Deoxyribose-5-Phosphate Aldolase As a Synthetic Catalyst'
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Accurate Enthalpies of Formation of Astromolecules: Energy, Stability and Abundance
Accurate Enthalpies of Formation of Astromolecules: Energy, Stability and Abundance Emmanuel E. Etim and Elangannan Arunan* Inorganic and Physical Chemistry Department, Indian Institute of Science Bangalore, India-560012 *email: [email protected] ABSTRACT: Accurate enthalpies of formation are reported for known and potential astromolecules using high level ab initio quantum chemical calculations. A total of 130 molecules comprising of 31 isomeric groups and 24 cyanide/isocyanide pairs with atoms ranging from 3 to 12 have been considered. The results show an interesting, surprisingly not well explored, relationship between energy, stability and abundance (ESA) existing among these molecules. Among the isomeric species, isomers with lower enthalpies of formation are more easily observed in the interstellar medium compared to their counterparts with higher enthalpies of formation. Available data in literature confirm the high abundance of the most stable isomer over other isomers in the different groups considered. Potential for interstellar hydrogen bonding accounts for the few exceptions observed. Thus, in general, it suffices to say that the interstellar abundances of related species are directly proportional to their stabilities. The immediate consequences of this relationship in addressing some of the whys and wherefores among astromolecules and in predicting some possible candidates for future astronomical observations are discussed. Our comprehensive results on 130 molecules indicate that the available experimental enthalpy -
Possible Gas-Phase Syntheses for Seven Neutral Molecules Studied Recently with the Green Bank Telescope
A&A 474, 521–527 (2007) Astronomy DOI: 10.1051/0004-6361:20078246 & c ESO 2007 Astrophysics Possible gas-phase syntheses for seven neutral molecules studied recently with the Green Bank Telescope D. Quan1 and E. Herbst2 1 Chemical Physics Program, The Ohio State University, Columbus, Ohio 43210, USA e-mail: [email protected] 2 Departments of Physics, Chemistry and Astronomy, The Ohio State University, Columbus, OH 43210, USA Received 9 July 2007 / Accepted 17 August 2007 ABSTRACT Aims. With the Green Bank telescope (GBT), seven neutral molecules have been newly detected or confirmed towards either the cold interstellar core TMC-1 or the hot core source Sgr B2(N) within the last 1–2 years. Towards TMC-1, the new molecules seen are cyanoallene (CH2CCHCN) and methyl triacetylene (CH3C6H) while methyl cyanoacetylene (CH3CCCN) and methyl cyanodiacety- lene (CH3C5N) were confirmed. Towards Sgr B2(N), the three newly detected molecules are cyclopropenone (c-C3H2O), ketenimine (CH2CNH), and acetamide (CH3CONH2); these are mainly seen in absorption and are primarily located in an envelope around the hot core. In this work, we report a detailed study of the gas-phase chemistry of all seven molecules. Methods. Starting with our updated gas-phase chemical reaction network osu.01.2007, we added formation and depletion reactions to treat the chemistry of each of the seven molecules. Some of these were already in our network but with incomplete chemistry, while most were not in the network at all prior to this work. We assumed the standard physical conditions for TMC-1 and assumed that these also hold for the envelope around Sgr B2(N). -
