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A Stringent Upper Limit of 20 Pptv for Methane on Mars and Constraints on Its Dispersion Outside Gale Crater F
A&A 650, A140 (2021) Astronomy https://doi.org/10.1051/0004-6361/202140389 & © F. Montmessin et al. 2021 Astrophysics A stringent upper limit of 20 pptv for methane on Mars and constraints on its dispersion outside Gale crater F. Montmessin1 , O. I. Korablev2 , A. Trokhimovskiy2 , F. Lefèvre3 , A. A. Fedorova2 , L. Baggio1 , A. Irbah1 , G. Lacombe1, K. S. Olsen4 , A. S. Braude1 , D. A. Belyaev2 , J. Alday4 , F. Forget5 , F. Daerden6, J. Pla-Garcia7,8 , S. Rafkin8 , C. F. Wilson4, A. Patrakeev2, A. Shakun2, and J. L. Bertaux1 1 LATMOS/IPSL, UVSQ Université Paris-Saclay, Sorbonne Université, CNRS, Guyancourt, France e-mail: [email protected] 2 Space Research Institute (IKI) RAS, Moscow, Russia 3 LATMOS/IPSL, Sorbonne Université, UVSQ Université Paris-Saclay, CNRS, Paris, France 4 AOPP, Oxford University, Oxford, UK 5 Laboratoire de Météorologie Dynamique, Sorbonne Université, Paris, France 6 BIRA-IASB, Bruxelles, Belgium 7 Centro de Astrobiología (CSIC?INTA), Torrejón de Ardoz, Spain 8 Southwest Research Institute, Boulder, CO, USA Received 20 January 2021 / Accepted 23 April 2021 ABSTRACT Context. Reports on the detection of methane in the Martian atmosphere have motivated numerous studies aiming to confirm or explain its presence on a planet where it might imply a biogenic or more likely a geophysical origin. Aims. Our intent is to complement and improve on the previously reported detection attempts by the Atmospheric Chemistry Suite (ACS) on board the ExoMars Trace Gas Orbiter (TGO). This latter study reported the results of a campaign that was a few months in length, and was significantly hindered by a dusty period that impaired detection performances. -
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. -
Global Ionosphere-Thermosphere-Mesosphere (ITM) Mapping Across Temporal and Spatial Scales a White Paper for the NRC Decadal
Global Ionosphere-Thermosphere-Mesosphere (ITM) Mapping Across Temporal and Spatial Scales A White Paper for the NRC Decadal Survey of Solar and Space Physics Andrew Stephan, Scott Budzien, Ken Dymond, and Damien Chua NRL Space Science Division Overview In order to fulfill the pressing need for accurate near-Earth space weather forecasts, it is essential that future measurements include both temporal and spatial aspects of the evolution of the ionosphere and thermosphere. A combination of high altitude global images and low Earth orbit altitude profiles from simple, in-the-medium sensors is an optimal scenario for creating continuous, routine space weather maps for both scientific and operational interests. The method presented here adapts the vast knowledge gained using ultraviolet airglow into a suggestion for a next-generation, near-Earth space weather mapping network. Why the Ionosphere, Thermosphere, and Mesosphere? The ionosphere-thermosphere-mesosphere (ITM) region of the terrestrial atmosphere is a complex and dynamic environment influenced by solar radiation, energy transfer, winds, waves, tides, electric and magnetic fields, and plasma processes. Recent measurements showing how coupling to other regions also influences dynamics in the ITM [e.g. Immel et al., 2006; Luhr, et al, 2007; Hagan et al., 2007] has exposed the need for a full, three- dimensional characterization of this region. Yet the true level of complexity in the ITM system remains undiscovered primarily because the fundamental components of this region are undersampled on the temporal and spatial scales that are necessary to expose these details. The solar and space physics research community has been driven over the past decade toward answering scientific questions that have a high level of practical application and relevance. -
Why Can't Cosmology Be More Open?
