1 UNIT 1 THEORIES of ORIGIN of LIFE Contents 1.0 Objectives 1.1
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Intelligent Design, Abiogenesis, and Learning from History: Dennis R
Author Exchange Intelligent Design, Abiogenesis, and Learning from History: Dennis R. Venema A Reply to Meyer Dennis R. Venema Weizsäcker’s book The World View of Physics is still keeping me very busy. It has again brought home to me quite clearly how wrong it is to use God as a stop-gap for the incompleteness of our knowledge. If in fact the frontiers of knowledge are being pushed back (and that is bound to be the case), then God is being pushed back with them, and is therefore continually in retreat. We are to find God in what we know, not in what we don’t know; God wants us to realize his presence, not in unsolved problems but in those that are solved. Dietrich Bonhoeffer1 am thankful for this opportunity to nature, is the result of intelligence. More- reply to Stephen Meyer’s criticisms over, this assertion is proffered as the I 2 of my review of his book Signature logical basis for inferring design for the in the Cell (hereafter Signature). Meyer’s origin of biological information: if infor- critiques of my review fall into two gen- mation only ever arises from intelli- eral categories. First, he claims I mistook gence, then the mere presence of Signature for an argument against bio- information demonstrates design. A few logical evolution, rendering several of examples from Signature make the point my arguments superfluous. Secondly, easily: Meyer asserts that I have failed to refute … historical scientists can show that his thesis by not providing a “causally a presently acting cause must have adequate alternative explanation” for the been present in the past because the origin of life in that the few relevant cri- proposed candidate is the only known tiques I do provide are “deeply flawed.” cause of the effect in question. -
Bayesian Analysis of the Astrobiological Implications of Life's
Bayesian analysis of the astrobiological implications of life's early emergence on Earth David S. Spiegel ∗ y, Edwin L. Turner y z ∗Institute for Advanced Study, Princeton, NJ 08540,yDept. of Astrophysical Sciences, Princeton Univ., Princeton, NJ 08544, USA, and zInstitute for the Physics and Mathematics of the Universe, The Univ. of Tokyo, Kashiwa 227-8568, Japan Submitted to Proceedings of the National Academy of Sciences of the United States of America Life arose on Earth sometime in the first few hundred million years Any inferences about the probability of life arising (given after the young planet had cooled to the point that it could support the conditions present on the early Earth) must be informed water-based organisms on its surface. The early emergence of life by how long it took for the first living creatures to evolve. By on Earth has been taken as evidence that the probability of abiogen- definition, improbable events generally happen infrequently. esis is high, if starting from young-Earth-like conditions. We revisit It follows that the duration between events provides a metric this argument quantitatively in a Bayesian statistical framework. By (however imperfect) of the probability or rate of the events. constructing a simple model of the probability of abiogenesis, we calculate a Bayesian estimate of its posterior probability, given the The time-span between when Earth achieved pre-biotic condi- data that life emerged fairly early in Earth's history and that, billions tions suitable for abiogenesis plus generally habitable climatic of years later, curious creatures noted this fact and considered its conditions [5, 6, 7] and when life first arose, therefore, seems implications. -
Origins of Life in the Universe Zackary Johnson