Hydroxyacetonitrile (HOCH2CN) As a Precursor for Formylcyanide (CHOCN), Ketenimine (CH2CNH), and Cyanogen (NCCN) in Astrophysical Conditions
A&A 549, A93 (2013) Astronomy DOI: 10.1051/0004-6361/201219779 & c ESO 2013 Astrophysics Hydroxyacetonitrile (HOCH2CN) as a precursor for formylcyanide (CHOCN), ketenimine (CH2CNH), and cyanogen (NCCN) in astrophysical conditions G. Danger1, F. Duvernay1, P. Theulé1, F. Borget1, J.-C. Guillemin2, and T. Chiavassa1 1 Aix-Marseille Univ, CNRS, PIIM UMR 7345, 13397 Marseille, France e-mail: [email protected] 2 Institut des Sciences Chimiques de Rennes, École Nationale Supérieure de Chimie de Rennes, CNRS, UMR 6226, Avenue du Général Leclerc, CS 50837, 35708 Rennes Cedex 7, France Received 8 June 2012 / Accepted 19 November 2012 ABSTRACT Context. The reactivity in astrophysical environments can be investigated in the laboratory through experimental simulations, which provide understanding of the formation of specific molecules detected in the solid phase or in the gas phase of these environments. In this context, the most complex molecules are generally suggested to form at the surface of interstellar grains and to be released into the gas phase through thermal or non-thermal desorption, where they can be detected through rotational spectroscopy. Here, we focus our experiments on the photochemistry of hydroxyacetonitrile (HOCH2CN), whose formation has been shown to compete with aminomethanol (NH2CH2OH), a glycine precursor, through the Strecker synthesis. Aims. We present the first experimental investigation of the ultraviolet (UV) photochemistry of hydroxyacetonitrile (HOCH2CN) as a pure solid or diluted in water ice. Methods. We used Fourier transform infrared (FT-IR) spectroscopy to characterize photoproducts of hydroxyacetonitrile (HOCH2CN) and to determine the different photodegradation pathways of this compound. To improve the photoproduct identifications, irradiations of hydroxyacetonitrile 14N and 15N isotopologues were performed, coupled with theoretical calculations. -
The Prebiotic Molecular Inventory of Serpens SMM1
Astronomy & Astrophysics manuscript no. SMM1_C2H3NO_isomers ©ESO 2021 January 1, 2021 The prebiotic molecular inventory of Serpens SMM1 I. An investigation of the isomers CH3NCO and HOCH2CN N.F.W. Ligterink1, A. Ahmadi2, A. Coutens3, Ł. Tychoniec2 H. Calcutt4; 5, E.F. van Dishoeck2; 6, H. Linnartz7, J.K. Jørgensen8, R.T. Garrod9, and J. Bouwman7 1 Physics Institute, University of Bern, Sidlerstrasse 5, 3012 Bern, Switzerland e-mail: [email protected] 2 Leiden Observatory, Leiden University, PO Box 9513, 2300 RA Leiden, The Netherlands 3 Laboratoire d’Astrophysique de Bordeaux, Univ. Bordeaux, CNRS, B18N, allée Geoffroy Saint-Hilaire, 33615 Pessac, France 4 Department of Space, Earth and Environment, Chalmers University of Technology, 41296, Gothenburg, Sweden 5 Institute of Astronomy, Faculty of Physics, Astronomy and Informatics, Nicolaus Copernicus University, Grudziadzka 5, 87-100 Torun, Poland 6 Max-Planck Institut für Extraterrestrische Physik (MPE), Giessenbachstr. 1, 85748 Garching, Germany 7 Laboratory for Astrophysics, Leiden Observatory, Leiden University, PO Box 9513, 2300 RA Leiden, The Netherlands 8 Centre for Star and Planet Formation, Niels Bohr Institute & Natural History Museum of Denmark, University of Copenhagen, Øster Voldgade 5–7, 1350 Copenhagen K., Denmark 9 Departments of Chemistry and Astronomy, University of Virginia, Charlottesville, VA 22904, USA Received October 8, 2020; accepted December 22, 2020 ABSTRACT Aims. Methyl isocyanate (CH3NCO) and glycolonitrile (HOCH2CN) are isomers and prebiotic molecules that are involved in the formation of peptide structures and the nucleobase adenine, respectively. These two species are investigated to study the interstellar chemistry of cyanides (CN) and isocyanates (NCO) and to gain insight into the reservoir of interstellar prebiotic molecules. -