ISSN: 2641-886X International Journal of Cosmology, Astronomy and Astrophysics Opinion Article Open Access Why can’t Cosmology be more open? Jayant Narlikar* Inter-University Centre for Astronomy and Astrophysics, Ganeshkhind, Post Bag 4, Pune-411007, India Article Info Keywords: Cosmology, Galaxy, Big Bang, Spectrum *Corresponding author: More than two millennia back, Pythagoreans believed that the Earth went round a Jayant Narlikar central fire, with the Sun lying well outside its orbit. When sceptics asked,” Why can’t we Emeritus Professor see the fire?”, theorists had to postulate that there was a ‘counter-Earth’ going around Inter-University Centre for Astronomy and Astrophysics the central fire in an inner orbit that blocked our view of the fire. The sceptics asked Ganeshkhind, Post Bag 4 again: why don’t we see this ‘counter-Earth’? The theorists replied that this happened Pune, India because Greece was facing away from it. In due course this explanation too was also Tel: +91-20-25604100 shot down by people sailing around and looking from other directions. Fax: +91-20-25604698 E-mail: [email protected] I have elaborated this ancient episode because it holds a moral for scientists. When you are on the wrong track, you may have to invoke additional assumptions, like the Received: November 5, 2018 counter-Earth, to prop up your original theory against an observed fact. If there is no Accepted: November 15, 2018 other independent support for these assumptions, the entire structure becomes suspect. Published: January 2, 2019 The scientific approach then requires a critical re-examination of the basic paradigm. -
Design of Low-Altitude Martian Orbits Using Frequency Analysis A
Design of Low-Altitude Martian Orbits using Frequency Analysis A. Noullez, K. Tsiganis To cite this version: A. Noullez, K. Tsiganis. Design of Low-Altitude Martian Orbits using Frequency Analysis. Advances in Space Research, Elsevier, 2021, 67, pp.477-495. 10.1016/j.asr.2020.10.032. hal-03007909 HAL Id: hal-03007909 https://hal.archives-ouvertes.fr/hal-03007909 Submitted on 16 Nov 2020 HAL is a multi-disciplinary open access L’archive ouverte pluridisciplinaire HAL, est archive for the deposit and dissemination of sci- destinée au dépôt et à la diffusion de documents entific research documents, whether they are pub- scientifiques de niveau recherche, publiés ou non, lished or not. The documents may come from émanant des établissements d’enseignement et de teaching and research institutions in France or recherche français ou étrangers, des laboratoires abroad, or from public or private research centers. publics ou privés. Design of Low-Altitude Martian Orbits using Frequency Analysis A. Noulleza,∗, K. Tsiganisb aUniversit´eC^oted'Azur, Observatoire de la C^oted'Azur, CNRS, Laboratoire Lagrange, bd. de l'Observatoire, C.S. 34229, 06304 Nice Cedex 4, France bSection of Astrophysics Astronomy & Mechanics, Department of Physics, Aristotle University of Thessaloniki, GR 541 24 Thessaloniki, Greece Abstract Nearly-circular Frozen Orbits (FOs) around axisymmetric bodies | or, quasi-circular Periodic Orbits (POs) around non-axisymmetric bodies | are of primary concern in the design of low-altitude survey missions. Here, we study very low-altitude orbits (down to 50 km) in a high-degree and order model of the Martian gravity field. We apply Prony's Frequency Analysis (FA) to characterize the time variation of their orbital elements by computing accurate quasi-periodic decompositions of the eccentricity and inclination vectors. -
Where Less May Be More: How the Rare Biosphere Pulls Ecosystems Strings
