Thermodynamics Simulation Performance of Rice Husk Combustion with a Realistic Decomposition Approach on the Devolatilization Stage

Total Page:16

File Type:pdf, Size:1020Kb

Thermodynamics Simulation Performance of Rice Husk Combustion with a Realistic Decomposition Approach on the Devolatilization Stage Thermodynamics simulation performance of rice husk combustion with a realistic decomposition approach on the devolatilization stage Soen Steven Institut Teknologi Bandung Pandit Hernowo Institut Teknologi Bandung Elvi Restiawaty Institut Teknologi Bandung Anton Irawan Universitas Sultan Ageng Tirtayasa Carolus Borromeus Rasrendra Institut Teknologi Bandung Yazid Bindar ( [email protected] ) Institut Teknologi Bandung Research Article Keywords: Biomass, Degree of freedom, Flue gas, Adiabatic ame temperature, Air to fuel ratio Posted Date: April 14th, 2021 DOI: https://doi.org/10.21203/rs.3.rs-359990/v1 License: This work is licensed under a Creative Commons Attribution 4.0 International License. Read Full License Thermodynamics simulation performance of rice husk combustion with a realistic decomposition approach on the devolatilization stage Soen Steven1, Pandit Hernowo1, Elvi Restiawaty1,2, Anton Irawan5, Carolus Borromeus Rasrendra1,3, and Yazid Bindar1,4* 1Department of Chemical Engineering 2Research Group on Design and Development of Chemical Engineering Processes 3Center for Catalysis and Reaction and Engineering 4Research Group on Biomass and Food Processing Technology Faculty of Industrial Technology, Institut Teknologi Bandung, Jl. Ganesha 10, Bandung 40132, Indonesia 5Chemical Engineering Department, Faculty of Engineering, Universitas Sultan Ageng Tirtayasa, Jl. Jendral Soedirman km 3 Cilegon, Banten, 42135, Indonesia * Corresponding author: [email protected] Abstract Rice husk has a great potential in its calorific value and silica content in ash which makes its valorization through combustion becomes important and interesting. This study presents the thermodynamics simulation performance of rice husk combustion using a realistic decomposition approach. A non-ideal gas approach and fugacity coefficient were also considered in the calculation. From this study, rice husk is devolatilized to form gases (63.37%), tar (8.69%), char (27.94%), and all of these are then oxidized to form flue gas. The realistic decomposition approach calculated that about 2.6 MJ/kg of specific combustion energy is produced, the maximum combustion temperature is up to 1457oC for perfect insulation condition, and up to 1400oC if there is a heat loss. It is found that combustion equipped with larger excess air could quench the heat produced and reduce the combustion efficiency but could maintain the temperature at 700oC. Furthermore, the thermodynamics simulation expressed that NO emission amount from rice husk combustion is negligible and there is still a probability for CO o and H2 to be produced at above 500 C due to Boudouard reaction and homogeneous water gas shift reaction (WGSR). The study showed that a realistic decomposition approach could predict the rice husk combustion performance with a reasonable and logical result. Supplying excess air of about 180-200% is advantageous to keep the combustion temperature at 700oC in order to prevent silica crystalline formation which harms human 1 health, as well as suppressing NO emission and reducing CO emission from the simultaneous Boudouard and WGSR. Keywords: Biomass, Degree of freedom, Flue