1. Nucleotides A. Pentose Sugars – 5-Carbon Sugar 1) Deoxyribose – in DNA 2) Ribose – in RNA B. Phosphate Group C. Nitroge
1. Nucleotides a. Pentose sugars – 5-Carbon sugar 1) Deoxyribose – in DNA 2) Ribose – in RNA b. Phosphate group c. Nitrogenous bases 1) Purines a) Adenine b) Guanine 2) Pyrimidines a) Cytosine b) Thymine 2. Types of Nucleic Acids a. DNA 1) Locations 2) Functions b. RNA 1) Locations 2) Functions E. High Energy Biomolecules 1. Adenosine triphosphate a. Uses 1) Active transport 2) Movement 3) Biosynthesis reactions b. Regeneration 1) ADP + Pi + Energy → ATP 4. Classes of proteins a. Structural – ex. Collagen, keratin b. Transport – Hemoglobin, many β-globulins c. Contractile – Actin and Myosin of muscle tissue d. Regulatory - Hormones e. Immunologic - Antibodies f. Clotting – Thrombin and Fibrin g. Osmotic - Albumin h. Catalytic – Enzymes 1) Characteristics of enzymes • Proteins (most); ribonucleoproteins (few/ribozymes) • Act as organic catalysts • Lower the activation energy of reactions • Not changed by the reaction • Bind to their substrates o Lock-and-key model of enzyme activity o Induced-fit model • Highly specific • Named by adding -ase to substrate name; e.g., maltose/maltase • May require cofactors which may be: o Nonprotein metal ions such as copper, manganese, potassium, sodium o Small organic molecules known as coenzymes. The B vitamins like thiamine (B1) riboflavin (B2) and nicotinamide are precursors of coenzymes. • May require activation; e.g., pepsinogen pepsin in stomach chief cells 4. Factors Affecting Enzyme Action • pH o pepsin (stomach) @ pH = 2; trypsin (small int.) @ pH = 8 • Temperature o Denatured by high temp’s. • Enzyme inhibitors o Competitive inhibitors o Noncompetitive inhibitors • Effect of substrate concentration and reversible reactions and the Law of Mass D. -
Multi-Enzymatic Cascades in the Synthesis of Modified Nucleosides
biomolecules Article Multi-Enzymatic Cascades in the Synthesis of Modified Nucleosides: Comparison of the Thermophilic and Mesophilic Pathways Ilja V. Fateev , Maria A. Kostromina, Yuliya A. Abramchik, Barbara Z. Eletskaya , Olga O. Mikheeva, Dmitry D. Lukoshin, Evgeniy A. Zayats , Maria Ya. Berzina, Elena V. Dorofeeva, Alexander S. Paramonov , Alexey L. Kayushin, Irina D. Konstantinova * and Roman S. Esipov Shemyakin and Ovchinnikov Institute of Bioorganic Chemistry RAS, Miklukho-Maklaya 16/10, 117997 GSP, B-437 Moscow, Russia; [email protected] (I.V.F.); [email protected] (M.A.K.); [email protected] (Y.A.A.); [email protected] (B.Z.E.); [email protected] (O.O.M.); [email protected] (D.D.L.); [email protected] (E.A.Z.); [email protected] (M.Y.B.); [email protected] (E.V.D.); [email protected] (A.S.P.); [email protected] (A.L.K.); [email protected] (R.S.E.) * Correspondence: [email protected]; Tel.: +7-905-791-1719 ! Abstract: A comparative study of the possibilities of using ribokinase phosphopentomutase ! nucleoside phosphorylase cascades in the synthesis of modified nucleosides was carried out. Citation: