Does Interstellar Dust Form the Largest Primordial Soup in the Universe?
Total Page:16
File Type:pdf, Size:1020Kb
Load more
Recommended publications
-
Regarding Belief in Primordial Soup to Explain the Origin of Life
Regarding Belief in Primordial Soup to explain the Origin of Life Belief in a primordial soup where life might spontaneously evolve is as wrong as believing the earth is flat, or, as Hoyle and Wickramasinghe (1981) suggest, as wrong as believing that the pre-Copernican idea that the earth is the center of the universe. They state, “It will be no bad thing to abandon this position” (p. 138). The belief in primordial soup goes something like this: “Somehow a brew of appropriate chemicals managed to get together, the organic soup, and somehow the chemicals managed to shuffle themselves into an early primitive life-form. From then on, all appeared to be plain-sailing, natural selection operating on randomly generated mutations would do the rest” (p. 131). Today we know that life does not arise spontaneously. In the 1860s, Louis Pasteur demonstrated that “the concept of spontaneous generation” was incorrect using “carefully designed experiments” (p. 36). Yet many biologists still “believe that life started on Earth through spontaneous processes” (p. 37). “The recourse to an organic soup to cross this biggest hurdle is evidently a blatant recourse to the spontaneous generation theory which Pasteur claimed to have destroyed. Nevertheless, most scientists, even to this day, have been satisfied to accept it” (p. 37). What scientific tests did Louis Pasteur conduct about spontaneous generation of life? How did he set up his experiment? What were his steps? What was his result? _________________________________________________________________ _________________________________________________________________ -
Laboratory Studies for Planetary Sciences
Laboratory Studies for Planetary Sciences A Planetary Decadal Survey White Paper Prepared by the American Astronomical Society (AAS) Working Group on Laboratory Astrophysics (WGLA) http://www.aas.org/labastro Targeted Panels: Terrestrial Planets; Outer Solar System Satellites; Small Bodies Lead Author: Murthy S. Gudipati Ice Spectroscopy Lab, Science Division, Mail Stop 183-301, Jet Propulsion Laboratory, California Institute of Technology, 4800 Oak Grove Drive, Pasadena, CA 91109. [email protected], 818-354-2637 Co-Authors: Michael A'Hearn - University of Maryland [email protected], 301-405-6076 Nancy Brickhouse - Harvard-Smithsonian Center for Astrophysics [email protected], 617-495-7438 John Cowan - University of Oklahoma [email protected], 405-325-3961 Paul Drake - University of Michigan [email protected], 734-763-4072 Steven Federman - University of Toledo [email protected], 419-530-2652 Gary Ferland - University of Kentucky [email protected], 859-257-879 Adam Frank - University of Rochester [email protected], 585-275-1717 Wick Haxton - University of Washington [email protected], 206-685-2397 Eric Herbst - Ohio State University [email protected], 614-292-6951 Michael Mumma - NASA/GSFC [email protected], 301-286-6994 Farid Salama - NASA/Ames Research Center [email protected], 650-604-3384 Daniel Wolf Savin - Columbia University [email protected], 212-854-4124, Lucy Ziurys – University of Arizona [email protected], 520-621-6525 1 Brief Description: The WGLA of the AAS promotes collaboration and exchange of knowledge between astronomy and planetary sciences and the laboratory sciences (physics, chemistry, and biology). -
The Primordial Earth: Hadean and Archean Eons
