Basalt Fibre Reinforced Geopolymer Made from Lunar Regolith Simulant
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Qiao Et Al., Sosigenes Pit Crater Age 1/51
Qiao et al., Sosigenes pit crater age 1 2 The role of substrate characteristics in producing anomalously young crater 3 retention ages in volcanic deposits on the Moon: Morphology, topography, 4 sub-resolution roughness and mode of emplacement of the Sosigenes Lunar 5 Irregular Mare Patch (IMP) 6 7 Le QIAO1,2,*, James W. HEAD2, Long XIAO1, Lionel WILSON3, and Josef D. 8 DUFEK4 9 1Planetary Science Institute, School of Earth Sciences, China University of 10 Geosciences, Wuhan 430074, China. 11 2Department of Earth, Environmental and Planetary Sciences, Brown University, 12 Providence, RI 02912, USA. 13 3Lancaster Environment Centre, Lancaster University, Lancaster LA1 4YQ, UK. 14 4School of Earth and Atmospheric Sciences, Georgia Institute of Technology, Atlanta, 15 Georgia 30332, USA. 16 *Corresponding author E-mail: [email protected] 17 18 19 20 Key words: Lunar/Moon, Sosigenes, irregular mare patches, mare volcanism, 21 magmatic foam, lava lake, dike emplacement 22 23 24 25 1/51 Qiao et al., Sosigenes pit crater age 26 Abstract: Lunar Irregular Mare Patches (IMPs) are comprised of dozens of small, 27 distinctive and enigmatic lunar mare features. Characterized by their irregular shapes, 28 well-preserved state of relief, apparent optical immaturity and few superposed impact 29 craters, IMPs are interpreted to have been formed or modified geologically very 30 recently (<~100 Ma; Braden et al. 2014). However, their apparent relatively recent 31 formation/modification dates and emplacement mechanisms are debated. We focus in 32 detail on one of the major IMPs, Sosigenes, located in western Mare Tranquillitatis, 33 and dated by Braden et al. -
How a Young-Looking Lunar Volcano Hides Its True Age 28 March 2017, by Kevin Stacey
How a young-looking lunar volcano hides its true age 28 March 2017, by Kevin Stacey formed in the recent geologic past, we just don't think that's the case," said Jim Head, co-author of the paper and professor in Brown's Department of Earth, Environmental and Planetary Sciences. "The model we've developed for Ina's formation puts it firmly within the period of peak volcanic activity on the Moon several billion years ago." Youthful appearance Ina sits near the summit of a gently sloped mound of basaltic rock, leading many scientists to conclude that it was likely the caldera of an ancient lunar volcano. But just how ancient wasn't clear. While the flanks of the volcano look billions of years old, the Ina caldera itself looks much younger. One The feature known as Ina, as seen by NASA's Lunar sign of youth is its bright appearance relative to its Reconnaissance Orbiter, was likely formed by an surroundings. The brightness suggests Ina hasn't eruption of fluffy 'magmatic foam,' new research shows. had time to accumulate as much regolith, the layer Credit: NASA/GSFC/ASU of loose rock and dust that builds up on the surface over time. Then there are Ina's distinctive mounds—80 or so While orbiting the Moon in 1971, the crew of Apollo smooth hills of rock, some standing as tall as 100 15 photographed a strange geological feature—a feet, which dominate the landscape within the bumpy, D-shaped depression about two miles long caldera. The mounds appear to have far fewer and a mile wide—that has fascinated planetary impact craters on them compared to the scientists ever since. -
WO 2012/028419 Al
(12) INTERNATIONAL APPLICATION PUBLISHED UNDER THE PATENT COOPERATION TREATY (PCT) (19) World Intellectual Property Organization International Bureau (10) International Publication Number (43) International Publication Date 8 March 2012 (08.03.2012) WO 2012/028419 Al (51) International Patent Classification: (81) Designated States (unless otherwise indicated, for every C04B 28/10 (2006.01) kind of national protection available): AE, AG, AL, AM, AO, AT, AU, AZ, BA, BB, BG, BH, BR, BW, BY, BZ, (21) International Application Number: CA, CH, CL, CN, CO, CR, CU, CZ, DE, DK, DM, DO, PCT/EP201 1/063629 DZ, EC, EE, EG, ES, FI, GB, GD, GE, GH, GM, GT, (22) International Filing Date: HN, HR, HU, ID, IL, IN, IS, JP, KE, KG, KM, KN, KP, 8 August 201 1 (08.08.201 