Furnace Atmospheres No. 6. Sintering of Steels
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On Increasing Powder Carbon Steels Properties Using Activating Additives
Int. J. of Applied Mechanics and Engineering, 2020, vol.25, No.2, pp.192-201 DOI: 10.2478/ijame-2020-0029 Brief note ON INCREASING POWDER CARBON STEELS PROPERTIES USING ACTIVATING ADDITIVES L. DYACHKOVA O.V. Roman Powder Metallurgy Institute Belarusian National Academy of Sciences 41, Platonov st., 220005 Minsk, BELARUS E-mail: [email protected] In this paper, the possibility of increasing powder carbon steels properties by activation of carbon diffusion into the iron base during sintering process due to the introduction of the thermally split graphite (TSG), macromolecular compounds (MC) and sodium bicarbonate was investigated. It was found that the introduction of these additives allows obtaining homogeneous structures at a sintering temperature of 100–200 °C lower than that traditionally used for sintering of powder carbon steels. Such structures provide increased mechanical properties of powder carbon steels. The addition of sodium bicarbonate increases the diffusion rate of carbon into iron at a temperature of 950 C by 1.8 times, at 1000 °C by 1.5 times, and at 1100 °C by 1.2 times. Key words: powder carbon steels, activating additives, structure, mechanical properties. 1. Introduction Powder metallurgy is one of the most progressive processes for parts manufactured for various purposes. Numerous technological processes of powder metallurgy can reduce the consumption of materials, manufacturing energy and allow automation of the process. The necessary combination of manufacturability and reliability of parts, as well as obtaining the required material properties, are ensured by controlling the processes of structure formation. The structure and properties of powder carbon steels, in which carbon is the main alloying element, depend on the degree of homogeneity of the structure formed during sintering. -
"J ;70 Potential New Sensor for Use with Conventional Gas Carburizing
/,,"J _;70 NASA Contractor Report 202306 Potential New Sensor for Use With Conventional Gas Carburizing W.A. de Groot NYMA Inc. Brook Park, Ohio January 1997 Prepared for Lewis Research Center Under Contract NAS3-27186 National Aeronautics and Space Administration Potential New Sensor for Use with Conventional Gas Carburizing W.A. de Groot NYMA Inc., Brook Park, Ohio Abstract The working p'rmciple of most endothermic gas generators is based on passing a mixture of natural gas and air over a heated catalyst. The comb'marion of heat and Diagnostics developed for in-situ monitoring of rocket combustion environments have been adapted for use in heat catalyst converts the air and natural gas into the endothermic treating furnaces. Simultaneous, in-situ monitoring of the gas mixture (a purely catalytic reaction, no combustion). The carbon monoxide, carbon dioxide, methane, water, nitrogen composition of this endothermic gas, and the percentages of carbon monoxide and methane critical for carburization, and hydrogen concentrations in the endothermic gas of a heat varies as a result of fluctuations in composition of the natural treating furnace has been demonsWated under a Space Act gas supply, gas/air ratio, the condition of the catalyst bed, and Agreement between NASA Lewis, the Heat Treating other variables. This in turn leads to a variation in carbon Network, and Akron Steel Treating Company. Equipment installed at the Akron Steel Treating Company showed the potential which could lead to an unacceptable quality of the feasibility of the method. Clear and well-defined spectra of steel product. Adequate monitoring and control of the gas composition carbon monoxide, nitrogen and hydrogen were obtained by means of an optical probe mounted on the endothermic gas of the protective atmosphere is required to ensure product line of a gas generator inside the plant, with the data quality. -
Electrons, Life and the Evolution of Earth's Chemical Cycles
Electrons, Life and the Evolution of Earth’s Chemical Cycles OCN 623 – Chemical Oceanography 23 April 2013 Adaption of Brian Glazer lecture (based on Falkowski and Godfrey (2008) Phil. Trans. R. Soc. B, 363: 2705-2716) © 2013 F.J. Sansone Outline Earth’s geological, geochemical and biological co- evolution since formation - Early Earth - Origins of life - The great oxidation event - Linkage between global O and N cycles - Alternate explanations for the great oxidation event - The rise of oxygen and the evolution of life - The Phanerozoic How Does the Earth Work as a Biosphere? All organisms derive energy for growth and maintenance by moving electrons from a substrate to a product All substrates and products must ultimately be recycled All metabolic processes on Earth are prokaryotic and were developed in the Archean and/or Proterozoic Eons Earth’s Geological, Geochemical and Biological Co-evolution Since Formation Earth, ~3.5 Ga Ago • Earth cools to <100˚C • Shallow sea environment – Land covered by low egg- shaped hills and pillow lavas – Silt layers – Scattered volcanic islands and evaporite lagoons • Tides higher – Moon closer to Earth, days shorter • Atmosphere –CO2-rich, no O2 – UV-drenched landscape Faint Sun Paradox High atmospheric CO2 and CH4 important in early Earth -- balanced weak Sun to maintain temp Recycling of Atmospheric CO2 Liquid water on early Earth allowed a hydrologic cycle, carbonate and silicate mineral weathering to develop: 2+ - CaCO3 + CO2 + H2O = Ca + 2HCO3 2+ - CaSiO3 +2CO2 +3H2O = Ca + 2HCO3 + H4SIO4 Uptake -
Is Extraterrestrial Organic Matter Relevant to the Origin of Life on Earth?
