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(2016), Volume 4, Issue 2, 77-90
ISSN 2320-5407 International Journal of Advanced Research (2016), Volume 4, Issue 2, 77-90 Journal homepage: http://www.journalijar.com INTERNATIONAL JOURNAL OF ADVANCED RESEARCH RESEARCH ARTICLE LICHENOMETRIC DATING CURVE AS APPLIED TO GLACIER RETREAT STUDIES IN THE HIMALAYAS. Gaurav K. Mishra, Santosh Joshi and Dalip K. Upreti. Lichenology Laboratory, CSIR-National Botanical Research Institute, Rana Pratap Marg, Lucknow- 226001. Manuscript Info Abstract Manuscript History: The study critically favours the importance of lichens in estimating palaeoclimatic events and its use in depicting the future discretion regarding Received: 14 December 2015 Final Accepted: 19 January 2016 glacier retreat. Besides the various lichenometric studies carried out in Indian Published Online: February 2016 Himalayan region, the world-wide classical work of different glaciologist and geologist on different applications of lichenometry is also well focused. Key words: The study also highlights the benefits, restrains, and drawbacks associated Lichens, lichenometry,glacier with the lichenometry. Being a globally accepted biological technique retreat,India. particular emphasis is given on the need of innovative approach in implementation of lichenometry in Indian Himalayan region. *Corresponding Author Gaurav K. Mishra. Copy Right, IJAR, 2016,. All rights reserved. Introduction:- Lichens are slow growing organisms and take several years to get established in nature. Lichens are a unique group of plants, comprising of two micro-organisms, fungus (mycobiont), an organism capable of producing food via photosynthesis and alga (photobiont). These photobionts are predominantly members of the chlorophyta (green algae) or cynophyta (blue-green algae or cynobacteria). The peculiar nature of lichens enables them to colonize variety of substrate like rock, boulders, bark, soil, leaf and man-made buildings. -
Can Parietin Transfer Energy Radiatively to Photosynthetic Pigments?
molecules Communication Can Parietin Transfer Energy Radiatively to Photosynthetic Pigments? Beatriz Fernández-Marín 1, Unai Artetxe 1, José María Becerril 1, Javier Martínez-Abaigar 2, Encarnación Núñez-Olivera 2 and José Ignacio García-Plazaola 1,* ID 1 Department Plant Biology and Ecology, University of the Basque Country (UPV/EHU), 48940 Leioa, Spain; [email protected] (B.F.-M.); [email protected] (U.A.); [email protected] (J.M.B.) 2 Faculty of Science and Technology, University of La Rioja (UR), 26006 Logroño (La Rioja), Spain; [email protected] (J.M.-A.); [email protected] (E.N.-O.) * Correspondence: [email protected]; Tel.: +34-94-6015319 Received: 22 June 2018; Accepted: 16 July 2018; Published: 17 July 2018 Abstract: The main role of lichen anthraquinones is in protection against biotic and abiotic stresses, such as UV radiation. These compounds are frequently deposited as crystals outside the fungal hyphae and most of them emit visible fluorescence when excited by UV. We wondered whether the conversion of UV into visible fluorescence might be photosynthetically used by the photobiont, thereby converting UV into useful energy. To address this question, thalli of Xanthoria parietina were used as a model system. In this species the anthraquinone parietin accumulates in the outer upper cortex, conferring the species its characteristic yellow-orange colouration. In ethanol, parietin absorbed strongly in the blue and UV-B and emitted fluorescence in the range 480–540 nm, which partially matches with the absorption spectra of photosynthetic pigments. In intact thalli, it was determined by confocal microscopy that fluorescence emission spectra shifted 90 nm towards longer wavelengths. -
Planetary Report Report
