Seismic Evidence for Water Deep in Earth's Upper Mantle

Total Page:16

File Type:pdf, Size:1020Kb

Seismic Evidence for Water Deep in Earth's Upper Mantle R EPORTS million years ago (Ma), subduction mainly took place in the eastern Mediterranean with Seismic Evidence for Water Deep mostly south- and eastward-dipping subduc- tion. Remnants of the subducted slab can be in Earth’s Upper Mantle found in the lower mantle between 1300 and 1900 km depth under locations such as Egypt Mark van der Meijde,* Federica Marone, Domenico Giardini, and Libya (18). Subduction was ubiquitous Suzan van der Lee after 80 Ma. At present, active subduction zones are found in southern Italy and Greece. Water in the deep upper mantle can influence the properties of seismic dis- We investigated seismic discontinuities in the continuities in the mantle transition zone. Observations of converted seismic deep upper mantle of the Mediterranean re- waves provide evidence of a 20- to 35-kilometer-thick discontinuity near a gion by searching seismograms for seismic S depth of 410 kilometers, most likely explained by as much as 700 parts per waves that converted from P waves at the million of water by weight. discontinuities. Our search was facilitated by a recent temporary deployment of mobile Two major seismic velocity discontinuities, lies in the mantle transition zone would broadband seismic stations [MIDSEA (19)] at nominal depths of 410 and 660 km, border have no seismically observable effect on along the plate boundary between Eurasia the transition zone of Earth’s mantle. The the thickness of the 660-km discontinuity and Africa. We analyzed over 500 seismo- 410-km discontinuity is the result of the tran- (7), whereas the effect on the 520-km dis- grams recorded in the Mediterranean region sition from olivine to wadsleyite. The 660- continuity is unknown. at 18 temporary and 6 permanent broadband km discontinuity is caused by the transition Both temperature and water content of the stations (Fig. 1). We identified converted from ringwoodite to perovskite and magne- upper mantle vary spatially. A variety of waves by analyzing receiver functions (20). siowu¨stite. Both phase transition intervals are evidence (11–14) has indicated that amounts We found P-to-S converted waves from reported to be sharp (about 4 to 10 km thick) of 1500 parts per million (ppm) of water can the 410- and 660-km discontinuity for prac- (1–3). However, there are conditions under be present locally in the uppermost mantle. tically all stations. The conversions from the which the transition interval of the 410-km This water is carried there by subducting 410-km discontinuity are small in amplitude discontinuity can be thickened, such as by an oceanic plates, which release most of the for receiver functions that are low-passed increase in water content in olivine or by a subducted water at depths shallower than 150 with corner frequencies higher than 0.5 Hz. decrease in temperature. Theoretical studies km into the mantle wedge overlying the plate The amplitudes increase with decreasing cor- (4, 5) have shown how water influences the (15). Reports of water being able to reside ner frequency. This effect is not observed for properties of the olivine-wadsleyite phase below this depth are based on high-pressure conversions from the 660-km discontinuity, transition. Because water is preferentially in- experiments (16) and seismic tomography which show comparable amplitudes through- corporated into wadsleyite rather than oli- (17). It is, however, unknown whether and out the whole frequency range. vine, it stabilizes wadsleyite over a wider how much water is transported down to 400 Because of the temporary deployment of range of pressures and temperatures, thereby km and below. To investigate whether water the network and differences in site character- thickening the transition interval. This has resides near the mantle transition zone, we istics, not all seismic stations yielded equally been confirmed by experiments (6) showing studied the properties of seismic discontinui- robust results. Receiver functions for nine that under hydrous conditions, the zone of ties beneath the Mediterranean region (Fig. stations, however, had a sufficiently high coexistence of olivine and wadsleyite can 1). This region has been heavily affected by signal-to-noise ratio to show unambiguous thicken to as much as 40 km. A decrease in the subduction of oceanic lithosphere for the evidence for this frequency dependence of temperature would also thicken the transition past 190 million years. Between 190 and 110 the P-to-S conversion from the 410-km dis- interval (7), but the effect of temperature on the transition-interval thickness is much smaller than the effect of water. A large temperature reduction of 800 K would thick- en the discontinuity by only 10 km (5). In- creased water content in the mantle transition zone would have the opposite effect on the thickness of the phase