Life As a Guide to Prebiotic Nucleotide Synthesis
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A Dicarboxylate/4-Hydroxybutyrate Autotrophic Carbon Assimilation Cycle in the Hyperthermophilic Archaeum Ignicoccus Hospitalis
A dicarboxylate/4-hydroxybutyrate autotrophic carbon assimilation cycle in the hyperthermophilic Archaeum Ignicoccus hospitalis Harald Huber*†, Martin Gallenberger*, Ulrike Jahn*, Eva Eylert‡, Ivan A. Berg§, Daniel Kockelkorn§, Wolfgang Eisenreich‡, and Georg Fuchs§ *Lehrstuhl fu¨r Mikrobiologie und Archaeenzentrum, Universita¨t Regensburg, Universitaetsstrasse 31, D-93053 Regensburg, Germany; ‡Lehrstuhl fu¨r Biochemie, Department Chemie, Technische Universita¨t Mu¨ nchen, Lichtenbergstrasse 4, D-85748 Garching, Germany; and §Lehrstuhl fu¨r Mikrobiologie, Universita¨t Freiburg, Scha¨nzlestrasse 1, D-79104 Freiburg, Germany Edited by Dieter So¨ll, Yale University, New Haven, CT, and approved April 1, 2008 (received for review February 1, 2008) Ignicoccus hospitalis is an anaerobic, autotrophic, hyperthermophilic starting from acetyl-CoA (4). On the basis of these data, pyruvate Archaeum that serves as a host for the symbiotic/parasitic Archaeum synthase and phosphoenolpyruvate (PEP) carboxylase were pos- Nanoarchaeum equitans. It uses a yet unsolved autotrophic CO2 tulated as CO2 fixing enzymes, with PEP carboxylase serving as the fixation pathway that starts from acetyl-CoA (CoA), which is reduc- only enzyme used for oxaloacetate synthesis. In addition, the tively carboxylated to pyruvate. Pyruvate is converted to phosphoe- operation of an incomplete ‘‘horseshoe-type’’ citric acid cycle, in nol-pyruvate (PEP), from which glucogenesis as well as oxaloacetate which 2-oxoglutarate oxidation does not take place, was demon- formation branch off. Here, we present the complete metabolic cycle strated. Enzyme and labeling data indicated a conventional glu- by which the primary CO2 acceptor molecule acetyl-CoA is regener- coneogenesis, but with some enzymes unrelated to those of the ated. Oxaloacetate is reduced to succinyl-CoA by an incomplete classical pathway. -
Recreating Ancient Metabolic Pathways Before Enzymes Kamila B
Recreating ancient metabolic pathways before enzymes Kamila B. Muchowska, Elodie Chevallot-Beroux, Joseph Moran To cite this version: Kamila B. Muchowska, Elodie Chevallot-Beroux, Joseph Moran. Recreating ancient metabolic path- ways before enzymes. Bioorganic and Medicinal Chemistry, Elsevier, 2019, 27 (12), pp.2292-2297. 10.1016/j.bmc.2019.03.012. hal-02516541 HAL Id: hal-02516541 https://hal.archives-ouvertes.fr/hal-02516541 Submitted on 23 Mar 2020 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. Graphical Abstract To create your abstract, type over the instructions in the template box below. Fonts or abstract dimensions should not be changed or altered. Recreating ancient metabolic pathways Leave this area blank for abstract info. before enzymes Kamila B. Muchowskaa* , Elodie Chevallot-Berouxa, and Joseph Morana* University of Strasbourg, CNRS, ISIS UMR 7006, 67000 Strasbourg, France Bioorganic & Medicinal Chemistry journal homepage: www.elsevier.com Recreating ancient metabolic pathways before enzymes Kamila B. Muchowska,a* Elodie Chevallot-Beroux,a and Joseph Morana* a University of Strasbourg, CNRS, ISIS UMR 7006, 67000 Strasbourg, France. ARTICLE INFO ABSTRACT Article history: The biochemistry of all living organisms uses complex, enzyme-catalyzed metabolic reaction Received networks. -
Interferometric Observations of Large Biologically Interesting Interstellar and Cometary Molecules
SPECIAL FEATURE: PERSPECTIVE Interferometric observations of large biologically interesting interstellar and cometary molecules Lewis E. Snyder* Department of Astronomy, University of Illinois, 1002 West Green Street, Urbana, IL 61801 Edited by William Klemperer, Harvard University, Cambridge, MA, and approved May 26, 2006 (received for review March 3, 2006) Interferometric observations of high-mass regions in interstellar molecular clouds have revealed hot molecular cores that have sub- stantial column densities of large, partly hydrogen-saturated molecules. Many of these molecules are of interest to biology and thus are labeled ‘‘biomolecules.’’ Because the clouds containing these molecules provide the material for star formation, they may provide insight into presolar nebular chemistry, and the biomolecules may provide information about the potential of the associated inter- stellar chemistry for seeding newly formed planets with prebiotic organic chemistry. In this overview, events are outlined that led to the current interferometric array observations. Clues that connect this interstellar hot core chemistry to the solar system can be found in the cometary detection of methyl formate and the interferometric maps of cometary methanol. Major obstacles to under- standing hot core chemistry remain because chemical models are not well developed and interferometric observations have not been very sensitive. Differentiation in the molecular isomers glycolaldehdye, methyl formate, and acetic acid has been observed, but not explained. The extended source structure for certain sugars, aldehydes, and alcohols may require nonthermal formation mechanisms such as shock heating of grains. Major advances in understanding the formation chemistry of hot core species can come from obser- vations with the next generation of sensitive, high-resolution arrays. -
A Survey of Carbon Fixation Pathways Through a Quantitative Lens
Journal of Experimental Botany, Vol. 63, No. 6, pp. 2325–2342, 2012 doi:10.1093/jxb/err417 Advance Access publication 26 December, 2011 REVIEW PAPER A survey of carbon fixation pathways through a quantitative lens Arren Bar-Even, Elad Noor and Ron Milo* Department of Plant Sciences, The Weizmann Institute of Science, Rehovot 76100, Israel * To whom correspondence should be addressed. E-mail: [email protected] Received 15 August 2011; Revised 4 November 2011; Accepted 8 November 2011 Downloaded from Abstract While the reductive pentose phosphate cycle is responsible for the fixation of most of the carbon in the biosphere, it http://jxb.oxfordjournals.org/ has several natural substitutes. In fact, due to the characterization of three new carbon fixation pathways in the last decade, the diversity of known metabolic solutions for autotrophic growth has doubled. In this review, the different pathways are analysed and compared according to various criteria, trying to connect each of the different metabolic alternatives to suitable environments or metabolic goals. The different roles of carbon fixation are discussed; in addition to sustaining autotrophic growth it can also be used for energy conservation and as an electron sink for the recycling of reduced electron carriers. Our main focus in this review is on thermodynamic and kinetic aspects, including thermodynamically challenging reactions, the ATP requirement of each pathway, energetic constraints on carbon fixation, and factors that are expected to limit the rate of the pathways. Finally, possible metabolic structures at Weizmann Institute of Science on July 3, 2016 of yet unknown carbon fixation pathways are suggested and discussed. -
'Impossible' Cloud on Titan Explained
‘Impossible’ Cloud on Titan Explained Cloud crystals in the super-cold environment of Titan are revealing surprising solid-state chemical processes that illuminate similar chemistry occurring in Earth’s polar stratospheric clouds. Titan’s spring brings polar ice clouds made of dicyanoacetylene (C4N2) molecules. The presence of these polar clouds seemed impossible, because Cassini infrared measurements showed there is not enough C4N2 in the stratosphere to form the observed ice clouds. So where does the C4N2 come from? Cassini found that springtime sunshine kicks off an ‘on-site’ manufacturing process that produces the icy raw material for the C4N2 clouds. Photochemical reactions between hydrogen cyanide (HCN) and cyanoacetylene (HC3N) in Titan’s stratosphere were found to produce C4N2 .This unexpected photochemical effect on icy solids explains how these Titan’s Icy Polar Clouds The cloud at right seemingly ‘impossible’ clouds form in Titan’s springtime polar contains HCN. Some stratosphere! other polar stratospheric clouds are made of Something similar occurs in Earth’s polar stratosphere, where dicyanoacetylene (C4N2) which is produced from solid-state chemistry involving chlorine is at the heart of ozone sunlight-driven processes loss in Earth’s atmosphere. Comparison of the atmospheres of occurring on frozen Earth and Titan informs us on the fundamental processes that organic particles. A similar process is seen in occur throughout nature. Earth’s stratosphere between gases and water Solid-state photochemistry as a formation mechanism for Titan's stratospheric ice particles. C4N2 ice clouds. C. Anderson, R. Samuelson, Y. Yung and J. McLain, Geophysical Research Letters, 43, 3088-3094, 2016. . -