11/4/2007 Origins of Life in the Universe Zackary Johnson OCN201 Fall 2007 [email protected] Zackary Johnson http://www.soest.hawaii.edu/oceanography/zij/education.html Uniiiversity of Hawaii Department of Oceanography Class Schedule Nov‐2Originsof Life and the Universe Nov‐5 Classification of Life Nov‐7 Primary Production Nov‐9Consumers Nov‐14 Evolution: Processes (Steward) Nov‐16 Evolution: Adaptation() (Steward) Nov‐19 Marine Microbiology Nov‐21 Benthic Communities Nov‐26 Whale Falls (Smith) Nov‐28 The Marine Food Web Nov‐30 Community Ecology Dec‐3 Fisheries Dec‐5Global Ecology Dec‐12 Final Major Concepts TIMETABLE Big Bang! • Life started early, but not at the beginning, of Earth’s Milky Way (and other galaxies formed) history • Abiogenesis is the leading hypothesis to explain the beginning of life on Earth • There are many competing theories as to how this happened • Some of the details have been worked out, but most Formation of Earth have not • Abiogenesis almost certainly occurred in the ocean 20‐15 15‐94.5Today Billions of Years Before Present 1 11/4/2007 Building Blocks TIMETABLE Big Bang! • Universe is mostly hydrogen (H) and helium (He); for Milky Way (and other galaxies formed) example –the sun is 70% H, 28% He and 2% all else! Abundance) e • Most elements of interest to biology (C, N, P, O, etc.) were (Relativ 10 produced via nuclear fusion Formation of Earth Log at very high temperature reactions in large stars after Big Bang 20‐13 13‐94.7Today Atomic Number Billions of Years Before Present ORIGIN OF LIFE ON EARTH Abiogenesis: 3 stages Divine Creation 1. -
Laboratory Astrophysics: from Observations to Interpretation
April 14th – 19th 2019 Jesus College Cambridge UK IAU Symposium 350 Laboratory Astrophysics: From Observations to Interpretation Poster design by: D. Benoit, A. Dawes, E. Sciamma-O’Brien & H. Fraser Scientific Organizing Committee: Local Organizing Committee: Farid Salama (Chair) ★ P. Barklem ★ H. Fraser ★ T. Henning H. Fraser (Chair) ★ D. Benoit ★ R Coster ★ A. Dawes ★ S. Gärtner ★ C. Joblin ★ S. Kwok ★ H. Linnartz ★ L. Mashonkina ★ T. Millar ★ D. Heard ★ S. Ioppolo ★ N. Mason ★ A. Meijer★ P. Rimmer ★ ★ O. Shalabiea★ G. Vidali ★ F. Wa n g ★ G. Del-Zanna E. Sciamma-O’Brien ★ F. Salama ★ C. Wa lsh ★ G. Del-Zanna For more information and to contact us: www.astrochemistry.org.uk/IAU_S350 [email protected] @iaus350labastro 2 Abstract Book Scheduley Sunday 14th April . Pg. 2 Monday 15th April . Pg. 3 Tuesday 16th April . Pg. 4 Wednesday 17th April . Pg. 5 Thursday 18th April . Pg. 6 Friday 19th April . Pg. 7 List of Posters . .Pg. 8 Abstracts of Talks . .Pg. 12 Abstracts of Posters . Pg. 83 yPlenary talks (40') are indicated with `P', review talks (30') with `R', and invited talks (15') with `I'. Schedule Sunday 14th April 14:00 - 17:00 REGISTRATION 18:00 - 19:00 WELCOME RECEPTION 19:30 DINNER BAR OPEN UNTIL 23:00 Back to Table of Contents 2 Monday 15th April 09:00 { 10:00 REGISTRATION 09:00 WELCOME by F. Salama (Chair of SOC) SESSION 1 CHAIR: F. Salama 09:15 E. van Dishoeck (P) Laboratory astrophysics: key to understanding the Universe From Diffuse Clouds to Protostars: Outstanding Questions about the Evolution of 10:00 A. -
Six Phases of Cosmic Chemistry
Six Phases of Cosmic Chemistry Lukasz Lamza The Pontifical University of John Paul II Department of Philosophy, Chair of Philosophy of Nature Kanonicza 9, Rm. 203 31-002 Kraków, Poland e-mail: [email protected] 1. Introduction The steady development of astrophysical and cosmological sciences has led to a growing appreciation of the continuity of cosmic history throughout which all known phenomena come to being. This also includes chemical phenomena and there are numerous theoretical attempts to rewrite chemistry as a “historical” science (Haken 1978; Earley 2004). It seems therefore vital to organize the immense volume of chemical data – from astrophysical nuclear chemistry to biochemistry of living cells – in a consistent and quantitative fashion, one that would help to appreciate the unfolding of chemical phenomena throughout cosmic time. Although numerous specialist reviews exist (e.g. Shaw 2006; Herbst 2001; Hazen et al. 2008) that illustrate the growing appreciation for cosmic chemical history, several issues still need to be solved. First of all, such works discuss only a given subset of cosmic