transition interval at 660 km. This phase transition interval would become thinner because ringwoodite can hold much more water than perovskite, thereby extending its stability phase (8). Moreover, recent studies indicate that the phase transi- tion interval from wadsleyite to ringwoodite, nominally at a depth of 520 km, can be sharper under hydrous conditions (9)(Ͻ15 km thick) than under anhydrous conditions (10)(ϳ60 km thick). Temperature anoma- Fig. 1. Map of the Mediterranean region with seismic station and approximate plate boundary locations. Stations for which results are discussed in this paper are represented by black triangles Institute of Geophysics, Eidgeno¨ssische Technische and labeled with the station name (table S1); other analyzed stations are represented by black Hochschule–Ho¨nggerberg (HPP)/Swiss Federal Insti- squares. Curves with a sawtooth pattern indicate the present location of the convergent boundary, tute of Technology CH–8093 Zu¨rich, Switzerland. with sawteeth pointing in the direction of subduction or underthrusting. Strike-slip is represented *To whom correspondence should be addressed. E- by arrows. The gray scale indicates topography ranging from higher than 2.5 km in white to deeper mail: [email protected] than –2.5 km in dark gray. 1556 6 JUNE 2003 VOL 300 SCIENCE www.sciencemag.org R EPORTS continuity (Fig. 2). For the other stations, the servations (1–3), we found that the phase- 410-km discontinuity. Trace elements in oli- receiver functions were more ambiguous and transition interval at 660 km is relatively thin vine are unlikely to be the cause of the broad- did not allow a significant interpretation of (Ͻ5 km) beneath seven of the nine stations ening, because their presence would thicken the frequency dependence. For these nine (Fig. 2, fig. S1, and table S2). the phase transition interval by no more than stations, the amplitude of the converted Because of limited azimuthal coverage, 2km(26). waves from the 410-km discontinuity de- owing to the location of the Mediterranean We interpret the broadening of the 410-km pends on frequency with 75% confidence, on with respect to seismogenic zones, we could discontinuity deduced here as being caused by average, whereas this confidence is only 21% not investigate the azimuthal influence on the water in the mantle minerals at this depth. for the 660-km discontinuity (table S2). This frequency dependence of the converted These minerals can contain a substantial indicates that the observed frequency depen- waves. However, the conversion points at the amount of water: as much as 1000 ppm by dence is almost four times more probable for 410-km discontinuity beneath most stations weight of water in olivine and about 20,000 conversions from the 410-km discontinuity fall within a radius of 100 km. Synthetic tests ppm by weight of water in wadsleyite (27). The than for those from the 660-km discontinuity. (24) (fig. S3) showed that topography on the estimated water content in olivine for a transi- We observed converted energy from the discontinuity as large as 20 to 40 km on a tion interval of 20 to 25 km is around 500 ppm 410-km discontinuity that is significant (20) 100-km length scale cannot be responsible by weight (Fig. 3). To broaden the transition to above the 95% confidence level for corner for the observed frequency dependence. To- 30 to 40 km, olivine would need to contain 700 frequencies around 0.2 and 0.25 Hz for most pography on the 410-km discontinuity would to 1000 ppm by weight of water. This amount stations. For station PAB, the amplitude of mainly decrease the amplitudes of P-to-S of water is an underestimate because the con- the wave converted at the 410-km disconti- converted waves but could not be responsible verted waves are the most sensitive to the lower nuity becomes comparable to that of the wave for the observed frequency dependence. We part of the phase transition interval, where the converted at the 660-km discontinuity for also excluded scattering of converted energy fraction of wadsleyite increases more rapidly frequencies as low as 0.15 Hz. This frequen- from discontinuities at shallower depths as a with increasing depth (Fig. 3) and the corre- cy dependence of the amplitudes and the possible cause for the observed frequency sponding gradient in seismic velocity is the significance allows us to estimate the thick- dependence, because the standard deviation steepest. ness of the phase transition interval (20). of the converted wave from the 410-km dis- For some stations (Fig. 2), we also ob- These findings indicate that the phase continuity is comparable to the standard de- served, above the 95% confidence level, transition around 410 km depth is not sharp viation of the converted wave from the 660- waves that converted at the 520-km disconti- and occurs over depth intervals of about 20 to km discontinuity. Seismic tomography (25) nuity. Water would make the corresponding 25 km for these stations (fig.