1) KR, KZ, LA, LC, LK, LR, LS, LT, LU, LY, MA, MD, ME, MG, MK, MN, MW, MX, MY, MZ, NA, NG, NI, (25) Filing Language: English NO, NZ, OM, PE, PG, PH, PL, PT, QA, RO, RS, RU, (26) Publication Langi English SC, SD, SE, SG, SK, SL, SM, ST, SV, SY, TH, TJ, TM, TN, TR, TT, TZ, UA, UG, US, UZ, VC, VN, ZA, ZM, (30) Priority Data: ZW. 1014577.9 2 September 2010 (02.09.2010) GB (84) Designated States (unless otherwise indicated, for every (71) Applicant (for all designated States except US): NO- kind of regional protection available): ARIPO (BW, GH, VACEM LIMITED [GB/GB]; The Incubator, Bessemer GM, KE, LR, LS, MW, MZ, NA, SD, SL, SZ, TZ, UG, Building, Imperial College, South Kensington London ZM, ZW), Eurasian (AM, AZ, BY, KG, KZ, MD, RU, TJ, SW7 2AZ (GB). -
Effect of Admixing Fly Ash on Cementing Characteristics of Magnesium Oxychloride Cement
International Journal of Recent Technology and Engineering (IJRTE) ISSN: 2277-3878, Volume-9 Issue-5, January 2021 Effect of Admixing Fly Ash on Cementing Characteristics of Magnesium Oxychloride Cement Rekha Sharma, R. N. Yadav Abstract: Investigations pertaining to the effect of admixing The manufacturing process of MOC binders is not only free different amounts of fly ash on setting characteristics and from any carbon dioxide gas emissions, but due to carbon compressive strength of magnesium oxychloride cement has been sequestration potential, these binders actually act as “sinks” carried out in this paper. For this purpose, two different dry mix for atmospheric carbon dioxide [13]. The important compositions (1:0 and 1:1) of magnesia and dolomite were commercial applications of MOC binders include floorings prepared and 5 %, 10 %, 15 % and 20 % fly ash were added in dry mixes. The dry mixes were then gauged with 24 °Be of industries and hospitals, grinding wheels and wall concentration of magnesium chloride gauging solution. It was insulation panels due to its marble like gloss. The industrial observed that initial and final setting times of cement blocks tend applications of MOC cement has been limited because of the to increase with increasing amount of fly ash in dry mix. MOC associated problems of poor water resistance, volume cement blocks of 1:1 composition admixed with fly ash displayed instability, cracking and sweating etc. The magnesium good cementing characteristics. oxychloride binder system exhibits excellent bonding Keywords: Compressive strength, fly ash, Gauging solution, capacity to a large variety of organic and inorganic Inert filler, MOC, Setting time. -
Conceptual Lunar Missions to the Ina Lunar Irregular Mare Patch: Distinguishing Between Ancient and Modern Volcanism Models
52nd Lunar and Planetary Science Conference 2021 (LPI Contrib. No. 2548) 1799.pdf CONCEPTUAL LUNAR MISSIONS TO THE INA LUNAR IRREGULAR MARE PATCH: DISTINGUISHING BETWEEN ANCIENT AND MODERN VOLCANISM MODELS. L. Qiao1, J. W. Head2, L. Wilson3 and Z. Ling1, 1Inst. Space Sci., Shandong Univ., Weihai, Shandong, 264209, China ([email protected]), 2Dep. Earth, Env. & Planet. Sci., Brown Univ., Providence, RI, 02912, USA, 3Lancaster Env. Centre, Lancaster Univ., Lancaster LA1 4YQ, UK. Introduction: The Ina Irregular Mare Patch (IMP), to volcanism having waned in middle lunar history and a distinctive ~2×3 km D-shaped depression located atop ceased sometime in the last ~1 Ga [9]. The Young a 22 km-diameter shield volcano in the nearside lunar Model, however, raises a line of questions that conflicts maria, is composed of unusual bulbous-shaped mounds with the above lunar evolution model, and indeed re- surrounded by optically immature hummocky and quires the overall evolution history to be very different blocky floor units. Its peculiar shape and interior struc- in various aspects including lunar interior thermal status, tures intrigued lunar scientists for decades. Previous in- abundance of lunar heat-producing elements, and stress vestigations have documented substantial geological status of the lunar lithosphere. characteristics of Ina in various aspects, and called on CriticAl Unresolved Issues About the Two End- various models to interpret its formation mechanism and Member (Young And Old) Models. Questions raised age, including sublimation -
Foam Glass Lightened Sorel's Cement Composites Doped with Coal Fly