The ISME Journal (2017) 11, 853–862 OPEN © 2017 International Society for Microbial Ecology All rights reserved 1751-7362/17 www.nature.com/ismej MINI REVIEW Where less may be more: how the rare biosphere pulls ecosystems strings Alexandre Jousset1, Christina Bienhold2,3, Antonis Chatzinotas4,5, Laure Gallien6,7, Angélique Gobet8, Viola Kurm9, Kirsten Küsel10,5, Matthias C Rillig11,12, Damian W Rivett13, Joana F Salles14, Marcel GA van der Heijden15,16,17, Noha H Youssef18, Xiaowei Zhang19, Zhong Wei20 and WH Gera Hol9 1Utrecht University, Department of Biology, Institute of Environmental Biology, Ecology and Biodiversity Group, Utrecht, The Netherlands; 2Alfred Wegener Institute Helmholtz Centre for Polar and Marine Research, Bremerhaven, Germany; 3Max Planck Institute for Marine Microbiology, Bremen, Germany; 4Helmholtz Centre for Environmental Research – UFZ, Leipzig, Germany; 5German Centre for Integrative Biodiversity Research (iDiv), Halle-Jena-Leipzig, Leipzig, Germany; 6Swiss Federal Institute for Forest, Snow and Landscape Research WSL, Birmensdorf, Switzerland; 7Center for Invasion Biology, Department of Botany & Zoology, Stellenbosch University, Matieland, South Africa; 8Sorbonne Universités, UPMC Université Paris 06, CNRS, UMR 8227, Integrative Biology of Marine Models, Station Biologique de Roscoff, F-29688, Roscoff Cedex, France; 9Netherlands Institute of Ecology, Department of Terrestrial Ecology, Wageningen, The Netherlands; 10Friedrich Schiller University Jena, Institute of Ecology, Jena, Germany; 11Freie Universtät Berlin, -
Experimental and Statistical Analysis of Nutritional Requirements for the Growth of the Extremophile Deinococcus Geothermalis DSM 11300
Experimental and statistical analysis of nutritional requirements for the growth of the extremophile Deinococcus geothermalis DSM 11300 Julie Bornot, Cesar Arturo Aceves-Lara, Carole Molina-Jouve, Jean-Louis Uribelarrea, Nathalie Gorret To cite this version: Julie Bornot, Cesar Arturo Aceves-Lara, Carole Molina-Jouve, Jean-Louis Uribelarrea, Nathalie Gor- ret. Experimental and statistical analysis of nutritional requirements for the growth of the ex- tremophile Deinococcus geothermalis DSM 11300. Extremophiles, Springer Verlag, 2014, 18 (6), pp.1009-1021. 10.1007/s00792-014-0671-8. hal-01268947 HAL Id: hal-01268947 https://hal.archives-ouvertes.fr/hal-01268947 Submitted on 11 Mar 2019 HAL is a multi-disciplinary open access L’archive ouverte pluridisciplinaire HAL, est archive for the deposit and dissemination of sci- destinée au dépôt et à la diffusion de documents entific research documents, whether they are pub- scientifiques de niveau recherche, publiés ou non, lished or not. The documents may come from émanant des établissements d’enseignement et de teaching and research institutions in France or recherche français ou étrangers, des laboratoires abroad, or from public or private research centers. publics ou privés. OATAO is an open access repository that collects the work of Toulouse researchers and makes it freely available over the web where possible This is an author’s version published in: http://oatao.univ-toulouse.fr/22999 Official URL: https://doi.org/10.1007/s00792-014-0671-8 To cite this version: Bornot, Julie and Aceves-Lara, César-Arturo and Molina-Jouve, Carole and Uribelarrea, Jean-Louis and Gorret, Nathalie Experimental and statistical analysis of nutritional requirements for the growth of the extremophile Deinococcus geothermalis DSM 11300. -
Performance and Contributions of the Green Industry to Utah's Economy
Utah State University DigitalCommons@USU All Graduate Plan B and other Reports Graduate Studies 5-2021 Performance and Contributions of the Green Industry to Utah's Economy Lara Gale Utah State University Follow this and additional works at: https://digitalcommons.usu.edu/gradreports Part of the Regional Economics Commons Recommended Citation Gale, Lara, "Performance and Contributions of the Green Industry to Utah's Economy" (2021). All Graduate Plan B and other Reports. 1551. https://digitalcommons.usu.edu/gradreports/1551 This Report is brought to you for free and open access by the Graduate Studies at DigitalCommons@USU. It has been accepted for inclusion in All Graduate Plan B and other Reports by an authorized administrator of DigitalCommons@USU. For more information, please contact [email protected]. PERFORMANCE AND CONTRIBUTIONS OF THE GREEN INDUSTRY TO UTAH’S ECONOMY by Lara Gale A research paper submitted in the partial fulfillment of the requirements for the degree of MASTER OF SCIENCE in Applied Economics Approved: ____________________________ ______________________________ Man Keun Kim, Ph.D. Ruby Ward, Ph.D. Major Professor