gas, Adiabatic flame temperature, Air to fuel ratio Statement of Novelty So far, many established simulations have proposed a simple approach to the devolatilization stage. This is unrealistic because assumes that biomass will decompose to C, H, O, N elements before entering oxidation. In the realistic decomposition approach, biomass is devolatilized not to form C, H, O, N elements but light gases, liquid as tar, and solid as char. Interestingly, there is still a lack of study on it and therefore, This study discussed the rice husk combustion simulation performance with a realistic decomposition approach on the devolatilization stage. The results perform that this approach gives a reasonable agreement with the other researchers’ results in terms of specific combustion energy, maximal combustion temperature, and flue gas composition analysis. 1. Introduction Recently, biomass utilization as an alternative fossil fuel and chemicals surrogates has become a major concern. Rice husk is one of the abundant biomass in Indonesia which occupies approximately 20%-wt from paddy, consists of nearly 20%-wt rice husk ash, contains silica as much as 87%-wt from its ash, and has a calorific value of 14-17 MJ/kg [1–3]. The high calorific value, as well as rich silica in ash, make rice husk important and interesting to be valorized. There are several stages occurred in the rice husk combustion, that is drying, devolatilization, oxidation, and ash formation [1, 4, 5]. So far, energy production through rice husk combustion mostly relied on direct experiments and then validate the results with thermodynamics simulation. They have focused on specific combustion energy calculation, rice husk combustion temperature monitoring, and flue gas composition prediction and analysis. A study on combined heat power fuelled by rice husk with a maximal temperature of about 1100oC gave a specific rice husk consumption of 1.2-1.7 kg/kWh [6] or recalculated as specific energy produced in the range of 2.12- 3.00 MJ/kg. Apart from that, the case study from Pakistan stated that as much as 4947.28 MWh of energy could be generated from 6432 tonnes of rice husk combustion [7] or equal to specific combustion energy of about 2.77 MJ/kg. The energy balance evaluation on 2.8 g/s rice husk combustion for steam and hot air generation resulted 2 in 21.09 kJ/s of utilized energy [8] and it is equal to 7.53 MJ/kg of specific energy. Meanwhile, the rice husk combustion modelling study in a grate bed furnace had a maximum combustion temperature of 1406.85oC and o flue gas exhaust temperature of 693.85 C with the composition of N2, CO, CO2, H2O, and remaining O2 [9]. The thermodynamics study from the research papers and well-established textbooks mostly proposed that at the devolatilization stage, biomass will decompose to C, H, O, N elements prior to being oxidized to form flue gas [10–12]. This approach is simple but quite unrealistic so that it should be developed with a more realistic one. Realistic decomposition assumes that rice husk devolatilization products are not C, H, O, N elements but gases, tar, and char [10]. Nevertheless, there is still a lack of study on it and therefore, this study intends to discuss the thermodynamics simulation performance of rice husk combustion with a realistic decomposition approach. The discussion comprises of problem preliminary analysis, devolatilized products result, specific energy produced from rice husk combustion, adiabatic flame temperature, air supply strategy for maintaining rice husk combustion temperature, and the flue gas composition analysis due to the attendance of Boudouard reaction and homogeneous water gas shift reaction (WGSR). 