Most Important 1: Chemical Bonding Occurs When One Or More Electrons Are Simultaneously Attracted to Two Nuclei
Total Page:16
File Type:pdf, Size:1020Kb
Load more
Recommended publications
-
Physical and Analytical Electrochemistry: the Fundamental
Electrochemical Systems The simplest and traditional electrochemical process occurring at the boundary between an electronically conducting phase (the electrode) and an ionically conducting phase (the electrolyte solution), is the heterogeneous electro-transfer step between the electrode and the electroactive species of interest present in the solution. An example is the plating of nickel. Ni2+ + 2e- → Ni Physical and Analytical The interface is where the action occurs but connected to that central event are various processes that can Electrochemistry: occur in parallel or series. Figure 2 demonstrates a more complex interface; it represents a molecular scale snapshot The Fundamental Core of an interface that exists in a fuel cell with a solid polymer (capable of conducting H+) as an electrolyte. of Electrochemistry However, there is more to an electrochemical system than a single by Tom Zawodzinski, Shelley Minteer, interface. An entire circuit must be made and Gessie Brisard for measurable current to flow. This circuit consists of the electrochemical cell plus external wiring and circuitry The common event for all electrochemical processes is that (power sources, measuring devices, of electron transfer between chemical species; or between an etc). The cell consists of (at least) electrode and a chemical species situated in the vicinity of the two electrodes separated by (at least) one electrolyte solution. Figure 3 is electrode, usually a pure metal or an alloy. The location where a schematic of a simple circuit. Each the electron transfer reactions take place is of fundamental electrode has an interface with a importance in electrochemistry because it regulates the solution. Electrons flow in the external behavior of most electrochemical systems. -
Constraint Closure Drove Major Transitions in the Origins of Life
entropy Article Constraint Closure Drove Major Transitions in the Origins of Life Niles E. Lehman 1 and Stuart. A. Kauffman 2,* 1 Edac Research, 1879 Camino Cruz Blanca, Santa Fe, NM 87505, USA; [email protected] 2 Institute for Systems Biology, Seattle, WA 98109, USA * Correspondence: [email protected] Abstract: Life is an epiphenomenon for which origins are of tremendous interest to explain. We provide a framework for doing so based on the thermodynamic concept of work cycles. These cycles can create their own closure events, and thereby provide a mechanism for engendering novelty. We note that three significant such events led to life as we know it on Earth: (1) the advent of collective autocatalytic sets (CASs) of small molecules; (2) the advent of CASs of reproducing informational polymers; and (3) the advent of CASs of polymerase replicases. Each step could occur only when the boundary conditions of the system fostered constraints that fundamentally changed the phase space. With the realization that these successive events are required for innovative forms of life, we may now be able to focus more clearly on the question of life’s abundance in the universe. Keywords: origins of life; constraint closure; RNA world; novelty; autocatalytic sets 1. Introduction The plausibility of life in the universe is a hotly debated topic. As of today, life is only known to exist on Earth. Thus, it may have been a singular event, an infrequent event, or a common event, albeit one that has thus far evaded our detection outside our own planet. Herein, we will not attempt to argue for any particular frequency of life. -
Basic Concepts of Chemical Bonding
