Space Biology Virtual Workshop January 20–21, 2021 Program and Abstracts
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ANNUAL REPORT Academic Year 2019-2020
ANNUAL REPORT Academic Year 2019-2020 International Space University The International Space University, founded in 1987 in Massachusetts, US, and now headquartered in Stras- bourg, France, is the world’s premier international space education institution. It is supported by major space agencies and aerospace organizations from around the world. The graduate level programs offered by ISU are dedicated to promoting international, interdisciplinary and intercultural cooperation in space activities. ISU offers the Master of Science in Space Studies program at its Central Campus in Strasbourg. Since the summer of 1988, ISU conducts the two-month Space Studies Program at different host institutions in locations spanning the globe; more recently the Southern Hemisphere Space Studies Program; and the online Interactive Space Program. ISU programs are delivered by over 100 ISU faculty members in concert with invited industry and agency experts from institutions around the world. Since its founding, more than 5000 students from 110 countries graduated from ISU. Contact Info: 1 rue Jean-Dominique Cassini Parc d’Innovation 67400 Illkirch-Graffenstaden, France [email protected] Phone: +33-3-88-65-54-30 Fax: +33-3-88-65-54-47 Table of Contents INTRODUCTION Page 1 1. Summary and Key Figures Page 3 2. Master of Space Studies - MSS20 Page 4 3. Interactive Space Program - ISP20 in lieu of SSP20 Page 9 4. Southern Hemisphere Space Studies Program - SHSSP20 Page 12 5. Commercial Space Course - CSP20 Page 15 6. Short Courses Page 17 7. Research and Publications Page 19 8. Space start-up Incubator Page 23 9. Alumni Affairs Page 24 10. Faculty and Executive Appointments Page 27 11. -
Climate Change and Human Health: Risks and Responses
Climate change and human health RISKS AND RESPONSES Editors A.J. McMichael The Australian National University, Canberra, Australia D.H. Campbell-Lendrum London School of Hygiene and Tropical Medicine, London, United Kingdom C.F. Corvalán World Health Organization, Geneva, Switzerland K.L. Ebi World Health Organization Regional Office for Europe, European Centre for Environment and Health, Rome, Italy A.K. Githeko Kenya Medical Research Institute, Kisumu, Kenya J.D. Scheraga US Environmental Protection Agency, Washington, DC, USA A. Woodward University of Otago, Wellington, New Zealand WORLD HEALTH ORGANIZATION GENEVA 2003 WHO Library Cataloguing-in-Publication Data Climate change and human health : risks and responses / editors : A. J. McMichael . [et al.] 1.Climate 2.Greenhouse effect 3.Natural disasters 4.Disease transmission 5.Ultraviolet rays—adverse effects 6.Risk assessment I.McMichael, Anthony J. ISBN 92 4 156248 X (NLM classification: WA 30) ©World Health Organization 2003 All rights reserved. Publications of the World Health Organization can be obtained from Marketing and Dis- semination, World Health Organization, 20 Avenue Appia, 1211 Geneva 27, Switzerland (tel: +41 22 791 2476; fax: +41 22 791 4857; email: [email protected]). Requests for permission to reproduce or translate WHO publications—whether for sale or for noncommercial distribution—should be addressed to Publications, at the above address (fax: +41 22 791 4806; email: [email protected]). The designations employed and the presentation of the material in this publication do not imply the expression of any opinion whatsoever on the part of the World Health Organization concerning the legal status of any country, territory, city or area or of its authorities, or concerning the delimitation of its frontiers or boundaries. -
Orbital Debris Quarterly News 22-1
National Aeronautics and Space Administration Orbital Debris Quarterly News Volume 22, Issue 1 February 2018 Inside... Two Anomalous Events in GEO Summer 2017 was marred by two apparently platform. Spacecraft dry mass is estimated to be on Space Debris Sensor anomalous events in the geosynchronous orbit the order of 2000 kg. On-board stored energy sources Launches Aboard (GEO) belt. Both incidents have been observed by include fuel and pressurized components, as well as the commercial space situation awareness providers, but as battery subsystem. SpaceX-13 2 of 26 December 2017 no debris from either event have The Indonesian GEO communications spacecraft entered the public catalog. TELKOM-1 (1999-042A, SSN catalog number 25880) SEM Analysis The GEO communications spacecraft AMC-9 experienced an energetic event on or about 25 August Results of (International Designator 2003-024A, U.S. Strategic 2017, after over 18.1 years on-orbit—3 years past Returned ISS Command [USSTRATCOM] Space Surveillance its nominal operational lifetime. An examination of Network [SSN] catalog number 27820), formerly known the Two Line Element data indicates an observable PMA-2 Cover 4 as GE-12, experienced an energetic event estimated to change in spacecraft orbit between 26 and 29 August. have occurred at approximately 07:10 GMT on 17 June At the beginning of this time interval, approximately CubeSat Study 2017, after approximately 14 years on-orbit. Fig. 1 Project Review 6 depicts the orbital evolution of the spacecraft in 2017. continued on page 2 SES, the spacecraft owner- operator, described this AMC‐9 (SSN 27820, 2003‐024A) 360 36300 Space Debris Sensor event as a “serious anomaly.” Installation 8 Following this event, the 36200 spacecraft began a westward 300 Monthly Object Type drift in the GEO belt. -