Fateev, I.V.; Kostromina, Recombinant phosphopentomutase from Thermus thermophilus HB27 was obtained for the first time: M.A.; Abramchik, Y.A.; Eletskaya, a strain producing a soluble form of the enzyme was created, and a method for its isolation and B.Z.; Mikheeva, O.O.; Lukoshin, D.D.; chromatographic purification was developed. It was shown that cascade syntheses of modified nu- Zayats, E.A.; Berzina, M.Y..; cleosides can be carried out both by the mesophilic and thermophilic routes from D-pentoses: ribose, Dorofeeva, E.V.; Paramonov, A.S.; 2-deoxyribose, arabinose, xylose, and 2-deoxy-2-fluoroarabinose. -
Dimethyl Sulfoxide Oxidation of Primary Alcohols
Western Michigan University ScholarWorks at WMU Master's Theses Graduate College 8-1966 Dimethyl Sulfoxide Oxidation of Primary Alcohols Carmen Vargas Zenarosa Follow this and additional works at: https://scholarworks.wmich.edu/masters_theses Part of the Chemistry Commons Recommended Citation Zenarosa, Carmen Vargas, "Dimethyl Sulfoxide Oxidation of Primary Alcohols" (1966). Master's Theses. 4374. https://scholarworks.wmich.edu/masters_theses/4374 This Masters Thesis-Open Access is brought to you for free and open access by the Graduate College at ScholarWorks at WMU. It has been accepted for inclusion in Master's Theses by an authorized administrator of ScholarWorks at WMU. For more information, please contact [email protected]. DIMETHYL SULFOXIDE OXIDATION OF PRIMARY ALCOHOLS by Carmen Vargas Zenarosa A thesis presented to the Faculty of the School of Graduate Studies in partial fulfillment of the Degree of Master of Arts Western Michigan University Kalamazoo, Michigan August, 1966 ACKNOWLEDGMENTS The author wishes to express her appreciation to the members of her committee, Dr, Don C. Iffland and Dr. Donald C, Berndt, for their helpful suggestions and most especially to Dr, Robert E, Harmon for his patience, understanding, and generous amount of time given to insure the completion of this work. Appreciation is also expressed for the assistance given by her. colleagues. The author acknowledges the assistance given by the National Institutes 0f Health for this research project. Carmen Vargas Zenarosa ii TABLE OF CONTENTS Page -
DNA Stands for Deoxyribose Nucleic Acid
DNA and Protein Synthesis DNA • DNA stands for deoxyribose nucleic acid. • This chemical substance is found in the nucleus of all cells in all living organisms • DNA controls all the chemical changes which take place in cells • The kind of cell which is formed, (muscle, blood, nerve etc) is controlled by DNA Ribose is a sugar, like glucose, but with only five carbon atoms in its molecule. Deoxyribose is almost the same but lacks one oxygen atom. The nitrogen bases are: o ADENINE (A) o THYMINE (T) o CYTOSINE (C) o GUANINE (G) Nucleotides • A molecule of DNA is formed by millions of nucleotides joined together in a long chain. • DNA is a very large molecule made up of a long chain of sub-units. • The sub-units are called nucleotides. • Each nucleotide is made up of a sugar called deoxyribose, a phosphate group -PO4 and an organic (Nitrogen) base: A, T, C, G BASE PAIRING RULE amount of C= amount of G AND amount of A= amount of T • Adenine always pairs with thymine, and guanine always pairs with cytosine. DNA STRUCTURE • The nucleotide bases will point to the inside of the DNA molecule while the outside (backbone) of the DNA molecule will be made of the sugar and phosphate molecules. • When complete the DNA molecule forms a double helix (two spiral sides wrapped together). • The paired strands are coiled into a spiral called A DOUBLE HELIX. Genes • Each chromosome contains hundreds of genes. • Most of your characteristics: hair color, height, how things taste to a person, are determined by the kinds of proteins cells make (gene). -
