Radiolysis Generates a Complex Organosynthetic Chemical Network
Total Page:16
File Type:pdf, Size:1020Kb
Load more
Recommended publications
-
Modelling Panspermia in the TRAPPIST-1 System
October 13, 2017 Modelling panspermia in the TRAPPIST-1 system James A. Blake1,2*, David J. Armstrong1,2, Dimitri Veras1,2 Abstract The recent ground-breaking discovery of seven temperate planets within the TRAPPIST-1 system has been hailed as a milestone in the development of exoplanetary science. Centred on an ultra-cool dwarf star, the planets all orbit within a sixth of the distance from Mercury to the Sun. This remarkably compact nature makes the system an ideal testbed for the modelling of rapid lithopanspermia, the idea that micro-organisms can be distributed throughout the Universe via fragments of rock ejected during a meteoric impact event. We perform N-body simulations to investigate the timescale and success-rate of lithopanspermia within TRAPPIST-1. In each simulation, test particles are ejected from one of the three planets thought to lie within the so-called ‘habitable zone’ of the star into a range of allowed orbits, constrained by the ejection velocity and coplanarity of the case in question. The irradiance received by the test particles is tracked throughout the simulation, allowing the overall radiant exposure to be calculated for each one at the close of its journey. A simultaneous in-depth review of space microbiological literature has enabled inferences to be made regarding the potential survivability of lithopanspermia in compact exoplanetary systems. 1Department of Physics, University of Warwick, Coventry, CV4 7AL 2Centre for Exoplanets and Habitability, University of Warwick, Coventry, CV4 7AL *Corresponding author: [email protected] Contents Universe, and can propagate from one location to another. This interpretation owes itself predominantly to the works of William 1 Introduction1 Thompson (Lord Kelvin) and Hermann von Helmholtz in the 1.1 Mechanisms for panspermia...............2 latter half of the 19th Century. -
Prebiological Evolution and the Metabolic Origins of Life
Prebiological Evolution and the Andrew J. Pratt* Metabolic Origins of Life University of Canterbury Keywords Abiogenesis, origin of life, metabolism, hydrothermal, iron Abstract The chemoton model of cells posits three subsystems: metabolism, compartmentalization, and information. A specific model for the prebiological evolution of a reproducing system with rudimentary versions of these three interdependent subsystems is presented. This is based on the initial emergence and reproduction of autocatalytic networks in hydrothermal microcompartments containing iron sulfide. The driving force for life was catalysis of the dissipation of the intrinsic redox gradient of the planet. The codependence of life on iron and phosphate provides chemical constraints on the ordering of prebiological evolution. The initial protometabolism was based on positive feedback loops associated with in situ carbon fixation in which the initial protometabolites modified the catalytic capacity and mobility of metal-based catalysts, especially iron-sulfur centers. A number of selection mechanisms, including catalytic efficiency and specificity, hydrolytic stability, and selective solubilization, are proposed as key determinants for autocatalytic reproduction exploited in protometabolic evolution. This evolutionary process led from autocatalytic networks within preexisting compartments to discrete, reproducing, mobile vesicular protocells with the capacity to use soluble sugar phosphates and hence the opportunity to develop nucleic acids. Fidelity of information transfer in the reproduction of these increasingly complex autocatalytic networks is a key selection pressure in prebiological evolution that eventually leads to the selection of nucleic acids as a digital information subsystem and hence the emergence of fully functional chemotons capable of Darwinian evolution. 1 Introduction: Chemoton Subsystems and Evolutionary Pathways Living cells are autocatalytic entities that harness redox energy via the selective catalysis of biochemical transformations. -
Chemical Evolution Theory of Life's Origins the Lattimer, AST 248, Lecture 13 – P.2/20 Organics
