Overview of VOC Emissions and Chemistry from PTR-TOF-MS Measurements During the Suskat-ABC Campaign
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Interstellar Formamide (NH2CHO), a Key Prebiotic Precursor
Interstellar formamide (NH2CHO), a key prebiotic precursor Ana López-Sepulcre,∗,y,z Nadia Balucani,{ Cecilia Ceccarelli,y Claudio Codella,x,y François Dulieu,k and Patrice Theulé? yUniv. Grenoble Alpes, IPAG, F-38000 Grenoble, France zInstitut de Radioastronomie Millimétrique (IRAM), 300 rue de la piscine, F-38406 Saint-Martin d’Hères, France {Dipartimento di Chimica, Biologia e Biotecnologie, Università degli Studi di Perugia, I-06123 Perugia, Italy xINAF, Osservatorio Astrofisico di Arcetri, Largo E. Fermi 5, I-50125, Firenze, Italy kUniversité de Cergy-Pontoise, Observatoire de Paris, PSL University, Sorbonne Université, CNRS, LERMA, F-95000, Cergy-Pontoise, France ?Aix-Marseille Université, PIIM UMR-CNRS 7345, 13397 Marseille, France E-mail: [email protected] Abstract Formamide (NH2CHO) has been identified as a potential precursor of a wide variety arXiv:1909.11770v1 [astro-ph.SR] 25 Sep 2019 of organic compounds essential to life, and many biochemical studies propose it likely played a crucial role in the context of the origin of life on our planet. The detection of formamide in comets, which are believed to have –at least partially– inherited their current chemical composition during the birth of the Solar System, raises the question whether a non-negligible amount of formamide may have been exogenously delivered onto a very young Earth about four billion years ago. A crucial part of the effort to 1 answer this question involves searching for formamide in regions where stars and planets are forming today in our Galaxy, as this can shed light on its formation, survival, and chemical re-processing along the different evolutionary phases leading to a star and planetary system like our own. -
Urea Decomposition and SCR Performance at Low Temperature
Urea Decomposition and SCR Performance at Low Temperature Scott Sluder, John Storey, Sam Lewis, Linda Lewis, Oak Ridge National Laboratory 10th Annual DEER Workshop Coronado, CA September 2, 2004 Sponsors: DOE-OFCVT, Steve Goguen and Kevin Stork OAK RIDGE NATIONAL LABORATORY U. S. DEPARTMENT OF ENERGY 1 Why study urea decomposition? • Under light-duty conditions (< 250 °C), there is negligible urea decomposition in the gas phase. Current models assume NH3 as input to catalyst. • It appears that urea decomposition kinetics on catalyst surfaces has to be understood. This will affect the length of the catalyst that is used for urea decomposition. OAK RIDGE NATIONAL LABORATORY U. S. DEPARTMENT OF ENERGY 2 Urea/SCR Chemistry Ideally, injected urea decomposes to NH3 O Heat NH3 + HCNO H2O, O2 isocyanic acid H 2N NH2 Heat HCNO NH3 + CO2 isocyanic acid H2O then reacts with NOX to form N2. 2 NH3 + NO + NO2 ⇔ 2 N2 + 3 H2O OAK RIDGE NATIONAL LABORATORY U. S. DEPARTMENT OF ENERGY 3 Unusual things can happen, such as ammonium nitrate formation and decomposition at T < 200 °C. 2NH3 + 2NO2 →NH4NO3 + N2 + 3 H2O NH4NO3 ⇔ NH3 + HNO3 2HNO3 + NO → 3 NO2 + H2O M. Koebel et al. in Ind.Eng.Chem.Res.: 39,p. 4120; 40, p. 52; 41, p.4008; 42, p.2093 Also in Catal.Today, 73, p.239 OAK RIDGE NATIONAL LABORATORY U. S. DEPARTMENT OF ENERGY 4 Experimental Approach • Use engine controls to: − Vary temperature − Keep constant: NOX and exhaust flow. • Investigate urea decomposition (if any) upstream of SCR catalyst. • Analyze exhaust products exiting undersized monoliths to elucidate urea decomposition − 3” and 6” monoliths = space velocities of 25K and 50K − const. -