Recommended publications
  • Quantification of Water in Hydrous Ringwoodite
    ORIGINAL RESEARCH ARTICLE published: 28 January 2015 EARTH SCIENCE doi: 10.3389/feart.2014.00038 Quantification of water in hydrous ringwoodite Sylvia-Monique Thomas 1*,StevenD.Jacobsen2, Craig R. Bina 2, Patrick Reichart 3, Marcus Moser 3, Erik H. Hauri 4, Monika Koch-Müller 5,JosephR.Smyth6 and Günther Dollinger 3 1 Department of Geoscience, University of Nevada Las Vegas, Las Vegas, NV, USA 2 Department of Earth and Planetary Sciences, Northwestern University, Evanston, IL, USA 3 Department für Luft- und Raumfahrttechnik LRT2, Universität der Bundeswehr München, Neubiberg, Germany 4 Department of Terrestrial Magnetism, Carnegie Institution of Washington, Washington, DC, USA 5 Helmholtz-Zentrum Potsdam, Deutsches GeoForschungsZentrum (GFZ), Potsdam, Germany 6 Department of Geological Sciences, University of Colorado Boulder, Boulder, CO, USA Edited by: Ringwoodite, γ-(Mg,Fe)2SiO4, in the lower 150 km of Earth’s mantle transition zone Mainak Mookherjee, Cornell (410–660 km depth) can incorporate up to 1.5–2wt% H2O as hydroxyl defects. We University, USA present a mineral-specific IR calibration for the absolute water content in hydrous Reviewed by: ringwoodite by combining results from Raman spectroscopy, secondary ion mass Geoffrey David Bromiley, University of Edinburgh, UK spectrometry (SIMS) and proton-proton (pp)-scattering on a suite of synthetic Mg- and Marc Blanchard, CNRS - Université Fe-bearing hydrous ringwoodites. H2O concentrations in the crystals studied here Pierre et Marie Curie, France range from 0.46 to 1.7wt% H2O (absolute methods), with the maximum H2Oin *Correspondence: the same sample giving 2.5 wt% by SIMS calibration. Anchoring our spectroscopic Sylvia-Monique Thomas, results to absolute H-atom concentrations from pp-scattering measurements, we report Department of Geoscience, University of Nevada Las Vegas, frequency-dependent integrated IR-absorption coefficients for water in ringwoodite −1 −2 4505 S.