Potential European Contributions to Europa Lander Mission
The Europa Initiative for ESA’s M5 mission Report to OPAG Michel Blanc, Geraint Jones, Olga Prieto-Ballesteros, Veerle Sterken, Javier Gomez-Elvira, David Mimoun, Adam Masters, Sascha Kempf, Luciano Iess, John Cooper, Zita Martins, Ralph Lorenz, Jérémie lasue, Nicolas André, Bruce Bills, Gael Choblet, Geoff Collins, Philippe Garnier, Kevin Hand, Paul Hartogh, Krishan Khurana, Andrea Longobardo, Katrin Stephan, Federico Tosi, Steve Vance, Tim van Hoolst, Roland Wagner, Frances Westall, Martin Wolverk, William Desprats, Ryan Russell, Georges Balmino, Julien Laurent-Varin and the Europa Initiative team August 11th, 2016 1 EI WORKING SCHEME Europa M5 for an ESA contribution to the Europa Lander mission Initiative Penetrator Contribution to Cubesat? Orbiter or… NASA lander A – GLOBAL GEOPHYSICSMagnetospheric interactions CHARACTERIZE EUROPA AS A COMPLEX DYNAMICAL SYSTEM B – ExosphereOF COUPLED LAYERS(neutrals, dust, plumes) FROM CORE TO PLASMA ENVELOPE THROUGH OCEAN AND CRYOSPHERE dimension RESPONDING TO E – Geophysics (internalJUPITER SYSTEM FORCING: TIDAL, MAGNETOSPHERICstructure, incl. Characterization of the ocean) themes ASTROBIOLOGY CONTRIBUTE TO NASA’s LANDER SCIENCE Science AND PROVIDE AN ADDITIONAL ELEMENT (AWL) As resources permit « Spacecraft » dimension EI contribution to EUROPA LanDer : SubmitteD LOI’s Joint Europa Mission (Blanc/Prieto-Ballesteros) • Baseline: Carrier-Orbiter + lander joint NASA/ESA mission: – P1a: Carrier-Orbiter provided by ESA, operated by NASA; – P1b: Alternative option: Carrier-Orbiter provided and operated by NASA; science platform (+ sub-systems?) provided by ESA – Science platform open to both ESA member states and NASA • Option 1: Augmented surface science: Astrobiology Wet Laboratory (AWL) provided by ESA + Member States to enhance landing site exploration. • Option 2: Augmented orbital science - cubesat released from carrier. -
Space Weathering of Itokawa Particles: Implications for Regolith Evolution
46th Lunar and Planetary Science Conference (2015) 2351.pdf SPACE WEATHERING OF ITOKAWA PARTICLES: IMPLICATIONS FOR REGOLITH EVOLUTION. Eve L. Berger1 and Lindsay P. Keller2, 1Geocontrol Systems – Jacobs JETS contract – NASA Johnson Space Center, Houston TX 77058, [email protected], 2NASA Johnson Space Center Introduction: Space weathering processes such as tion rate of 4.1 ±1.2 × 104 tracks/cm2/year at 1AU [6] solar wind irradiation and micrometeorite impacts are are: ~80,000 years for 0211, ~70,000 years for 0192, known to alter the the properties of regolith materials and ~24,000 years for 0125. exposed on airless bodies [1]. The rates of space Discussion: Cosmic-ray exposure: Measurements weathering processes however, are poorly constrained of cosmic-ray exposure (CRE) ages of Itokawa parti- for asteroid regoliths, with recent estimates ranging cles [6-8] reveal that these grains are relatively young, over many orders of magnitude [e.g., 2, 3]. The return of surface samples by JAXA’s Hayabusa mission to ≤1−1.5 Ma, when compared to the distribution of ex- asteroid 25143 Itokawa, and their laboratory analysis posure ages for LL chondrite meteorites (8−50Ma) [9]. provides “ground truth” to anchor the timescales for The CRE ages for Itokawa grains are consistent with a space weathering processes on airless bodies. Here, we stable regolith at meter-depths for ~106 years. use the effects of solar wind irradiation and the Solar flare particle tracks: Based on the solar flare accumulation of solar flare tracks recorded in Itokawa particle track production rate in olivine at 1AU [6], the grains to constrain the rates of space weathering and Itokawa grains recorded solar flare tracks over time- yield information about regolith dynamics on these scales of <105 years. -
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. -
Detection of a Bacterial Group Within the Phylum Chloroflexi And