chemistry (astrochemistry, chemistry of life etc.) using the usual tools and languages of these particular disciplines which does not facilitate drawing large-scale conclusions. Second, they discuss the history of chemical structures and not chemical processes – which implicitly leaves out half of the totality chemical phenomena as non-historical. While it may now seem obvious that certain chemical structures such as aromatic hydrocarbons or pyrazines have a certain cosmic “history”, it might cause more controversy to argue that chemical processes such as catalysis or polymerization also have their “histories”. -
Bayesian Analysis of the Astrobiological Implications of Lifets
Bayesian analysis of the astrobiological implications of life’s early emergence on Earth David S. Spiegela,b,1 and Edwin L. Turnerb,c aSchool of Natural Sciences, Institute for Advanced Study, Princeton, NJ 08540; bDepartment of Astrophysical Sciences, Princeton University, Princeton, NJ 08544; and cInstitute for the Physics and Mathematics of the Universe, University of Tokyo, Kashiwa 227-8568, Japan Edited by Neta A. Bahcall, Princeton University, Princeton, NJ, and approved October 26, 2011 (received for review July 19, 2011) Life arose on Earth sometime in the first few hundred million years tween when Earth achieved prebiotic conditions suitable for after the young planet had cooled to the point that it could support abiogenesis plus generally habitable climatic conditions (5–7) and water-based organisms on its surface. The early emergence of when life first arose, therefore, seems to serve as a basis for life on Earth has been taken as evidence that the probability of estimating λ. Revisiting and quantifying this analysis is the subject abiogenesis is high, if starting from young Earth-like conditions. of this paper. We revisit this argument quantitatively in a Bayesian statistical We note several previous quantitative attempts to address this framework. By constructing a simple model of the probability issue in the literature, of which one (8) found, as we do, that early of abiogenesis, we calculate a Bayesian estimate of its posterior abiogenesis is consistent with life being rare, and the other (9) probability, given the data that life emerged fairly early in Earth’s found that Earth’s early abiogenesis points strongly to life being history and that, billions of years later, curious creatures noted common on Earth-like planets (we compare our approach to the this fact and considered its implications. -
Answers to Common Misconceptions About Biological Evolution Leah M
University of Nebraska - Lincoln DigitalCommons@University of Nebraska - Lincoln Papers in Evolution Papers in the Biological Sciences 5-2017 Answers to common misconceptions about biological evolution Leah M. Abebe University of Nebraska-Lincoln Blake Bartels University of Nebraska-Lincoln Kaitlyn M. Caron University of Nebraska-Lincoln Adam M. Gleeson University of Nebraska-Lincoln Samuel N. Johnson University of Nebraska-Lincoln See next page for additional authors Follow this and additional works at: http://digitalcommons.unl.edu/bioscievolution Part of the Evolution Commons Abebe, Leah M.; Bartels, Blake; Caron, Kaitlyn M.; Gleeson, Adam M.; Johnson, Samuel N.; Kluza, Tyler J.; Knopik, Nicholas W.; Kramer, Kristen N.; Maza, Masiel S.; Stava, Kaitlyn A.; Sullivan, Kaitlyn; Trimble, Jordan T.; and Zink, Robert M. , editor, "Answers to common misconceptions about biological evolution" (2017). Papers in Evolution. 4. http://digitalcommons.unl.edu/bioscievolution/4 This Article is brought to you for free and open access by the Papers in the Biological Sciences at DigitalCommons@University of Nebraska - Lincoln. It has been accepted for inclusion in Papers in Evolution by an authorized administrator of DigitalCommons@University of Nebraska - Lincoln. Authors Leah M. Abebe; Blake Bartels; Kaitlyn M. Caron; Adam M. Gleeson; Samuel N. Johnson; Tyler J. Kluza; Nicholas W. Knopik; Kristen N. Kramer; Masiel S. Maza; Kaitlyn A. Stava; Kaitlyn Sullivan; Jordan T. Trimble; and Robert M. Zink , editor This article is available at DigitalCommons@University of Nebraska - Lincoln: http://digitalcommons.unl.edu/bioscievolution/4 Answers to common misconceptions about biological evolution Class of BIOS 472, University of Nebraska, Lincoln, Spring 2017 Students: Leah M. Abebe, Blake Bartels, Kaitlyn M. -