    [Show full text]
  • Influence of the Ringwoodite-Perovskite Transition on Mantle Convection in Spherical Geometry As a Function of Clapeyron Slope A
    Discussion Paper | Discussion Paper | Discussion Paper | Discussion Paper | Solid Earth Discuss., 3, 713–741, 2011 Solid Earth www.solid-earth-discuss.net/3/713/2011/ Discussions doi:10.5194/sed-3-713-2011 © Author(s) 2011. CC Attribution 3.0 License. This discussion paper is/has been under review for the journal Solid Earth (SE). Please refer to the corresponding final paper in SE if available. Influence of the Ringwoodite-Perovskite transition on mantle convection in spherical geometry as a function of Clapeyron slope and Rayleigh number M. Wolstencroft1,* and J. H. Davies1 1School of Earth and Ocean Sciences, Cardiff University, Main Building, Park Place, Cardiff, Wales, CF10 3AT, UK *now at: University of Ottawa, Ottawa, Ontario, Canada Received: 21 July 2011 – Accepted: 27 July 2011 – Published: 4 August 2011 Correspondence to: J. H. Davies ([email protected]) Published by Copernicus Publications on behalf of the European Geosciences Union. 713 Discussion Paper | Discussion Paper | Discussion Paper | Discussion Paper | Abstract We investigate the influence on mantle convection of the negative Clapeyron slope ringwoodite to perovskite and ferro-periclase mantle phase transition, which is corre- lated with the seismic discontinuity at 660 km depth. In particular, we focus on un- 5 derstanding the influence of the magnitude of the Clapeyron slope (as measured by the Phase Buoyancy parameter, P ) and the vigour of convection (as measured by the Rayleigh number, Ra) on mantle convection. We have undertaken 76 simulations of isoviscous mantle convection in spherical geometry varying Ra and P . Three domains of behaviour were found: layered convection for high Ra and more negative P , whole 10 mantle convection for low Ra and less negative P and transitional behaviour in an inter- vening domain.
    [Show full text]
  • The Upper Mantle and Transition Zone
    The Upper Mantle and Transition Zone Daniel J. Frost* DOI: 10.2113/GSELEMENTS.4.3.171 he upper mantle is the source of almost all magmas. It contains major body wave velocity structure, such as PREM (preliminary reference transitions in rheological and thermal behaviour that control the character Earth model) (e.g. Dziewonski and Tof plate tectonics and the style of mantle dynamics. Essential parameters Anderson 1981). in any model to describe these phenomena are the mantle’s compositional The transition zone, between 410 and thermal structure. Most samples of the mantle come from the lithosphere. and 660 km, is an excellent region Although the composition of the underlying asthenospheric mantle can be to perform such a comparison estimated, this is made difficult by the fact that this part of the mantle partially because it is free of the complex thermal and chemical structure melts and differentiates before samples ever reach the surface. The composition imparted on the shallow mantle by and conditions in the mantle at depths significantly below the lithosphere must the lithosphere and melting be interpreted from geophysical observations combined with experimental processes. It contains a number of seismic discontinuities—sharp jumps data on mineral and rock properties. Fortunately, the transition zone, which in seismic velocity, that are gener- extends from approximately 410 to 660 km, has a number of characteristic ally accepted to arise from mineral globally observed seismic properties that should ultimately place essential phase transformations (Agee 1998). These discontinuities have certain constraints on the compositional and thermal state of the mantle. features that correlate directly with characteristics of the mineral trans- KEYWORDS: seismic discontinuity, phase transformation, pyrolite, wadsleyite, ringwoodite formations, such as the proportions of the transforming minerals and the temperature at the discontinu- INTRODUCTION ity.