The PLANETARYPLANETARY REPORT REPORT Volume XXIX Number 1 January/February 2009 Beyond The Moon From The Editor he Internet has transformed the way science is On the Cover: Tdone—even in the realm of “rocket science”— The United States has the opportunity to unify and inspire the and now anyone can make a real contribution, as world’s spacefaring nations to create a future brightened by long as you have the will to give your best. new goals, such as the human exploration of Mars and near- In this issue, you’ll read about a group of amateurs Earth asteroids. Inset: American astronaut Peggy A. Whitson who are helping professional researchers explore and Russian cosmonaut Yuri I. Malenchenko try out training Mars online, encouraged by Mars Exploration versions of Russian Orlan spacesuits. Background: The High Rovers Project Scientist Steve Squyres and Plane- Resolution Camera on Mars Express took this snapshot of tary Society President Jim Bell (who is also head Candor Chasma, a valley in the northern part of Valles of the rovers’ Pancam team.) Marineris, on July 6, 2006. Images: Gagarin Cosmonaut Training This new Internet-enabled fun is not the first, Center. Background: ESA nor will it be the only, way people can participate in planetary exploration. The Planetary Society has been encouraging our members to contribute Background: their minds and energy to science since 1984, A dust storm blurs the sky above a volcanic caldera in this image when the Pallas Project helped to determine the taken by the Mars Color Imager on Mars Reconnaissance Orbiter shape of a main-belt asteroid. -
Human Exploration of the Moon and Cislunar Space (1) Author: Ms
Paper ID: 47143 69th International Astronautical Congress 2018 oral 21st IAA SYMPOSIUM ON HUMAN EXPLORATION OF THE SOLAR SYSTEM (A5) Human Exploration of the Moon and Cislunar Space (1) Author: Ms. Dorota Budzyn European Space Agency (ESA/EAC), Germany, [email protected] Mr. Herv´eStevenin European Space Agency - Astronaut Training Center, Germany, [email protected] Dr. Matthias Maurer ESA/EAC, Germany, [email protected] Ms. Loredana Bessone ESA, European Astronaut Centre (EAC), Germany, [email protected] Mr. Francesco Sauro Alma Mater Studiorum - University of Bologna, Italy, [email protected] PROTOTYPING OF LUNAR SURFACE GEOLOGICAL SAMPLING TOOLS FOR MOON SPACEWALK SIMULATIONS BY ESA Abstract Apollo Lunar missions returned to scientists on Earth the first collection of geological extra-terrestrial planetary samples, other than meteorites. Scientists around the world are still studying rocks and soil samples that were collected, by the Apollo 11 through 17 missions, using modern equipment, methods and technologies. The return of samples has allowed the field of planetary science to advance in ways unthinkable with the restrictions of in-situ analysis and remote observations. As for every other aspect of the Apollo programme, the design and manufacturing of the tools uti- lized by astronauts for sample collection had to meet rigorous planetary protection requirements, whilst respecting stringent environmental and operability constraints. Many of those tools went through various redesign efforts, based on feedback from the very skillful and resourceful astronauts using them. In future planetary exploration missions, geological and geo-microbiological sampling will be a key to further devel- opment of our understanding of the evolution of the solar system, and to develop successful technologies for in-situ resource utilization and 3D printing. -
Viability of the Lichen Xanthoria Elegans and Its Symbionts After 18 Months of Space Exposure and Simulated Mars Conditions on the ISS
International Journal of Astrobiology 14 (3): 411–425 (2015) doi:10.1017/S1473550414000214 © Cambridge University Press 2014 Viability of the lichen Xanthoria elegans and its symbionts after 18 months of space exposure and simulated Mars conditions on the ISS Annette Brandt1, Jean-Pierre de Vera2, Silvano Onofri3 and Sieglinde Ott1 1Institute of Botany, Heinrich-Heine-University, Universitätsstr. 1, 40225 Düsseldorf, Germany 2Institute of Planetary Research, German Aerospace Center (DLR), Rutherfordstr. 2, 12489 Berlin, Germany 3Department of Ecological and Biological Sciences (DEB), Tuscia University, Largo dell’Università, 01100 Viterbo, Italy e-mail: [email protected] Abstract: The lichen Xanthoria elegans has been exposed to space conditions and simulated Mars-analogue conditions in the lichen and fungi experiment (LIFE) on the International Space Station (ISS). After several simulations and short space exposure experiments such as BIOPAN, this was the first long-term exposure of eukaryotic organisms to the hostile space conditions of the low Earth orbit (LEO). The biological samples were integrated in the EXPOSE-E facility and exposed for 1.5 years outside the ISS to the combined impact of insolation, ultraviolet (UV)-irradiation, cosmic radiation, temperatures and vacuum conditions of LEO space. Additionally, a subset of X. elegans samples was exposed to simulated Martian environmental conditions by applying Mars-analogue atmosphere and suitable solar radiation filters. After their return to Earth the viability of the lichen samples was ascertained by viability analysis of LIVE/DEAD staining and confocal laser-scanning microscopy, but also by analyses of chlorophyll a fluorescence. According to the LIVE/DEAD staining results, the lichen photobiont showed an average viability rate of 71%, whereas the even more resistant lichen mycobiont showed a rate of 84%. -