IS EXTRATERRESTRIAL ORGANIC MATTER RELEVANT TO THE ORIGIN OF LIFE ON EARTH? D. C. B. WHITTET Department of Physics, Applied Physics and Astronomy, Rensselaer Polytechnic Institute, Troy, NY 12180, U.S.A. (Received 19 August 1996) Abstract. I review the relative importance of internal and external sources of prebiotic molecules on Earth at the time of life's origin 3.7 Gyr ago. The ef®ciency of synthesis in the Earth's atmosphere was critically dependent on its oxidation state. If the early atmosphere was non-reducing and CO2- dominated, external delivery might have been the dominant source. Interplanetary dust grains and micrometeorites currently deliver carbonaceous matter to the Earth's surface at a rate of 3 5 7 10 kg/yr (equivalent to a biomass in 2 Gyr), but this may have been as high as 5 10 kg/yr (a biomass in only 10 Myr) during the epoch of late bombardment. Much of the incoming material is in the form of chemically inactive kerogens and amorphous carbon; but if the Earth once had a dense (10-bar) atmosphere, small comets rich in a variety of prebiotic molecules may have been suf®ciently air-braked to land non-destructively. Lingering uncertainties regarding the impact history of the Earth and the density and composition of its early atmosphere limit our ability to draw ®rm conclusions. 1. Introduction In at least one sense, a connection between the Universe at large and life in our small corner of it is inevitable. The hydrogen, carbon, nitrogen, oxygen, and other elements that make up our bodies and other living things were created billions of years ago in the interiors of stars and, in the case of hydrogen, in the the Big Bang itself (see Trimble, 1997, in this volume for an eloquent review). -
Life in the Outer Solar System Jupiter
Life in the Outer Solar System Jupiter Big R = 11R⊕ Massive M = 300 M⊕ = 2.5 all the rest Thick Atmosphere Mostly H2, He But also more complex molecules Colors, storms Like Miller - Urey Life in Jupiter Atmosphere? Sagan-Salpeter, etc. Sinkers (Plankton) Floaters (Fish) Hunters (Fish) Galileo Results on Jupiter Reached Jupiter Dec. 1995 Sent probe into Jupiter’s atmosphere at 100,000 mile/hour Decelerated at 230 g Lasted for 57 min. Found: Strong winds Turbulence, little lightning Life less likely? Surprise: Little or no H2O May have entered in an unusual place (fewer clouds) Europa (Moon of Jupiter) Surface: Fractured Ice Subsurface Oceans? (Heated from Inside) Close-up of “ice floes” Galileo - Jupiter’s Moons http://www.jpl.nasa.gov/galileo/index.html Europa has a (THIN!) atmosphere UV H H H O=O T hin O O2 H2O ATM Pressure ~ 10–11 Earth More evidence for resurfacing along cracks by “ice geysers” fluid ice or liquid water Organic molecules on Callisto & Ganymede, maybe Europa? Saturn • Big (9.4 R⊕) • Massive (95 M⊕) • Year 29.5 years • Day 0.43 days • Composition similar to Jupiter Titan • Moon of Saturn • Diameter ~0.4 Earth • Atmospheric Pressure = 1.5 × Earth • 85% Nitrogen BUT • Cold (~90 K) • Reducing atmosphere • Haze • Lab for prebiotic chemistry The Cassini-Huygens Mission • Launched 10/13/97 • Arrived Saturn 7/2004 • Cassini studies – Saturn – Moons • Huygens – Dropped onto Titan – Study atmosphere – Surface CASSINI SPACECRAFT Huygens Probe • Released from Cassini • Slowed by heat shield • Parachute deploys • Soft landing • Sample -
REOXIDATION of SPONGE IRON IS an EXOTHERMIC PROCESS DUE to REMOVAL of HYDROGEN‖ Prof