2. Methods 2.1. Devolatilized products prediction calculation In this study, rice husk has a calorific value of 14.95 MJ/kg. The ultimate and proximate analysis results are given in Table 1. The proximate analysis procedure is performed at 900oC follows ASTM 3175-07 procedure, whereas the combustion occurred at = 700oC. 푇Table 1. Ultimate and proximate analyses of rice husk Ultimate Analysis (Dry Basis) Proximate Analysis (As-received) C 37.95% Moisture 8.98% H 5.41% Volatile Matter 58.13% O 36.56% Fixed Carbon 15.49% N 0.96% Ash 17.40% A volatile enhancement factor , which is commonly found in 0.8-1.3, plays a role to correct the devolatilized product at a temperature beyond푉퐸 900oC [10, 11]. To determine , the biomass type number ( ) should be calculated first as in equation 1a. The value is then applied to푉 퐸determine the predicted volatile푁퐶푇 matter value ( ), equation 1b. Subsequently, equation푁퐶푇 1c is a temperature correction function, in oC unit, which is later ′ employed푌푉푀 in equation 1d to obtain the predicted devolatilized products mass fraction푓5(푇) ( ). Afterward, is ′ calculated following equation 1e [10, 11]. Rice husk devolatilization produces gases, tar,푌 푉푌and char. Gases 푉were퐸 3 represented with CO, H2, CO2, CH4, HCN, and H2O. Tar was assumed to consist of C16H18, C10H14O2, C7H8O, and C9H7N. Char was presumed to contain only C. Each product amount is determined from equation 2 and should consistent with the value from dry-ash-free basis of proximate and ultimate analysis [10, 11]. (1a) 2 퐶,푢푙푡 퐶푇 푌 푁 = 퐻,푢푙푡 푂,푢푙푡 (1b) ′ 푌 . 푌 2 푉푀 퐶푇 퐶푇 (1c) 푌 = 푒푥푝[0.031 −5 0.029 푙푛 푁 − 0.4038(푙푛 푁 ) ] 3 2 푇 푇 푇 푇 푇 푓5(푇) = 3.87 ( ) − 28.28 ( ) + 80.87 ( ) − 112.8 ( ) + 77.07 ( ) − 20.26 (1d) ′ ′ 900 900 900 900 900 푉푌 푉푀 5 (1e) 푌 = 푌′ . 푒푥푝[푓 (푇)] 푌푉푌 푌푉푌 푉퐸 = ′ = 푌푉푀 푌푉푀 (2a) 푐ℎ푎푟 푉푌 푖 푌 = 1 − 푌 = 1 − ∑ 푌 (2b) 푌퐶,푖. 퐴푟퐶 푌퐶,푢푙푡 = 푌푐ℎ푎푟 + ∑ ( ) 푀푟푖 (2c) 푌퐻,푖. 퐴푟퐻 푌퐻,푢푙푡 = ∑ ( ) 푀푟푖 (2d) 푌푂,푖. 퐴푟푂 푌푂,푢푙푡 = ∑ ( ) 푀푟푖 (2e) 푌푁,푖. 퐴푟푁 푁,푢푙푡 푌 = ∑ ( 푖 ) where is the푀푟 actual devolatilized products mass fraction, is the volatile matter value from proximate analysis푌 푉푌on dry-ash-free basis, is the ith component of actual 푌devolatilized푉푀 products mass fraction, is the char fraction, is the number푌 푖of C atoms in ith component, is the number of H atoms in ith component,푌푐ℎ푎푟 퐶,푖 퐻,푖 푂,푖 is the number 푌of O atoms in ith component, is the number푌 of N atoms in ith component, is the C-H-O-푌N 푁,푖 푢푙푡 content ultimate analysis in dry-ash-free basis,푌 is the atomic weight for C-H-O-N, and 푌 is the molecular weight of ith component. 퐴푟 푀푟푖 In the rice husk combustor, all devolatilized products react with oxygen from the air. The air amount was varied under stoichiometric and excess conditions. The flue gas temperature was also varied from 200-700oC. The excess air ( ) is calculated from equation 3 and the O2 and CO2 percentages in the flue gas are acquired from equation 4, respectively.퐸퐴 (3) 푛푎 − 푛푠 퐸퐴 = 푥 100% 푛푠 (4a) 푛푂2,푎 − 푛푂2,푠 푂2 푖푛 푓푙푢푒 푔푎푠 = 푥 100% 푛푓푔 (4b) 푛퐶푂2 퐶푂2 푖푛 푓푙푢푒 푔푎푠 = 푥 100% 푛푓푔 4 where is the actual air amount; is the stoichiometric air amount; is the actual oxygen amount; is 푎 푠 푂2,푎 푂2,푠 the stoichiometric푛 oxygen amount;푛 and is the carbon dioxide amount;푛 and is the flue gas amount.푛 퐶푂2 푓푔 푛 푛 2.2.