(12) United States Patent (10) Patent No.: US 8,604,000 B2 De Kort Et Al
USOO8604000B2 (12) United States Patent (10) Patent No.: US 8,604,000 B2 de Kort et al. (45) Date of Patent: Dec. 10, 2013 (54) PALATABLE NUTRITIONAL COMPOSITION 2011/0027391 A1 2/2011 De Kort et al. COMPRISING ANUCLEOTDE AND/ORA 2013, OO12469 A1 1/2013 De Kort et al. NUCLEOSDE AND A TASTE MASKING 2013, OO18012 A1 1/2013 Hageman et al. AGENT FOREIGN PATENT DOCUMENTS (75) Inventors: Esther Jacqueline de Kort, Wageningen EP O 175468 A2 3, 1986 (NL); Martine Groenendijk, EP 1216 041 B1 6, 2002 EP 1282 365 B1 2, 2003 Barendrecht (NL); Patrick Joseph EP 1656 839 A1 5, 2006 Gerardus Hendrikus Kamphuis, EP 1666 092 A2 6, 2006 Utrecht (NL) EP 18OO 675 A1 6, 2007 JP 64-080250 A 3, 1989 (73) Assignee: N.V. Nutricia, Zoetermeer (NL) JP 06-237734. A 8, 1994 JP 10-004918 A 1, 1998 JP 10-136937 A 5, 1998 (*) Notice: Subject to any disclaimer, the term of this JP 11-071274. A 3, 1999 patent is extended or adjusted under 35 WO WO-0038829 A1 T 2000 U.S.C. 154(b) by 213 days. WO WO-01 (32034 A1 5, 2001 WO WO-02/088159 A1 11, 2002 WO WO-02/096464 A1 12/2002 (21) Appl. No.: 12/809,431 WO WO-03 (013276 A1 2, 2003 WO WO-03/041701 A2 5, 2003 (22) PCT Filed: Dec. 22, 2008 WO WO-2005/039597 A2 5, 2005 WO WO-2006/031683 A2 3, 2006 (86). PCT No.: PCT/NL2O08/050843 WO WO-2006,118665 A2 11/2006 WO WO-2006, 127620 A2 11/2006 S371 (c)(1), WO WO-2007/001883 A2 1, 2007 (2), (4) Date: Dec. -
Ketenes 25/01/2014 Part 1
Baran Group Meeting Hai Dao Ketenes 25/01/2014 Part 1. Introduction Ph Ph n H Pr3N C A brief history Cl C Ph + nPr NHCl Ph O 3 1828: Synthesis of urea = the starting point of modern organic chemistry. O 1901: Wedekind's proposal for the formation of ketene equivalent (confirmed by Staudinger 1911) Wedekind's proposal (1901) 1902: Wolff rearrangement, Wolff, L. Liebigs Ann. Chem. 1902, 325, 129. 2 Wolff adopt a ketene structure in 1912. R 2 hν R R2 1905: First synthesis and characterization of a ketene: in an efford to synthesize radical 2, 1 ROH R C Staudinger has synthesized diphenylketene 3, Staudinger, H. et al., Chem. Ber. 1905, 1735. N2 1 RO CH or Δ C R C R1 1907-8: synthesis and dicussion about structure of the parent ketene, Wilsmore, O O J. Am. Chem. Soc. 1907, 1938; Wilsmore and Stewart Chem. Ber. 1908, 1025; Staudinger and Wolff rearrangement (1902) O Klever Chem. Ber. 1908, 1516. Ph Ph Cl Zn Ph O hot Pt wire Zn Br Cl Cl CH CH2 Ph C C vs. C Br C Ph Ph HO O O O O O O O 1 3 (isolated) 2 Wilsmore's synthesis and proposal (1907-8) Staudinger's synthesis and proposal (1908) wanted to make Staudinger's discovery (1905) Latest books: ketene (Tidwell, 1995), ketene II (Tidwell, 2006), Science of Synthesis, Vol. 23 (2006); Latest review: new direactions in ketene chemistry: the land of opportunity (Tidwell et al., Eur. J. Org. Chem. 2012, 1081). Search for ketenes, Google gave 406,000 (vs. -
Effects of Metal Ions in Free Radical Reactions Richard Duane Kriens Iowa State University
