Fungal Biology in the Origin and Emergence of Life
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The Aromatic Universe.Pdf
The aromatic universe Alessandra Candian, Junfeng Zhen, and Alexander G. G. M. Tielens Citation: Physics Today 71, 11, 38 (2018); doi: 10.1063/PT.3.4068 View online: https://doi.org/10.1063/PT.3.4068 View Table of Contents: https://physicstoday.scitation.org/toc/pto/71/11 Published by the American Institute of Physics ARTICLES YOU MAY BE INTERESTED IN When condensed-matter physics became king Physics Today 72, 30 (2019); https://doi.org/10.1063/PT.3.4110 Quantum foundations still not cemented Physics Today 71, 51 (2018); https://doi.org/10.1063/PT.3.4070 Measuring cosmic distances with standard sirens Physics Today 71, 34 (2018); https://doi.org/10.1063/PT.3.4090 Astrophysical high-energy neutrinos Physics Today 71, 36 (2018); https://doi.org/10.1063/PT.3.4043 Humans control complex objects by guiding them toward stability Physics Today 71, 16 (2018); https://doi.org/10.1063/PT.3.4060 Has elegance betrayed physics? Physics Today 71, 57 (2018); https://doi.org/10.1063/PT.3.4022 aromaticThe UNIVERSE Alessandra Candian, Junfeng Zhen, and Alexander G. G. M. Tielens The rich molecular structures of polycyclic aromatic hydrocarbons— essentially planar flakes of fused benzene rings—and their fullerene cousins are revealed through their vibrational and electronic spectra. The Mountains of Creation in the Eagle Nebula. (Courtesy of NASA/JPL-Caltech/L. Allen, Harvard–Smithsonian CfA.) Alessandra Candian is a Veni Research Fellow and Xander Tielens is a professor of physics and chemistry of the interstellar medium, both at the Leiden Observatory at Leiden University in the Netherlands. -
Cometary Panspermia a Radical Theory of Life’S Cosmic Origin and Evolution …And Over 450 Articles, ~ 60 in Nature
35 books: Cosmic origins of life 1976-2020 Physical Sciences︱ Chandra Wickramasinghe Cometary panspermia A radical theory of life’s cosmic origin and evolution …And over 450 articles, ~ 60 in Nature he combined efforts of generations supporting panspermia continues to Prof Wickramasinghe argues that the seeds of all life (bacteria and viruses) Panspermia has been around may have arrived on Earth from space, and may indeed still be raining down some 100 years since the term of experts in multiple fields, accumulate (Wickramasinghe et al., 2018, to affect life on Earth today, a concept known as cometary panspermia. ‘primordial soup’, referring to Tincluding evolutionary biology, 2019; Steele et al., 2018). the primitive ocean of organic paleontology and geology, have painted material not-yet-assembled a fairly good, if far-from-complete, picture COMETARY PANSPERMIA – cultural conceptions of life dating back galactic wanderers are normal features have argued that these could not into living organisms, was first of how the first life on Earth progressed A SOLUTION? to the ideas of Aristotle, and that this of the cosmos. Comets are known to have been lofted from the Earth to a coined. The question of how from simple organisms to what we can The word ‘panspermia’ comes from the may be the source of some of the have significant water content as well height of 400km by any known process. life’s molecular building blocks see today. However, there is a crucial ancient Greek roots ‘sperma’ meaning more hostile resistance the idea of as organics, and their cores, kept warm Bacteria have also been found high in spontaneously assembled gap in mainstream understanding - seed, and ‘pan’, meaning all. -
General Disclaimer One Or More of the Following Statements May Affect This Document