Nanopore Sequencing in Space: One Small Step for a Minion, One Giant Leap for Spaceflight Research
Nanopore Sequencing in Space: One Small Step for a MinION, One Giant Leap for Spaceflight Research Sarah Wallace, Ph.D. NASA Johnson Space Center Biomedical Research and Environmental Sciences Division Microbiology Laboratory [email protected] 1 To Sequence Where No One Has Sequenced Before OUTLINE • Why sequence in space? • The Molecular Space Age • Biomolecule Sequencer • Sample Prep • NEEMO • Genes in Space-3 • BEST 2 Why Molecular Biology in Space? • Operational environmental monitoring FGB • Identification of contaminating microbes panel • Infectious disease diagnosis Clogged SRV-K • Reduce down mass (sample return for environmental monitoring, crew line health, etc.) • Research • Human • Animal • Microbes/Cell lines Changes in the • Plants genome? • Med Ops Changes in gene Control LSMMG expression? • Response to countermeasures • Radiation • Real-time analysis can influence medical intervention • Support astrobiology science investigations • Technology superiorly suited to in situ nucleic acid-based life detection • Functional testing for integration into robotics for extra-planetary exploration mission 3 Microbial Monitoring on the ISS EHS Water Kit – Environmental SSK - Surface Sampling Kit MAS – Microbial Air Sampler Health Systems Water Kit 2016: The Molecular Space Age 2 April 19: The first 2 molecular biology assay in 0 0 space is completed, as DNA 1 is amplified using the 1 6 miniPCR thermal cycler 6 Biomolecule Sequencer • The first device to assess the capability of DNA and RNA sequencing in the microgravity environment of space • Capable of DNA, RNA, and protein sequencing • First launched July 18, 2016 (SpaceX-9) MinION by Oxford Nanopore-based sequencers measure changes in current caused by DNA strands migrating through the pore. -
Retour Des Réponses Le 06/01/2020 À [email protected] PARTIE I
Episode 2 – Énoncé des énigmes le 04/11/2019 ; retour des réponses le 06/01/2020 à [email protected] PARTIE I – Questions à choix multiples – Trouver la bonne réponse pour chacune des questions ! Question 1. Comparons nos deux planètes telluriques voisines La Terre et Mars. Quelle est la réponse fausse parmi les suivantes ? o Le diamètre de la planète Mars est plus petit que celui de la Terre o Ces deux planètes rocheuses ont la même masse volumique o Ces deux planètes sont rocheuses et ont chacune au moins un satellite o L’atmosphère de Mars est 61 fois plus fine que celle de la Terre o la gravité de surface sur Mars est seulement 38 % de celle de la Terre Question 2. Il n'y a pas que sur la Terre qu'il y a des volcans. Le volcanisme de la planète Mars serait apparu il y a près de quatre milliards d'années. Il aurait connu son intensité maximale à entre 3,7 et 3,2 Ga, puis se serait progressivement affaibli. Il a produit de nombreux volcans tels que Olympus Mons, Pavonis Mons, Ascraeus Mons, Elysium Mons, Arsia Mons. Localisez chacun de ces volcans sur la carte ci dessous : o volcan 1 > o volcan 2 > o volcan 3 > o volcan 4 > o volcan 5 > Question 3. Classez ces volcans par altitude. Le plus haut en premier (A), le moins haut en dernier (E) o volcan A le plus haut > o volcan B > o volcan C > o volcan D > o volcan E le moins haut > Question 4. -
Molecular Phylogenetic Study at the Generic Boundary Between the Lichen-Forming Fungi Caloplaca and Xanthoria (Ascomycota, Teloschistaceae)