5th International Symposium on Strong Electromagnetic Fields and Neutron Stars 10 –13 of May, 2017 -Varadero, Cuba HABITABILITY OF THE MILKY WAY REVISITED Rolando Cárdenas and Rosmery Nodarse-Zulueta e-mail: [email protected] Planetary Science Laboratory Universidad Central “Marta Abreu” de Las Villas, Santa Clara, Cuba Abstract • The discoveries of the last three decades on deep sea and deep crust of planet Earth show that life can thrive in many places where solar radiation does not reach, using chemosynthesis instead of photosynthesis for primary production. • Underground life is relatively well protected from hazardous ionizing cosmic radiation, so above mentioned discoveries reopen the habitability budget of the Milky Way, turning potentially habitable even planetary bodies without atmosphere. • Considering this, in this work the habitability potential of the Milky Way is reconsidered. Energy Sources for Primary Habitability: - Photosynthesis: Electromagnetic Waves, mostly in the range 400-700 nm. Dominant in planetary surface. - Chemosynthesis: Energy released by redox chemical reactions. Dominant in deep sea and crust. Circumstellar Habitable Zone https://en.wikipedia.org/wiki/Circumstellar_habitable_zone. Accessed on 2017.04.28 Liquid water at surface: biased towards surface (photosynthetic) life Chemosynthesis: More common than previously thought… - Any redox process giving at least 20 kJ/mol of free energy can support microbial metabolism. The following gives 794 kJ/mol: Pohlman, J.: The biogeochemistry of anchialine caves: -
Quantification of Peptide Bond Types in Human Proteome Indicates How
ics om & B te i ro o P in f f o o r l m Nahalka, J Proteomics Bioinform 2011, 4:8 a Journal of a n t r i c u s DOI: 10.4172/jpb.1000184 o J ISSN: 0974-276X Proteomics & Bioinformatics Research Article Article OpenOpen Access Access Quantification of Peptide Bond Types in Human Proteome Indicates How DNA Codons were Assembled at Prebiotic Conditions Jozef Nahalka1,2* 1Institute of Chemistry, Center for Glycomics, Slovak Academy of Sciences, Dúbravská cesta 9, SK-84538 Bratislava, Slovak Republic 2Institute of Chemistry, Center of excellence for white-green biotechnology, Slovak Academy of Sciences, Trieda Andreja Hlinku 2, SK-94976 Nitra, Slovak Republic Abstract [GADV]-protein world hypothesis [1] leaded me to quantification of decapeptides assembled from G, A, V, D in human proteome. The G, A, V, and D amino acids were related to the nucleotides Guanine (g), Cystosine (c), Uracil (u), and Adenine (a). The search revealed agreement with the genetic code. The types of prebiotic peptide bonds represent probably the first selection power that established the base order in the codons. The genetic code underwent three phases of formation, which explain why modern codons have their particular order of nucleotides: the monobase, dibase and the modern phase (tribase). Sequence alignments and 3D structures of aminoacyl-tRNA synthetases confirm the depicted picture of “relatedness” and the picture indicates how “relatedness” is used by aminoacyl-tRNA synthetases for navigation into and within of the C-terminal anticodon-binding domain. The findings presented here illustrate the novel concept of possible translation of the amino acid sequence into a nucleotide sequence that can be in interactive or contrary mode regarding to desired protein-RNA interactions. -
SIDE GROUP ADDITION to the POLYCYCLIC AROMATIC HYDROCARBON CORONENE by PROTON IRRADIATION in COSMIC ICE ANALOGS Max P
The Astrophysical Journal, 582:L25–L29, 2003 January 1 ᭧ 2003. The American Astronomical Society. All rights reserved. Printed in U.S.A. SIDE GROUP ADDITION TO THE POLYCYCLIC AROMATIC HYDROCARBON CORONENE BY PROTON IRRADIATION IN COSMIC ICE ANALOGS Max P. Bernstein,1,2 Marla H. Moore,3 Jamie E. Elsila,4 Scott A. Sandford,2 Louis J. Allamandola,2 and Richard N. Zare4 Received 2002 July 23; accepted 2002 November 5; published 2002 December 6 ABSTRACT ∼ Ices at 15 K consisting of the polycyclic aromatic hydrocarbon coronene (C24H12) condensed either with H2O, CO2, or CO in the ratio of 1 : 100 or greater have been subjected to MeV proton bombardment from a Van de Graaff generator. The resulting reaction products have been examined by infrared transmission- reflection-transmission spectroscopy and by microprobe laser-desorption laser-ionization mass spectrometry. Just as in the case of