materials Article Foam Glass Lightened Sorel’s Cement Composites Doped with Coal Fly Ash Adam Pivák 1 , Milena Pavlíková 1 , Martina Záleská 1 , Michal Lojka 2, Anna-Marie Lauermannová 2 , Ivana Faltysová 2, OndˇrejJankovský 2 and Zbyšek Pavlík 1,* 1 Department of Materials Engineering and Chemistry, Faculty of Civil Engineering, Czech Technical University in Prague, Thákurova 7, 166 29 Prague 6, Czech Republic; [email protected] (A.P.); [email protected] (M.P.); [email protected] (M.Z.) 2 Department of Inorganic Chemistry, Faculty of Chemical Technology, University of Chemistry and Technology, Technická 5, 166 28 Prague 6, Czech Republic; [email protected] (M.L.); [email protected] (A.-M.L.); [email protected] (I.F.); [email protected] (O.J.) * Correspondence: [email protected]; Tel.: +420-224-354-371 Abstract: Lightweight Sorel’s cement composites doped with coal fly ash were produced and tested. Commercially available foam granulate was used as lightening aggregate. For comparison, reference composites made of magnesium oxychloride cement (MOC) and quartz sand were tested as well. The performed experiments included X-ray diffraction, X-ray fluorescence, scanning electron microscopy, light microscopy, and energy dispersive spectroscopy analyses. The macro- and microstructural parameters, mechanical resistance, stiffness, hygric, and thermal parameters of the 28-days matured composites were also researched. The combined use of foam glass and fly ash enabled to get a material of low weight, high porosity, sufficient strength and stiffness, low water imbibition, and Citation: Pivák, A.; Pavlíková, M.; greatly improved thermal insulation performance. -
Rethinking Lunar Mare Basalt Regolith Formation: 4 New Concepts of Lava Flow Protolith 5 and 6 Evolution of Regolith Thickness and Internal Structure 7 8 James W
1 1 2 3 Rethinking Lunar Mare Basalt Regolith Formation: 4 New Concepts of Lava Flow Protolith 5 and 6 Evolution of Regolith Thickness and Internal Structure 7 8 James W. Head1 and Lionel Wilson2,1 9 10 1Department of Earth, Environmental and Planetary Science, 11 Brown University, Providence, Rhode Island 02912 USA. 12 13 2Lancaster Environment Centre, Lancaster University, Lancaster LA1 4YQ UK 14 15 Submitted to Geophysical Research Letters 16 #2020GL088334 17 April 9, 2020 18 Revised September 21, 2020 19 20 21 Abstract: Lunar mare regolith is traditionally thought to have formed by impact bombardment 22 of newly emplaced coherent solidified basaltic lava. We use new models for initial 23 emplacement of basalt magma to predict and map out thicknesses, surface topographies and 24 internal structures of the fresh lava flows and pyroclastic deposits that form the lunar mare 25 regolith parent rock, or protolith. The range of basaltic eruption types produce widely varying 26 initial conditions for regolith protolith, including 1) “auto-regolith”, a fragmental meters-thick 27 surface deposit that forms upon eruption and mimics impact-generated regolith in physical 28 properties, 2) lava flows with significant near-surface vesicularity and macro-porosity, 3) 29 magmatic foams, and 4) dense, vesicle-poor flows. Each protolith has important implications for 30 the subsequent growth, maturation and regional variability of regolith deposits, suggesting 31 wide spatial variations in the properties and thickness of regolith of similar age. Regolith may 32 thus provide key insights into mare basalt protolith and its mode of emplacement. 33 34 Plain Language Summary: Following recent studies of how lava eruptions are emplaced on the 35 lunar surface, we show that solid basalt is only one of a wide range of starting conditions in the 36 process of forming lunar soil (regolith). -
Carbon Dioxide Uptake by MOC-Based Materials