Mycol. Res. 107 (11): 1266–1276 (November 2003). f The British Mycological Society 1266 DOI: 10.1017/S0953756203008529 Printed in the United Kingdom. Molecular phylogenetic study at the generic boundary between the lichen-forming fungi Caloplaca and Xanthoria (Ascomycota, Teloschistaceae) Ulrik SØCHTING1 and Franc¸ ois LUTZONI2 1 Department of Mycology, Botanical Institute, University of Copenhagen, O. Farimagsgade 2D, DK-1353 Copenhagen K, Denmark. 2 Department of Biology, Duke University, Durham, NC 27708-0338, USA. E-mail : [email protected] Received 5 December 2001; accepted 5 August 2003. A molecular phylogenetic analysis of rDNA was performed for seven Caloplaca, seven Xanthoria, one Fulgensia and five outgroup species. Phylogenetic hypotheses are constructed based on nuclear small and large subunit rDNA, separately and in combination. Three strongly supported major monophyletic groups were revealed within the Teloschistaceae. One group represents the Xanthoria fallax-group. The second group includes three subgroups: (1) X. parietina and X. elegans; (2) basal placodioid Caloplaca species followed by speciations leading to X. polycarpa and X. candelaria; and (3) a mixture of placodioid and endolithic Caloplaca species. The third main monophyletic group represents a heterogeneous assemblage of Caloplaca and Fulgensia species with a drastically different metabolite content. We report here that the two genera Caloplaca and Xanthoria, as well as the subgenus Gasparrinia, are all polyphyletic. The taxonomic significance of thallus morphology in Teloschistaceae and the current delimitation of the genus Xanthoria is discussed in light of these results. INTRODUCTION Taxonomy of Teloschistaceae and its genera The Teloschistaceae is a well-delimited family of Hawksworth & Eriksson (1986) assigned the Teloschis- lichenized fungi. -
A Critique of Phanerozoic Climatic Models Involving Changes in The
Earth-Science Reviews 56Ž. 2001 1–159 www.elsevier.comrlocaterearscirev A critique of Phanerozoic climatic models involving changes in the CO2 content of the atmosphere A.J. Boucot a,), Jane Gray b,1 a Department of Zoology, Oregon State UniÕersity, CorÕallis, OR 97331, USA b Department of Biology, UniÕersity of Oregon, Eugene, OR 97403, USA Received 28 April 1998; accepted 19 April 2001 Abstract Critical consideration of varied Phanerozoic climatic models, and comparison of them against Phanerozoic global climatic gradients revealed by a compilation of Cambrian through Miocene climatically sensitive sedimentsŽ evaporites, coals, tillites, lateritic soils, bauxites, calcretes, etc.. suggests that the previously postulated climatic models do not satisfactorily account for the geological information. Nor do many climatic conclusions based on botanical data stand up very well when examined critically. Although this account does not deal directly with global biogeographic information, another powerful source of climatic information, we have tried to incorporate such data into our thinking wherever possible, particularly in the earlier Paleozoic. In view of the excellent correlation between CO2 present in Antarctic ice cores, going back some hundreds of thousands of years, and global climatic gradient, one wonders whether or not the commonly postulated Phanerozoic connection between atmospheric CO2 and global climatic gradient is more coincidence than cause and effect. Many models have been proposed that attempt to determine atmospheric composition and global temperature through geological time, particularly for the Phanerozoic or significant portions of it. Many models assume a positive correlation between atmospheric CO2 and surface temperature, thus viewing changes in atmospheric CO2 as playing the critical role in r regulating climate temperature, but none agree on the levels of atmospheric CO2 through time. -
First DJ in Space 15 August 2019
First DJ in space 15 August 2019 operational activities, Luca also explained the goal of his Beyond mission and demonstrated life on board the Station to the audience in Ibiza. All these activities were key to widening awareness of ESA to a young European audience and bringing the focus on space in an inspirational and accessible setting. Luca's set was followed by that of his mentor, German DJ Le Shuuk. Luca had taken time out of his busy pre-flight training schedule earlier this year to work with Le Shuuk and receive a briefing on how to mix tracks. Le Shuuk prepared a personal playlist for Luca to take with him to the Station, and provided specialist DJ software that was uploaded ESA astronaut Luca Parmitano made