Basic Concepts of Chemical Bonding Cover 8.1 to 8.7 EXCEPT 1. Omit Energetics of Ionic Bond Formation Omit Born-Haber Cycle 2. Omit Dipole Moments ELEMENTS & COMPOUNDS • Why do elements react to form compounds ? • What are the forces that hold atoms together in molecules ? and ions in ionic compounds ? Electron configuration predict reactivity Element Electron configurations Mg (12e) 1S 2 2S 2 2P 6 3S 2 Reactive Mg 2+ (10e) [Ne] Stable Cl(17e) 1S 2 2S 2 2P 6 3S 2 3P 5 Reactive Cl - (18e) [Ar] Stable CHEMICAL BONDSBONDS attractive force holding atoms together Single Bond : involves an electron pair e.g. H 2 Double Bond : involves two electron pairs e.g. O 2 Triple Bond : involves three electron pairs e.g. N 2 TYPES OF CHEMICAL BONDSBONDS Ionic Polar Covalent Two Extremes Covalent The Two Extremes IONIC BOND results from the transfer of electrons from a metal to a nonmetal. COVALENT BOND results from the sharing of electrons between the atoms. Usually found between nonmetals. The POLAR COVALENT bond is In-between • the IONIC BOND [ transfer of electrons ] and • the COVALENT BOND [ shared electrons] The pair of electrons in a polar covalent bond are not shared equally . DISCRIPTION OF ELECTRONS 1. How Many Electrons ? 2. Electron Configuration 3. Orbital Diagram 4. Quantum Numbers 5. LEWISLEWIS SYMBOLSSYMBOLS LEWISLEWIS SYMBOLSSYMBOLS 1. Electrons are represented as DOTS 2. Only VALENCE electrons are used Atomic Hydrogen is H • Atomic Lithium is Li • Atomic Sodium is Na • All of Group 1 has only one dot The Octet Rule Atoms gain, lose, or share electrons until they are surrounded by 8 valence electrons (s2 p6 ) All noble gases [EXCEPT HE] have s2 p6 configuration. -
Ocw-5.112-Lec24 the Following Content Is Provided by MIT Opencourseware Under a Creative Commons License
MITOCW | ocw-5.112-lec24 The following content is provided by MIT OpenCourseWare under a Creative Commons license. Additional information about our license and MIT OpenCourseWare in general is available at ocw.mit.edu. Today I would like to start by discussing a timeline. And you will see in a moment what this timeline has to do with. It is obviously only a partial timeline. But let's start here in 1916, as we have done this semester, by talking about the Lewis theory of electronic structure. And his electron pair theory is something we are going to come back to a couple of times during lecture today. Let's move on to 1954. 1954 was an important year in electronic structure theory, because in that year there was awarded, to Linus Pauling, the Nobel Prize in chemistry. Let me write down Pauling here. And if you are interested in knowing something about what Pauling was awarded the Nobel Prize in chemistry for, I will show you over here on the side boards. What you are going to see here, if you read this citation for Linus Carl Pauling in 1954 for the Nobel Prize in chemistry, his prize was awarded principally for his contributions to our understanding of the nature of the chemical bond. If you think back to the elegant title of the paper by Lewis that we started out our discussion of acid-base theory with, it was a paper entitled "The Atom and the Molecule." And now we have gotten to Pauling, in 1954, who is being awarded a Nobel Prize in chemistry for the nature of the chemical bond. -
Astrochemistry in Galaxies of the Local Universe Authors: David S
Astrochemistry in Galaxies of the Local Universe Authors: David S. Meier (New Mexico Tech), Jean Turner (UCLA), An- thony Remijan (NRAO), Juergen Ott (NRAO) and Alwyn Wootten (NRAO) Contact Author: David S. Meier New Mexico Institute of Mining and Technology Phone: 575-835-5340 Fax: 575-835-5707 E-mail: [email protected] Science Frontier Area: Galactic Neighborhood Abstract To understand star formation in galaxies we must know the molecular fuel out of which the stars form. Telescopes coming online in the upcoming decade will enable us to understand the molecular ISM from a new and powerful global perspective. In this white paper we focus on the use of astrochemistry—the observation, analysis and theoretical modeling of many molecular lines and their correlations—to answer some of the outstanding questions regarding the evolution of star formation and galactic structure in nearby galaxies. The 2 mm spectral line survey of the nearby starburst spiral, NGC 253 (Martin et al. 2006), overlaid on the 2 MASS near infrared JHK color image. The spectrum shows the richness of the millimeter spectrum. 1 Introduction Galactic structure and its evolution across cosmic time is driven by the gaseous component of galaxies. Our knowledge of the gaseous universe beyond the Milky Way is sketchy at present. Least studied of all is molecular gas, the component most closely linked to star formation. How has the gaseous structure of galaxies changed through cosmic time? What is the nature of intergalactic gas and its interaction with galaxies? How do galaxies accrete gas to form disks, giant molecular clouds (GMCs), stars and star clusters? How are GMCs affected by their environment? What is the relative importance of secular evolution and impulsive dynamical interactions in the histories of different kinds of galaxies? In this white paper we focus on how to concretely address these questions through astrochemistry. -