This Item Was Submitted to Loughborough University
This item was submitted to Loughborough University as an MPhil thesis by the author and is made available in the Institutional Repository (https://dspace.lboro.ac.uk/) under the following Creative Commons Licence conditions. For the full text of this licence, please go to: http://creativecommons.org/licenses/by-nc-nd/2.5/ LOUGHBOROUGH UNIVERSITY OF TECHNOLOGY LIBRARY AUTHOR/FILING TITLE . -------------~§'~£~~~-~-;::r------_...: __________ i , ----------------!.------------------------ -- ----- - .....- , ACCESSION/COPY NO. --------------___ _L~~~~~/~~-----~- _____ ______ _ VOL. NO. CLASS MARK ISO C YA N I C ACID B Y D. J. BEL SON N .rkl ' A'~OCIORAL THESIS SUBMITTED IN PARTIAL FULFILMENT OF THE REQUIREMENTS FOR , . ." , THE AWARD OF ~,_~,.' , ~ kf\S-r.. tt ; ~eCTeR OF PHILOSOPHY OF THE LOUGHBOROUGH UNIVERSITY OF TECHNOLOGY - 1981\ SUPERVISOR: DRI A, N, STRACHAN DEPARTMENT OF CHEM I STRY © BY D. J. BELSON J 1981. ..... ~- ~~c. \0) 'to 'b/O"2- .-'-' , C O,N TEN T S Chapter 1 Intr6duction .. 1 2 Preparation and storage of isocyanic acid. 3 3 Physical properties and structure of isocyanic acid. 11 4 Methods of analysis for isocyanic acid. 17 5 The polymerisation of isocyanic acid. 21 6 Pyrolysis and photolysis of isocyanicacid. 34 7 Reactions in water. 36 8: Reaction 'with alcohols. 48 9 Reactions with ammonia and amines. 52 10 Other addition reactions across th'e N=C double bond. 57· 11 Addition of isocyanic acid to unsaturated molecules. 65 12 Summary and conclUsions. 69 Acknowledgements. 82 Ref erenc es. 83 Figures Opposite Page 1 Van't Hoff equation plot for the gas- 23 phase depolymerisation of cyanuric acid. 2 Values of pKfor isocyanic acid 37 dissociation~;'- plotted against temperature. -
15 Aug 2017 Sims Ue2,2021 23, June Srnm Astrophysics & Astronomy .Codella C
Astronomy & Astrophysics manuscript no. codella˙astroph˙solisIII c ESO 2021 June 23, 2021 Letter to the Editor Seeds of Life in Space (SOLIS) III. Formamide in protostellar shocks: evidence for gas-phase formation C. Codella1, C. Ceccarelli2,1, P. Caselli3, N. Balucani4,1, V. Barone5, F. Fontani1, B. Lefloch2, L. Podio1, S. Viti6, S. Feng3, R. Bachiller7, E. Bianchi1,8, F. Dulieu9, I. Jim´enez-Serra10, J. Holdship6, R. Neri11, J. Pineda3, A. Pon12, I. Sims13, S. Spezzano3, A.I. Vasyunin3,14, F. Alves3, L. Bizzocchi3, S. Bottinelli15,16, E. Caux15,16, A. Chac´on-Tanarro3, R. Choudhury3, A. Coutens6, C. Favre1,2, P. Hily-Blant2, C. Kahane2, A. Jaber Al-Edhari2,17, J. Laas3, A. L´opez-Sepulcre11, J. Ospina2, Y. Oya18, A. Punanova3, C. Puzzarini19, D. Quenard10, A. Rimola20, N. Sakai21, D. Skouteris5, V. Taquet22,1, L. Testi23,1, P. Theul´e24, P. Ugliengo25, C. Vastel15,16, F. Vazart5, L. Wiesenfeld2, and S. Yamamoto18 1 INAF, Osservatorio Astrofisico di Arcetri, Largo E. Fermi 5, 50125 Firenze, Italy 2 Univ. Grenoble Alpes, CNRS, Institut de Plan´etologie et d’Astrophysique de Grenoble (IPAG), 38000 Grenoble, France 3 Max-Planck-Institut f¨ur extraterrestrische Physik (MPE), Giessenbachstrasse 1, 85748 Garching, Germany 4 Dipartimento di Chimica, Biologia e Biotecnologie, Via Elce di Sotto 8, 06123 Perugia, Italy 5 Scuola Normale Superiore, Piazza dei Cavalieri 7, 56126 Pisa, Italy 6 Department of Physics and Astronomy, University College London, Gower Street, London, WC1E 6BT, UK 7 IGN, Observatorio Astron´omico Nacional, Calle Alfonso XII, 28004 Madrid, Spain 8 Dipartimento di Fisica e Astronomia, Universit`adegli Studi di Firenze, Italy 9 LERMA, Universit´ede Cergy-Pontoise, Observatoire de Paris, PSL Research University, CNRS, Sorbonne Universit´e, UPMC, Univ. -
