends on water content and is consistent with significant water in the early Moon.

Competitive fitness of a predominant pelagic calcifier impaired by ocean acidification   pp19 - 23
Ulf Riebesell, Lennart T. Bach, Richard G. J. Bellerby, J. Rafael Bermúdez Monsalve, Tim Boxhammer et al.
doi:10.1038/ngeo2854
Ocean acidification can affect growth and calcification rates of calcifying phytoplankton. Mesocosm experiments reveal that acidification can also cause declines in population size and inhibit bloom formation.

N2 production rates limited by nitrite availability in the Bay of Bengal oxygen minimum zone   pp24 - 29
L. A. Bristow, C. M. Callbeck, M. Larsen, M. A. Altabet, J. Dekaezemacker et al.
doi:10.1038/ngeo2847
Nitrogen losses have not been observed in the Bay of Bengal, unlike in other ocean oxygen minimum zones. Chemical and molecular analyses reveal that trace levels of oxygen inhibit nitrate formation, largely preventing microbial N2 production.

Metabolism in anoxic permeable sediments is dominated by eukaryotic dark fermentation   pp30 - 35
Michael F. Bourke, Philip J. Marriott, Ronnie N. Glud, Harald Hasler-Sheetal, Manoj Kamalanathan et al.
doi:10.1038/ngeo2843
Bacteria have been assumed to dominate organic matter decomposition in marine sediments. In flow-through reactor experiments, algae were revealed to be primarily responsible for anaerobically metabolizing organic matter in permeable sediments.
See also: News and Views by Rao

Global atmospheric teleconnections during Dansgaard–Oeschger events   pp36 - 40
Bradley R. Markle, Eric J. Steig, Christo Buizert, Spruce W. Schoenemann, Cecilia M. Bitz et al.
doi:10.1038/ngeo2848
Abrupt glacial climate changes were slowly communicated between hemispheres by oceanic heat transport. Ice core data point to more rapid atmospheric teleconnections linking the North Atlantic, tropics, and southern storm track.
See also: News and Views by Abram

Constraints on ocean carbonate chemistry and pCO2 in the Archaean and Palaeoproterozoic   pp41 - 45
C. L. Blättler, L. R. Kump, W. W. Fischer, G. Paris, J. J. Kasbohm et al.
doi:10.1038/ngeo2844
The composition of the oceans on early Earth has been challenging to assess. Calcium isotope records from carbonate rocks formed 1.9 to 2.7 billion years ago rule out high alkalinity, and are consistent with moderate to high CO2 concentrations.

Metamorphic record of catastrophic pressure drops in subduction zones   pp46 - 50
P. Yamato & J. P. Brun
doi:10.1038/ngeo2852
Rocks are altered by high pressure during subduction. Analysis of exhumed metamorphic rocks suggests that the peak pressures recorded within minerals mark a change in tectonic regime within a subduction zone, rather than burial depth.

Subduction megathrust creep governed by pressure solution and frictional–viscous flow   pp51 - 57
Åke Fagereng & Sabine A. M. den Hartog
doi:10.1038/ngeo2857
The controls on fast versus slow fault slip in subduction zones are unclear. Rock deformation experiments suggest that faults within the seismogenic region of a subduction zone may slip aseismically due to pressure solution creep.

Decrease in oceanic crustal thickness since the breakup of Pangaea   pp58 - 61
Harm J. A. Van Avendonk, Joshua K. Davis, Jennifer L. Harding & Lawrence A. Lawver
doi:10.1038/ngeo2849
Thicker oceanic crust forms from a hot mantle. Observations of unusually thick oceanic crust that formed 170 million years ago in the Atlantic and Indian oceans suggest that the ancient supercontinent Pangaea helped insulate and warm the mantle.
See also: News and Views by Lenardic

An accelerating high-latitude jet in Earth's core   pp62 - 68
Philip W. Livermore, Rainer Hollerbach & Christopher C. Finlay
doi:10.1038/ngeo2859
Satellite observations have detected localized magnetic field changes at high latitudes. Simulations suggest these changes can be explained by a westward jet in the liquid core, which has been accelerating over the past 15 years.

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