Chemical Evolution Theory of Life's Origins 1. the synthesis and accumulation of small organic molecules, or monomers, such as amino acids and nucleotides. • Production of glycine (an amino acid) energy 3HCN+2H2O −→ C2H5O2N+CN2H2. • Production of adenine (a base): 5 HCN → C5H5N5, • Production of ribose (a sugar): 5H2CO → C5H10O5. 2. the joining of these monomers into polymers, including proteins and nucleic acids. Bernal showed that clay-like materials could serve as sites for polymerization. 3. the concentration of these molecules into droplets, called protobionts, that had chemical characteristics different from their surroundings. This relies heavily on the formation of a semi-permeable membrane, one that allows only certain materials to flow one way or the other through it. Droplet formation requires a liquid with a large surface tension, such as water. Membrane formation naturally occurs if phospholipids are present. 4. The origin of heredity, or a means of relatively error-free reproduction. It is widely, but not universally, believed that RNA-like molecules were the first self-replicators — the RNA world hypothesis. They may have been preceded by inorganic self-replicators. Lattimer, AST 248, Lecture 13 – p.1/20 Acquisition of Organic Material and Water • In the standard model of the formatio of the solar system, volatile materials are concentrated in the outer solar system. Although there is as much carbon as nearly all other heavy elements combined in the Sun and the bulk of the solar nebula, the high temperatures in the inner solar system have lead to fractional amounts of C of 10−3 of the average. -
Nomination Background: Dihydroxyacetone (CASRN: 96-26-4)
SUMMARY OF DATA FOR CHEMICAL SELECTION Dihydroxyacetone 96-26-4 BASIS OF NOMINATION TO THE CSWG As consumers have become more mindful of the hazards ofa "healthy tan," more individuals have turned to sunless tanning. Sunless tanning products represent about 10% of the $400 million market for suntan preparations, and these products are the fastest growing segment of the suntanning preparation market. All sunless tanners contain dihydroxyacetone. Information on the toxicity of dihydroxyacetone appears contradictory. A mutagen that induces DNA strand breaks, dihydroxyacetone is also an intermediate in carbohydrate metabolism in higher plants and animals. Such contradictions are not unprecedented, and it has been suggested that autooxidation of cx-hydroxycarbonyl compounds including reducing sugars may play a role in diseases associated with age and diabetes (Morita, 1991 ). When dihydroxyacetone was applied to the skin of mice, no carcinogenic effect was observed. It is unclear whether this negative response was caused by a failure ofthe compound to penetrate the skin. If so, extrapolating the dermal results to other routes of exposure would not be appropriate. NCI is nominating dihydroxyacetone to the NTP for dermal penetration studies in rats and mice to determine whether dihydroxyacetone can penetrate the skin. This information will clarify whether additional testing of dihydroxyacetone is warranted. Dihydroxyacetone 96-26-4 CHEMICAL IDENTIFICATION CAS Registry Number: 96-26-4 Chemical Abstracts Service Name: 1,3-Dihydroxy-2-propanone (9CI; 8CI) Synonyms and Tradenames: 1,3-Dihydroxydimethyl ketone; Chromelin; CTF A 00816; Dihyxal; Otan; Oxantin; Oxatone; Soleal; Triulose; Viticolor Structural Class: Ketone, ketotriose compound Structure. Molecular Formula. and Molecular Weight: 0 II /c"-. -
Ganymede Science Questions and Future Exploration
Planetary Science Decadal Survey Community White Paper Ganymede science questions and future exploration Geoffrey C. Collins, Wheaton College, Norton, Massachusetts [email protected] Claudia J. Alexander, Jet Propulsion Laboratory Edward B. Bierhaus, Lockheed Martin Michael T. Bland, Washington University in St. Louis Veronica J. Bray, University of Arizona John F. Cooper, NASA Goddard Space Flight Center Frank Crary, Southwest Research Institute Andrew J. Dombard, University of Illinois at Chicago Olivier Grasset, University of Nantes Gary B. Hansen, University of Washington Charles A. Hibbitts, Johns Hopkins University Applied Physics Laboratory Terry A. Hurford, NASA Goddard Space Flight Center Hauke Hussmann, DLR, Berlin Krishan K. Khurana, University of California, Los Angeles Michelle R. Kirchoff, Southwest Research Institute Jean-Pierre Lebreton, European Space Agency Melissa A. McGrath, NASA Marshall Space Flight Center William B. McKinnon, Washington University in St. Louis Jeffrey M. Moore, NASA Ames Research Center Robert T. Pappalardo, Jet Propulsion Laboratory G. Wesley Patterson, Johns Hopkins University Applied Physics Laboratory Louise M. Prockter, Johns Hopkins University Applied Physics Laboratory Kurt Retherford, Southwest Research Institute James H. Roberts, Johns Hopkins University Applied Physics Laboratory Paul M. Schenk, Lunar and Planetary Institute David A. Senske, Jet Propulsion Laboratory Adam P. Showman, University of Arizona Katrin Stephan, DLR, Berlin Federico Tosi, Istituto Nazionale di Astrofisica, Rome Roland J. Wagner, DLR, Berlin Introduction Ganymede is a planet-sized (larger than Mercury) moon of Jupiter with unique characteristics, such as being the largest satellite in the solar system, the most centrally condensed solid body in the solar system, and the only solid body in the outer solar system known to posses an internally generated magnetic field. -