Recommended publications
  • Hypothesis Paper Many Chemistries Could Be Used to Build Living
    ASTROBIOLOGY Volume 4, Number 2, 2004 © Mary Ann Liebert, Inc. Hypothesis Paper Many Chemistries Could Be Used to Build Living Systems WILLIAM BAINS ABSTRACT It has been widely suggested that life based around carbon, hydrogen, oxygen, and nitrogen is the only plausible biochemistry, and specifically that terrestrial biochemistry of nucleic acids, proteins, and sugars is likely to be “universal.” This is not an inevitable conclusion from our knowledge of chemistry. I argue that it is the nature of the liquid in which life evolves that defines the most appropriate chemistry. Fluids other than water could be abun- dant on a cosmic scale and could therefore be an environment in which non-terrestrial bio- chemistry could evolve. The chemical nature of these liquids could lead to quite different biochemistries, a hypothesis discussed in the context of the proposed “ammonochemistry” of the internal oceans of the Galilean satellites and a more speculative “silicon biochemistry” in liquid nitrogen. These different chemistries satisfy the thermodynamic drive for life through different mechanisms, and so will have different chemical signatures than terrestrial biochemistry. Key Words: Carbon, hydrogen, oxygen, and nitrogen life—Planetary liquid— Silicon. Astrobiology 4, xxx–xxx. INTRODUCTION ISCUSSIONS of nonterrestrial life generally as- Dsume that the biochemistry of life will be similar to that which we see on Earth. Almost all There is a famous book published about writers assume that carbon is the central element 1912 by Lawrence J. Henderson . in which in any plausible biochemistry, and that its com- Henderson concludes that life necessarily bination with hydrogen, nitrogen, and oxygen is must be based on carbon and water, and the core of any living system.
    [Show full text]
  • Geology 111 – Discovering Planet Earth
    Geology 111 – Discovering Planet Earth A1) Early History of the Earth The earth and the rest of the solar system were formed about 4.57 billion years ago from an enormous cloud of fragments of both icy and rocky material which was produced from the explosions (super novae) of one or more large stars - [see page 11]1. It is likely that the proportions of elements in this material were generally similar to those shown in the diagram below. Although most of the cloud was made of hydrogen and helium, the material that accumulated to form the earth also included a significant amount of the heavier elements, especially elements like carbon, oxygen, iron, aluminum, magnesium and silicon2. As the cloud started to contract, most of the mass accumulated towards the centre to become the sun. Once a critical mass had been reached the sun started to heat up through nuclear fusion of hydrogen into helium. In the region relatively close to the sun - within the orbit of what is now Mars - the heat was sufficient for most of the lighter elements to evaporate, and these were driven outward by the solar wind to the area of the orbits of Jupiter and the other gaseous planets. As a result, the four inner planets - Mercury, Venus, Earth and Mars are "rocky" in their composition, while the four major outer planets, Jupiter, Saturn, Neptune and Uranus are "gaseous". As the ball of fragments and dust that was to eventually become the earth grew, it began to heat up - firstly from the heat of colliding particles - but more importantly from the heat generated by radioactive decay (fission) of uranium, thorium, and potassium (figure below).
    [Show full text]
  • 19126634.Pdf
    View metadata, citation and similar papers at core.ac.uk brought to you by CORE provided by Estudo Geral Analytical Biochemistry 385 (2009) 176–178 Contents lists available at ScienceDirect Analytical Biochemistry journal homepage: www.elsevier.com/locate/yabio Notes & Tips Biosensor plates detect mitochondrial physiological regulators and mutations in vivo Anabela P. Rolo a, Carlos M. Palmeira a, Gino A. Cortopassi b,* a Cen ter for Neu ro sci ences and Cell Biol ogy, Depart ment of Zool ogy, Uni ver sity of Coim bra, 3004-517 Coim bra, Por tu gal b VM: Molec u lar Bio sci ences, Uni ver sity of Cal i for nia at Davis, 1 Shields Ave nue, Davis, CA 95616, USA article info abstract Article history: The mea sure ment of mito chon drial activ ity in living cells is usu ally not straight for ward, even though Received 15 September 2008 it is quite impor tant in phys i o log i cal and path o phys i o log i cal pro cesses. We describe a high-through put Available online 7 October 2008 method for mea sure ment of mito chon drial oxy gen con sump tion in living cells, based on the Bec ton– Dick in son Bio sen sor plates. © 2008 Else vier Inc. All rights reserved. Mito chon dria are the primary energy-gen er at ing sys tem in The Bec ton–Dick in son Bio sen sor plates were orig i nally most eukary otic cells. As the site of oxi da tive phos phor y la tion, described in 2000 [2] and have been used mostly to mon i tor cell these dou ble-mem brane organ elles pro vide a highly efficient route pro lif er a tion and to per form cyto tox ic ity and via bil ity assays [2–4].