    [Show full text]
  • RINGWOODITE-OLIVINE ASSEMBLAGES in DHOFAR 922 L6 MELT VEINS. D. D. Badjukov1, F. Brandstaetter2, G. Kurat3, E. Libowitzky3 and J
    Lunar and Planetary Science XXXVI (2005) 1684.pdf RINGWOODITE-OLIVINE ASSEMBLAGES IN DHOFAR 922 L6 MELT VEINS. D. D. Badjukov1, F. Brandstaetter2, G. Kurat3, E. Libowitzky3 and J. Raitala4, 1V.I. Vernadsky Institute RAS, Kosygin str. 19, 11991, Moscow, Russia, [email protected], 2Naturhistorisches Museum, Burgring 7, A-1010 Wien, Austria, [email protected], 3Universität Wien, Institut für Geologische Wissenschaften, Althanstr. 14, A- 1090 Wien, Austria, [email protected], 3University of Oulu, FIN 90401, Finland, [email protected], Introduction. Shock-induced melt veins stand out gave in average a composition enriched in Al and Ca among different types of veins in ordinary chondrites relatively to the host chondrite, which is proposed to due to their specific mineral assemblages. They often be due to preferred melting of plagioclase. Embedded contain high pressure polymorphs of host chondrite in the veins are non-melted inclusions of the host minerals like wadsleyite, ringwoodite, majorite, chondrite which were converted to different phases, akimotoite and so on [1-4]. Because of a compositional common are ringwoodite, olivine, majorite, pyroxene similarity between chondrites and the Earth’s mantle, and plagioclase glass. Several areas contain also green the shock melt veins are an unique natural source of wadsleyite aggregates. Some majorite and ringwoodite study of mantle mineralogy. Two lithologies are clasts are enveloped by a silica mantle. Ringwoodite is characteristic for the veins: silicates, oxide(s), observed also at a distance of no more than ~0.5 mm sulfide(s) and metal crystallized from a melt and solid from vein walls in the host rock.
    [Show full text]
  • Spin Transition of Fe2+ in Ringwoodite (Mg,Fe)2Sio4 at High Pressures
    American Mineralogist, Volume 98, pages 1803–1810, 2013 2+ Spin transition of Fe in ringwoodite (Mg,Fe)2SiO4 at high pressures IGOR S. LYUBUTIN1, JUNG-FU LIN2, ALEXANDER G. GAVRILIUK1,3,*, ANNA A. MIRONOVICH3, ANNA G. IVANOVA1, VLADIMIR V. RODDATIS4 AND ALEXANDER L. VASILIEV1,4 1Shubnikov Institute of Crystallography, Russian Academy of Sciences, Moscow 119333, Russia 2Department of Geological Sciences, Jackson School of Geosciences, The University of Texas at Austin, Austin, Texas 78712-0254, U.S.A. 3Institute for Nuclear Research, Russian Academy of Sciences, 60-letiya Oktyabrya prospekt 7a, Moscow 117312, Russia 4National Scientific Center, “Kurchatov Institute,” Moscow 123098, Russia ABSTRACT Electronic spin transitions of iron in the Earth’s mantle minerals are of great interest to deep-Earth researchers because their effects on the physical and chemical properties of mantle minerals can significantly affect our understanding of the properties of the deep planet. Here we have studied the electronic spin states of iron in ringwoodite (Mg0.75Fe0.25)2SiO4 using synchrotron Mössbauer spec- troscopy in a diamond-anvil cell up to 82 GPa. The starting samples were analyzed extensively using transmission and scanning electron microscopes to investigate nanoscale crystal chemistry and local iron distributions. Analyses of the synchrotron Mössbauer spectra at ambient conditions reveal two 2+ 2+ non-equivalent iron species, (Fe )1 and (Fe )2, which can be attributed to octahedral and tetrahedral sites in the cubic spinel structure, respectively. High-pressure Mössbauer measurements show the disappearance of the hyperfine quadrupole splitting (QS) of the Fe2+ ions in both sites at approximately 45–70 GPa, indicating an electronic high-spin (HS) to low-spin (LS) transition.
