Notice: This is an archived and unmaintained page. For current information, please browse astrobiology.nasa.gov.

2010 Annual Science Report

University of Hawaii, Manoa Reporting  |  SEP 2009 – AUG 2010

Hydrogen in Nominally Anhydrous Minerals

Project Summary

The amount of water in the Earth’s interior is not known. Experiments have shown that at high pressure, the high-pressure forms of the minerals that make up the Earth’s mantle can contain significant hydrogen substituting for magnesium. We are carrying out a series of experiments to determine how much hydrogen (=water) can be contained in these high-pressure minerals. Mineral samples produced at mantle pressures in the presence of water are being measured using the Cameca ims 1280 ion microprobe at the Unversity of Hawaii to determine the maximum amount of water that each mineral can hold at high pressure, providing a constraint on the possible water content of the mantle.

4 Institutions
3 Teams
1 Publication
0 Field Sites
Field Sites

Project Progress

We have synthesized hydrous peridotite-composition samples at 13GPa and 1400°C with co-existing coarse grains (~100 micrometer) of olivine, wadsleyite, clinoenstatite, and melt in a multi-anvil press. The olivine grains contain fine-scale lamellae of wadsleyite and clinoenstatite that likely resulted from small temperature fluctuations during the four-hour experiment. Major-element compositions were determined by electron microprobe and H contents by secondary ion mass spectroscopy (SIMS). The olivine is about Fo93 in composition and contains about 650 ppm by weight H2O. The wadsleyite is about Fo87 in composition and contains about 1650 ppm H2O. The clinoenstatite is about En93 in composition and about 440 ppm H2O. High resolution transmission electron microscopy of the lamellae and host show that the olivine and wadsleyite share their close-packed oxygen planes so that the wadsleyite lamellae are nearly planar and perpendicular to the [1 0 0] of olivine. The wadsleyite lamellae thus have their [1 0 1] and [1 0 -1] directions parallel to the [1 0 0] of olivine. Additionally, a second orientation relation with the [001] of olivine parallel to [100] of wadsleyite is also found as are incoherent blebs of wadsleyite in olivine. The coexisting melt phase quenched to a feathery mass of mostly wadsleyite crystals. Neither a quenched glass phase nor a nominally hydrous phase was observed.

  • PROJECT INVESTIGATORS:
    Gary Huss Gary Huss
    Unspecified Role
    Joseph Smyth
    Unspecified Role
  • RELATED OBJECTIVES:
    Objective 1.1
    Formation and evolution of habitable planets.