General Disclaimer One or more of the Following Statements may affect this Document This document has been reproduced from the best copy furnished by the organizational source. It is being released in the interest of making available as much information as possible. This document may contain data, which exceeds the sheet parameters. It was furnished in this condition by the organizational source and is the best copy available. This document may contain tone-on-tone or color graphs, charts and/or pictures, which have been reproduced in black and white. This document is paginated as submitted by the original source. Portions of this document are not fully legible due to the historical nature of some of the material. However, it is the best reproduction available from the original submission. Produced by the NASA Center for Aerospace Information (CASI) 4. ti 4bASA-C6- 17 11j4s) itLSIULUT bESkAhLA ASSUCIA'k5b,LLS. ILSILLC'ICEAL A ► L SEbICb bbskAi /b AL LS: CEPLEIU161711S EAFt LLStARCH Al 'IH %^l kULPLLSILb LAL'CEA1rkV AuaUdi 441p i i tit kru}ulsio p Lal.) 61 F NE5-1E945 IU/%SA UuC I a s National A G31 ^ 9 01 C 94 etut outics and Space Admit -iistration 0 ./ r ^` l `i^ Resident Research Associateships Postdoctoral and Senior Research Awards 1984 OPPORTUNITIES FOR RESEARCH at tho JET PROPULSION LABORATORY California Institute of Technology Pasadena, California 91109 in association with the NATIONAL RESEARCH COUNCIL National Academy of Sciences National Academy of Engineering Institute of Medicine 2101 Constitution Avenue W3shington,D C 20418 ^WY T , a V- AW ^V O r^ 1 Foreword. -
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. -
The Diffuse Interstellar Bands
Proceedings of the International Astronomical Union IAU Symposium No. 297 IAU Symposium IAU Symposium 20–24 May 2013 This volume describes the current state of the art in research aimed at unraveling the carriers of the enigmatic diffuse interstellar bands 297 Noordwijkerhout, (DIBs). The DIBs are a set of hundreds of absorption bands that are The Netherlands seen from the near-ultraviolet to near-infrared wavelengths. Their interstellar origin is well established, but the precise chemical identity of the DIB carriers remains to date one of the greatest 20–24 May 2013 297 20–24 May 2013 The Diffuse unsolved mysteries in astronomical spectroscopy. These Noordwijkerhout, The Diffuse proceedings of IAU Symposium 297 include more than 70 Noordwijkerhout, contributions that cover a wide range of topics in observational The Netherlands Interstellar astronomy and astrophysics; laboratory astrophysics and The Netherlands Interstellar Bands spectroscopy; astrochemistry; and theoretical, experimental and computational chemistry. This interdisciplinary overview contains Bands all the required background material to make the volume an ideal starting point for researchers and graduate students to learn about the various aspects of DIBs and related topics. Proceedings of the International Astronomical Union Editor in Chief: Prof. Thierry Montmerle This series contains the proceedings of major scientifi c meetings held by the International Astronomical Union. Each volume contains a series of articles on a topic of current interest in astronomy, giving a timely overview of research in the fi eld. With contributions by leading scientists, these books are at a level The Diffuse suitable for research astronomers and graduate students. Interstellar Edited by Bands Cami Cox Jan Cami Nick L.J. -
First Life in Primordial-Planet Oceans: the Biological Big Bang Gibson/Wickramasinghe/Schild First Life in Primordial-Planet Oceans: the Biological Big Bang
Journal of Cosmology First life in primordial-planet oceans: the biological big bang Gibson/Wickramasinghe/Schild First life in primordial-planet oceans: the biological big bang Carl H. Gibson 1,2 1 University of California San Diego, La Jolla, CA 92093-0411, USA [email protected], http://sdcc3.ucsd.edu/~ir118 N. Chandra Wickramasinghe3,4 3Cardiff Centre for Astrobiology, 24 Llwynypia Road, Lisvane, Cardiff CF14 0SY [email protected] Rudolph E. Schild5,6 5 Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138, USA 6 [email protected] Abstract: A scenario is presented for the formation of first life in the universe based on hydro- gravitational-dynamics (HGD) cosmology. From