LIQUID DYNE PENS (#N001-002, #N001-015) Date Prepared: 5/1/03
*** MATERIAL SAFETY DATA SHEET *** DYNE SOLUTION-100CC (#N001-011), LIQUID DYNE PENS (#N001-002, #N001-015) Date Prepared: 5/1/03 SECTION A DISTRIBUTOR: UV PROCESS SUPPLY, INC 1229 W. CORTLAND ST. CHICAGO, IL 60614-4805 TELEPHONE: (773)248-0099 EMERGENCY #: (800)424-9300 SECTION B GENERAL PRODUCT INFORMATION PRODUCT NAME: CON-TROL-CURE DYNE TEST SOLUTIONS CON-TROL-CURE LIQUID DYNE PEN SET FORM: Liquid COLOR: Medium blue ODOR: Mild, non-residual; ethereal/ammoniacal SECTION C COMPOSITION/INGREDIENTS Constituent CAS No. Molecular Formula 2-ethoxyethanol, 100% pure (C)* 110-80-5 C2H5OC2H4OH Formamide, minimum 99.5% pure (F)** 75-12-7 HCONH2 Water (H) 7732-18-5 H2O Victoria Blue Dye, 100% pure 2185-86-6 no data *2-ethoxyethanol is also known as ethylene glycol monoethyl ether, cellosolve solvent, ehlyl cellosolve, and glycol ether EE. **Formamide is also known as methanamide. Mix Percentages by Dyne Level Level C (vol) F (vol) Level C (vol) F (vol) Level F (vol) H (vol) 30 100.0% 0.0% 44 22.0% 78.0% 57 100.0% 0.0% 31 97.5% 2.5% 45 19.7% 80.3% 58 81.2% 18.8% 32 89.5% 10.5% 46 17.2% 82.8% 59 73.1% 26.9% 33 81.0% 19.0% 47 15.0% 85.0% 60 65.0% 35.0% 34 73.5% 26.5% 48 13.0% 87.0% 61 56.0% 44.0% 35 65.0% 35.0% 49 11.1% 88.9% 62 47.0% 53.0% 36 57.5% 42.5% 50 9.3% 90.7% 63 38.8% 61.2% 37 51.5% 48.5% 51 7.8% 92.2% 64 30.6% 69.4% 38 46.0% 54.0% 52 6.3% 93.7% 65 24.4% 75.6% 39 41.0% 59.0% 53 4.9% 95.1% 66 18.2% 81.8% 40 36.5% 63.5% 54 3.5% 96.5% 67 13.4% 86.6% 41 32.5% 67.5% 55 2.2% 97.8% 68 8.6% 91.4% 42 28.5% 71.5% 56 1.0% 99.0% 69 6.1% 93.9% 43 25.3% 74.7% 70 3.6% 96.4% Concentration of Victoria Blue dye is 0.3 grams per liter. -
TR-541: Formamide (CASRN 75-12-7) in F344/N Rats and B6C3F1 Mice (Gavage Studies)
NTP TECHNICAL REPORT ON THE TOXICOLOGY AND CARCINOGENESIS STUDIES OF FORMAMIDE (CAS NO. 75-12-7) IN F344/N RATS AND B6C3F1 MICE (GAVAGE STUDIES) NATIONAL TOXICOLOGY PROGRAM P.O. Box 12233 Research Triangle Park, NC 27709 July 2008 NTP TR 541 NIH Publication No. 08-5884 National Institutes of Health Public Health Service U.S. DEPARTMENT OF HEALTH AND HUMAN SERVICES FOREWORD The National Toxicology Program (NTP) is an interagency program within the Public Health Service (PHS) of the Department of Health and Human Services (HHS) and is headquartered at the National Institute of Environmental Health Sciences of the National Institutes of Health (NIEHS/NIH). Three agencies contribute resources to the program: NIEHS/NIH, the National Institute for Occupational Safety and Health of the Centers for Disease Control and Prevention (NIOSH/CDC), and the National Center for Toxicological Research of the Food and Drug Administration (NCTR/FDA). Established in 1978, the NTP is charged with coordinating toxicological testing activities, strengthening the science base in toxicology, developing and validating improved testing methods, and providing information about potentially toxic substances to health regulatory and research agencies, scientific and medical communities, and the public. The Technical Report series began in 1976 with carcinogenesis studies conducted by the National Cancer Institute. In 1981, this bioassay program was transferred to the NTP. The studies described in the Technical Report series are designed and conducted to characterize and evaluate the toxicologic potential, including carcinogenic activity, of selected substances in laboratory animals (usually two species, rats and mice). Substances selected for NTP toxicity and carcinogenicity studies are chosen primarily on the basis of human exposure, level of production, and chemical structure. -