    [Show full text]
  • Whole-Mantle Convection and the Transition-Zone Water Filter
    hypothesis Whole-mantle convection and the transition-zone water filter David Bercovici & Shun-ichiro Karato Department of Geology and Geophysics, Yale University, PO Box 208109, New Haven, Connecticut 06520-8109, USA ........................................................................................................................................................................................................................... Because of their distinct chemical signatures, ocean-island and mid-ocean-ridge basalts are traditionally inferred to arise from separate, isolated reservoirs in the Earth’s mantle. Such mantle reservoir models, however, typically satisfy geochemical constraints, but not geophysical observations. Here we propose an alternative hypothesis that, rather than being divided into isolated reservoirs, the mantle is filtered at the 410-km-deep discontinuity. We propose that, as the ascending ambient mantle (forced up by the downward flux of subducting slabs) rises out of the high-water-solubility transition zone (between the 660 km and 410 km discontinuities) into the low-solubility upper mantle above 410 km, it undergoes dehydration-induced partial melting that filters out incompatible elements. The filtered, dry and depleted solid phase continues to rise to become the source material for mid-ocean-ridge basalts. The wet, enriched melt residue may be denser than the surrounding solid and accordingly trapped at the 410 km boundary until slab entrainment returns it to the deeper mantle. The filter could be suppressed for
    [Show full text]
  • Comparative Compressibility of Hydrous Wadsleyite and Ringwoodite
    PUBLICATIONS Journal of Geophysical Research: Solid Earth RESEARCH ARTICLE Comparative compressibility of hydrous wadsleyite 10.1002/2015JB012123 and ringwoodite: Effect of H2O and implications Key Points: for detecting water in the transition zone • Hydration reduces K0 of wadsleyite significantly Yun-Yuan Chang1,2, Steven D. Jacobsen1, Craig R. Bina1, Sylvia-Monique Thomas3, Joseph R. Smyth4, • fl Hydration does not in uence dK/dP of 5 5 5 6 7 wadslyeite Daniel J. Frost , Tiziana Boffa Ballaran , Catherine A. McCammon , Erik H. Hauri , Toru Inoue , 8 9 10 • Hydration reduces bulk sound velocity Hisayoshi Yurimoto , Yue Meng , and Przemyslaw Dera at transition zone conditions 1Department of Earth and Planetary Sciences, Northwestern University, Evanston, Illinois, USA, 2Now at Institute of Earth Sciences, Academia Sinica, Taipei, Taiwan, 3Department of Geoscience, University of Nevada, Las Vegas, Las Vegas, Nevada, USA, 4Department of Geological Sciences, University of Colorado Boulder, Boulder, Colorado, USA, 5Bayerisches Geoinstitut, Correspondence to: University of Bayreuth, Bayreuth, Germany, 6Department of Terrestrial Magnetism, Carnegie Institution of Washington, Y.-Y. Chang, 7 8 [email protected] Washington, District of Columbia, USA, Geodynamics Research Center, Ehime University, Matsuyama, Japan, Department of Natural History Sciences, Hokkaido University, Sapporo, Japan, 9High-Pressure Collaborative Access Team, Carnegie Institution of Washington, Argonne, Illinois, USA, 10Hawaii Institute of Geophysics and Planetology, University of Hawai‘iat Citation: Mānoa, Honolulu, Hawaii, USA Chang, Y.-Y., et al. (2015), Comparative compressibility of hydrous wadsleyite and ringwoodite: Effect of H2O and fl implications for detecting water in the Abstract Review of recent mineral physics literature shows consistent trends for the in uence of Fe and transition zone, J.
    [Show full text]
  • 5 Ringwoodite: Its Importance in Earth Sciences
    Fabrizio Nestola 5 Ringwoodite: its importance in Earth Sciences 5.1 History of ringwoodite The history of ringwoodite started in 1869 in a remote locality in the south-west of Queensland in Australia. Mr. Michael Hammond witnessed a meteorite shower close to the junction between Cooper and Kyabra Creeks (Lat. 25° 30 S., Long. 142° 40 E.), not far from Windorah (Queensland, Australia) and about 1000 km west of Brisbane. The meteorite fall was very impressive and in due course 102 stones were recovered. Mr. Hammond was the owner of the Tenham Station and from this the meteorite col- lection was named as “Tenham meteorites”. This collection was then offered in 1935 to the British Museum by Mr. Benjamin Dunstan, formerly Government Geologist of Queensland [1]. But why does this nice story match with ringwoodite? In 1969, exactly 100 years after Mr. Hammond observed the Tenham meteorite fall, R. A. Binns, R. J. Davies and S. J. B. Reed published in Nature [2] the first natural evidence of ringwoodite after studying a fragment of the Tenham meteorite. Thirty years later Chen et al. [3] reported clear images of some lamellae of about 1–2 μ in thickness showing a higher density than olivine but with identical composition (Fig. 5.1, modified from Chen et al. [3]). The Fig. 5.1: Back-scattered image of lamellae of ringwoodite in olivine (modified from [3]). The lamellae are evident being marked by a brighter grey. The darker grey corresponds to olivine. The blue solid lines are reported to indicate the directions along which ringwoodite grew.