States of Origin: Influences on Research Into the Origins of Life
COPYRIGHT AND USE OF THIS THESIS This thesis must be used in accordance with the provisions of the Copyright Act 1968. Reproduction of material protected by copyright may be an infringement of copyright and copyright owners may be entitled to take legal action against persons who infringe their copyright. Section 51 (2) of the Copyright Act permits an authorized officer of a university library or archives to provide a copy (by communication or otherwise) of an unpublished thesis kept in the library or archives, to a person who satisfies the authorized officer that he or she requires the reproduction for the purposes of research or study. The Copyright Act grants the creator of a work a number of moral rights, specifically the right of attribution, the right against false attribution and the right of integrity. You may infringe the author’s moral rights if you: - fail to acknowledge the author of this thesis if you quote sections from the work - attribute this thesis to another author - subject this thesis to derogatory treatment which may prejudice the author’s reputation For further information contact the University’s Director of Copyright Services sydney.edu.au/copyright Influences on Research into the Origins of Life. Idan Ben-Barak Unit for the History and Philosophy of Science Faculty of Science The University of Sydney A thesis submitted to the University of Sydney as fulfilment of the requirements for the degree of Doctor of Philosophy 2014 Declaration I hereby declare that this submission is my own work and that, to the best of my knowledge and belief, it contains no material previously published or written by another person, nor material which to a substantial extent has been accepted for the award of any other degree or diploma of a University or other institute of higher learning. -
A Statistical Estimation of the Occurrence of Extraterrestrial Intelligence in the Milky Way Galaxy
galaxies Article A Statistical Estimation of the Occurrence of Extraterrestrial Intelligence in the Milky Way Galaxy Xiang Cai 1, Jonathan H. Jiang 2,*, Kristen A. Fahy 2 and Yuk L. Yung 3 1 Grade 12, Santiago High School, Corona, CA 92881, USA; [email protected] 2 Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA 91109, USA; [email protected] 3 Division of Geological and Planetary Sciences, California Institute of Technology, Pasadena, CA 91125, USA; [email protected] * Correspondence: [email protected] Abstract: In the field of astrobiology, the precise location, prevalence, and age of potential extrater- restrial intelligence (ETI) have not been explicitly explored. Here, we address these inquiries using an empirical galactic simulation model to analyze the spatial–temporal variations and the prevalence of potential ETI within the Galaxy. This model estimates the occurrence of ETI, providing guidance on where to look for intelligent life in the Search for ETI (SETI) with a set of criteria, including well-established astrophysical properties of the Milky Way. Further, typically overlooked factors such as the process of abiogenesis, different evolutionary timescales, and potential self-annihilation are incorporated to explore the growth propensity of ETI. We examine three major parameters: (1) the likelihood rate of abiogenesis (λA); (2) evolutionary timescales (Tevo); and (3) probability of self- annihilation of complex life (Pann). We found Pann to be the most influential parameter determining the quantity and age of galactic intelligent life. Our model simulation also identified a peak location for ETI at an annular region approximately 4 kpc from the galactic center around 8 billion years (Gyrs), with complex life decreasing temporally and spatially from the peak point, asserting a high Citation: Cai, X.; Jiang, J.H.; Fahy, likelihood of intelligent life in the galactic inner disk. -