10: Alkenes and Alkynes. Electrophilic and Concerted Addition Reactions
(2/94)(8,9/96)(12/03)(1,2/04) Neuman Chapter 10 10: Alkenes and Alkynes. Electrophilic and Concerted Addition Reactions Addition Reactions Electrophilic Addition of H-X or X2 to Alkenes Addition of H-X and X2 to Alkynes Alkenes to Alcohols by Electrophilic Addition Alkenes to Alcohols by Hydroboration Addition of H2 to Alkenes and Alkynes Preview (To be added) 10.1 Addition Reactions We learned about elimination reactions that form C=C and Cº C bonds in Chapter 9. In this chapter we learn about reactions in which reagents add to these multiple bonds. General Considerations (10.1A) We show a general equation for an addition reaction with an alkene in Figure 10.01. Figure 10.01 (see Figure folder for complete figure) A¾ B A B | | C=C ® C¾ C This equation is the reverse of the general equation for an elimination reaction that we showed at the beginning of Chapter 9. This general equation does not show a mechanism for the addition process. There are a number of different types of mechanisms for addition reactions, but we can group them into the four broad categories of (1) electrophilic addition, (2) nucleophilic addition, (3) free radical addition, and (4) concerted addition. Electrophilic and nucleophilic addition reactions involve intermediate ions so they are ionic addition reactions. In contrast, free radical additions, and 1 (2/94)(8,9/96)(12/03)(1,2/04) Neuman Chapter 10 concerted addition reactions, are non-ionic addition reactions because they do not involve the formation of intermediate ions. Ionic Addition Reactions (10.1B) We compare general features of nucleophilic and electrophilic addition reactions here. -
Guidelines for Terms Related to Chemical Speciation and Fractionation of Elements. Definitions, Structural Aspects, and Methodological Approaches
Pure Appl. Chem., Vol. 72, No. 8, pp. 1453–1470, 2000. © 2000 IUPAC INTERNATIONAL UNION FOR PURE AND APPLIED CHEMISTRY ANALYTICAL CHEMISTRY DIVISION COMMISSION ON MICROCHEMICAL TECHNIQUES AND TRACE ANALYSIS CHEMISTRY AND THE ENVIRONMENT DIVISION COMMISSION ON FUNDAMENTAL ENVIRONMENTAL CHEMISTRY CHEMISTRY AND HUMAN HEALTH DIVISION CLINICAL CHEMISTRY SECTION, COMMISSION ON TOXICOLOGY GUIDELINES FOR TERMS RELATED TO CHEMICAL SPECIATION AND FRACTIONATION OF ELEMENTS. DEFINITIONS, STRUCTURAL ASPECTS, AND METHODOLOGICAL APPROACHES (IUPAC Recommendations 2000) Prepared for publication by DOUGLAS M. TEMPLETON1, FREEK ARIESE2, RITA CORNELIS3*, LARS-GÖRAN DANIELSSON4, HERBERT MUNTAU5, HERMAN P. VAN LEEUWEN6, AND RYSZARD ŁOBIŃSKI7 1Department of Laboratory Medicine and Pathobiology, University of Toronto, Canada; 2Department of Analytical Chemistry and Applied Spectroscopy, Vrije Universiteit Amsterdam, the Netherlands; 3Laboratory for Analytical Chemistry, Faculty of Sciences, University of Gent, Belgium; 4Department of Analytical Chemistry, Royal Institute of Technology, Stockholm, Sweden; 5Environmental Institute, Joint Research Centre Ispra, (VA) Italy; 6Department of Physical Chemistry and Colloid Science, Wageningen Agricultural University, the Netherlands; 7CNRS UMR 5034, Hélioparc, Pau, France, and Department of Chemistry, Warsaw University of Technology, Warszawa, Poland *Corresponding author: Laboratory for Analytical Chemistry, RUG, Proeftuinstraat 86, B-9000 Gent, Belgium; E-mail: [email protected] Republication or reproduction of this report or its storage and/or dissemination by electronic means is permitted without the need for formal IUPAC permission on condition that an acknowledgment, with full reference to the source along with use of the copyright symbol ©, the name IUPAC, and the year of publication, are prominently visible. Publication of a translation into another language is subject to the additional condition of prior approval from the relevant IUPAC National Adhering Organization. -
Stoichiometry of Chemical Reactions 175