    [Show full text]
  • Phase Relations in MAFSH System up to 21 Gpa: Implications for Water Cycles in Martian Interior
    minerals Article Phase Relations in MAFSH System up to 21 GPa: Implications for Water Cycles in Martian Interior Chaowen Xu 1,* and Toru Inoue 1,2,3 1 Geodynamics Research Center, Ehime University, 2-5 Bunkyo-cho, Matsuyama 790-8577, Japan; [email protected] 2 Department of Earth and Planetary Systems Science, Hiroshima University, 1-3-1 Kagamiyama, Higashi-Hiroshima 739-8526, Japan 3 Hiroshima Institute of Plate Convergence Region Research (HiPeR), Hiroshima University, Higashi-Hiroshima, Hiroshima 739-8526, Japan * Correspondence: [email protected]; Tel.: +81-050-3699-0952 Received: 3 August 2019; Accepted: 14 September 2019; Published: 16 September 2019 Abstract: To elucidate the water cycles in iron-rich Mars, we investigated the phase relation of a water-undersaturated (2 wt.%) analog of Martian mantle in simplified MgO-Al2O3-FeO-SiO2-H2O (MAFSH) system between 15 and 21 GPa at 900–1500 ◦C using a multi-anvil apparatus. Results showed that phase E coexisting with wadsleyite or ringwoodite was at least stable at 15–16.5 GPa and below 1050 ◦C. Phase D coexisted with ringwoodite at pressures higher than 16.5 GPa and temperatures below 1100 ◦C. The transition pressure of the loop at the wadsleyite-ringwoodite boundary shifted towards lower pressure in an iron-rich system compared with a hydrous pyrolite model of the Earth. Some evidence indicates that water once existed on the Martian surface on ancient Mars. The water present in the hydrous crust might have been brought into the deep interior by the convecting mantle. Therefore, water might have been transported to the deep Martian interior by hydrous minerals, such as phase E and phase D, in cold subduction plates.
    [Show full text]
  • Mccoy, T. J. Mineralogical Evolution of Meteorites. Elements
    Mineralogical Evolution of Meteorites Halite crystals from the Monahans chondrite contain fl uid inclusions, which indicate Timothy J. McCoy* signifi cant water–rock interactions in the 1811-5209/10/0006-0019$2.50 DOI: 10.2113/gselements.6.1.19 meteorite’s parent body. Image width ~5 mm. COURTESY OF M. he approximately 250 mineral species found in meteorites record the ZOLENSKY AND R. BODNAR earliest stages of the birth of our solar system. Refractory minerals but eventually transformed some that formed during the violent deaths of other stars and during conden- T asteroids into molten worlds that sation of our own solar nebula mixed with a wide range of silicates, sulfi des, formed crusts, mantles, and cores and metals to form the most primitive chondritic meteorites. Subsequent reminiscent of our own planet. It aqueous alteration, thermal metamorphism, and shock metamorphism further is this history—from the earliest beginnings to the melting of diversifi ed the minerals found in meteorites. Asteroidal melting at fi rst planets—that we explore in this increased and then dramatically decreased mineralogical diversity, before a article. new phase of igneous differentiation that presaged the processes that would occur in terrestrial planets. THE STELLAR CAULDRON Earth’s mineralogical evolution KEYWORDS: mineral evolution, meteorites, asteroids, metamorphism, began not in the heat of an early differentiation, shock molten planet but in the blast furnace of stars that predated our FRAGMENTS FROM THE BEGINNING solar system. More than 4.6 billion years ago, presolar As Earth evolved over the last 4.5 billion years, its miner- grains formed when temperatures in the expanding enve- alogy changed.