    [Show full text]
  • Systematics and Evaluation of Meteorite Classification 19
    Weisberg et al.: Systematics and Evaluation of Meteorite Classification 19 Systematics and Evaluation of Meteorite Classification Michael K. Weisberg Kingsborough Community College of the City University of New York and American Museum of Natural History Timothy J. McCoy Smithsonian Institution Alexander N. Krot University of Hawai‘i at Manoa Classification of meteorites is largely based on their mineralogical and petrographic charac- teristics and their whole-rock chemical and O-isotopic compositions. According to the currently used classification scheme, meteorites are divided into chondrites, primitive achondrites, and achondrites. There are 15 chondrite groups, including 8 carbonaceous (CI, CM, CO, CV, CK, CR, CH, CB), 3 ordinary (H, L, LL), 2 enstatite (EH, EL), and R and K chondrites. Several chondrites cannot be assigned to the existing groups and may represent the first members of new groups. Some groups are subdivided into subgroups, which may have resulted from aster- oidal processing of a single group of meteorites. Each chondrite group is considered to have sampled a separate parent body. Some chondrite groups and ungrouped chondrites show chemi- cal and mineralogical similarities and are grouped together into clans. The significance of this higher order of classification remains poorly understood. The primitive achondrites include ureil- ites, acapulcoites, lodranites, winonaites, and silicate inclusions in IAB and IIICD irons and probably represent recrystallization or residues from a low-degree partial melting of chondritic materials. The genetic relationship between primitive achondrites and the existing groups of chondritic meteorites remains controversial. Achondrites resulted from a high degree of melt- ing of chondrites and include asteroidal (angrites, aubrites, howardites-diogenites-eucrites, mesosiderites, 3 groups of pallasites, 15 groups of irons plus many ungrouped irons) and plane- tary (martian, lunar) meteorites.
    [Show full text]
  • Standard 1: CHEMISTRY of LIFE –REVIEW of BASICS O=C=O
    Standard 1: CHEMISTRY OF LIFE –REVIEW OF BASICS What are the six most common elements that make up living organisms? C H O N P S (carbon, hydrogen, oxygen, nitrogen, phosphorus, sulfur) What is an organic molecule? An organic molecule or compound contains the element carbon. Why is carbon the necessary element in organic compounds? Carbon can form 4 covalent bonds (strong bonds made by sharing pairs of electrons) with up to 4 different elements. Methane Carbon Dioxide Acetylene O=C=O Carbon with 4 single bonds Carbon with 2 double bonds Each carbon has one single and one triple bond What does the word ending –ose indicate? The –ose ending means the molecule is a sugar. What does the word ending –ase indicate? The –ose word ending indicates the molecule is an enzyme. What are enzymes? Enzymes are proteins that are catalysts – they speed up chemical reactions without being used up or changed. Enzyme activity can be affected by temperature and pH. What are the four categories of organic compounds? The four categories of organic compounds are Carbohydrates, Lipids, Proteins, and Nucleic Acids Complete this chart of the four major categories of organic compounds: CARBOHYDRATES LIPIDS PROTEINS NUCLEIC ACIDS ELEMENTS CHO CHO CHON (sometimes S) CHONP MONOMERS Monosaccharides are simple Glycerol and fatty acids Amino acids (20 Nucleotide (made of a sugar, (BUILDING sugars (glucose, galactose, Fatty acids are long different kinds) phosphate and nitrogen base) BLOCKS) fructose) chains of hydrocarbons Sugar names end in -ose (C and H) SHAPE/ Glucose Amino Acid (-R group DNA is shaped like a double STRUCTURE is different for each helix (twisted ladder) amino acid Proteins are chains of amino acids Glycerol is a 3-carbon Sequence of the amino acids determines the alcohol and each fatty Starch is a chain of glucose acid is a long chain of protein molecules that are chemically carbon atoms with bonded.