Mitochondrial Uncoupling and the Reprograming of Intermediary Metabolism in Leukemia Cells
REVIEW ARTICLE published: 02 April 2013 doi: 10.3389/fonc.2013.00067 Mitochondrial uncoupling and the reprograming of intermediary metabolism in leukemia cells Juliana Vélez 1, Numsen Hail Jr.2,3, Marina Konopleva2,3, Zhihong Zeng 2,3, Kensuke Kojima2,3, Ismael Samudio1* and Michael Andreeff 2,3* 1 Grupo de Terapia Celular y Molecular Laboratorio de Bioquimica, Pontificia Universidad Javeriana, Bogotá, Colombia 2 Section of Molecular Hematology and Therapy, The University of Texas MD Anderson Cancer Center, Houston, TX, USA 3 Department of Leukemia, The University of Texas MD Anderson Cancer Center, Houston, TX, USA Edited by: Nearly 60 years ago Otto Warburg proposed, in a seminal publication, that an irreparable Jozsef Dudas, Medical University defect in the oxidative capacity of normal cells supported the switch to glycolysis for energy Innsbru, Austria generation and the appearance of the malignant phenotype (Warburg, 1956). Curiously, Reviewed by: Daniel Christian Hoessli, International this phenotype was also observed by Warburg in embryonic tissues, and recent research Center for Chemical and Biological demonstrated that normal stem cells may indeed rely on aerobic glycolysis – fermenting Sciences, Switzerland pyruvate to lactate in the presence of ample oxygen – rather than on the complete oxidation Jozsef Dudas, Medical University of pyruvate in the Krebs cycle – to generate cellular energy (Folmes et al., 2012). However, Innsbruck, Austria it remains to be determined whether this phenotype is causative for neoplastic develop- *Correspondence: Ismael Samudio, Laboratorio de ment, or rather the result of malignant transformation. In addition, in light of mounting Bioquimica #301, Edificio Jesús evidence demonstrating that cancer cells can carry out electron transport and oxidative Emilio Ramírez, Pontificia Universidad phosphorylation, although in some cases predominantly using electrons from non-glucose Javeriana, Cra 7 No. -
Profile of Bob B. Buchanan PROFILE
PROFILE Profile of Bob B. Buchanan PROFILE Paul Gabrielsen, Science Writer On a clear June day in 1975, Bob Buchanan and two anaerobic fermentation pro- Oslo colleagues pulled up water samples from a lake cesses responsible for their in Norway, examining the microorganisms growing at beverages. Another friend at various depths. “When we got to 6 meters,” Buchanan Duke was Melinda Speas, a recalls, “there was a band of Chlorobium growing,” graduate student in zoology. referring to a genus of green bacteria (now called Their friendship was later Chlorobaculum) that belongs to a unique class of or- rekindled in California and they ganisms called photolithotrophs. These bacteria re- married in 1965. quire sunlight for photosynthesis but obtain cellular After earning his doctorate reductants from sulfur compounds rather than water. in 1962, Buchanan secured a The bacteria buck the traditional chemical pathways postdoctoral fellowship at the for energy production and carbon fixation and instead University of California, Berkeley, use pathways discovered by Buchanan, a member of where he would spend the next the National Academy of Sciences and emeritus pro- 55 years. He hoped to work fessor at the University of California, Berkeley. with renowned microbiologist H. A. Barker, but because From Appalachia to the Laboratory Barker was on sabbatical leave Buchanan was born in 1937 in Richmond, Virginia. at the time, Buchanan instead Fearing for the family’s safety during World War II, joined the group of Barker’s Buchanan’s mother took him and his two older sisters former student, Jesse Rabinowitz. to a family farm in Southwest Virginia, near the Ap- Buchanan and Rabinowitz crys- Bob B. -
Synthesis of Activated Pyrimidine Ribonucleotides in Prebiotically Plausible Conditions