space (and music) to the astronaut's tablets in space. history on 13 August 2019 when he broadcast the first DJ music set from orbit, performing to an audience of over 3000 people as part of the BigCityBeats WORLD CLUB DOME Cruise Edition. The results of his work were beamed to the main stage on board the cruise ship Norwegian Pearl moored at the Spanish island of Ibiza. His set of around 12 minutes was played as part of the regular programme of DJs at the festival. This was the first time that a DJ set has been played from the International Space Station and, indeed, from space. Credit: World Club Dome/ESA ESA astronaut Luca Parmitano made space (and music) history on 13 August when he broadcast the first DJ music set from orbit, performing to an audience of over 3000 people as part of the DJ Luca, ship at Ibiza. -
Lichen Life in Antarctica a Review on Growth and Environmental Adaptations of Lichens in Antarctica
Lichen Life in Antarctica A review on growth and environmental adaptations of lichens in Antarctica Individual Project for ANTA 504 for GCAS 08/09 Lorna Little Contents Antarctic Vegetation ...............................................................................................................................3 The Basics of Lichen Life .........................................................................................................................4 Environmental Influences .......................................................................................................................7 Nutrients .............................................................................................................................................7 Water Relations and Temperature .....................................................................................................7 UV‐B Radiation and Climate Change Effects.......................................................................................8 Variations in Lichen Growth and Colonisation......................................................................................10 Growth rate.......................................................................................................................................10 Case Studies of Antarctic Lichens .....................................................................................................13 Colonisation ......................................................................................................................................15 -
18Th EANA Conference European Astrobiology Network Association
18th EANA Conference European Astrobiology Network Association Abstract book 24-28 September 2018 Freie Universität Berlin, Germany Sponsors: Detectability of biosignatures in martian sedimentary systems A. H. Stevens1, A. McDonald2, and C. S. Cockell1 (1) UK Centre for Astrobiology, University of Edinburgh, UK ([email protected]) (2) Bioimaging Facility, School of Engineering, University of Edinburgh, UK Presentation: Tuesday 12:45-13:00 Session: Traces of life, biosignatures, life detection Abstract: Some of the most promising potential sampling sites for astrobiology are the numerous sedimentary areas on Mars such as those explored by MSL. As sedimentary systems have a high relative likelihood to have been habitable in the past and are known on Earth to preserve biosignatures well, the remains of martian sedimentary systems are an attractive target for exploration, for example by sample return caching rovers [1]. To learn how best to look for evidence of life in these environments, we must carefully understand their context. While recent measurements have raised the upper limit for organic carbon measured in martian sediments [2], our exploration to date shows no evidence for a terrestrial-like biosphere on Mars. We used an analogue of a martian mudstone (Y-Mars[3]) to investigate how best to look for biosignatures in martian sedimentary environments. The mudstone was inoculated with a relevant microbial community and cultured over several months under martian conditions to select for the most Mars-relevant microbes. We sequenced the microbial community over a number of transfers to try and understand what types microbes might be expected to exist in these environments and assess whether they might leave behind any specific biosignatures.