Problems of Planetology, Cosmochemistry and Meteoritica
Problems of Planetology, Cosmochemistry and Meteoritica Problems of Planetology, Cosmochemistry and Meteoritica Alexeev V.A., Pavlova T.A., Kalinina G.K. sample. The submitted work presents the analysis Some features of the radiation history of results of the distribution of the cosmic-ray exposure ureilites ages and masses of ureilites in comparison with those for ordinary chondrites, as well as the analysis results Vernadsky Institute of Geochemistry and Analytical of Wilkening and Marti (1976) of the track studies of Chemistry RAS, Moscow ([email protected]) the Kanne ureilite. Abstract. The analysis of the distributions of the cosmic- ray exposure ages and masses of ureilites in comparison with those for ordinary chondrites, as well as the analysis of the track study results of the Kenna ureilite are presented. The characteristic features found in the distributions are most likely associated with the presence of a larger proportion of ureilites with the small cosmic-ray exposure ages among the ureilites with small sizes. This fact may be due to the faster delivery of small-sized meteoroids on the orbits crossing the Earth’s orbit, which in turn is associated with the more efficient transfer of the small bodies from the region of the asteroid belt in the resonances regions mainly in result of the action of "daily" component of the Yarkovsky effect. Keywords: ureilites, cosmic-ray exposure ages, particle tracks Introduction. Among the meteorites, the total number of which exceeded 70,000, the ureilites account are less than 0.8% - only 553 meteorites (https://www.lpi.usra.edu/meteor/metbull.php). The most of these meteorites (~55%) were found in the deserts of northwestern Africa. -
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. -
Alexander Ruf Dissertation
TECHNISCHE UNIVERSITÄT MÜNCHEN Previously unknown organomagnesium compounds in astrochemical context Alexander Ruf Dissertation TECHNISCHE UNIVERSITÄT MÜNCHEN Fakultät Wissenschaftszentrum Weihenstephan für Ernährung, Landnutzung und Umwelt Lehrstuhl für Analytische Lebensmittelchemie Previously unknown organomagnesium compounds in astrochemical context Alexander Ruf Vollständiger Abdruck der von der Fakultät Wissenschaftszentrum Weihenstephan für Ernährung, Landnutzung und Umwelt der Technischen Universität München zur Erlangung des akademischen Grades eines Doktors der Naturwissenschaften (Dr. rer. nat.) genehmigten Dissertation. Vorsitzender: Prof. Dr. Erwin Grill Prüfer der Dissertation: 1. apl. Prof. Dr. Philippe Schmitt-Kopplin 2. Prof. Dr. Michael Rychlik 3. Prof. Eric Quirico, PhD (Université Grenoble Alpes) Die Dissertation wurde am 06.12.2017 bei der Technischen Universität München ein- gereicht und durch die Fakultät Wissenschaftszentrum Weihenstephan für Ernährung, Landnutzung und Umwelt am 18.01.2018 angenommen. Do we feel less open-minded, the more open-minded we are? A tribute to sensitivity and resolution... Acknowledgments This work has been prepared at the Helmholtz Zentrum München in the research unit Analytical BioGeoChemistry of apl. Prof. Dr. Philippe Schmitt-Kopplin, in collaboration with the Chair of Analytical Food Chemistry at the Technical Uni- versity of Munich. In the course of these years, I have relied on the courtesy and support of many to which I am grateful. The success of this PhD thesis would not have been possible without help and support of many wonderful people. First of all, I would like to thank the whole research group Analytical BioGeo- Chemistry for a very friendly, informal, and emancipated working atmosphere that formed day-by-day an enjoyable period of residence - it has felt like freedom! Small issues like having stimulating lunch discussions or going out into a bar, friendly peo- ple could be found herein to setting up a balance to scientific work.