HGD, the dark matter of galaxies is H-He gas dominated planets (primordial-fog-particle PFPs) in million solar mass clumps (protoglobularstar- cluster PGCs), which formed at the plasma to gas transition temperature 3000 K. Stars result from mergers of these hot-gas-planets. Over-accretion causes stars to explode as supernovae that scatter life-chemicals (C, N, O, P, S, Ca, Fe etc.) to other planets in PGC clumps and beyond. These chemicals were first collected gravitationally by merging PFPs to form H-saturated, high-pressure, dense oceans of critical-temperature 647 K water over iron-nickel cores at ~ 2 Myr. Stardust fertil- izes the formation of first life in a cosmic hot-ocean soup kitchen comprised of all planets and their moons in meteoric communication, > 10100 kg in total. Ocean freezing at 273 K slows this biologi- cal big bang at ~ 8 Myr. HGD cosmology confirms that the evolving seeds of life are scattered on intergalactic scales by Hoyle-Wickramasinghe cometary panspermia. -
Astrochemistry from Astronomy to Astrobiology
Astrochemistry from Astronomy to Astrobiology Astrochemistry from Astronomy to Astrobiology Andrew M. Shaw University of Exeter Copyright 2006 John Wiley & Sons Ltd, The Atrium, Southern Gate, Chichester, West Sussex PO19 8SQ, England Telephone (+44) 1243 779777 Email (for orders and customer service enquiries): [email protected] Visit our Home Page on www.wiley.com All Rights Reserved. No part of this publication may be reproduced, stored in a retrieval system or transmitted in any form or by any means, electronic, mechanical, photocopying, recording, scanning or otherwise, except under the terms of the Copyright, Designs and Patents Act 1988 or under the terms of a licence issued by the Copyright Licensing Agency Ltd, 90 Tottenham Court Road, London W1T 4LP, UK, without the permission in writing of the Publisher. Requests to the Publisher should be addressed to the Permissions Department, John Wiley & Sons Ltd, The Atrium, Southern Gate, Chichester, West Sussex PO19 8SQ, England, or emailed to [email protected], or faxed to (+44) 1243 770620. Designations used by companies to distinguish their products are often claimed as trademarks. All brand names and product names used in this book are trade names, service marks, trademarks or registered trademarks of their respective owners. The Publisher is not associated with any product or vendor mentioned in this book. This publication is designed to provide accurate and authoritative information in regard to the subject matter covered. It is sold on the understanding that the Publisher is not engaged in rendering professional services. If professional advice or other expert assistance is required, the services of a competent professional should be sought. -
A Study of the C3H2 Isomers and Isotopologues: first Interstellar Detection of HDCCC?
A&A 586, A110 (2016) Astronomy DOI: 10.1051/0004-6361/201527460 & c ESO 2016 Astrophysics A study of the C3H2 isomers and isotopologues: first interstellar detection of HDCCC? S. Spezzano1;3, H. Gupta2;??, S. Brünken3, C. A. Gottlieb4, P. Caselli1, K. M. Menten5, H. S. P. Müller3, L. Bizzocchi1, P. Schilke3, M. C. McCarthy4, and S. Schlemmer3 1 Max-Planck-Institut für extraterrestrische Physik, Giessenbachstr. 1, 85748 Garching, Germany e-mail: [email protected] 2 California Institute of Technology, 770 S. Wilson Ave., M/C 100-22, Pasadena, CA 91125, USA 3 I. Physikalisches Institut, Universität zu Köln, Zülpicher Str. 77, 50937 Köln, Germany 4 Harvard-Smithsonian Center for Astrophysics, and School of Engineering & Applied Sciences, Harvard University, Cambridge, MA 02138, USA 5 Max-Planck Institut für Radioastronomie, Auf dem Hügel 69, 53121 Bonn, Germany Received 28 September 2015 / Accepted 12 November 2015 ABSTRACT The partially deuterated linear isomer HDCCC of the ubiquitous cyclic carbene (c-C3H2) was observed in the starless cores TMC- 1C and L1544 at 96.9 GHz, and a confirming line was observed in TMC-1 at 19.38 GHz. To aid the identification in these narrow line sources, four centimetre-wave rotational transitions (two in the previously reported Ka = 0 ladder and two new ones in the Ka = 1 ladder) and 23 transitions in the millimetre band between 96 and 272 GHz were measured in high-resolution laboratory spectra. Ten spectroscopic constants in a standard asymmetric top Hamiltonian allow the main transitions of astronomical interest −1 in the Ka ≤ 3 rotational ladders to be calculated to within 0.1 km s in radial velocity up to 400 GHz. -