Committee Member ____________________________ Larry Rupp, Ph.D. Committee Member UTAH STATE UNIVERSITY Logan, Utah 2021 ii ABSTRACT PERFORMANCE AND CONTRIBUTIONS OF THE GREEN INDUSTRY TO UTAH’S ECONOMY by Lara Gale, MS in Applied Economics Utah State University, 2021 Major Professor: Dr. Man Keun Kim Department: Applied Economics Landscaping and nursery enterprises, commonly known as green industry enterprises, can be found everywhere in Utah, and are necessary to create both aesthetic appeal and human well-being in the built environment. In order to understand the impact that events such as economic shocks or policy changes may have on the green industry, the baseline performance and contribution of the industry must be specified for comparison following these shocks. -
The Mystery of Methane on Mars and Titan
The Mystery of Methane on Mars & Titan By Sushil K. Atreya MARS has long been thought of as a possible abode of life. The discovery of methane in its atmosphere has rekindled those visions. The visible face of Mars looks nearly static, apart from a few wispy clouds (white). But the methane hints at a beehive of biological or geochemical activity underground. Of all the planets in the solar system other than Earth, own way, revealing either that we are not alone in the universe Mars has arguably the greatest potential for life, either extinct or that both Mars and Titan harbor large underground bodies or extant. It resembles Earth in so many ways: its formation of water together with unexpected levels of geochemical activ- process, its early climate history, its reservoirs of water, its vol- ity. Understanding the origin and fate of methane on these bod- canoes and other geologic processes. Microorganisms would fit ies will provide crucial clues to the processes that shape the right in. Another planetary body, Saturn’s largest moon Titan, formation, evolution and habitability of terrestrial worlds in also routinely comes up in discussions of extraterrestrial biology. this solar system and possibly in others. In its primordial past, Titan possessed conditions conducive to Methane (CH4) is abundant on the giant planets—Jupiter, the formation of molecular precursors of life, and some scientists Saturn, Uranus and Neptune—where it was the product of chem- believe it may have been alive then and might even be alive now. ical processing of primordial solar nebula material. On Earth, To add intrigue to these possibilities, astronomers studying though, methane is special. -
The Puzzle of Lichen Symbiosis
Digital Comprehensive Summaries of Uppsala Dissertations from the Faculty of Science and Technology 1503 The puzzle of lichen symbiosis Pieces from Thamnolia IOANA ONUT, -BRÄNNSTRÖM ACTA UNIVERSITATIS UPSALIENSIS ISSN 1651-6214 ISBN 978-91-554-9887-0 UPPSALA urn:nbn:se:uu:diva-319639 2017 Dissertation presented at Uppsala University to be publicly examined in Lindhalsalen, EBC, Norbyvägen 14, Uppsala, Thursday, 1 June 2017 at 09:15 for the degree of Doctor of Philosophy. The examination will be conducted in English. Faculty examiner: Associate Professor Anne Pringle (University of Wisconsin-Madison, Department of Botany). Abstract Onuț-Brännström, I. 2017. The puzzle of lichen symbiosis. Pieces from Thamnolia. Digital Comprehensive Summaries of Uppsala Dissertations from the Faculty of Science and Technology 1503. 62 pp. Uppsala: Acta Universitatis Upsaliensis. ISBN 978-91-554-9887-0. Symbiosis brought important evolutionary novelties to life on Earth. Lichens, the symbiotic entities formed by fungi, photosynthetic organisms and bacteria, represent an example of a successful adaptation in surviving hostile environments. Yet many aspects of the lichen symbiosis remain unexplored. This thesis aims at bringing insights into lichen biology and the importance of symbiosis in adaptation. I am using as model system a successful colonizer of tundra and alpine environments, the worm lichens Thamnolia, which seem to only reproduce vegetatively through symbiotic propagules. When the genetic architecture of the mating locus of the symbiotic fungal partner was analyzed with genomic and transcriptomic data, a sexual self-incompatible life style was revealed. However, a screen of the mating types ratios across natural populations detected only one of the mating types, suggesting that Thamnolia has no potential for sexual reproduction because of lack of mating partners. -