    [Show full text]
  • Solar Elemental Abundances Table of Contents Summary
    Solar Elemental Abundances Katharina Lodders Department of Earth & Planetary Sciences and McDonnell Center for the Space Sciences Washington University, Campus Box 1169, 1 Brookings Drive, St. Louis MO 63130 November 2019, in press. Cite as: Lodders, K. 2020, Solar Elemental Abundances, in The Oxford Research Encyclopedia of Planetary Science, Oxford University Press. doi:[TBD] Table of Contents Summary ......................................................................................................................................... 1 Keywords ................................................................................................................................ 2 Definitions....................................................................................................................................... 2 Abundance Scales ........................................................................................................................... 3 Historical Background .................................................................................................................... 5 Meteoritic Abundances ................................................................................................................... 7 Abundances of the Elements in CI-Chondrites ......................................................................... 15 Solar Abundances of the Elements, Photosphere, Sunspots, Corona, and Solar Wind ................ 19 Photospheric Abundances ........................................................................................................
    [Show full text]
  • Sourcebook in Forensic Serology, Immunology, and Biochemistry Usually Said That Antigens Are Substances Which Elicit an One Cross-React with the Others
    UNIT I BACKGROUND MATERIAL Forensic serology, if taken in its broadest sense to include them to standard texts, review articles, and so forth. Just as all aspects of the medico-legal examination of blood and detailed documentation was not in order for this unit, neither body fluids, draws its methods and the basis of its activities was complete treatment of the various disciplines. Topics for from a number of traditional intellectual disciplines. Fore- inclusion were selected on the basis of their relevance to most among these are biochemistry, immunology and forensic serological tests or methods. A few topics which are . genetics. not particularly relevant to medico-legal practice, have been This being a sourcebook, an effort has been made to pro- briefly discussed for the sake of completeness. vide background on the various methods and concepts dis- The material included in the background chapters is not cussed as they come up. As a result, many aspects of bio- regarded as being essential to the use of the succeeding units chemistry, genetics and immunology are discussed in con- of the Sourcebook. Cross references have been included, nection with the various procedures and tests which are used where relevant, however, so that readers who may wish to in forensic practice. Such an approach necessarily presents consult the background material on a particular subject in much of the material of a particular unified body of knowl- some context will be able to locate it without undue edge in a rather disjoint manner. Unit I has been included in difficulty. order to provide some background material in the unified Unit I consists of two sections, the first consisting of back- diiiplines in a more organized fashion.
    [Show full text]
  • Elements & Macromolecules in Organisms
    Elements & Macromolecules in Organisms Most common elements in living things are carbon, hydrogen, nitrogen, and oxygen. These four elements constitute about 95% of your body weight. All compounds can be classified in two broad categories --- organic and inorganic compounds. Organic compounds are made primarily of carbon. Carbon has four outer electrons and can form four bonds. Carbon can form single bonds with another atom and also bond to other carbon molecules forming double, triple, or quadruple bonds. Organic compounds also contain hydrogen. Since hydrogen has only one electron, it can form only single bonds. Each small organic molecule can be a unit of a large organic molecule called a macromolecule. There are four classes of macromolecules (polysaccharides or carbohydrates, triglycerides or lipids, polypeptides or proteins, and nucleic acids such as DNA & RNA). Carbohydrates and lipids are made of only carbon, hydrogen, and oxygen (CHO). Proteins are made of carbon, hydrogen, oxygen, and nitrogen (CHON). Nucleic acids such as DNA and RNA contain carbon, hydrogen, oxygen, nitrogen, and phosphorus (CHON P). The body also needs trace amounts of other elements such as calcium, potassium, and sulfur for proper functioning of muscles, nerves, etc. Questions: 1. Name the 4 main elements that make up 95% of an organism. 2. Name the 4 types of bonds carbon can form. 3. What are macromolecules? 1 4. Name the 4 classes of macromolecules. 5. Give 2 examples of nucleic acids. 6. What elements make up carbohydrates & lipids (symbols)? 7. Name 3 elements your body needs trace amounts of for proper functioning. The four main classes of organic compounds (carbohydrates, lipids, proteins, and nucleic acids) that are essential to the proper functioning of all living things are known as polymers or macromolecules.