Abstract Book
Our Astro-Chemical History Past, Present, and Future Sept. 10-14 2018 Assen, The Netherlands Abstract Book Program Monday 12:30-14:00 Lunch 14:00-15:25 14:00 Welcome and logistics 14:10 Summary of activities/results from the Action (Laurent Wiesenfeld) 14:40 The Future of Astrochemistry - Farid Salama (NASA) 15:25-16:00 Coffee break 16:00-17:30 Formation of COMs: surface routes vs new gas-phase routes 16:00 Audrey Coutens (Bordeaux, FR) 16:30 Dimitrios Skouteris (Pisa, IT) 17:00 Alexey Potapov (University ofJena, DE) 17:30-18:30 Welcome reception/posters 19:00-20:00 Dinner Tuesday 9:00-10:30 Low temperature chemistry and kinetics and processes (gas & solid) 9:00 Sergiy Krasnokutskiy (Jena, DE) 9:30 Johannes Kästner (Stuttgart, DE) 10:00 Stanka Jerosimić (Belgrade, RS) 10:30-11:00 Coffee break 11:00-12:30 Isotopic fractionation pathways in space 11:00 Kenji Furuya (Tsukuba, JP) 11:30 Eva Wirström (Chalmers, SE) 12:00 Olli Sipilä (Helsinki, FI; MPE, DE) 12:30-14:00 Lunch 14:00-15:30 Nanoparticles: Condensation, reactivity and diffusion 14:00 Herma Cuppen (Nijmegen, NL) 14:30 David Gobrecht (Leuven, BE) 15:00 Antoni Macià Escatllar (Barcelona, ES) 15:30-16:30 Coffee break/poster session 16:30-18:00 16:30 Chemistry of Planetary Atmospheres - Christiane Helling (St Andrews, UK) 17:15 Comet chemistry - Kathrin Altwegg (Bern, CH) 19:00-20:00 Dinner Wednesday 9:00-11:00 Hydrocarbon chains and rings in space 9:00 Ricardo Urso (INAF, IT) 9:30 Maria Luisa Senent (CSIC, ES) 10:00 Thomas Pino (ISMO Paris, FR) 10:30 Sandra Wiersma (Amsterdam, NL) 11:00-11:30 -
Arxiv:1802.10216V1 [Physics.Chem-Ph] 28 Feb 2018 They Play an Important Role in Their Spectroscopic Characteriza- Not Been Systematically Investigated
Bound and continuum-embedded states of cyanopolyyne anions† Wojciech Skomorowski, Sahil Gulania, and Anna I. Krylova Cyanopolyyne anions were among the first anions discovered in the interstellar medium. The discovery have raised questions about routes of formation of these anions in space. Some of the proposed mechanisms assumed that anionic excited electronic states, either metastable or weakly bound, play a key role in the formation process. Verification of this hypothesis requires detailed knowledge of the electronic states of the anions. Here we investigate bound and continuum states of four cyanopolyyne anions, CN−,C3N−,C5N−, and C7N−, by means of ab initio calculations. We employ the equation-of-motion coupled-cluster method augmented with complex absorbing potential. We predict that already in CN−, the smallest anion in the family, there are several low-lying metastable states of both singlet and triplet spin symmetry. These states, identified as shape resonances, are located between 6.3–8.5 eV above the ground state of the anion (or 2.3–4.5 eV above the ground state of the parent radical) and have widths of a few tenths of eV up to 1 eV. We analyze the identified resonances in terms of leading molecular orbital contributions and Dyson orbitals. As the carbon chain length increases in the C2n+1N− series, these resonances gradually become stabilized and eventually turn into stable valence bound states. The trends in energies of the transitions leading to both resonance and bound excited states can be rationalized by means of the Hückel model. Apart from valence excited states, some of the cyanopolyynes can also support dipole bound states and dipole stabilized resonances, owing to a large dipole moment of the parent radicals in the lowest 2S+ state. -