Sources of Isocyanic Acid (HNCO) Indoors: a Focus on Cigarette Smoke
TSpace Research Repository tspace.library.utoronto.ca Sources of isocyanic acid (HNCO) indoors: a focus on cigarette smoke Rachel F. Hems, Chen Wang, Douglas B. Collins, Shouming Zhou, Nadine Borduas-Dedekind, Jeffrey A. Siegel, Jonathan P.D. Abbatt Version Post-print/Accepted Manuscript Citation Hems, R.F., Wang, C., Collins, D.B., Zhou, S., Borduas-Dedekind, N., (published version) Siegel, J.A., Abbatt, J.P.D., 2019. Sources of isocyanic acid (HNCO) indoors: a focus on cigarette smoke. Environ. Sci.: Processes Impacts, 21, 1334. https://doi.org/10.1039/C9EM00107G. How to cite TSpace items Always cite the published version, so the author(s) will receive recognition through services that track citation counts, e.g. Scopus. If you need to cite the page number of the author manuscript from TSpace because you cannot access the published version, then cite the TSpace version in addition to the published version using the permanent URI (handle) found on the record page. This article was made openly accessible by U of T Faculty. Please tell us how this access benefits you. Your story matters. 1 Sources of isocyanic acid (HNCO) indoors: a focus on cigarette smoke 2 Rachel F. Hems,† Chen Wang,† Douglas B. Collins,ǂ Shouming Zhou,† Nadine Borduas- 3 Dedekind,† Jeffrey A. Siegel,‡ Jonathan P.D. Abbatt*† 4 †Department of Chemistry, University of Toronto, 80 St. George Street, Toronto, Ontario M5S 5 3H6, Canada. 6 ‡Department of Civil and Mineral Engineering, University of Toronto, 35 Street George Street, 7 Toronto, Ontario M5S 1A4, Canada. 8 ǂDepartment of Chemistry, Bucknell University, 1 Dent Drive, Lewisburg, PA 17837, USA. -
Surface Chemistry and Kinetics of the Hydrolysis of Isocyanic Acid on Anatase
Technische Universität München Lehrstuhl 2 für Technische Chemie Surface chemistry and kinetics of the hydrolysis of isocyanic acid on TiO2 anatase Philipp Christian Dino Patrick Hauck Vollständiger Abdruck der von der Fakultät für Chemie der Technischen Universität München zur Erlangung des akademischen Grades eines Doktors der Naturwissenschaften (Dr.rer.nat.) genehmigten Dissertation. Vorsitzender: Univ.-Prof. Dr. Klaus Köhler Prüfer der Dissertation: 1. Univ.-Prof. Dr. Johannes A. Lercher 2. Univ.-Prof. Dr. Kai-Olaf Hinrichsen Die Dissertation wurde am 14.02.2007 bei der Technischen Universität München eingereicht und durch die Fakultät für Chemie am 16.04.2007 angenommen. Gott sei Dank! Nun ist’s vorbei mit der Übertäterei! Meine Damen und Herren, vielleicht hat niemand mehr damit gerechnet. Um so größer wird die Überraschung sein: Ich komme jetzt zum Ende. Wilhelm Busch (1832-1908) Acknowledgements Finally the PhD time has drawn to its close and the tamer of the isocyanic acid would like to say a few words of thank to a bunch of people who made a substantial contribution to the ultimate thesis. First of all I would like to thank Johannes (Prof. J.A. Lercher) for inviting me into his group and thus giving me the opportunity to work in a fairly international team on an adventurous project. Thank you for all the guidance, trust, fruitful, but also sharp- tongued discussions during the last three years three months and the sufficient freedom and independence with regard to structuring my work. The time at TC 2 has been an important and joyful part of my life for sure. -