International Journal Of advance research in Science and Engineering http://www.ijarse.com (IJARSE) 2012, Vol. No.1, Issue No. I, July ISSN-2319-8354 ―REOXIDATION OF SPONGE IRON IS AN EXOTHERMIC PROCESS DUE TO REMOVAL OF HYDROGEN‖ Prof. Pushpendra Kumar Sharma1, Neeraj Singh Rajput2, Prof. Sachin Jain3 1Head Mechanical Engineering Department, NIIST, Bhopal 2Post Graduate Student, NIIST, Bhopal 3Asst. Professor, NIIST, Bhopal [email protected] Abstract— In the present era scarcity of high grade coal, high valuable process of coke production is a headache. So to get release from this problem huge amount of electric arc furnace and sponge iron production is increased. Sometimes Sponge iron transportation is a problematic situation, because during transportation chances of spontaneous burning of sponge iron are found, that is the effect of re-oxidation of sponge iron. Re-oxidation of sponge iron phenomenon refers to oxidation of metallic sponge iron in moisture condition. Metallic iron forms a strongly bonded Fe (OH)2 compound which causes increase in mass of sponge iron. The re-oxidation phenomenon is an exothermic process. Sponge iron is spongy in structure having large in porous area. Thus it is very much reactive and seeks for high oxidation. So the sponge iron produced is highly susceptible to re-oxidation. So it is important to study the kinetic of sponge iron re-oxidation. Keywords—Sponge iron, Iron ore, Coal, Dolomite, Power unit for initial power consuming unit. INTRODUCTION The conventional route for making steel consists of sintering/pelletization plants, ovens, blast and basic oxygen furnaces. Such plants need huge capital expenses and raw materials as they are the stringent requirements. -
(5) Field: Session Topic: Speaker
(5) Field: Earth Science/Geoscience/Environment Session Topic: Stable Isotopes in Earth and Space Science Speaker: Shogo Tachibana, The University of Tokyo 1. Introduction The present Earth’s atmosphere is made up of 78% of nitrogen, 21% of oxygen (we breathe oxygen to live!), and 1% of other gases. However, the present oxygen-rich atmosphere is not the Earth’s original atmosphere. The atmosphere changed its chemical composition in the history of Earth. The present oxygen-rich atmosphere was built up by photosynthesis of cyanobacteria, and it has been known that the Earth’s atmosphere contained almost no oxygen in the Archean (>2.5 billion years ago (Ga)). There have been several geological indicators for the atmospheric oxygen level such as presence of detrital pyrite and uraninite in sedimentary rocks for the reducing atmosphere and presence banded iron formations and red beds for the oxidizing atmosphere. Geological records for transition from the reducing atmosphere to the oxidation atmosphere (Great Oxygenation Event) have been found in the Paleoproterozoic sedimentary rocks. 2. Mass-independent fractionation of sulfur isotopes and its relation to the atmospheric chemistry Sulfur has four stable isotopes (32S, 33S, 34S, and 36S). Their average relative abundances in the solar system are 95.02%, 0.75%, 4.22%, and 0.017% for 32S, 33S, 34S, and 36S, respectively, but they can be varied by various physical, chemical, and/or biological processes. The variations of relative abundances of 32S and 34S in minerals or rocks have been used to understand geological and biological processes on the Earth. Other two minor isotopes (33S and 36S) had not been measured intensively because their relative abundances were assumed to vary with following the mass-dependent fractionation law. -
Laboratory-Scale Investigation of the Removal of Hydrogen Sulfide From
Laboratory-scale investigation of the removal of hydrogen sulfide from biogas and air using industrial waste-based sorbents Olumide Wesley Awe, Doan Pham Minh, Nathalie Lyczko, Ange Nzihou, Yaqian Zhao To cite this version: Olumide Wesley Awe, Doan Pham Minh, Nathalie Lyczko, Ange Nzihou, Yaqian Zhao. Laboratory- scale investigation of the removal of hydrogen sulfide from biogas and air using industrial waste- based sorbents. Journal of Environmental Chemical Engineering, Elsevier, 2017, 5 (2), p.1809-1820. 