Evidence to Clinch the Theory of Extraterrestrial Life
obiolog str y & f A O u o l t a r e n a Chandra Wickramasinghe, Astrobiol Outreach 2015, 3:2 r c u h o J Journal of Astrobiology & Outreach DOI: 10.4172/2332-2519.1000e107 ISSN: 2332-2519 EditorialResearch Article OpenOpen Access Access Evidence to Clinch the Theory of Extraterrestrial Life Chandra Wickramasinghe N1,2,3 1Buckingham Centre for Astrobiology (BCAB), Buckingham University, UK 2Institute for the Study of Panspermia and Astroeconomics, Gifu, Japan 3University of Peradeniya, Peradeniya, Sri Lanka New data may serve to bring about the long overdue paradigm probe) appears to have been finally vindicated, both by the discovery of shift from theories of Earth-centred life to life being a truly cosmic organic molecules on the surface, and more dramatically by the recent phenomenon. The theory that bacteria and viruses similar to those discovery of time-variable spikes in methane observed by the Curiosity on Earth exist in comets, other planets and generally throughout the galaxy was developed as a serious scientific discipline from the early 1980’s [1-4]. Throughout the past three decades this idea has often been Relectivity Spectrum the subject of criticism, denial or even ridicule. Even though many discoveries in astronomy, geology and biology continued to provide supportive evidence for the theory of cosmic life, the rival theory of Earth-centered biology has remained deeply rooted in scientific culture. However, several recent developments are beginning to strain the credibility of the standard point of view. The great abundance of highly complex organic molecules in interstellar clouds [5], the plentiful existence of habitable planets in the galaxy numbering over 100 billion and separated one from another just by a few light years [6], the extreme space-survival properties of bacteria and viruses -make it exceedingly difficult to avoid the conclusion that the entire galaxy is a single connected biosphere. -
Laboratory Experiments of Titan Tholins Formed by Photochemistry of Cyanopolyynes
BIO Web of Conferences 2, 01005 (2014) DOI: 10.1051/bioconf/20140201005 C Owned by the authors, published by EDP Sciences, 2014 Laboratory Experiments of Titan Tholins formed by Photochemistry of Cyanopolyynes I. Couturier-Tamburelli1, I. N. Piétri1 1Aix Marseille Université, Laboratoire PIIM, UMR 6633, 13397 Marseille cedex 20 France. Tholins are complex organic materials produced by irradiation of several carbon and nitrogen rich atmosphere. It has been proposed that Tholins could have played an important role in the origin of life on Earth [1]. We investigate the formation of polymer (Tholins) from the photolysis of dicyanoacetylene. As of today, nitriles molecules have been identified in Titan atmosphere. Among these nitriles, the cyanopolyynes (HCnN) are very important since they are the essential constituents in building block amino acids. It is known that a rich phochemistry takes place in the Titan aerosols, and contributes to the evolution of molecular diversity in this atmosphere. These compounds evolve through polymerization processes in aerosol particles, which grow by coagulation and rain down to the surface of Titan containing water ice. We present photochemical processes of larger cyanopolyyne formation from small precursor molecules submitted to long wavelength photons. Under UV irradiation cyanopolyynes are known to induce izomerization process (figure 1) [2] and formation of longer cyanopolyynes [3]. Figure 1: Izomerisation process of cyanopolyynes. We provide the photochemical processes of Titan Tholins formation (figure 2) from cyanopolyyne precursor molecules submitted to long wavelength photons. Such photons penetrate down into the stratosphere and troposphere (figure 3). The photoreactivity of the cyanopolyynes with other Titan molecules are also presented.