Vol 459 | 14 May 2009 | doi:10.1038/nature08013 LETTERS Synthesis of activated pyrimidine ribonucleotides in prebiotically plausible conditions Matthew W. Powner1,Be´atrice Gerland1 & John D. Sutherland1 At some stage in the origin of life, an informational polymer must we have discovered a short, highly efficient route to activated pyrimi- have arisen by purely chemical means. According to one version of dine ribonucleotides from these same precursors that proceeds by way the ‘RNA world’ hypothesis1–3 this polymer was RNA, but attempts of alternative intermediates (Fig. 1, green arrows). By contrast with to provide experimental support for this have failed4,5. In parti- previously investigated routes to ribonucleotides, ours bypasses ribose cular, although there has been some success demonstrating that and the free pyrimidine nucleobases. Mixed nitrogenous–oxygenous ‘activated’ ribonucleotides can polymerize to form RNA6,7,itis chemistry first results in the reaction of cyanamide 8 and glycolalde- far from obvious how such ribonucleotides could have formed from hyde 10, giving 2-amino-oxazole 11, and this heterocycle then adds to their constituent parts (ribose and nucleobases). Ribose is difficult glyceraldehyde 9 to give the pentose amino-oxazolines including the to form selectively8,9, and the addition of nucleobases to ribose is arabinose derivative 12. Reaction of 12 with cyanoacetylene 7 then inefficient in the case of purines10 and does not occur at all in the gives the anhydroarabinonucleoside 13, which subsequently under- case of the canonical pyrimidines11. Here we show that activated goes phosphorylation with rearrangement to furnish b-ribocytidine- pyrimidine ribonucleotides can be formed in a short sequence that 29,39-cyclic phosphate 1. -
10 Metabolism
Route to life by chemical networks P. L. Luisi Mol Syst Biol. 2014, 10, 729 Metabolism-first vs. Genes-first Genetics/replication-first: an information-carrying polymer capable of replication (RNA or something simpler) spontaneously arose from available prebiotic molecules available on early Earth. Metabolism incorporated later as a mean to receive energy from the surroundings in a controlled manner. Metabolism-first: primitive metabolic cycles spontaneously assembled from simple prebiotic organic molecules or inorganic carbon sources as CO2. And the cycles produced a set or more or less complex molecules needed for the replication process and construction of the genetic apparatus. The supposed proto-metabolism would differ from the currently known one, because the chemical reactions were not catalysed by efficient enzymes, nor were aminoacid and peptide sequences determined by DNA. The involved reactions were either spontaneous, or catalysed by inorganic catalysts or peptides. Inorganic catalysts would be molecules, or ions, in solutions or on surfaces of solids such as clays or pyrites. Peptides (or peptoids) formed either by random oligomerization or mutual catalysis. Metabolism and self-organization of chemical networks One of pre-conditions for life is to be far from thermodynamic equilibrium. Life uses non-linear effects to amplify and stabilize minor environmental effects Spatial and temporal synchronisation of reactive processes provides molecules with patterns of collective behavior. Under certain conditions far from thermodynamic equilibrium, heterogenous mixtures can trigger emergent properties at the collective level. Oscilatory and autocatalytic processes are very common in biological systems. Examples include: metabolic cycles, immune response, or apoptosis. Oscilatory reactions – importance for homeostasis. -
The Dissipative Photochemical Origin of Life: UVC Abiogenesis of Adenine
entropy Article The Dissipative Photochemical Origin of Life: UVC Abiogenesis of Adenine Karo Michaelian Department of Nuclear Physics and Applications of Radiation, Instituto de Física, Universidad Nacional Autónoma de México, Circuito Interior de la Investigación Científica, Cuidad Universitaria, Mexico City, C.P. 04510, Mexico; karo@fisica.unam.mx Abstract: The non-equilibrium thermodynamics and the photochemical reaction mechanisms are described which may have been involved in the dissipative structuring, proliferation and complex- ation of the fundamental molecules of life from simpler and more common precursors under the UVC photon flux prevalent at the Earth’s surface at the origin of life. Dissipative structuring of the fundamental molecules is evidenced by their strong and broad wavelength absorption bands in the UVC and rapid radiationless deexcitation. Proliferation arises from the auto- and cross-catalytic nature of the intermediate products. Inherent non-linearity gives rise to numerous stationary states permitting the system to evolve, on amplification of a fluctuation, towards concentration profiles providing generally greater photon dissipation through a thermodynamic selection