UV photolysis, oxygen atoms are added to coronene, yielding, in the case of H2O ices, the addition of one or more alcohol (i OH) and ketone (1CuO) side chains to the coronene scaffolding. There are, however, significant differences between the products formed by proton irradiation and the products formed by UV photolysis of coronene containing CO and CO2 ices. The formation of a coronene carboxylic i acid ( COOH) by proton irradiation is facile in solid CO but not in CO2, the reverse of what was previously observed for UV photolysis under otherwise identical conditions. This work presents evidence that cosmic- ray irradiation of interstellar or cometary ices should have contributed to the formation of aromatics bearing ketone and carboxylic acid functional groups in primitive meteorites and interplanetary dust particles. -
Computational Surface Modelling of Ices and Minerals of Interstellar Interest—Insights and Perspectives
minerals Review Computational Surface Modelling of Ices and Minerals of Interstellar Interest—Insights and Perspectives Albert Rimola 1,* , Stefano Ferrero 1, Aurèle Germain 2 , Marta Corno 2 and Piero Ugliengo 2,3 1 Departament de Química, Universitat Autònoma de Barcelona, 08193 Bellaterra, Catalonia, Spain; [email protected] 2 Dipartimento di Chimica, Università degli Studi di Torino, 10125 Torino, Italy; [email protected] (A.G.); [email protected] (M.C.); [email protected] (P.U.) 3 Nanostructured Interfaces and Surfaces (NIS) Centre, Università degli Studi di Torino, 10125 Torino, Italy * Correspondence: [email protected]; Tel.: +34-93-581-3723 Abstract: The universe is molecularly rich, comprising from the simplest molecule (H2) to complex organic molecules (e.g., CH3CHO and NH2CHO), some of which of biological relevance (e.g., amino acids). This chemical richness is intimately linked to the different physical phases forming Solar-like planetary systems, in which at each phase, molecules of increasing complexity form. Interestingly, synthesis of some of these compounds only takes place in the presence of interstellar (IS) grains, i.e., solid-state sub-micron sized particles consisting of naked dust of silicates or carbonaceous materials that can be covered by water-dominated ice mantles. Surfaces of IS grains exhibit particular characteristics that allow the occurrence of pivotal chemical reactions, such as the presence of binding/catalytic sites and the capability to dissipate energy excesses through the grain phonons. The present know-how on the physicochemical features of IS grains has been obtained by the fruitful synergy of astronomical observational with astrochemical modelling and laboratory experiments. -
Interstellar Dust Within the Life Cycle of the Interstellar Medium K
EPJ Web of Conferences 18, 03001 (2011) DOI: 10.1051/epjconf/20111803001 C Owned by the authors, published by EDP Sciences, 2011 Interstellar dust within the life cycle of the interstellar medium K. Demyk1,2,a 1Université de Toulouse, UPS-OMP, IRAP, Toulouse, France 2CNRS, IRAP, 9 Av. colonel Roche, BP. 44346, 31028 Toulouse Cedex 4, France Abstract. Cosmic dust is omnipresent in the Universe. Its presence influences the evolution of the astronomical objects which in turn modify its physical and chemical properties. The nature of cosmic dust, its intimate coupling with its environment, constitute a rich field of research based on observations, modelling and experimental work. This review presents the observations of the different components of interstellar dust and discusses their evolution during the life cycle of the interstellar medium. 1. INTRODUCTION Interstellar dust grains are found everywhere in the Universe: in the Solar System, around stars at all evolutionary stages, in interstellar clouds of all kind, in galaxies and in the intergalactic medium. Cosmic dust is intimately mixed with the gas-phase and represents about 1% of the gas (in mass) in our Galaxy. The interstellar extinction and the emission of diffuse interstellar clouds is reproduced by three dust components: a population of large grains, the BGs (Big Grains, ∼10–500 nm) made of silicate and a refractory mantle, a population of carbonaceous nanograins, the VSGs (Very Small Grains, 1–10 nm) and a population of macro-molecules the PAHs (Polycyclic Aromatic Hydrocarbons) [1]. These three components are more or less abundant in the diverse astrophysical environments reflecting the coupling of dust with the environment and its evolution according to the physical and dynamical conditions. -