Chapter 4 Stoichiometry of Chemical Reactions 175 Chapter 4 Stoichiometry of Chemical Reactions Figure 4.1 Many modern rocket fuels are solid mixtures of substances combined in carefully measured amounts and ignited to yield a thrust-generating chemical reaction. (credit: modification of work by NASA) Chapter Outline 4.1 Writing and Balancing Chemical Equations 4.2 Classifying Chemical Reactions 4.3 Reaction Stoichiometry 4.4 Reaction Yields 4.5 Quantitative Chemical Analysis Introduction Solid-fuel rockets are a central feature in the world’s space exploration programs, including the new Space Launch System being developed by the National Aeronautics and Space Administration (NASA) to replace the retired Space Shuttle fleet (Figure 4.1). The engines of these rockets rely on carefully prepared solid mixtures of chemicals combined in precisely measured amounts. Igniting the mixture initiates a vigorous chemical reaction that rapidly generates large amounts of gaseous products. These gases are ejected from the rocket engine through its nozzle, providing the thrust needed to propel heavy payloads into space. Both the nature of this chemical reaction and the relationships between the amounts of the substances being consumed and produced by the reaction are critically important considerations that determine the success of the technology. This chapter will describe how to symbolize chemical reactions using chemical equations, how to classify some common chemical reactions by identifying patterns of reactivity, and how to determine the quantitative relations between the amounts of substances involved in chemical reactions—that is, the reaction stoichiometry. 176 Chapter 4 Stoichiometry of Chemical Reactions 4.1 Writing and Balancing Chemical Equations By the end of this section, you will be able to: • Derive chemical equations from narrative descriptions of chemical reactions. -
Organic and Biological Chemistry
CHAPTER 23 Organic and Biological Chemistry CONTENTS HO H 23.1 ▶ Organic Molecules and Their C Structures: Alkanes H H C 23.2 ▶ Families of Organic Compounds: HO O O C C Functional Groups 23.3 ▶ Naming Organic Compounds H CC 23.4 ▶ Carbohydrates:HO A Biological Example HO OH of Isomers H 23.5 ▶ Valence Bond TCheory and Orbital OverlapH Pictures H C 23.6 ▶ Lipids:HO A Biological EOxample ofO Cis–Trans IsomerismC C 23.7 ▶ Formal Charge and Resonance in Organic CompoundsH CC 23.8 ▶ Conjugated SystemsHO OH 23.9 ▶ Proteins: A Biological Example of Conjugation 23.10 ▶ Aromatic Compounds and Molecular Ascorbic acid, also known as vitamin C, is an essential nutrient in the human diet Orbital Theory because it is not synthesized in our body. We can eat citrus fruits or take pills that contain vitamin C to maintain health. 23.11 ▶ Nucleic Acids: A Biological Example of Aromaticity ? Which Is Better, Natural or Synthetic? The answer to this question can be found in the INQUIRY ▶▶▶ on page 1021. STUDY GUIDE M23_MCMU3170_07_SE_C23.indd 978 27/11/14 2:11 AM f the ultimate goal of chemistry is to understand the world around us on a molecular level, then a knowledge of biochemistry—the chemistry of living organisms—is a central part Iof that goal. Biochemistry, in turn, is a branch of organic chemistry, a term originally used to mean the study of compounds from living organisms while inorganic chemistry was used for the study of compounds from nonliving sources. Today, however, we know that there are no fundamental differences between organic and inorganic compounds; the same principles apply to both. -
1: Organic Molecules and Chemical Bonding
(4,5,9,11,12/98)(1,9,10/99) Neuman Chapter 1 1: Organic Molecules and Chemical Bonding Organic Molecules Chemical Bonds Organic Chemistry Bon voyage Preview Organic chemistry describes the structures, properties, preparation, and reactions of a vast array of molecules that we call organic compounds. There are many different types of organic compounds, but all have carbon as their principal constituent atom. These carbon atoms form a carbon skeleton or carbon backbone that has other bonded atoms such as H, N, O, S, and the halogens (F, Cl, Br, and I). We frequently hear the term "organic" in everyday language where it describes or refers to substances that are "natural". This is probably a result of the notion of early scientists that all organic compounds came from living systems and possessed a "vital force". However, chemists learned over 170 years ago that this is not the case. Organic compounds are major components of living systems, but chemists can make many of them in the laboratory from substances that have no direct connection with living systems. Chemically speaking, a pure sample of an organic compound such as Vitamin C prepared in a laboratory is chemically identical to a pure sample of Vitamin C isolated from a natural source such as an orange or other citrus fruit. Your journey through organic chemistry will be challenging because of the large amount of information that you will need to learn and understand. However, we will explore this subject in a systematic manner so that it is not a vast collection of isolated facts. -