A Future Mars Environment for Science and Exploration
Planetary Science Vision 2050 Workshop 2017 (LPI Contrib. No. 1989) 8250.pdf A FUTURE MARS ENVIRONMENT FOR SCIENCE AND EXPLORATION. J. L. Green1, J. Hol- lingsworth2, D. Brain3, V. Airapetian4, A. Glocer4, A. Pulkkinen4, C. Dong5 and R. Bamford6 (1NASA HQ, 2ARC, 3U of Colorado, 4GSFC, 5Princeton University, 6Rutherford Appleton Laboratory) Introduction: Today, Mars is an arid and cold world of existing simulation tools that reproduce the physics with a very thin atmosphere that has significant frozen of the processes that model today’s Martian climate. A and underground water resources. The thin atmosphere series of simulations can be used to assess how best to both prevents liquid water from residing permanently largely stop the solar wind stripping of the Martian on its surface and makes it difficult to land missions atmosphere and allow the atmosphere to come to a new since it is not thick enough to completely facilitate a equilibrium. soft landing. In its past, under the influence of a signif- Models hosted at the Coordinated Community icant greenhouse effect, Mars may have had a signifi- Modeling Center (CCMC) are used to simulate a mag- cant water ocean covering perhaps 30% of the northern netic shield, and an artificial magnetosphere, for Mars hemisphere. When Mars lost its protective magneto- by generating a magnetic dipole field at the Mars L1 sphere, three or more billion years ago, the solar wind Lagrange point within an average solar wind environ- was allowed to directly ravish its atmosphere.[1] The ment. The magnetic field will be increased until the lack of a magnetic field, its relatively small mass, and resulting magnetotail of the artificial magnetosphere its atmospheric photochemistry, all would have con- encompasses the entire planet as shown in Figure 1. -
First Results from the Solar Mesosphere Explorer
N_A_ru_RE_v_o_L_JOS_I _SEPTE__ MB_E_R_I_98_3 ---------- NEWSANDVIEWS------------------15 and changes in environmental variables demonstrating the complementarity of the getic particles - caused by a solar proton (such as food density) are well known. two approaches. 0 event4, for example. The largest event in Previously, comparative studies and op the current solar cycle occurred on 13 July timality theory have addressed rather dif 1982, and the notable decrease of ozone ferent kinds of ethological issue. The ap Paul H. Harvey is a lecturer in the School of concentration it caused was measured by plication of optimal foraging models to Biological Sciences, University of Sussex, SME. Proton events of this kind inject large data on interspecies differences in territory BrightonBN19RH, andGeorginaM. Mace is a research associate at London Zoo and at the numbers of high-energy protons into the size may throw light on the precise form of Department of Anthropology, University Col middle atmosphere, changing the concen cross-species relationships, as well as lege ofLondon, London WCIE 6BT. trations of ionized hydrogen, nitrogen and oxygen, and thus the ozone destruction rate and density. SME's near-infrared Atmospheric chemistry spectrometer observed ozone depletion reaching 70 per cent at 65° latitude, 78 km altitude, on the morning side and 10-20 per First results from the cent on the afternoon side. All the observations, including those of Solar Mesosphere Explorer the proton event, have been satisfactorily from Guy Brasseur compared with a particularly elaborate two-dimensional model which takes into THE first results from the Solar Meso foreseen by the Chapman theory in 1930, account most chemical reactions related to sphere Explorer (SME), a satellite designed and show that atmospheric temperature is the mesosphere and the fundamental specially to study atmospheric ozone, are the principal cause of changes in ozone dynamical mechanisms5•6 • now becoming available (Geophys.