A Comparative View of Radiation, Xa9745787 Photo and Photocatalytically Induced Oxidation of Water Pollutants
A COMPARATIVE VIEW OF RADIATION, XA9745787 PHOTO AND PHOTOCATALYTICALLY INDUCED OXIDATION OF WATER POLLUTANTS N. GETOFF Institute for Theoretical Chemistry and Radiation Chemistry, University of Vienna, Vienna, Austria Abstract Water resources are presently overloaded with biologically resistant (refractory) pollutants. Several oxidation methods have been developed for their degradation, the most efficient of which is iradiation treatment, particularly that based on e-beam processing in the presence of Q/O3. The next-best method is photoinduced pollutant oxidation with VUV- and/or UV-light, using HjO2 or H2O2/O3 as an additional source of OH radicals. The photocatalytic method, using e.g. TiQ as a catalyst in combination with oxidation agents such as If Oj or H2O2/O3, is also recommended. The suitability of these three methods is illustrated by examples and they are briefly discussed and compared on the basis of theirenergy consumption and efficiency. Other methods, such as ozone treatment, the photo-Fenton process, ultrasonic and elctrochemical treatments, as well as the well known biological process and thermal oxidation of refractory pollutants, are briefly mentioned. 1. INTRODUCTION Current water resources are strongly overloaded with biologically resistant pollutants, as a result of global population growth and the development of certain industries in the past few decades. The disposal of chemical waste in rivers, seas and oceans has contributed to possibly-irrepairable destruction of marine life. The application of fertilizers, pesticides etc. in modern agriculture has exacerbated the situation. Hence, urgent measures are necessary for remediation of water resources. For the degradation of water pollutants, a number of oxidation methods, based on processes initiated by ionizing radiation, UV- and visible light, photocatalytic induced reactions, as well as combinations of these, have been developed. -
Investigations of Moon-Magnetosphere Interactions by the Europa Clipper Mission
EPSC Abstracts Vol. 13, EPSC-DPS2019-366-1, 2019 EPSC-DPS Joint Meeting 2019 c Author(s) 2019. CC Attribution 4.0 license. Investigations of Moon-Magnetosphere Interactions by the Europa Clipper Mission Haje Korth (1), Robert T. Pappalardo (2), David A. Senske (2), Sascha Kempf (3), Margaret G. Kivelson (4,5), Kurt Retherford (6), J. Hunter Waite (6), Joseph H. Westlake (1), and the Europa Clipper Science Team (1) Johns Hopkins University Applied Physics Laboratory, Maryland, USA, (2) Jet Propulsion Laboratory, California, USA, (3) University of Colorado, Colorado, USA, (4) University of Michigan, Michigan, USA, (5) University of California, California, USA, (6) Southwest Research Institute, Texas, USA. ([email protected]) 1. Introduction magnetic fields inducing eddy currents in the ocean. By measuring the induced field response at multiple The influence of the Jovian space environment on frequencies, the ice shell thickness and the ocean Europa is multifaceted, and observations of moon- layer thickness and conductivity can be uniquely magnetosphere interaction by the Europa Clipper will determined. The ECM consists of four fluxgate provide an understanding of the satellite’s interior sensors mounted on a 5-m-long boom and a control structure and compositional makeup among others. electronics hosted in a vault shielding it from The variability of Jupiter’s magnetic field at Europa radiation damage. The use of four sensors allows for induces electric currents within the moon’s dynamic removal of higher-order spacecraft- conducting ocean layer, the magnitude of which generated magnetic fields on a boom that is short depends on the ocean’s location, extent, and compared with the spacecraft dimensions. -
Quantitative Estimation of Track Segment Yields of Water Radiolysis