    [Show full text]
  • Suppressing the Martian Dynamo with Ongoing Hydrogenation of the Core by Hydrated Mantle Minerals
    49th Lunar and Planetary Science Conference 2018 (LPI Contrib. No. 2083) 2390.pdf SUPPRESSING THE MARTIAN DYNAMO WITH ONGOING HYDROGENATION OF THE CORE BY HYDRATED MANTLE MINERALS. J. G. O’Rourke and S.-H. Shim, School of Earth and Space Exploration, Arizona State University, Tempe, AZ ([email protected]). Introduction: Mars lacks an internally generated to drive a dynamo. Geophysical missions like InSight magnetic field today. However, crustal remanent mag- could detect several signatures of a hydrogen-rich core. netism discovered by Mars Global Surveyor evidences Delivering hydrogen to the core: We focus on the dynamo activity prior to ~4.1 billion years ago [e.g., 1]. mass of hydrogen that is available for transport into the Vigorous fluid motions must constantly occur in the core over geologic time. Hydrogen that is already mixed core to drive a magnetic dynamo. Any field would dis- in the core immediately after accretion does not affect sipate within ~104 years after the fluid stagnates [e.g., the dynamo except by reducing the liquidus tempera- 2]. Thermal and/or compositional convection, in partic- tures—thus delaying the formation of an inner core. ular, requires a minimum amount of heat flow across the Total mass budget: Minerals like wadsleyite and core/mantle boundary. Popular explanations for the ces- ringwoodite—found in the transition zone between sation of internal magnetism on Mars rely on a decrease depths of 410 and 660 km on Earth—can host up to ~2.5 in the rate of core cooling as mantle convection becomes wt% of water in their crystal structures.
    [Show full text]
  • The Coexistence of Wadsleyite and Ringwoodite in L/LL Chondrite SAH 293: Constraints on Shock Pressure Conditions and Olivine Transformation
    45th Lunar and Planetary Science Conference (2014) 2237.pdf The Coexistence of Wadsleyite and Ringwoodite in L/LL Chondrite SAH 293: Constraints on Shock Pressure Conditions and Olivine Transformation. C. Fudge, J. Hu and T.G. Sharp 1School of Earth And Space Explora- tion, Arizona State University, Tempe, AZ 85278, U.S.A. [email protected] Introduction: and within melt veins and ranges from colorless to The presence of high pressure minerals in highly deep blue. shocked chondrites provides information on the pres- Wadsleyite and ringwoodite are constrained within sure and duration of shock resulting from impact pro- and in contact with melt veins, whereas maskelynite is cesses on parent bodies in the main asteroid belt. less localized, but still occurs predominantly along Ringwoodite, the spinel structured polymorph of oli- melt veins and pockets. The presence of ringwoodite in vine, is the most common high-pressure polymorph in the sample are consistent with shock stage S6 [2], how- ordinary chondrites. Ringwoodite forms by either the ever the presence of plagioclase away from the shock solid-state transformation of olivine fragments within vein indicates a shock stage ~S5. The localization of shock veins, or by crystallization from the shock melt. S6 features to shock melt illustrates the importance of Wadsleyite, the other high-pressure polymorph of high temperatures in shock-induced phase transitions. olivine, is much less common in meteorites and has Contrast variations in BES images (Figure 3a & 3b) only been found in the Peace River L6 chondrite [1]. In show internal textures consistent with partial transfor- this study, we observed pervasive wadsleyite in ordi- mation of olivine.
    [Show full text]