Cosmic-Ray Soil Water Monitoring: the Development, Status & Potential of the COSMOS- India Network Ross Morrison, J
Cosmic-ray soil water monitoring: the development, status & potential of the COSMOS- India network Ross Morrison, J. G. Evans, S. S. Angadi, L. Ball, T. Chakraborty, H. Cooper, M. Fry, G. Geet, M. Goswami, N. Ganeshi, O. Hitt, S. Jain, M. Krishnan, R. Krishnan, A. Kumar, M. Mujumdar, M. Nema, G. Rees, M. Sekhar, O. Swain, R. Thayyen, S. Tripathi, D. Upadhyaya & A. Jenkins COSMOS-India: outline o Background & rationale o Basics of measurement principle o COSMOS-India network & sites o Selected results o Future work COSMOS-India: objectives o Collaborative development of soil moisture (SM) network in India using cosmic ray (COSMOS) sensors o Deliver high temporal frequency SM observations at the intermediate spatial scale in near real-time o Development of national COSMOS-India data system & near real time data portal o Integrate with Earth Observation datasets for validated SM maps of India o Empower many other applications… Acknowledgment: other COSMOS networks cosmos.hwr.arizona.edu cosmos.ceh.ac.uk Why measure soil moisture (SM)? o Controls exchanges of energy & mass between land surface & atmosphere o Hydrology: controls evapotranspiration, partitioning between runoff & infiltration, groundwater recharge o Meteorology: partitioning solar energy into sensible, latent & soil heat fluxes, surface-boundary layer interactions o Plant growth & soil biogeochemistry https://www2.ucar.edu/atmosnews/people/aiguo-dai https://nevada.usgs.gov/water/et/measured.htm Applications of soil moisture data SM observation techniques o Challenge: SM observations at spatial & temporal resolution relevant Measuringto applications soil (e.g.moisture gridded models, content field scale) o Point scale: high temporal resolution & low cost o Issues - spatial heterogeneity & sensor placement (e.g. -
Cosmic-Ray Studies with Experimental Apparatus at LHC
S S symmetry Article Cosmic-Ray Studies with Experimental Apparatus at LHC Emma González Hernández 1, Juan Carlos Arteaga 2, Arturo Fernández Tellez 1 and Mario Rodríguez-Cahuantzi 1,* 1 Facultad de Ciencias Físico Matemáticas, Benemérita Universidad Autónoma de Puebla, Av. San Claudio y 18 Sur, Edif. EMA3-231, Ciudad Universitaria, 72570 Puebla, Mexico; [email protected] (E.G.H.); [email protected] (A.F.T.) 2 Instituto de Física y Matemáticas, Universidad Michoacana, 58040 Morelia, Mexico; [email protected] * Correspondence: [email protected] Received: 11 September 2020; Accepted: 2 October 2020; Published: 15 October 2020 Abstract: The study of cosmic rays with underground accelerator experiments started with the LEP detectors at CERN. ALEPH, DELPHI and L3 studied some properties of atmospheric muons such as their multiplicity and momentum. In recent years, an extension and improvement of such studies has been carried out by ALICE and CMS experiments. Along with the LHC high luminosity program some experimental setups have been proposed to increase the potential discovery of LHC. An example is the MAssive Timing Hodoscope for Ultra-Stable neutraL pArticles detector (MATHUSLA) designed for searching of Ultra Stable Neutral Particles, predicted by extensions of the Standard Model such as supersymmetric models, which is planned to be a surface detector placed 100 meters above ATLAS or CMS experiments. Hence, MATHUSLA can be suitable as a cosmic ray detector. In this manuscript the main results regarding cosmic ray studies with LHC experimental underground apparatus are summarized. The potential of future MATHUSLA proposal is also discussed. Keywords: cosmic ray physics at CERN; atmospheric muons; trigger detectors; muon bundles 1. -