www.nature.com/scientificreports OPEN Quantitative estimation of track segment yields of water radiolysis species under heavy ions around Bragg peak energies using Geant4‑DNA Kentaro Baba1, Tamon Kusumoto2, Shogo Okada3, Ryo Ogawara4, Satoshi Kodaira2, Quentin Rafy5, Rémi Barillon5, Nicolas Ludwig5, Catherine Galindo5, Philippe Peaupardin5 & Masayori Ishikawa1,6* − · We evaluate the track segment yield G′ of typical water radiolysis products (eaq , OH and H2O2) under heavy ions (He, C and Fe ions) using a Monte Carlo simulation code in the Geant4‑DNA. Furthermore, we reproduce experimental results of ·OH of He and C ions around the Bragg peak energies (< 6 MeV/u). In the relatively high energy region (e.g., > 10 MeV/u), the simulation results using Geant4‑DNA have agreed with experimental results. However, the G‑values of water radiolysis species have not been properly evaluated around the Bragg peak energies, at which high ionizing density can be expected. Around the Bragg peak energy, dense continuous secondary products are generated, so that it is necessary to simulate the radical–radical reaction more accurately. To do so, we added the role of secondary products formed by irradiation. Consequently, our simulation results are in good agreement with experimental results and previous simulations not only in the high‑energy region but also around the Bragg peak. Several future issues are also discussed regarding the roles of fragmentation and multi‑ionization to realize more realistic simulations. Cancer patients can nowadays select several modalities in radiotherapy such as conventional X-ray therapy and particle therapies (e.g., proton therapy, heavy ion therapy and boron neutron capture therapy). -
Radiolysis of H2O:CO2 Ices by Heavy Energetic Cosmic Ray Analogs
A&A 523, A77 (2010) Astronomy DOI: 10.1051/0004-6361/201015123 & c ESO 2010 Astrophysics Radiolysis of H2O:CO2 ices by heavy energetic cosmic ray analogs S. Pilling1, E. Seperuelo Duarte2, A. Domaracka3,H.Rothard3, P. Boduch3, and E. F. da Silveira4 1 IP&D/UNIVAP, Av. Shishima Hifumi, 2911, São Jose dos Campos, SP, Brazil e-mail: [email protected] 2 Grupo de Física e Astronomia, CEFET/Química de Nilópolis, Rua Lúcio Tavares, 1052, CEP 2653-060, Nilópolis, Brazil 3 Centre de Recherche sur les Ions, les Matériaux et la Photonique (CEA/CNRS/ENSICAEN/Université de Caen-Basse Normandie), CIMAP – CIRIL – GANIL, Boulevard Henri Becquerel, BP 5133, 14070 Caen Cedex 05, France 4 Departamento de Física, Pontifícia Universidade Católica do Rio de Janeiro (PUC-Rio), Rua Marquês de São Vicente 225, CEP 22453-900, Rio de Janeiro, Brazil Received 1 June 2010 / Accepted 3 August 2010 ABSTRACT 58 13+ An experimental study of the interaction of heavy, highly charged, and energetic ions (52 MeV Ni ) with pure H2O, pure CO2 and mixed H2O:CO2 astrophysical ice analogs is presented. This analysis aims to simulate the chemical and the physicochemical interactions induced by heavy cosmic rays inside dense and cold astrophysical environments, such as molecular clouds or protostellar clouds. The measurements were performed at the heavy ion accelerator GANIL (Grand Accélérateur National d’Ions Lourds in Caen, France). The gas samples were deposited onto a CsI substrate at 13 K. In-situ analysis was performed by a Fourier transform infrared (FTIR) spectrometer at different fluences. Radiolysis yields of the produced species were quantified. -
Origin and Temperature Dependence of Radiation Damage in Biological Samples at Cryogenic Temperatures
Origin and temperature dependence of radiation damage in biological samples at cryogenic temperatures Alke Meentsa,b,1,2, Sascha Gutmanna,1,3, Armin Wagnerc, and Clemens Schulze-Briesea aPaul Scherrer Institut, Swiss Light Source, CH-5232 Villigen, Switzerland bHamburger Synchrotronstrahlungslabor, Deutsches Elektronen Synchrotron, D-22607 Hamburg, Germany cDiamond Light Source, Harwell Science and Innovations Campus, Didcot, OX11 0DE, United Kingdom Edited by Venkatraman Ramakrishnan, Medical Research Council, Cambridge, United Kingdom, and approved November 23, 2009 (received for review May 20, 2009) Radiation damage is the major impediment for obtaining structural electrons with energies of a few up to severals tens of eV (4, 5). information from biological samples by using ionizing radiation Subsequent radiolytic reactions caused by products of primary such as x-rays or electrons. The knowledge of underlying processes damage are classified as secondary damage. Possible consequences especially at cryogenic temperatures