applied sciences Article Carbon Dioxide Uptake by MOC-Based Materials OndˇrejJankovský 1, Michal Lojka 1, Anna-Marie Lauermannová 1, Filip Antonˇcík 1, Milena Pavlíková 2, Zbyšek Pavlík 2 and David Sedmidubský 1,* 1 Department of Inorganic Chemistry, Faculty of Chemical Technology, University of Chemistry and Technology, Technická 5, 166 28 Prague 6, Czech Republic; [email protected] (O.J.); [email protected] (M.L.); [email protected] (A.-M.L.); fi[email protected] (F.A.) 2 Department of Materials Engineering and Chemistry, Faculty of Civil Engineering, Czech Technical University in Prague, Thákurova 7, 166 29 Prague 6, Czech Republic; [email protected] (M.P.); [email protected] (Z.P.) * Correspondence: [email protected]; Tel.: +420-2-2044-4122 Received: 6 March 2020; Accepted: 24 March 2020; Published: 26 March 2020 Featured Application: The highest potential of magnesium oxychloride cement (MOC) is its capability to be used as a component of low-energy building composite materials while acting as a CO2 sink. The results of this contribution also show that MOC can be used as a binder in advanced building materials that have particular properties, and therefore specific application potentials. Formation and hardening of this material are rather fast, so the material can be used in quick repairs as well as a protection layer. This property is also beneficial for use in prefabrication, due to the possibility of unmolding after a shorter time compared to Portland cement (PC) materials, so the whole production process can be considered more effective. Somewhat significant importance should be given to its ability to capture CO2, which not only makes it more eco-friendly, but also improves its mechanical properties. -
Ina Pit Crater on the Moon: Extrusion of Waning-Stage Lava Lake Magmatic Foam Results in Extremely Young Crater Retention Ages
Lunar and Planetary Science XLVIII (2017) 1126.pdf INA PIT CRATER ON THE MOON: EXTRUSION OF WANING-STAGE LAVA LAKE MAGMATIC FOAM RESULTS IN EXTREMELY YOUNG CRATER RETENTION AGES. L. Qiao1, 2, J. W. Head2, L. Wil- son3, L. Xiao1, M. Kreslavsky4 and J. Dufek5, 1Planet. Sci. Inst., China Univ. Geosci., Wuhan 430074, China, 2Dep. Earth, Env. & Planet. Sci., Brown Univ., Providence, RI, 02906, USA, 3Lancaster Env. Centre, Lancaster Univ., Lancaster LA1 4YQ, UK, 4Earth & Planet. Sci., UC Santa Cruz, Santa Cruz, CA 95064, USA , 5Sch. Earth & Atmos. Sci., GA Tech, Atlanta, GA, 30332, USA. Contact: [email protected], [email protected]. Introduction: Ina is an unusual lunar feature in Lacus Felicitatis (18.65°N, 5.30°E), ~170 km southeast of the Imbrium impact basin, first discovered in Apollo 15 data [1]. Located in the midst of mare deposits interpreted to be ancient basalts, the ~2×3 km D-shaped shallow de- pression consists of dozens of mounds with cross-section resembling a convex meniscus shape, surrounded by a relatively optically fresh hummocky and blocky floor (Fig. 1). The Ina interior is defined by an inward-facing wall (5–10°) and a relatively flat basal terrace/ledge with a steep (10–30°) inward-facing scarp up to ~12 m high. The floor is generally flat, slopes gently (<2°) toward the interior, and mainly lies about 40–60 m below the rim. About 50% of the interior terrain is made up of the unu- Fig. 1. Perspective view of the Ina interior, based on sual bleb-like mounds with the remainder composed of LROC NAC frame M119815703 overlaid on LROC NAC DTM, VEX.=~3. -
Evidence for Basaltic Volcanism on the Moon Within the Past 100 Million Years
LETTERS PUBLISHED ONLINE: 12 OCTOBER 2014 | DOI: 10.1038/NGEO2252 Evidence for basaltic volcanism on the Moon within the past 100 million years S. E. Braden1*, J. D. Stopar1, M. S. Robinson1, S. J. Lawrence1, C. H. van der Bogert2 and H. Hiesinger2 The bulk of basaltic magmatism on the Moon occurred Stratigraphic relationships at all IMPs indicate that the smooth from 3.9 to 3.1 billion years ago on the ancient lunar mare deposits generally superpose—and are higher in elevation than—the plains1. There is evidence for basaltic volcanism as recently uneven deposits. as 2.9 billion years ago from crystallization ages2 and a billion Crater size-frequency distributions (CSFDs; refs 10,11) of years ago from stratigraphy3,4. An enigmatic surface formation superposed craters with D ≥ 10 m yield model ages for the smooth named Ina (18.65◦ N, 5.30◦ E) may represent much younger deposits of individual IMPs (Fig.3), but the uneven deposits have mare volcanism, but age estimates are poorly constrained5–8. too few craters to provide statistically significant CSFDs (Methods Here we investigate 70 small topographic anomalies, termed section); however, their inferred stratigraphic position below the irregular mare patches (100–5,000 m maximum dimension), smooth deposits suggests an older age. Model ages are 58 ± 4 Myr on the lunar nearside with irregular morphologies and textures for the Cauchy-5 IMP (smooth deposit area D 1.3 km2/, 33±2 Myr similar to Ina, using Lunar Reconnaissance Orbiter narrow for Ina (smooth deposit area D 1.7 km2/ and 18 ± 1 Myr for the angle camera images9, digital terrain models and wide angle Sosigenes IMP (smooth deposit area D 4.5 km2/ (Supplementary camera colour ratios. -