Microbes Environ. Vol. 21, No. 3, 154–162, 2006 http://wwwsoc.nii.ac.jp/jsme2/ Detection of a Bacterial Group within the Phylum Chloroflexi and Reductive-Dehalogenase-Homologous Genes in Pentachlorobenzene- Dechlorinating Estuarine Sediment from the Arakawa River, Japan KYOSUKE SANTOH1, ATSUSHI KOUZUMA1, RYOKO ISHIZEKI2, KENICHI IWATA1, MINORU SHIMURA3, TOSHIO HAYAKAWA3, TOSHIHIRO HOAKI4, HIDEAKI NOJIRI1, TOSHIO OMORI2, HISAKAZU YAMANE1 and HIROSHI HABE1*† 1 Biotechnology Research Center, The University of Tokyo, 1–1–1 Yayoi, Bunkyo-ku, Tokyo 113–8657, Japan 2 Department of Industrial Chemistry, Faculty of Engineering, Shibaura Institute of Technology, Minato-ku, Tokyo 108–8548, Japan 3 Environmental Biotechnology Laboratory, Railway Technical Research Institute, 2–8–38 Hikari-cho, Kokubunji-shi, Tokyo 185–8540, Japan 4 Technology Research Center, Taisei Corporation, 344–1 Nase, Totsuka-ku, Yokohama 245–0051, Japan (Received April 21, 2006—Accepted June 12, 2006) We enriched a pentachlorobenzene (pentaCB)-dechlorinating microbial consortium from an estuarine-sedi- ment sample obtained from the mouth of the Arakawa River. The sediment was incubated together with a mix- ture of four electron donors and pentaCB, and after five months of incubation, the microbial community structure was analyzed. Both DGGE and clone library analyses showed that the most expansive phylogenetic group within the consortium was affiliated with the phylum Chloroflexi, which includes Dehalococcoides-like bacteria. PCR using a degenerate primer set targeting conserved regions in reductive-dehalogenase-homologous (rdh) genes from Dehalococcoides species revealed that DNA fragments (approximately 1.5–1.7 kb) of rdh genes were am- plified from genomic DNA of the consortium. The deduced amino acid sequences of the rdh genes shared sever- al characteristics of reductive dehalogenases. -
Molecular Biology for Computer Scientists
CHAPTER 1 Molecular Biology for Computer Scientists Lawrence Hunter “Computers are to biology what mathematics is to physics.” — Harold Morowitz One of the major challenges for computer scientists who wish to work in the domain of molecular biology is becoming conversant with the daunting intri- cacies of existing biological knowledge and its extensive technical vocabu- lary. Questions about the origin, function, and structure of living systems have been pursued by nearly all cultures throughout history, and the work of the last two generations has been particularly fruitful. The knowledge of liv- ing systems resulting from this research is far too detailed and complex for any one human to comprehend. An entire scientific career can be based in the study of a single biomolecule. Nevertheless, in the following pages, I attempt to provide enough background for a computer scientist to understand much of the biology discussed in this book. This chapter provides the briefest of overviews; I can only begin to convey the depth, variety, complexity and stunning beauty of the universe of living things. Much of what follows is not about molecular biology per se. In order to 2ARTIFICIAL INTELLIGENCE & MOLECULAR BIOLOGY explain what the molecules are doing, it is often necessary to use concepts involving, for example, cells, embryological development, or evolution. Bi- ology is frustratingly holistic. Events at one level can effect and be affected by events at very different levels of scale or time. Digesting a survey of the basic background material is a prerequisite for understanding the significance of the molecular biology that is described elsewhere in the book. -
ESA Strategy for Science at the Moon
ESA UNCLASSIFIED - Releasable to the Public ESA Strategy for Science at the Moon ESA UNCLASSIFIED - Releasable to the Public EXECUTIVE SUMMARY A new era of space exploration is beginning, with multiple international and private sector actors engaged and with the Moon as its cornerstone. This renaissance in lunar exploration will offer new opportunities for science across a multitude of disciplines from planetary geology to astronomy and astrobiology whilst preparing the knowledge humanity will need to explore further into the Solar System. Recent missions and new analyses of samples retrieved during Apollo have transformed our understanding of the Moon and the science that can be performed there. We now understand the scientific importance of further exploration of the Moon to understand the origins and evolution of Earth and the cosmic context of life’s emergence on Earth and our future in space. ESA’s priorities for scientific activities at the Moon in the next ten years are: • Analysis of new and diverse samples from the Moon. • Detection and characterisation of polar water ice and other lunar volatiles. • Deployment of geophysical instruments and the build up a global geophysical network. • Identification and characterisation of potential resources for future exploration. • Deployment long wavelength radio astronomy receivers on the lunar far side. • Characterisation of the dynamic dust, charge and plasma environment. • Characterisation of biological sensitivity to the lunar environment. ESA UNCLASSIFIED - Releasable to the Public -
Department of Pharmacology (GRAD) 1