Iowa State University Capstones, Theses and Retrospective Theses and Dissertations Dissertations 1963 Effects of metal ions in free radical reactions Richard Duane Kriens Iowa State University Follow this and additional works at: https://lib.dr.iastate.edu/rtd Part of the Organic Chemistry Commons Recommended Citation Kriens, Richard Duane, "Effects of metal ions in free radical reactions " (1963). Retrospective Theses and Dissertations. 2544. https://lib.dr.iastate.edu/rtd/2544 This Dissertation is brought to you for free and open access by the Iowa State University Capstones, Theses and Dissertations at Iowa State University Digital Repository. It has been accepted for inclusion in Retrospective Theses and Dissertations by an authorized administrator of Iowa State University Digital Repository. For more information, please contact [email protected]. This dissertation has been 64—3880 microfilmed exactly as received KRIENS, Richard Duane, 1932- EFFECTS OF METAL IONS IN FREE RADICAL REACTIONS. Iowa State University of Science and Technology Ph.D„ 1963 Chemistry, organic University Microfilms, Inc., Ann Arbor, Michigan EFFECTS OF METAL IONS IN FREE RADICAL REACTIONS by Richard Duane Kriens A Dissertation Submitted to the Graduate Faculty in Partial Fulfillment of The Requirements for the Degree of DOCTOR OF PHILOSOPHY Major Subject: Organic Chemistry Approved: Signature was redacted for privacy. In Charge of Major Work Signature was redacted for privacy. ead of Major Departmei^ Signature was redacted for privacy. Iowa State University Of Science and Technology Ames, Iowa 1963 11 TABLE OF CONTENTS Page PART I. REACTIONS OF RADICALS WITH METAL SALTS. ... 1 INTRODUCTION 2 REVIEW OF LITERATURE 3 RESULTS AND DISCUSSION 17 EXPERIMENTAL 54 Chemicals 54 Apparatus and Procedure 66 Reactions of compounds with the 2-cyano-2-propyl radical 66 Reactions of compounds with the phenyl radical 67 Procedure for Sandmeyer type reaction. -
Nucleosides & Nucleotides
Nucleosides & Nucleotides Biochemistry Fundamentals > Genetic Information > Genetic Information NUCLEOSIDE AND NUCLEOTIDES SUMMARY NUCLEOSIDES  • Comprise a sugar and a base NUCLEOTIDES  • Phosphorylated nucleosides (at least one phosphorus group) • Link in chains to form polymers called nucleic acids (i.e. DNA and RNA) N-BETA-GLYCOSIDIC BOND  • Links nitrogenous base to sugar in nucleotides and nucleosides • Purines: C1 of sugar bonds with N9 of base • Pyrimidines: C1 of sugar bonds with N1 of base PHOSPHOESTER BOND • Links C3 or C5 hydroxyl group of sugar to phosphate NITROGENOUS BASES  • Adenine • Guanine • Cytosine • Thymine (DNA) 1 / 8 • Uracil (RNA) NUCLEOSIDES • =sugar + base • Adenosine • Guanosine • Cytidine • Thymidine • Uridine NUCLEOTIDE MONOPHOSPHATES – ADD SUFFIX 'SYLATE' • = nucleoside + 1 phosphate group • Adenylate • Guanylate • Cytidylate • Thymidylate • Uridylate Add prefix 'deoxy' when the ribose is a deoxyribose: lacks a hydroxyl group at C2. • Thymine only exists in DNA (deoxy prefix unnecessary for this reason) • Uracil only exists in RNA NUCLEIC ACIDS (DNA AND RNA)  • Phosphodiester bonds: a phosphate group attached to C5 of one sugar bonds with - OH group on C3 of next sugar • Nucleotide monomers of nucleic acids exist as triphosphates • Nucleotide polymers (i.e. nucleic acids) are monophosphates • 5' end is free phosphate group attached to C5 • 3' end is free -OH group attached to C3 2 / 8 FULL-LENGTH TEXT • Here we will learn about learn about nucleoside and nucleotide structure, and how they create the backbones of nucleic acids (DNA and RNA). • Start a table, so we can address key features of nucleosides and nucleotides. • Denote that nucleosides comprise a sugar and a base.