Performance of a Novel Sustainable Binder Under Extreme Dynamic Loading Conditions
University of Rhode Island DigitalCommons@URI Open Access Master's Theses 2017 Performance of a Novel Sustainable Binder Under Extreme Dynamic Loading Conditions Paul David Schmidt University of Rhode Island, [email protected] Follow this and additional works at: https://digitalcommons.uri.edu/theses Recommended Citation Schmidt, Paul David, "Performance of a Novel Sustainable Binder Under Extreme Dynamic Loading Conditions" (2017). Open Access Master's Theses. Paper 1049. https://digitalcommons.uri.edu/theses/1049 This Thesis is brought to you for free and open access by DigitalCommons@URI. It has been accepted for inclusion in Open Access Master's Theses by an authorized administrator of DigitalCommons@URI. For more information, please contact [email protected]. PERFORMANCE OF A NOVEL SUSTAINABLE BINDER UNDER EXTREME DYNAMIC LOADING CONDITIONS BY PAUL DAVID SCHMIDT A THESIS SUBMITTED IN PARTIAL FULFILLMENT OF THE REQUIREMENTS FOR THE DEGREE OF MASTER OF SCIENCE IN CIVIL AND ENVIRONMENTAL ENGINEERING UNIVERSITY OF RHODE ISLAND 2017 MASTER OF SCIENCE OF PAUL DAVID SCHMIDT APPROVED: Thesis Committee: Major Professor Sumanta Das George Tsiatas Arun Shukla Nasser H. Zawia DEAN OF THE GRADUATE SCHOOL UNIVERSITY OF RHODE ISLAND 2017 ABSTRACT Iron Carbonate is a novel carbon-negative sustainable binder that is made from metallic iron powder waste and utilizes the chemistry of iron carbonation. To produce the binder, usually landfilled iron powder and other constituents (fly ash, limestone powder, metakaolin, sodium carbonate, sodium bicarbonate, powdered organic reducing agent, and water) are mixed together and exposed to a pressurized CO2 regime that leads to slow external diffusion. The carbonation of iron particles results in the formation of complex iron carbonates that have binding capabilities and mechanical properties similar or better compared to ordinary Portland cement (OPC)- based binders. -
Magnesium Oxychloride Cement with Partial Replacement of Fly Ash and Magnesium Sulphate
International Research Journal of Engineering and Technology (IRJET) e-ISSN: 2395-0056 Volume: 07 Issue: 02 | Feb 2020 www.irjet.net p-ISSN: 2395-0072 Magnesium Oxychloride Cement with partial replacement of fly ash and Magnesium Sulphate Vignesh R1, Suresh Babu KP2, Vengadesh P3, Sriram S4, Selvam B5 1234UG Student, 5Assistant Professor, Department of Civil Engineering, Sree Sakthi Engineering College, Coimbatore, India ---------------------------------------------------------------------***---------------------------------------------------------------------- Abstract – Magnesium Oxychloride Cement with addition of The well crystallized needle-like structure of phase 5 of fly ash has been evaluated. MOC Fly ash mix material with chemically bonded MOC has been described as scroll-tubular various composition of fly ash having good workability and whiskers. The mechanical interlocking and unique fibrous attains early strength. MOC Fly ash mix attains 20-68 MPa as microstructure resulting from the intergrowth of the crystals compressive strength after the air curing. Concrete sets within is a major source for the strength development of MOC 4hrs. Very good aggregate-cement bonding and excellent cement. Therefore, the physical properties of MOC cement failure patterns are observed. Fly ash as 20% addition with the depend largely on the phase’s formation and subsequently MgO gives high strength with comparing other combinations. on the appropriate proportions of the starting materials. (Karthikeyan N 2014) Key Words: MOC Fly ash mix, fly ash, Chemical reaction, Magnesium Sulphate, Compressive strength. 1.2 Scope of research 1.INTRODUCTION MOC cement draws much research interests recently due to the energy saving consideration as it can be used as Portland Magnesium Oxychloride Cement (MOC, Sorel’s cement/ cement replacement on many occasions.