    [Show full text]
  • Earth's Earliest Atmospheres
    Downloaded from http://cshperspectives.cshlp.org/ at UNIV OF CHICAGO on February 4, 2015 - Published by Cold Spring Harbor Laboratory Press Earth’s Earliest Atmospheres Kevin Zahnle1, Laura Schaefer2, and Bruce Fegley2 1Space Science Division, NASA Ames Research Center, MS 245-3, Moffett Field, California 94035 2Planetary Chemistry Laboratory, Department of Earth and Planetary Sciences and McDonnell Center for the Space Sciences, Washington University, St Louis, Missouri 63130 Correspondence: [email protected] Earth is the one known example of an inhabited planet and to current knowledge the likeliest site of the one known origin of life. Here we discuss the origin of Earth’s atmosphere and ocean and some of the environmental conditions of the early Earth as they may relate to the origin of life. A key punctuating event in the narrative is the Moon-forming impact, partly because it made Earth for a short time absolutely uninhabitable, and partly because it sets the boundary conditions for Earth’s subsequent evolution. If life began on Earth, as opposed to having migrated here, it would have done so after the Moon-forming impact. What took place before the Moon formed determined the bulk properties of the Earth and probably determined the overall compositions and sizes of its atmospheres and oceans. What took place afterward animated these materials. One interesting consequence of the Moon-forming impact is that the mantle is devolatized, so that the volatiles subsequently fell out in a kind of condensation sequence. This ensures that the volatiles were concentrated toward the surface so that, for example, the oceans were likely salty from the start.
    [Show full text]
  • Name: MACROMOLECULES Date: I. ELEMENTS AND
    Name: MACROMOLECULES Date: I. ELEMENTS AND MACROMOLECULES IN ORGANISMS: Most common elements in living things are carbon, hydrogen, nitrogen, and oxygen. These four elements constitute about 95% of your body weight. All compounds can be classified in two broad categories --- organic and inorganic compounds. Organic compounds are made primarily of carbon. Carbon has four outer electrons and can form four bonds. Carbon can also bond to other carbon molecules forming double, triple, or quadruple bonds. Organic compounds also contain hydrogen. Since hydrogen has only one electron, it can form only single bonds. Each small organic molecule can be a unit of a large organic molecule called a macromolecule. There are four classes of macromolecules (polysaccharides or carbohydrates, triglycerides or lipids, polypeptides or proteins, and nucleic acids such as DNA & RNA). Carbohydrates and lipids are made of only carbon, hydrogen, and oxygen (CHO). Proteins are made of carbon, hydrogen, oxygen, and nitrogen (CHON). Nucleic acids such as DNA and RNA contain carbon, hydrogen, oxygen, nitrogen, and phosphorus (CHON P).The body also needs trace amounts of other elements such as calcium, potassium, and sulfur for proper functioning of muscles, nerves, etc. The four main classes of organic compounds (carbohydrates, lipids, proteins, and nucleic acids) that are essential to the proper functioning of all living things are known as polymers or macromolecules. All of these compounds are built primarily of carbon, hydrogen, and oxygen but in different ratios. This gives each compound different properties. Questions: 1. What are the 4 main elements that make up 95% of an organism? 2. What are macromolecules? 3.
