Organic synthesis during fluid mixing in hydrothermal systems

被引:197
作者
Shock, EL [1 ]
Schulte, MD [1 ]
机构
[1] Washington Univ, Dept Earth & Planetary Sci, McDonnell Ctr Space Sci, GEOPIG, St Louis, MO 63130 USA
关键词
D O I
10.1029/98JE02142
中图分类号
P3 [地球物理学]; P59 [地球化学];
学科分类号
0708 ; 070902 ;
摘要
Hydrothermal circulation can lead to fluid mixing on any planet with liquid water and a source of heat. Aqueous fluids with differing compositions, especially different oxidation states, are likely to be far from thermodynamic equilibrium when they mix, and provide a source of free energy that can drive organic synthesis from CO2 and H-2, and/or supply a source of geochemical energy-to chemolithoautotrophic organisms. Results are presented that quantify the potential for organic synthesis during unbuffered fluid mixing in present submarine hydrothermal systems, as well as hypothetical systems that may have existed on the early Earth and Mars. Dissolved hydrogen, present in submarine hydrothermal fluids owing to the high-temperature reduction of H2O as seawater reacts with oceanic crustal rocks, provides the reduction potential and the thermodynamic drive for organic synthesis from CO, (or bicarbonate) as hydrothermal fluids mix with seawater. The potential for organic synthesis is a strong function of the H-2 content of the hydrothermal fluid, which is, in turn, a function of the prevailing oxidation state controlled by the composition of the rock that hosts the hydrothermal system. Hydrothermal fluids with initial oxidation states at or below those set by the fayalite-magnetite-quartz mineral assemblage show the greatest potential for driving organic synthesis. These calculations show that it is thermodynamically possible for 100% of the carbon in the mixed fluid to be reduced to a mixture of carboxylic acids, alcohols, and ketone in the range 250-50 degrees C as cold seawater mixes with the hydrothermal fluid. As the temperature drops, larger organic molecules are favored, which implies that fluid mixing could drive the geochemical equivalent of a metabolic system. This enormous reduction potential probably drives a large portion of the primary productivity around present seafloor hydrothermal vents and would have been present in hydrothermal systems on the early Earth or Mars. The single largest control on the potential for organic synthesis is the composition of the rock that hosts the hydrothermal system.
引用
收藏
页码:28513 / 28527
页数:15
相关论文
共 88 条
[11]   A MODEL FOR THE HYDROLOGIC AND CLIMATIC BEHAVIOR OF WATER ON MARS [J].
CLIFFORD, SM .
JOURNAL OF GEOPHYSICAL RESEARCH-PLANETS, 1993, 98 (E6) :10973-11016
[12]  
Corliss J. B., 1981, Oceanologica Acta, V4, P59
[13]  
FRENCH BM, 1964, THESIS J HOPKINS U B
[14]   A GEOCHEMICAL MODEL FOR THE FORMATION OF HYDROTHERMAL CARBONATES ON MARS [J].
GRIFFITH, LL ;
SHOCK, EL .
NATURE, 1995, 377 (6548) :406-408
[15]   Hydrothermal hydration of martin crust: Illustration via geochemical model calculations [J].
Griffith, LL ;
Shock, EL .
JOURNAL OF GEOPHYSICAL RESEARCH-PLANETS, 1997, 102 (E4) :9135-9143
[16]   NEW CONSTRAINTS ON PRECAMBRIAN OCEAN COMPOSITION [J].
GROTZINGER, JP ;
KASTING, JF .
JOURNAL OF GEOLOGY, 1993, 101 (02) :235-243
[17]   HOT-SPRING DEPOSITS ON THE EAST PACIFIC RISE AT 21-DEGREES-N - PRELIMINARY DESCRIPTION OF MINERALOGY AND GENESIS [J].
HAYMON, RM ;
KASTNER, M .
EARTH AND PLANETARY SCIENCE LETTERS, 1981, 53 (03) :363-381
[18]   PETROLEUM, OIL-FIELD WATERS, AND AUTHIGENIC MINERAL ASSEMBLAGES - ARE THEY IN METASTABLE EQUILIBRIUM IN HYDROCARBON RESERVOIRS [J].
HELGESON, HC ;
KNOX, AM ;
OWENS, CE ;
SHOCK, EL .
GEOCHIMICA ET COSMOCHIMICA ACTA, 1993, 57 (14) :3295-3339
[19]   THERMODYNAMICS OF HYDROTHERMAL SYSTEMS AT ELEVATED TEMPERATURES AND PRESSURES [J].
HELGESON, HC .
AMERICAN JOURNAL OF SCIENCE, 1969, 267 (07) :729-&
[20]  
HELGESON HC, 1978, AM J SCI, V278, P1