of dissipative efficacy. An example is given of photochemical dissipative abiogenesis of adenine from the precursor HCN in water solvent within a fatty acid vesicle floating on a hot ocean surface and driven far from equilibrium by the incident UVC light. The kinetic equations for the photochemical reactions with diffusion are resolved under different environmental conditions and the results analyzed within the framework of non-linear Classical Irreversible Thermodynamic theory. Keywords: origin of life; dissipative structuring; prebiotic chemistry; abiogenesis; adenine; organic molecules; non-equilibrium thermodynamics; photochemical reactions Citation: Michaelian, K. The Dissipative Photochemical Origin of MSC: 92-10; 92C05; 92C15; 92C40; 92C45; 80Axx; 82Cxx Life: UVC Abiogenesis of Adenine. -
Pyrolysis and Combustion of Acetonitrile (Ch3cn)
OAK RIDGE ORNL/TM-2002/113 NATIONAL LABORATORY MANAGED BY UT-BATTELLE FOR THE DEPARTMENT OF ENERGY Pyrolysis and Combustion of Acetonitrile (CH3CN) Phillip F. Britt DOCUMENT AVAILABILITY Reports produced after January 1, 1996, are generally available free via the U.S. Department of Energy (DOE) Information Bridge. Web site http://www.osti.gov/bridge Reports produced before January 1, 1996, may be purchased by members of the public from the following source. National Technical Information Service 5285 Port Royal Road Springfield, VA 22161 Telephone 703-605-6000 (1-800-553-6847) TDD 703-487-4639 Fax 703-605-6900 E-mail [email protected] Web site http://www.ntis.gov/support/ordernowabout.htm Reports are available to DOE employees, DOE contractors, Energy Technology Data Exchange (ETDE) representatives, and International Nuclear Information System (INIS) representatives from the following source. Office of Scientific and Technical Information P.O. Box 62 Oak Ridge, TN 37831 Telephone 865-576-8401 Fax 865-576-5728 E-mail [email protected] Web site http://www.osti.gov/contact.html This report was prepared as an account of work sponsored by an agency of the United States Government. Neither the United States Government nor any agency thereof, nor any of their employees, makes any warranty, express or implied, or assumes any legal liability or responsibility for the accuracy, completeness, or usefulness of any information, apparatus, product, or process disclosed, or represents that its use would not infringe privately owned rights. Reference herein to any specific commercial product, process, or service by trade name, trademark, manufacturer, or otherwise, does not necessarily constitute or imply its endorsement, recommendation, or favoring by the United States Government or any agency thereof. -
Investigating the Chemical Composition of the CIRS-Observed 160 Cm-1 Ice Cloud in Titan’S Stratosphere
EPSC Abstracts Vol. 14, EPSC2020-423, 2020 https://doi.org/10.5194/epsc2020-423 Europlanet Science Congress 2020 © Author(s) 2021. This work is distributed under the Creative Commons Attribution 4.0 License. Investigating the Chemical Composition of the CIRS-Observed 160 cm-1 Ice Cloud in Titan’s Stratosphere Melissa Ugelow1,2 and Carrie Anderson1 1NASA Goddard Space Flight Center, Astrochemistry Laboratory, Greenbelt, MD, United States of America 2Universities Space Research Association, Columbia, MD, United States of America Remote sensing observations from Voyager 1’s InfraRed Interferometer Spectrometer (IRIS) and Cassini’s Composite InfraRed Spectrometer (CIRS) confirmed the presence of nitrile ice clouds in Titan’s stratosphere (Samuelson 1985, 1992; Khanna, R.K. et al., 1987; Samuelson et al., 1997, 2007; Coustenis, A. et al., 1999; Mayo and Samuelson, 2005; Anderson, C.M. et al., 2010, 2018a,b; Anderson and Samuelson, 2011). While individual gases in Titan’s stratosphere are expected to condense to form pure ices, some of these gases will enter altitude regions where they undergo simultaneous saturation, or co-condensation, and form a mixed ice. The infrared spectral features resulting from a mixed ice have their own unique spectral signatures that notably diverge from the weighted sum of the individual species, and must therefore be experimentally determined as functions of temperature and mixing ratio (Anderson and Samuelson, 2011; Anderson et al. 2018a,b). The first observation of a co-condensate in Titan’s stratosphere was acquired by CIRS, which revealed a spectrally broad quasi-continuum ice emission feature with a spectral peak near 160 cm-1.