10.1016/j.jece.2017.03.023. hal-01619255 HAL Id: hal-01619255 https://hal.archives-ouvertes.fr/hal-01619255 Submitted on 20 Oct 2018 HAL is a multi-disciplinary open access L’archive ouverte pluridisciplinaire HAL, est archive for the deposit and dissemination of sci- destinée au dépôt et à la diffusion de documents entific research documents, whether they are pub- scientifiques de niveau recherche, publiés ou non, lished or not. The documents may come from émanant des établissements d’enseignement et de teaching and research institutions in France or recherche français ou étrangers, des laboratoires abroad, or from public or private research centers. publics ou privés. Laboratory-scale investigation of the removal of hydrogen sulfide from biogas and air using industrial waste-based sorbents a,b, b, b b Olumide Wesley Awe *, Doan Pham Minh **, Nathalie Lyczko , Ange Nzihou , a Yaqian Zhao a Dooge Centre for Water Resources Research, School of Civil Engineering, University College Dublin, Newstead, Belfield, Dublin 4, Ireland b Universite’ de Toulouse, Mines Albi, CNRS UMR 5302, Centre RAPSODEE, Campus Jarlard, Albi, F-81013 cedex 09, France A B S T R A C T Biogas is a valuable renewable energy that can be used as a fuel or as raw material for the production of hydrogen, synthesis gas and chemicals. -
Vacuum & Atmosphere Endothermic Gas Generator
The Marketplace for Surface Technology. New and Used Process Equipment & Machinery. Home > Ovens & FurnacesIndustrial Furnaces > Vacuum & Atmosphere Endothermic Gas Generator Stock Code: OU1469 Model: Endothermic Gas Generator New or Used: Used (Second Hand) Other Info: Endogas 20 - 60 m³/hr output Weight: 1300 External Dimensions (WxDxH): 1200 x 1600 x 2650 Vacuum & Atmosphere Endothermic Gas Generator The endothermic generator creates an atmosphere to provide a positive pressure in a heat treating furnace, and a platform on which a carburizing or decarburizing environment can be formulated, by addition of enriching gas or dilution air. This tried and tested design has been based upon the IPSEN G2000 Endothermic Gas Generator Introduction Vacuum & Atmosphere endothermic gas generators are used to produce atmospheres necessary for the scale free hardening, carburizing and carbon restoration of steel as well as the cover gas for the annealing of copper and for the silver brazing and sintering processes. Riley Industries Ltd A subsidiary of Barry Riley & Sons Ltd. Directors: R T Barry Riley, M P A Riley, Secretary: J C Riley Registered in England no. 1965748 Page 1/2 The Marketplace for Surface Technology. New and Used Process Equipment & Machinery. Home > Ovens & FurnacesIndustrial Furnaces > Vacuum & Atmosphere Endothermic Gas Generator A typical use would be in the case hardening of steel gears where the carbon content of the steel has to be tightly controlled. Endothermic generators built by Vacuum & Atmosphere are compact, air cooled, efficient and reliable producers of these atmospheres. An endothermic generator is comprised of a heavily insulated, heated chamber; a nickel catalyst filled retort; a feedstock gas metering system, a chamber heating system and an output gas cooling system. -
High Temperature, Reducing Atmosphere, Continuous Furnaces to 1800°C (3272°F)
industrial and laboratory furnaces www.cmfurnaces.com HIGH TEMPERATURE, REDUCING ATMOSPHERE, CONTINUOUS FURNACES TO 1800°C (3272°F) The CM 300 Series furnaces are available in a variety the 300 Series muffle design furnaces. When automated of configurations from manually loaded lab-scale units the pusher plates (carrier trays) form a train and are to fully automated production systems. These furnaces pushed through the furnace by an external stoker employ a molybdenum wound aluminum oxide muffle, device. All automation is located outside the heat typically D-shaped, designed to operate from 800°C envelope for ease of maintenance and long life. (1472°F) to 1700°C (3100°F) on the standard models Hydrogen, dissociated ammonia, forming gas or any and as high as 1800°C (3272°F) for special applications. other reducing atmosphere compatible the refractory The base model includes inclined doors with protective metal heating elements can be employed. The standard atmosphere flushes, high heat section, and a cooling gas panel includes all necessary pressure regulators, section. Depending on application requirements other flow meters, solenoids and