    [Show full text]
  • Agilent E1431A User Guide
    Full-service, independent repair center -~ ARTISAN® with experienced engineers and technicians on staff. TECHNOLOGY GROUP ~I We buy your excess, underutilized, and idle equipment along with credit for buybacks and trade-ins. Custom engineering Your definitive source so your equipment works exactly as you specify. for quality pre-owned • Critical and expedited services • Leasing / Rentals/ Demos equipment. • In stock/ Ready-to-ship • !TAR-certified secure asset solutions Expert team I Trust guarantee I 100% satisfaction Artisan Technology Group (217) 352-9330 | [email protected] | artisantg.com All trademarks, brand names, and brands appearing herein are the property o f their respective owners. Find the Keysight / Agilent E1431A at our website: Click HERE HP E1431A 25.6 kHz Eight Channel VXI Input Module User's Guide HEWLETT PACKARD Part Number E 1431-90005 Microfiche Number E 1431-90205 Printed in U.S.A. Print Date: June 1995 OHewlett-Packard Company, 1994-1995. All rights reserved. 8600 Soper Hill Road Everett, Washington 98205-1298 U.S.A. Artisan Technology Group - Quality Instrumentation ... Guaranteed | (888) 88-SOURCE | www.artisantg.com HEWLETT Fa PACKARD NOTICE The ~nformationcontained in this document is subject to change without notice. HEWLETT-PACKARD MAKES NO WARRANTY OF ANY KIND WITH REGARD TO THIS MANUAL, INCLUDING, BUT NOT LIMITED TO, THE IMPLIED WARRANTIES OF MERCHANTABILITY AND FITNESS FOR A PARTICULAR PURPOSE. Hewlett-Packard shall not be liable for errors contained herein or direct, indirect, special, incidental or consequential damages in connection with the furnishmg, performance, or use of this material. WARRANTY A ccrpy of the speafi warmnty tenns applicable to your Haolet&Packard product and mplacement parts can be obtainedfiom your local Sales and senvice Qj%ce.
    [Show full text]
  • Vaporization and Thermodynamics of Forsterite-Rich Olivine and Some Implications for Silicate
    Vaporization and thermodynamics of forsterite-rich olivine and some implications for silicate atmospheres of hot rocky exoplanets a , a b Gustavo C.C. Costa ∗, Nathan S. Jacobson , Bruce Fegley Jr. a NASA Glenn Research Center, 210 0 0 Brookpark Road, MS 106-1, Cleveland, OH, 44135, USA b Planetary Chemistry Laboratory, McDonnell Center for the Space Sciences, Department of Earth and Planetary Sciences, Washington University in St. Louis, Campus Box 1169, 1 Brookings Dr, St. Louis, MO, 63130-4899, USA a r t i c l e i n f o a b s t r a c t Article history: We describe an experimental and theoretical study of olivine [Mg 2 SiO 4 (Fo)–Fe 2 SiO 4 (Fa)] vaporization The vaporization Received 12 May 2016 behavior and thermodynamic properties of a fosterite-rich olivine (Fo 95 Fa 5 ) have been explored by high-temperature Knudsen Revised 16 November 2016 Accepted 14 effusion mass spectrometry (KEMS) from 1750 to 2250 K. The gases observed (in order of decreasing partial pressure) are Fe, February 2017 Available online 16 February 2017 SiO, Mg, O 2 and O. We measured the solidus temperature ( ∼2050 K), partial pressures of individual gases, the total vapor pressure, and thermodynamic activities and partial molar enthalpies of MgO, ‘FeO’, and SiO 2 for the Fo 95 Fa 5 olivine. The results are compared to other measurements and models of the olivine system. Our experimental data show olivine vaporizes incongruently. We discuss this system both as a psuedo-binary of Fo-Fa and a psuedo-ternary of MgO–‘FeO’–SiO 2 .
    [Show full text]