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The Fe–C–O–H–N system at 6.3–7.8 GPa and 1200–1400 °C : implications for deep carbon and nitrogen cycles. / Sokol, Alexander G.; Tomilenko, Anatoly A.; Bul’bak, Taras A. и др.

в: Contributions to Mineralogy and Petrology, Том 173, № 6, 47, 01.06.2018.

Результаты исследований: Научные публикации в периодических изданияхстатьяРецензирование

Harvard

Sokol, AG, Tomilenko, AA, Bul’bak, TA, Kruk, AN, Zaikin, PA, Sokol, IA, Seryotkin, YV & Palyanov, YN 2018, 'The Fe–C–O–H–N system at 6.3–7.8 GPa and 1200–1400 °C: implications for deep carbon and nitrogen cycles', Contributions to Mineralogy and Petrology, Том. 173, № 6, 47. https://doi.org/10.1007/s00410-018-1472-3

APA

Sokol, A. G., Tomilenko, A. A., Bul’bak, T. A., Kruk, A. N., Zaikin, P. A., Sokol, I. A., Seryotkin, Y. V., & Palyanov, Y. N. (2018). The Fe–C–O–H–N system at 6.3–7.8 GPa and 1200–1400 °C: implications for deep carbon and nitrogen cycles. Contributions to Mineralogy and Petrology, 173(6), [47]. https://doi.org/10.1007/s00410-018-1472-3

Vancouver

Sokol AG, Tomilenko AA, Bul’bak TA, Kruk AN, Zaikin PA, Sokol IA и др. The Fe–C–O–H–N system at 6.3–7.8 GPa and 1200–1400 °C: implications for deep carbon and nitrogen cycles. Contributions to Mineralogy and Petrology. 2018 июнь 1;173(6):47. doi: 10.1007/s00410-018-1472-3

Author

Sokol, Alexander G. ; Tomilenko, Anatoly A. ; Bul’bak, Taras A. и др. / The Fe–C–O–H–N system at 6.3–7.8 GPa and 1200–1400 °C : implications for deep carbon and nitrogen cycles. в: Contributions to Mineralogy and Petrology. 2018 ; Том 173, № 6.

BibTeX

@article{ce780b74caf8415e871ae3445b95972e,
title = "The Fe–C–O–H–N system at 6.3–7.8 GPa and 1200–1400 °C: implications for deep carbon and nitrogen cycles",
abstract = "Interactions in a Fe–C–O–H–N system that controls the mobility of siderophile nitrogen and carbon in the Fe0-saturated upper mantle are investigated in experiments at 6.3–7.8 GPa and 1200–1400 °C. The results show that the γ-Fe and metal melt phases equilibrated with the fluid in a system unsaturated with carbon and nitrogen are stable at 1300 °C. The interactions of Fe3C with an N-rich fluid in a graphite-saturated system produce the ε-Fe3N phase (space group P63/mmc or P6322) at subsolidus conditions of 1200–1300 °C, while N-rich melts form at 1400 °C. At IW- and MMO-buffered hydrogen fugacity (fH2), fluids vary from NH3- to H2O-rich compositions (NH3/N2 > 1 in all cases) with relatively high contents of alkanes. The fluid derived from N-poor samples contains less H2O and more carbon which mainly reside in oxygenated hydrocarbons, i.e., alcohols and esters at MMO-buffered fH2 and carboxylic acids at unbuffered fH2 conditions. In unbuffered conditions, N2 is the principal nitrogen host (NH3/N2 ≤ 0.1) in the fluid equilibrated with the metal phase. Relatively C- and N-rich fluids in equilibrium with the metal phase (γ-Fe, melt, or Fe3N) are stable at the upper mantle pressures and temperatures. According to our estimates, the metal/fluid partition coefficient of nitrogen is higher than that of carbon. Thus, nitrogen has a greater affinity for iron than carbon. The general inference is that reduced fluids can successfully transport volatiles from the metal-saturated mantle to metal-free shallow mantle domains. However, nitrogen has a higher affinity for iron and selectively accumulates in the metal phase, while highly mobile carbon resides in the fluid phase. This may be a controlling mechanism of the deep carbon and nitrogen cycles.",
keywords = "Carbon, Fluid, Gas chromatography–mass spectrometry, Hydrocarbons, Mantle, Metal, Nitrogen, TERRESTRIAL CARBON, HIGH-PRESSURE, OXYGEN FUGACITY, EARTHS MANTLE, MAGMA OCEAN, Gas chromatography-mass spectrometry, SILICATE MELTS, METALLIC IRON, CORE FORMATION, PHASE-RELATIONS, DIAMOND CRYSTAL-GROWTH",
author = "Sokol, {Alexander G.} and Tomilenko, {Anatoly A.} and Bul{\textquoteright}bak, {Taras A.} and Kruk, {Alexey N.} and Zaikin, {Pavel A.} and Sokol, {Ivan A.} and Seryotkin, {Yurii V.} and Palyanov, {Yury N.}",
year = "2018",
month = jun,
day = "1",
doi = "10.1007/s00410-018-1472-3",
language = "English",
volume = "173",
journal = "Contributions to Mineralogy and Petrology",
issn = "0010-7999",
publisher = "Springer Nature",
number = "6",

}

RIS

TY - JOUR

T1 - The Fe–C–O–H–N system at 6.3–7.8 GPa and 1200–1400 °C

T2 - implications for deep carbon and nitrogen cycles

AU - Sokol, Alexander G.