Arxiv:1510.07052V1 [Astro-Ph.EP] 23 Oct 2015 99 Lae Ta.20,Adrfrne Therein)
A Chemical Kinetics Network for Lightning and Life in Planetary Atmospheres P. B. Rimmer1 and Ch Helling School of Physics and Astronomy, University of St Andrews, St Andrews, KY16 9SS, United Kingdom ABSTRACT There are many open questions about prebiotic chemistry in both planetary and exoplane- tary environments. The increasing number of known exoplanets and other ultra-cool, substellar objects has propelled the desire to detect life and prebiotic chemistry outside the solar system. We present an ion-neutral chemical network constructed from scratch, Stand2015, that treats hydrogen, nitrogen, carbon and oxygen chemistry accurately within a temperature range between 100 K and 30000 K. Formation pathways for glycine and other organic molecules are included. The network is complete up to H6C2N2O3. Stand2015 is successfully tested against atmo- spheric chemistry models for HD209458b, Jupiter and the present-day Earth using a simple 1D photochemistry/diffusion code. Our results for the early Earth agree with those of Kasting (1993) for CO2, H2, CO and O2, but do not agree for water and atomic oxygen. We use the network to simulate an experiment where varied chemical initial conditions are irradiated by UV light. The result from our simulation is that more glycine is produced when more ammonia and methane is present. Very little glycine is produced in the absence of any molecular nitrogen and oxygen. This suggests that production of glycine is inhibited if a gas is too strongly reducing. Possible applications and limitations of the chemical kinetics network are also discussed. Subject headings: astrobiology — atmospheric effects — molecular processes — planetary systems 1. Introduction The input energy source and the initial chem- istry have been varied across these different ex- The potential connection between a focused periments. -
Investigating Diesel Engines As an Atmospheric Source of Isocyanic Acid in Urban Areas
Atmos. Chem. Phys., 17, 8959–8970, 2017 https://doi.org/10.5194/acp-17-8959-2017 © Author(s) 2017. This work is distributed under the Creative Commons Attribution 3.0 License. Investigating diesel engines as an atmospheric source of isocyanic acid in urban areas Shantanu H. Jathar1, Christopher Heppding1, Michael F. Link2, Delphine K. Farmer2, Ali Akherati1, Michael J. Kleeman3, Joost A. de Gouw4,5, Patrick R. Veres4,5, and James M. Roberts4 1Department of Mechanical Engineering, Colorado State University, Fort Collins, CO 80523, USA 2Department of Chemistry, Colorado State University, Fort Collins, CO 80523, USA 3Department of Civil and Environmental Engineering, University of California Davis, Davis, CA 95616, USA 4NOAA Earth System Research Laboratory, Chemical Sciences Division, Boulder, CO 80305, USA 5Cooperative Institute for Research in Environmental Sciences, University of Colorado, Boulder, CO 80305, USA Correspondence to: Shantanu H. Jathar ([email protected]) Received: 20 January 2017 – Discussion started: 22 February 2017 Revised: 18 May 2017 – Accepted: 19 May 2017 – Published: 26 July 2017 Abstract. Isocyanic acid (HNCO), an acidic gas found in implied that diesel-powered engines were the largest source tobacco smoke, urban environments, and biomass-burning- of HNCO in urban areas. The CTM also predicted that daily- affected regions, has been linked to adverse health outcomes. averaged concentrations of HNCO reached a maximum of Gasoline- and diesel-powered engines and biomass burning ∼ 110 pptv but were an order of magnitude lower than the are known to emit HNCO and hypothesized to emit pre- 1 ppbv level that could be associated with physiological ef- cursors such as amides that can photochemically react to fects in humans. -