Chemical Bonding and Molecular Structure
100 CHEMISTRY UNIT 4 CHEMICAL BONDING AND MOLECULAR STRUCTURE Scientists are constantly discovering new compounds, orderly arranging the facts about them, trying to explain with the existing knowledge, organising to modify the earlier views or After studying this Unit, you will be evolve theories for explaining the newly observed facts. able to • understand KÖssel-Lewis approach to chemical bonding; • explain the octet rule and its Matter is made up of one or different type of elements. limitations, draw Lewis Under normal conditions no other element exists as an structures of simple molecules; independent atom in nature, except noble gases. However, • explain the formation of different a group of atoms is found to exist together as one species types of bonds; having characteristic properties. Such a group of atoms is • describe the VSEPR theory and called a molecule. Obviously there must be some force predict the geometry of simple which holds these constituent atoms together in the molecules; molecules. The attractive force which holds various • explain the valence bond constituents (atoms, ions, etc.) together in different approach for the formation of chemical species is called a chemical bond. Since the covalent bonds; formation of chemical compounds takes place as a result • predict the directional properties of combination of atoms of various elements in different of covalent bonds; ways, it raises many questions. Why do atoms combine? Why are only certain combinations possible? Why do some • explain the different types of hybridisation involving s, p and atoms combine while certain others do not? Why do d orbitals and draw shapes of molecules possess definite shapes? To answer such simple covalent molecules; questions different theories and concepts have been put forward from time to time. -
The Mystery of Life's Origin
The Mystery of Life’s Origin The Continuing Controversy CHARLES B. THAXTON, WALTER L. BRADLEY, ROGER L. OLSEN, JAMES TOUR, STEPHEN MEYER, JONATHAN WELLS, GUILLERMO GONZALEZ, BRIAN MILLER, DAVID KLINGHOFFER Seattle Discovery Institute Press Description e origin of life from non-life remains one of the most enduring mysteries of modern science. e Mystery of Life’s Origin: e Continuing Controversy investigates how close scientists are to solving that mystery and explores what we are learning about the origin of life from current research in chemistry, physics, astrobiology, biochemistry, and more. e book includes an updated version of the classic text e Mystery of Life’s Origin by Charles axton, Walter Bradley, and Roger Olsen, and new chapters on the current state of the debate by chemist James Tour, physicist Brian Miller, astronomer Guillermo Gonzalez, biologist Jonathan Wells, and philosopher of science Stephen C. Meyer. Copyright Notice Copyright © 2020 by Discovery Institute, All Rights Reserved. Library Cataloging Data e Mystery of Life’s Origin: e Continuing Controversy by Charles B. axton, Walter L. Bradley, Roger L, Olsen, James Tour, Stephen Meyer, Jonathan Wells, Guillermo Gonzalez, Brian Miller, and David Klinghoffer 486 pages, 6 x 9 x 1.0 inches & 1.4 lb, 229 x 152 x 25 mm. & 0.65 kg Library of Congress Control Number: 9781936599745 ISBN-13: 978-1-936599-74-5 (paperback), 978-1-936599-75-2 (Kindle), 978-1-936599-76-9 (EPUB) BISAC: SCI013040 SCIENCE / Chemistry / Organic BISAC: SCI013030 SCIENCE / Chemistry / Inorganic BISAC: SCI007000 SCIENCE / Life Sciences / Biochemistry BISAC: SCI075000 SCIENCE / Philosophy & Social Aspects Publisher Information Discovery Institute Press, 208 Columbia Street, Seattle, WA 98104 Internet: http://www.discoveryinstitutepress.com/ Published in the United States of America on acid-free paper.