AU - Tomilenko, Anatoly A.

AU - Bul’bak, Taras A.

AU - Kruk, Alexey N.

AU - Zaikin, Pavel A.

AU - Sokol, Ivan A.

AU - Seryotkin, Yurii V.

AU - Palyanov, Yury N.

PY - 2018/6/1

Y1 - 2018/6/1

N2 - Interactions in a Fe–C–O–H–N system that controls the mobility of siderophile nitrogen and carbon in the Fe0-saturated upper mantle are investigated in experiments at 6.3–7.8 GPa and 1200–1400 °C. The results show that the γ-Fe and metal melt phases equilibrated with the fluid in a system unsaturated with carbon and nitrogen are stable at 1300 °C. The interactions of Fe3C with an N-rich fluid in a graphite-saturated system produce the ε-Fe3N phase (space group P63/mmc or P6322) at subsolidus conditions of 1200–1300 °C, while N-rich melts form at 1400 °C. At IW- and MMO-buffered hydrogen fugacity (fH2), fluids vary from NH3- to H2O-rich compositions (NH3/N2 > 1 in all cases) with relatively high contents of alkanes. The fluid derived from N-poor samples contains less H2O and more carbon which mainly reside in oxygenated hydrocarbons, i.e., alcohols and esters at MMO-buffered fH2 and carboxylic acids at unbuffered fH2 conditions. In unbuffered conditions, N2 is the principal nitrogen host (NH3/N2 ≤ 0.1) in the fluid equilibrated with the metal phase. Relatively C- and N-rich fluids in equilibrium with the metal phase (γ-Fe, melt, or Fe3N) are stable at the upper mantle pressures and temperatures. According to our estimates, the metal/fluid partition coefficient of nitrogen is higher than that of carbon. Thus, nitrogen has a greater affinity for iron than carbon. The general inference is that reduced fluids can successfully transport volatiles from the metal-saturated mantle to metal-free shallow mantle domains. However, nitrogen has a higher affinity for iron and selectively accumulates in the metal phase, while highly mobile carbon resides in the fluid phase. This may be a controlling mechanism of the deep carbon and nitrogen cycles.

AB - Interactions in a Fe–C–O–H–N system that controls the mobility of siderophile nitrogen and carbon in the Fe0-saturated upper mantle are investigated in experiments at 6.3–7.8 GPa and 1200–1400 °C. The results show that the γ-Fe and metal melt phases equilibrated with the fluid in a system unsaturated with carbon and nitrogen are stable at 1300 °C. The interactions of Fe3C with an N-rich fluid in a graphite-saturated system produce the ε-Fe3N phase (space group P63/mmc or P6322) at subsolidus conditions of 1200–1300 °C, while N-rich melts form at 1400 °C. At IW- and MMO-buffered hydrogen fugacity (fH2), fluids vary from NH3- to H2O-rich compositions (NH3/N2 > 1 in all cases) with relatively high contents of alkanes. The fluid derived from N-poor samples contains less H2O and more carbon which mainly reside in oxygenated hydrocarbons, i.e., alcohols and esters at MMO-buffered fH2 and carboxylic acids at unbuffered fH2 conditions. In unbuffered conditions, N2 is the principal nitrogen host (NH3/N2 ≤ 0.1) in the fluid equilibrated with the metal phase. Relatively C- and N-rich fluids in equilibrium with the metal phase (γ-Fe, melt, or Fe3N) are stable at the upper mantle pressures and temperatures. According to our estimates, the metal/fluid partition coefficient of nitrogen is higher than that of carbon. Thus, nitrogen has a greater affinity for iron than carbon. The general inference is that reduced fluids can successfully transport volatiles from the metal-saturated mantle to metal-free shallow mantle domains. However, nitrogen has a higher affinity for iron and selectively accumulates in the metal phase, while highly mobile carbon resides in the fluid phase. This may be a controlling mechanism of the deep carbon and nitrogen cycles.

KW - Carbon

KW - Fluid

KW - Gas chromatography–mass spectrometry

KW - Hydrocarbons

KW - Mantle

KW - Metal

KW - Nitrogen

KW - TERRESTRIAL CARBON

KW - HIGH-PRESSURE

KW - OXYGEN FUGACITY

KW - EARTHS MANTLE

KW - MAGMA OCEAN

KW - Gas chromatography-mass spectrometry

KW - SILICATE MELTS

KW - METALLIC IRON

KW - CORE FORMATION

KW - PHASE-RELATIONS

KW - DIAMOND CRYSTAL-GROWTH

UR - http://www.scopus.com/inward/record.url?scp=85047405082&partnerID=8YFLogxK

U2 - 10.1007/s00410-018-1472-3

DO - 10.1007/s00410-018-1472-3

M3 - Article

AN - SCOPUS:85047405082

VL - 173

JO - Contributions to Mineralogy and Petrology

JF - Contributions to Mineralogy and Petrology

SN - 0010-7999

IS - 6

M1 - 47

ER -

ID: 13595344