Olivine water contents in the continental lithosphere and the longevity of cratons

Nature ◽  
2010 ◽  
Vol 467 (7311) ◽  
pp. 78-81 ◽  
Author(s):  
Anne H. Peslier ◽  
Alan B. Woodland ◽  
David R. Bell ◽  
Marina Lazarov
Author(s):  
Jens Konnerup-Madsen

NOTE: This article was published in a former series of GEUS Bulletin. Please use the original series name when citing this article, for example: Konnerup-Madsen, J. (2001). A review of the composition and evolution of hydrocarbon gases during solidification of the Ilímaussaq alkaline complex, South Greenland. Geology of Greenland Survey Bulletin, 190, 159-166. https://doi.org/10.34194/ggub.v190.5187 _______________ Fluid inclusions in minerals from agpaitic nepheline syenites and hydrothermal veins in the Ilímaussaq complex and in similar agpaitic complexes on the Kola Peninsula, Russia, are dominated by hydrocarbon gases (predominantly methane) and hydrogen. Such volatile compositions differ considerably from those of most other igneous rocks and their formation and entrapment in minerals reflects low oxygen fugacities and a wide range of crystallisation temperatures extending to a low-temperature solidus. Their composition reflects initial low carbon contents and high water contents of the magma resulting in the exsolution of a waterrich CO2–H2O dominated vapour phase. Fractionation of chlorides into the vapour phase results in high salinities and the subsequent development of a heterogeneous vapour phase with a highly saline aqueous-rich fraction and a methane-dominated fraction, with preferential entrapment of the latter, possibly due to different wetting characteristics. The light stable isotope compositions support an abiogenic origin for the hydrocarbons in agpaitic nepheline syenite complexes.


1990 ◽  
Vol 54 (2) ◽  
pp. 555-557 ◽  
Author(s):  
Ralph G. Nash ◽  
M. Leroy Beall
Keyword(s):  

2017 ◽  
Author(s):  
Adam Nordling ◽  
◽  
Elizabeth McTaggart ◽  
Elizabeth A. Johnson ◽  
Madison L. Myers ◽  
...  
Keyword(s):  

2017 ◽  
Author(s):  
Elizabeth McTaggart ◽  
◽  
Adam Nordling ◽  
Elizabeth A. Johnson ◽  
Madison L. Myers ◽  
...  

2020 ◽  
Author(s):  
Julia Chen ◽  
◽  
Barbara Ratschbacher ◽  
Barbara Ratschbacher ◽  
Claire E. Bucholz ◽  
...  

Author(s):  
Karel Schrijver

This chapter describes how the first found exoplanets presented puzzles: they orbited where they should not have formed or where they could not have survived the death of their stars. The Solar System had its own puzzles to add: Mars is smaller than expected, while Venus, Earth, and Mars had more water—at least at one time—than could be understood. This chapter shows how astronomers worked through the combination of these puzzles: now we appreciate that planets can change their orbits, scatter water-bearing asteroids about, steal material from growing planets, or team up with other planets to stabilize their future. The special history of Jupiter and Saturn as a pair bringing both destruction and water to Earth emerged from the study of seventeenth-century resonant clocks, from the water contents of asteroids, and from experiments with supercomputers imposing the laws of physics on virtual worlds.


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