The Nature of Reduction in Space Weathering

Details The Nature of Reduction in Space Weathering The Nature of Reduction in Space Weathering

Jul 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993metic..28r.394m&link_type=abstract

Meteoritics, vol. 28, no. 3, volume 28, page 394

Computer Science

2

Agglutinates, Iron-Nickel, Regolith, Weathering

Scientific paper

Space weathering is a broad term that includes a number of complex effects of the exposure of materials to the environment of space. The processes that drive space weathering include micrometeorite impact, radiation from the Sun and cosmic rays, and exposure to the vacuum of space. One of the important effects caused by these processes is the tendency for chemical reduction of oxide and silicate materials (including glasses), with accompanying loss of oxygen and production of reduced metal. Such chemical reduction and accompanying metal production may have an important influence on the chemistry of the outermost volume of individual grains as well as on the optical properties of this material. Hapke [1] discussed five processes that have been suggested for producing submicroscopic iron metal in the lunar soil: (1) shock reduction, (2) heating in a thermal blanket in vacuum, (3) shock heating of solar-wind-impregnated grains, (4) coatings deposited by solar wind sputtering, and (5) coatings deposited by impact vaporization. As noted by Hapke, "Processes (1) and (2) have been refuted by laboratory experiments. Processes (4) and (5) have produced submicroscopic iron metal in laboratory simulations. Although no experiments have been done to simulate process (3), it is widely accepted." We have been performing experimental reduction of simulated and actual lunar materials [2-5] and have shown that, under conditions of exposure to hydrogen at elevated temperatures, reduction of FeO readily occurs in ilmenite and lunar composition glass, and occurs at a slower rate in pyroxene and olivine. Even plagioclase feldspar containing minor FeO is readily reduced with formation of metallic iron blebs on surfaces [4]. A comparison of natural lunar samples to hydrogen-reduced samples or simulants in which we are searching for reduction evidence in various soil phases is underway. Preliminary data for mature soils show, in agreement with earlier results, that reduced iron produced in the regolith is most commonly formed in agglutinitic glass rather than in minerals including ilmenite, even though experimental reduction of ilmenite occurs as rapidly, if not more so, than reduction of FeO in glass. Several explanations are possible. Ilmenite may melt and dissolve readily into the impact-formed melt, providing FeO to the glass. Then the reduced iron is derived from the melt rather than from the mineral. Relic reduced ilmenite grains, similar to experimentally reduced ilmenites, therefore may not normally be formed. Second, similar to the process for making impact breccias as proposed by Simonds et al. [6], the impact process may tend to completely melt everything within a small volume, including iron-bearing minerals such as ilmenite and pyroxene. This superheated volume is partially reduced almost instantly by included solar wind hydrogen or carbon as summarized in Hapke [1], forming abundant metallic iron blebs. Then this melted volume encounters cold mineral and lithic grains and incorporates them as clasts, chilling rapidly without heating the clasts sufficiently to produce significant reduction. This explanation seems to better fit the observation that apparently totally unreduced ilmenite clasts are found in glass containing abundant reduced iron. Implications for space weathering are that reduction mainly occurs in melting processes (and also in vaporization processes [7]), but that solid-state reduction may be rare in micrometeorite impact-driven processes. However, impact-driven reduction from events larger than micrometeorite impacts may still provide elevated temperatures over a long enough time span to drive solid-state reduction. Solid-state reduction produced by shock effects has also been proposed to explain metal blebs in plagioclase [8]. While hydrogen is usually cited as the main reducing agent in the lunar regolith, we note that recent analyses of interplanetary dust particles show carbon contents of up to 40% by weight [9]; such particles added to the regolith may supply abundant carbon for supporting space weathering reduction processes during impacts. References: [1] Hapke B. (1993) LPI Tech. Rpt. 93-01, 8-9. [2] Allen C. C. et al. (1992) In Engineering, Construction, and Operations in Space III, 629-640, Am. Soc. Civil Engineers, New York. [3] Allen C. C. et al. (1992) LPS XXIII, 21-22. [4] Allen C. C. et al. (1993) Icarus, submitted. [5] Allen C. C. et al. (1993) LPS XXIV, 19-20. [6] Simonds C. H. et al. (1976) Proc. LSC 7th, 2509-2528. [7] Keller L. P. and McKay D. S. (1992) LPS XXIll, 673-674. [8] Sclar C. B. and Bauer J. F. (1976) Proc. LSC 7th, 2493-2508. [9] Thomas K. L. et al. (1993) GCA, in press.

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