pressure switches for both features are added such as preheat sections, binder primary processing atmosphere and standby safety removal sections, multiple zone controls, low or high nitrogen. All furnaces come complete with the CM dewpoint features, and turn-key automated pusher combustion atmosphere safety system. Full details are systems. available on request. The furnaces are constructed of heavy gauge steel that Temperature control is by microprocessor based is welded and reinforced. All power components and setpoint controllers operating in conjunction with controls are located on the main frame assembly. -
Atmospheric Nitrogen Evolution on Earth and Venus
Atmospheric nitrogen evolution on Earth and Venus The Harvard community has made this article openly available. Please share how this access benefits you. Your story matters Citation Wordsworth, R.D. 2016. “Atmospheric Nitrogen Evolution on Earth and Venus.” Earth and Planetary Science Letters 447 (August): 103–111. doi:10.1016/j.epsl.2016.04.002. http://dx.doi.org/10.1016/ j.epsl.2016.04.002. Published Version doi:10.1016/j.epsl.2016.04.002 Citable link http://nrs.harvard.edu/urn-3:HUL.InstRepos:27846862 Terms of Use This article was downloaded from Harvard University’s DASH repository, and is made available under the terms and conditions applicable to Open Access Policy Articles, as set forth at http:// nrs.harvard.edu/urn-3:HUL.InstRepos:dash.current.terms-of- use#OAP Atmospheric nitrogen evolution on Earth and Venus R. D. Wordsworth Harvard Paulson School of Engineering and Applied Sciences, Harvard University, Cambridge, MA 02138, Department of Earth and Planetary Sciences, Harvard University, Cambridge, MA 02138 Abstract Nitrogen is the most common element in Earth’s atmosphere and also appears to be present in significant amounts in the mantle. However, its long-term cycling between these two reservoirs remains poorly understood. Here a range of biotic and abiotic mechanisms are evaluated that could have caused nitrogen exchange between Earth’s surface and interior over time. In the Archean, biological nitrogen fixation was likely strongly limited by nutrient and/or electron acceptor constraints. Abiotic fixation of dinitrogen becomes efficient in strongly reducing atmospheres, but only once temperatures exceed around 1000 K. -
Formation of Amino Acids and Nucleotide Bases in a Titan Atmosphere Simulation Experiment
ASTROBIOLOGY Volume 12, Number 9, 2012 Research Article ª Mary Ann Liebert, Inc. DOI: 10.1089/ast.2011.0623 Formation of Amino Acids and Nucleotide Bases in a Titan Atmosphere Simulation Experiment S.M. Ho¨rst,1,2 R.V. Yelle,2 A. Buch,3 N. Carrasco,4 G. Cernogora,4 O. Dutuit,5 E. Quirico,5 E. Sciamma-O’Brien,6 M.A. Smith,7,8 A´ . Somogyi,8 C. Szopa,4 R. Thissen,5 and V. Vuitton5 Abstract The discovery of large ( > 100 u) molecules in Titan’s upper atmosphere has heightened astrobiological interest in this unique satellite. In particular, complex organic aerosols produced in atmospheres containing C, N, O, and H, like that of Titan, could be a source of prebiotic molecules. In this work, aerosols produced in a Titan atmosphere simulation experiment with enhanced CO (N2/CH4/CO gas mixtures of 96.2%/2.0%/1.8% and 93.2%/5.0%/ 1.8%) were found to contain 18 molecules with molecular formulae that correspond to biological amino acids and nucleotide bases. Very high-resolution mass spectrometry of isotopically labeled samples confirmed that C4H5N3O, C4H4N2O2,C5H6N2O2,C5H5N5, and C6H9N3O2 are produced by chemistry in the simulation chamber. Gas chromatography–mass spectrometry (GC-MS) analyses of the non-isotopic samples confirmed the presence of cytosine (C4H5N3O), uracil (C5H4N2O2), thymine (C5H6N2O2), guanine (C5H5N5O), glycine (C2H5NO2), and alanine (C3H7NO2). Adenine (C5H5N5) was detected by GC-MS in isotopically labeled samples. The remaining prebiotic molecules were detected in unlabeled samples only and may have been affected by contamination in the chamber.