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. -
Origin of Life
Origin of life An explanation of what is needed for abiogenesis (or biopoiesis) Don Batten Introduction The origin of life is also known as abiogenesis or sometimes chemical evolution. Life is based on long information-rich molecules such as DNA and RNA that contain instructions for making proteins, upon which life depends. But the reading of the DNA/RNA to make proteins, and the replication of DNA or RNA to make new cells (reproduction, the mark of ‘life’) both depend on a large suite of proteins that are coded on the DNA/RNA. Both the DNA/RNA and the proteins need to be present at the same time for life to begin—a serious chicken-and-egg conundrum. Thus, the origin of life is a vexing problem for those who insist that life arose through purely natural processes (physics and chemistry alone). Some evolutionists claim that the origin of life is not a part of evolution. However, probably every evolutionary biology textbook has a section on the origin of life in the chapters on evolution. The University of California, Berkeley, has the origin of life included in their ‘Evolution 101’ course, in a section titled “From Soup to Cells—the Origin of Life”.1High-profile defenders of ‘all-things- evolutionary’, such as P.Z. Myers and Nick Matzke, agree that the origin of life is part of evolution, as does Richard Dawkins.2 A well-known evolutionist of the past, G.A. Kerkut, did make a distinction between the General Theory of Evolution (GTE), which included the origin of life, and the Special Theory of Evolution (STE) that only dealt with the diversification of life (the supposed topic of Darwin’s 1859 book).3 It is only recently that some defenders of evolution have tried to divorce the origin of life from consideration. -
Coulomb Explosion of Polycyclic Aromatic Hydrocarbons Induced by Heavy Cosmic Rays: Carbon Chains Production Rates
Coulomb explosion of polycyclic aromatic hydrocarbons induced by heavy cosmic rays: carbon chains production rates M Chabot1 ∗, K B´eroff2, E Dartois2, and T Pino2 1Institut de Physique Nucl´eaired'Orsay (IPNO), CNRS-IN2P3, Univ. Paris Sud, Universit´eParis-Saclay, F-91406 Orsay, France 2Institut des Sciences Mol´eculairesd'Orsay (ISMO), CNRS, Univ. Paris Sud, Universit´eParis-Saclay, F-91405 Orsay, France Synopsis The interstellar medium contains both polycyclic aromatic hydrocarbons and cosmic rays. The frontal impact of a single heavy cosmic ray strips out many electrons. The highly charged species then relax by multi-fragmentation, potentially feeding the interstellar medium with hydrocarbon chains. We model both ionization(s) and fragmentation processes and compute the fragments production rates of particular interest for astrophysical models. Low energy CRs consist of projectiles from ties of Q fold ionization's for an iron projectile proton to nickel with energy from 10 keV to GeV. at 5MeV/u on a C60 is shown in Fig.1 as an ex- Astrophysical PAHs are carbons structures with ample of such calculation. cycles containing from ten's to few hundred's of To calculate the charge state above which carbon atoms. We report on the coulomb explo- the PAH multi-fragments, we used a statistical sion of highly positively charged PAHs induced model in a microcanonical formalism based on by the interstellar low energy CRs leading to the the experimental work of S. Martin [3]. The in- formation of long carbon chains. ternal energy was compute with the IAE model. To retrieve the figure of fragmentation in the 250 multi fragmentation process of the multi-charged 1 species, we extend a statistical model construct 200 initially for small multi-charged carbon Cn(n=2 150 3 to 10)[2].