is still fragmentary, and a con- of primary and secondary radiation damage reactions include sistent mechanism has not been found yet. By using a combination breakage of chemical bonds, redox processes, and generation of of single-crystal x-ray diffraction, small-angle scattering, and qual- free radicals. Alterations of the sample at primary and secondary itative and quantitative radiolysis experiments, we show that hy- damage sites may eventually cause long-range rearrangements of drogen gas, formed inside the sample during irradiation, rather molecules in crystals or other assemblies. The loss of crystalline than intramolecular bond cleavage between non-hydrogen atoms, order has been referred to as tertiary or global damage (1). is mainly responsible for the loss of high-resolution information In crystallography, radiation damage results in the decrease of and contrast in diffraction experiments and microscopy. -
Arxiv:1910.06396V4 [Physics.Pop-Ph] 12 Jun 2021 ∗ Rmtv Ieeitdi H R-Oa Eua(Vni H C System)
Nebula-Relay Hypothesis: Primitive Life in Nebula and Origin of Life on Earth Lei Feng1,2, ∗ 1Key Laboratory of Dark Matter and Space Astronomy, Purple Mountain Observatory, Chinese Academy of Sciences, Nanjing 210023 2Joint Center for Particle, Nuclear Physics and Cosmology, Nanjing University – Purple Mountain Observatory, Nanjing 210093, China Abstract A modified version of panspermia theory, named Nebula-Relay hypothesis or local panspermia, is introduced to explain the origin of life on Earth. Primitive life, acting as the seeds of life on Earth, originated at pre-solar epoch through physicochemical processes and then filled in the pre- solar nebula after the death of pre-solar star. Then the history of life on the Earth can be divided into three epochs: the formation of primitive life in the pre-solar epoch; pre-solar nebula epoch; the formation of solar system and the Earth age of life. The main prediction of our model is that primitive life existed in the pre-solar nebula (even in the current nebulas) and the celestial body formed therein (i.e. solar system). arXiv:1910.06396v4 [physics.pop-ph] 12 Jun 2021 ∗Electronic address: [email protected] 1 I. INTRODUCTION Generally speaking, there are several types of models to interpret the origin of life on Earth. The two most persuasive and popular models are the abiogenesis [1, 2] and pansper- mia theory [3]. The modern version of abiogenesis is also known as chemical origin theory introduced by Oparin in the 1920s [1], and Haldane proposed a similar theory independently [2] at almost the same time. In this theory, the organic compounds are naturally produced from inorganic matters through physicochemical processes and then reassembled into much more complex living creatures. -
Safety Analysis Report and Associated Documentation, TH
This page intentionally left blank to facilitate duplex printing. RH-TRU Payload Appendices Rev. 1, February 2011 TABLE OF CONTENTS 1.0 INTRODUCTION 2.0 GAS GENERATION METHODOLOGY 2.1 Radiolytic G Values for Waste Materials 2.2 G Values for RH-TRU 72-B Waste 2.3 Shipping Period – General Case 2.4 Shipping Period – Controlled Shipments 2.5 Compliance Methodology for Gas Generation Requirements 3.0 ASSESSMENT METHODS 3.1 Gas Generation Test Plan for Remote-Handled Transuranic (RH-TRU) Waste Containers 3.2 Summary of the Flammability Assessment Methodology Program 4.0 SUPPORTING EVALUATIONS 4.1 Chemical Compatibility of Waste Forms 4.2 Free Halides in the RH-TRU 72-B Payload – Source Term and Release Rate Estimates 4.3 Payload Compatibility with Butyl Rubber O-Ring Seals 4.4 Volatile Organic Compounds (VOCs) in the RH-TRU 72-B Payload – Source Term and Release Rate Estimates 4.5 Biological Activity Assessment 4.6 Thermal Stability of Payload Materials at Transport Temperatures 5.0 PAYLOAD CONTAINER DESIGN BASIS EVALUATIONS 5.1 Description of Neutron Shielded Canister i RH-TRU Payload Appendices Rev. 1, February 2011 This page intentionally left blank. ii RH-TRU Payload Appendices Rev. 1, February 2011 1.0 INTRODUCTION This document, the RH-TRU Payload Appendices, accompanies the Remote-Handled Transuranic Waste Authorized Methods for Payload Control (RH-TRAMPAC) and is provided as supplemental information pertaining to issues related to the transportation of remote-handled transuranic (RH-TRU) waste in the RH-TRU 72-B packaging. The RH-TRAMPAC contains all information, including requirements and methods of compliance, required for the qualification of a payload for transport in the RH-TRU 72-B packaging.