Department of Pharmacology (GRAD) 1 faculty participate fully at all levels. The department has the highest DEPARTMENT OF level of NIH funding of all pharmacology departments and a great diversity of research areas is available to trainees. These areas PHARMACOLOGY (GRAD) include cell surface receptors, G proteins, protein kinases, and signal transduction mechanisms; neuropharmacology; nucleic acids, cancer, Contact Information and antimicrobial pharmacology; and experimental therapeutics. Cell and molecular approaches are particularly strong, but systems-level research Department of Pharmacology such as behavioral pharmacology and analysis of knock-in and knock-out Visit Program Website (http://www.med.unc.edu/pharm/) mice is also well-represented. Excellent physical facilities are available for all research areas. Henrik Dohlman, Chair Students completing the training program will have acquired basic The Department of Pharmacology offers a program of study that leads knowledge of pharmacology and related fields, in-depth knowledge in to the degree of doctor of philosophy in pharmacology. The curriculum is their dissertation research area, the ability to evaluate scientific literature, individualized in recognition of the diverse backgrounds and interests of mastery of a variety of laboratory procedures, skill in planning and students and the broad scope of the discipline of pharmacology. executing an important research project in pharmacology, and the ability The department offers a variety of research areas including to communicate results, analysis, and interpretation. These skills provide a sound basis for successful scientific careers in academia, government, 1. Receptors and signal transduction or industry. 2. Ion channels To apply to BBSP, students must use The Graduate School's online 3. -
Standard 2: CELL BIOLOGY – REVIEW of BASICS
Standard 2: CELL BIOLOGY – REVIEW OF BASICS CELL PART OR TYPE OF CELL WHERE FOUND WHAT DOES IT FUNCTION: MISCELLANEOUS ORGANELLE Prokaryotic cell Plant cell LOOK LIKE: Job it does in INFORMATION: things Eukaryotic cell Animal cell Describe or Draw the cell such as color, what it is Both Both made of, size, etc. plasma/cell See diagram Holds cell together Phospholipid bilayer with membrane both both Regulates what goes proteins in/out of cell Semipermeable cytoplasm both Clear thick jelly- Supports/protects both like material in cell cell organelles See diagram Control center nucleus eukaryotic both Contains DNA See diagram Where proteins are ribosome both both made See diagram Process proteins Golgi complex eukaryotic both that go to other /apparatus parts of cell Membrane-bound Digests materials lysosome eukaryotic animal sac of digestive within the cell enzymes Membrane-bound Stores water, food, One large one in plants vacuole eukaryotic both storage area waste and dissolved Many smaller ones in minerals animals endoplasmic Network of Transport materials Can be rough (with reticulum eukaryotic both membrane tubes throughout the cell ribosomes attached) or smooth (without ribosomes) See diagram Where cell respiration Called Powerhouse of cell mitochondria eukaryotic both occurs (releases Makes ATP from energy for cell to use) breaking down glucose See diagram Where photosynthesis Contains chlorophyll chloroplast eukaryotic plant takes place Converts light energy into chemical energy in glucose Some pro- and plant (also fungi Rigid structure -
Exploration of the Moon
Exploration of the Moon The physical exploration of the Moon began when Luna 2, a space probe launched by the Soviet Union, made an impact on the surface of the Moon on September 14, 1959. Prior to that the only available means of exploration had been observation from Earth. The invention of the optical telescope brought about the first leap in the quality of lunar observations. Galileo Galilei is generally credited as the first person to use a telescope for astronomical purposes; having made his own telescope in 1609, the mountains and craters on the lunar surface were among his first observations using it. NASA's Apollo program was the first, and to date only, mission to successfully land humans on the Moon, which it did six times. The first landing took place in 1969, when astronauts placed scientific instruments and returnedlunar samples to Earth. Apollo 12 Lunar Module Intrepid prepares to descend towards the surface of the Moon. NASA photo. Contents Early history Space race Recent exploration Plans Past and future lunar missions See also References External links Early history The ancient Greek philosopher Anaxagoras (d. 428 BC) reasoned that the Sun and Moon were both giant spherical rocks, and that the latter reflected the light of the former. His non-religious view of the heavens was one cause for his imprisonment and eventual exile.[1] In his little book On the Face in the Moon's Orb, Plutarch suggested that the Moon had deep recesses in which the light of the Sun did not reach and that the spots are nothing but the shadows of rivers or deep chasms.