2015Unpublished venueRequires access

Formation of hydrogen gas and alkane during peridotite serpentinization

Gh Zhang, Bx Han, Ruifang Huang, Zhongyue Zhou, X. Y. Bi, Sh Dai, Sun Wei-dong, Wei Ming Huang, Dh Chen, Xing Ding, Xin Wang, Liu Jiqiang, Sheng Gy, Fu Jm, Wenhuan Zhan

Open publisher page 2 citations

Abstract

Serpentinization potentially contributes to the origin and evolution of life during early history of Earth and other planets, indicated by biological activities in hydrothermal fields those are supplied with hydrogen gas, alkanes and organic acids produced during serpentinization. Previous studies have been investigated on olivine serpentinization, and temperatures and pressures were very limited (<= 300 degrees C, 500bar). Here, we performed a series of hydrothermal experiments at 300 similar to 500 degrees C and 1 similar to 3kbar to explore the formation of hydrogen gas and alkanes during serpentinization of olivine, orthopyroxene, clinopyroxene, peridotite, basalt, and mixtures of peridotite and basalt. At 300 degrees C and 3kbar, the quantity of hydrogen gas after olivine serpentinization is much higher than that after pyroxene alteration. As temperatures increase, e. g., at 400 similar to 500 degrees C and 3kbar, the amount of hydrogen gas after olivine alteration is much lower due to its sluggish alteration rate, which is slightly less than that after orthopyroxene serpentinization. Clinopyroxene is completely unaltered after experiments, and therefore no hydrogen gas and alkanes are produced. Compared to peridotite, the quantity of hydrogen gas after olivine and orthopyroxene at 400 similar to 500 degrees C is identical, while the amounts of alkanes are much less. The quantities of hydrogen gas and alkane during basalt alteration are comparable with those after hydration of mixtures of basalt and peridotite, but they are much lower than those after peridotite alteration. This is mainly due to production of Fe2+ -rich diopside (similar to 8. 1% FeO) after basalt alteration, which dramatically reduces the amount of Fe3+ and consequently hydrogen gas. This study suggests that olivine and pyroxene cannot completely represent peridotite for the formation of hydrogen gas and alkanes during serpentinization. Moreover, hydrogen gas and alkane are produced not only after serpentinization of abyssal peridotite, which could be also formed during hydration of oceanic crust in subduction zones. However, the amounts of hydrogen and alkane during hydration of oceanic crust should be very low due to incorporation of basalt.

About this research paper

What this paper is about

Serpentinization potentially contributes to the origin and evolution of life during early history of Earth and other planets, indicated by biological activities in hydrothermal fields those are supplied with hydrogen gas, alkanes and organic acids produced during serpentinization. Previous studies have been investigated on olivine serpentinization, and temperatures and pressures were very limited (<= 300 degrees C, 500bar). Here, we performed a series of hydrothermal experiments at 300 similar to 500 degrees C and 1 similar to 3kbar to explore the formation of hydrogen gas and alkanes during serpentinization of olivine, orthopyroxene, clinopyroxene, peridotite, basalt, and mixtures of peridotite and basalt. At 300 degrees C and 3kbar, the quantity of hydrogen gas after olivine serpentinization is much higher than that after pyroxene alteration. As temperatures increase, e. g., at 400 similar to 500 degrees C and 3kbar, the amount of hydrogen gas after olivine alteration is much lower due to its sluggish alteration rate, which is slightly less than that after orthopyroxene serpentinization. Clinopyroxene is completely unaltered after experiments, and therefore no hydrogen gas and alkanes are produced. Compared to peridotite, the quantity of hydrogen gas after olivine and orthopyroxene at 400 similar to 500 degrees C is identical, while the amounts of alkanes are much less. The quantities of hydrogen gas and alkane during basalt alteration are comparable with those after hydration of mixtures of basalt and peridotite, but they are much lower than those after peridotite alteration. This is mainly due to production of Fe2+ -rich diopside (similar to 8. 1% FeO) after basalt alteration, which dramatically reduces the amount of Fe3+ and consequently hydrogen gas. This study suggests that olivine and pyroxene cannot completely represent peridotite for the formation of hydrogen gas and alkanes during serpentinization. Moreover, hydrogen gas and alkane are produced not only after serpentinization of abyssal peridotite, which could be also formed during hydration of oceanic crust in subduction zones. However, the amounts of hydrogen and alkane during hydration of oceanic crust should be very low due to incorporation of basalt.

Why it matters

OpenAlex reports 2 citations for this work. Citation counts describe recorded attention and do not establish research quality.

Key contribution

A contribution statement is not available in the OpenAlex record.

Method / approach

Method details are not available in the OpenAlex metadata.

Main findings

Findings are not separately available in the OpenAlex metadata.

Limitations

Limitations are not available in the OpenAlex metadata.

Applications

Application details are not available in the OpenAlex metadata.

Available abstract

Serpentinization potentially contributes to the origin and evolution of life during early history of Earth and other planets, indicated by biological activities in hydrothermal fields those are supplied with hydrogen gas, alkanes and organic acids produced during serpentinization. Previous studies have been investigated on olivine serpentinization, and temperatures and pressures were very limited (<= 300 degrees C, 500bar). Here, we performed a series of hydrothermal experiments at 300 similar to 500 degrees C and 1 similar to 3kbar to explore the formation of hydrogen gas and alkanes during serpentinization of olivine, orthopyroxene, clinopyroxene, peridotite, basalt, and mixtures of peridotite and basalt. At 300 degrees C and 3kbar, the quantity of hydrogen gas after olivine serpentinization is much higher than that after pyroxene alteration. As temperatures increase, e. g., at 400 similar to 500 degrees C and 3kbar, the amount of hydrogen gas after olivine alteration is much lower due to its sluggish alteration rate, which is slightly less than that after orthopyroxene serpentinization. Clinopyroxene is completely unaltered after experiments, and therefore no hydrogen gas and alkanes are produced. Compared to peridotite, the quantity of hydrogen gas after olivine and orthopyroxene at 400 similar to 500 degrees C is identical, while the amounts of alkanes are much less. The quantities of hydrogen gas and alkane during basalt alteration are comparable with those after hydration of mixtures of basalt and peridotite, but they are much lower than those after peridotite alteration. This is mainly due to production of Fe2+ -rich diopside (similar to 8. 1% FeO) after basalt alteration, which dramatically reduces the amount of Fe3+ and consequently hydrogen gas. This study suggests that olivine and pyroxene cannot completely represent peridotite for the formation of hydrogen gas and alkanes during serpentinization. Moreover, hydrogen gas and alkane are produced not only after serpentinization of abyssal peridotite, which could be also formed during hydration of oceanic crust in subduction zones. However, the amounts of hydrogen and alkane during hydration of oceanic crust should be very low due to incorporation of basalt.

Key concepts: Peridotite, Olivine, Basalt, Geology, Hydrogen, Geochemistry, Pyroxene, Alkane

Related papers

Back to paper searchBrowse research topicsOriginal source
Formation of hydrogen gas and alkane during peridotite serpentinization — Research Paper | ScholarLens