Evaluation of Chemical and Particle Exposures During Vehicle Fire Suppression Training
This Health Hazard Evaluation (HHE) report and any recommendations made herein are for the specific facility evaluated and may not be universally applicable. Any recommendations made are not to be considered as final statements of NIOSH policy or of any agency or individual involved. Additional HHE reports are available at http://www.cdc.gov/niosh/hhe/ Workplace Safety and Health Evaluation of Chemical and Particle Exposures During Vehicle Fire Suppression Training Kenneth W. Fent, PhD Douglas E. Evans, PhD James Couch, MS, CIH Health Hazard Evaluation Report HETA 2008-0241-3113 Miami Township Fire and Rescue Yellow Springs, Ohio July 2010 Department of Health and Human Services Centers for Disease Control and Prevention National Institute for Occupational Safety and Health The employer shall post a copy of this report for a period of 30 calendar days at or near the workplace(s) of affected employees. The employer shall take steps to insure that the posted determinations are not altered, defaced, or covered by other material during such period. [37 FR 23640, November 7, 1972, as amended at 45 FR 2653, January 14, 1980]. CONTENTS REPO R T Abbreviations .......................................................................ii Highlights of the NIOSH Health Hazard Evaluation ............iv Summary ............................................................................vi Introduction ..........................................................................1 Assessment .........................................................................3 -
Overview of VOC Emissions and Chemistry from PTR-TOF-MS Measurements During the Suskat-ABC Campaign
Overview of VOC emissions and chemistry from PTR-TOF-MS measurements during the SusKat-ABC campaign: high acetaldehyde, isoprene and isocyanic acid in wintertime air of the Kathmandu Valley by C. Sarkar et al., 2015 (ACPD) We thank the anonymous referee 1 for his/her helpful comments and the generally positive remarks concerning the novelty of the work and its importance. Please find the referee’s comments in black and our point wise replies in blue for easy perusal. REFEREE 1: The study produced a lot of important, unique content of great interest to ACP readers. However, the presentation is not quite there. For example, the references have unwanted numbers appended throughout. We thank the referee for appreciating the importance and content of the work and deeming it of great interest to ACP readers. Regarding improving the overall presentation and discussion, we found several of Referee 1’s specific comments very helpful and these are now reflected in the revised submission (changes are specified in replies and manuscript version with “tracked changes” given at the end of the responses here). Concerning the specific point of “references having unwanted numbers appended”, we note that those “numbers” are actually page numbers at which the references have been cited in the ACPD manuscript and were inserted during the typesetting process by the editorial office as it seems to be a feature of their LATEX template for submissions to ACPD. As authors we only followed the journal’s submission procedure. More importantly, the length should be cut in half while both clarifying and focusing on the main points that are most strongly supported as discussed below.