NASA Is Looking for Life in the Sky at First, NASA Thinks That Life on The
Total Page:16
File Type:pdf, Size:1020Kb

Load more
Recommended publications
-
20 Years Building Astrobiology
ASTROBIOLOGY Volume 20, Number 9, 2020 Special Collection Articles Mary Ann Liebert, Inc. DOI: 10.1089/ast.2020.0804 Introduction—Centro de Astrobiologı´a: 20 Years Building Astrobiology Vı´ctor Parro,1 J. Miguel Mas-Hesse,1 Javier Gomez-Elvira,1,2 A´ lvaro Gime´nez,1 and Juan Pe´rez-Mercader3 The Origins example of life, and we do not know how it was generated. It would require a team of scientists with a truly scientific he Centro de AstroBiologı´a (CAB) was founded in and professional knowledge and understanding of the TNovember 1999 as a joint institute between the Spanish various components of the puzzle. National Research Council (CSIC) and the National Institute That team began to emerge in Madrid, with scientists for Aerospace Technologies (INTA). Located in Madrid working in galactic astrophysics, planetary science, evolu- (Spain), CAB became the first astrobiology organization outside tion of life and of viruses, origins-of-life chemistry, meta- the United States to be associated with the NASA Astrobiology bolic processes in biochemistry, evolution of planets, Institute (NAI)—formally becoming an associate member in bioinformatics, extremophiles, and physics, together with the year 2000. Astrobiology considers life as a natural conse- engineers to design and produce instrumentation. This group, quence of the evolution of the Universe, and CAB aims to study from a variety of universities and government research cen- the origin, evolution, distribution, and future of life in the ters, such as INTA (Instituto Nacional de Te´cnica Aero- Universe, from an integrative transdisciplinary approach. espacial) and CSIC (Consejo Superior de Investigaciones CAB’s foundation was the result of a profound interest Cientı´ficas), started informal discussions; and a passion for in applying the scientific method to life—in the sense of the subject of astrobiology began to burn. -
OPENING CEREMONY 9:00 A.M
81st Annual Meeting of The Meteoritical Society 2018 (LPI Contrib. No. 2067) sess201.pdf Monday, July 23, 2018 OPENING CEREMONY 9:00 a.m. Concert Hall of the Academy of Science Building 9:00 a.m. Opening Ceremony Marina Ivanova, Vernadsky Institute, Convener for 81st Annual Meeting of The Meteoritical Society Eric Galimov, Vernadsky Institute, Scientific Advisor Dmitry Badyukov, Vernadsky Institute, Head of the Meteoritics Laboratory AWARD CEREMONY 9:30 a.m. Concert Hall of the Academy of Science Building Chairs: Trevor Ireland Meenakshi Wadhwa 9:30 a.m. Leonard Medal Recipient: Alexander N. Krot Citation: Kevin D. McKeegan The Leonard Medal is given to individuals who have made outstanding original contributions to the science of meteoritics or closely allied fields. The Meteoritical Society recognizes Alexander “Sasha” Krot with its 2018 Leonard Medal in recognition of his fundamental contributions to understanding the role oxygen isotopes in early solar system processes and aqueous alteration processes on asteroids. 9:45 a.m. Barringer Medal Recipient: Thomas Kenkmann Citation: Kai Wünnemann The Barringer Medal is given for outstanding work in the field of impact crating. The 2018 Barringer Medal is awarded to Professor Thomas Kenkmann for his fundamental contributions to our understanding of the structure mechanics and tectonics of rock displacement associated with the formation of hypervelocity impact craters. 10:00 a.m. Nier Prize Recipient: Lydia Hallis Citation: Martin Lee The Nier Prize is given for significant research in the field of meteoritics and closely related fields by a young scientist under the age of 35. The Meteoritical Society recognizes Lydia Hallis with its 2018 Nier Prize for her contributions to the understanding of the origin of volatiles in planets. -
Curriculum Vitae
DANTE S. LAURETTA Lunar and Planetary Laboratory Department of Planetary Sciences University of Arizona Tucson, AZ 85721-0092 Cell: (520) 609-2088 Email: [email protected] CHRONOLOGY OF EDUCATION Washington University, St. Louis, MO Dept. of Earth and Planetary Sciences Ph.D. in Earth and Planetary Sciences, 1997 Thesis: Theoretical and Experimental Studies of Fe-Ni-S, Be, and B Cosmochemistry Advisor: Bruce Fegley, Jr. University of Arizona, Tucson, AZ Depts. of Physics, Mathematics, and East Asian Studies B.S. in Physics and Mathematics, Cum Laude, 1993 B.A. in Oriental Studies (emphasis: Japanese), Cum Laude, 1993 CHRONOLOGY OF EMPLOYMENT Professor, Lunar and Planetary Laboratory, Dept. of Planetary Sciences, University of Arizona, Tucson, AZ; 2012 – present. Principal Investigator, OSIRIS-REx Asteroid Sample Return Mission, NASA New Frontiers Program, 2011 – present. Deputy Principal Investigator, OSIRIS-REx Asteroid Sample Return Mission, NASA New Frontiers Program, 2008 – 2011. Associate Professor, Lunar and Planetary Laboratory, Dept. of Planetary Sciences, University of Arizona, Tucson, AZ; 2006 – 2012. Assistant Professor, Lunar and Planetary Laboratory, Dept. of Planetary Sciences, University of Arizona, Tucson, AZ; 2001 – 2006. Associate Research Scientist, Dept. of Chemistry & Biochemistry, Arizona State University, Tempe, AZ; 1999 – 2001. Postdoctoral Research Associate, Dept. of Geology, Arizona State University, Tempe, AZ Primary project: Transmission electron microscopy of meteoritic minerals. Supervisor: Peter R. Buseck; Dates: 1997 – 1999. Research Assistant, Dept. of Earth and Planetary Sciences, Washington Univ., St. Louis, MO Primary project: Experimental studies of sulfide formation in the solar nebula. Advisor: Bruce Fegley, Jr.; Dates: 1993 – 1997. Research Intern, NASA Undergraduate Research Program, University of Arizona, Tucson, AZ Primary project: Development of a logic-based language for S.E.T.I. -
Leshin Web CV Short Feb14
Laurie A. Leshin, Ph.D. Professional Experience WORCESTER POLYTECHNIC INSTITUTE, STARTING JULY, 2014 President RENSSELAER POLYTECHNIC INSTITUTE, 2011-PRESENT Dean, School of Science and Professor, Department of Earth & Environmental Sciences NATIONAL AERONAUTICS AND SPACE ADMINISTRATION, 2005-2011 Deputy Associate Administrator, Exploration Systems Mission Directorate, NASA HQ, 2010-2011 Deputy Center Director for Science & Technology, NASA Goddard Space Flight Center, 2008-2009 Director of Sciences and Exploration Directorate, NASA Goddard Space Flight Center, 2005-2007 ARIZONA STATE UNIVERSITY, 1998-2005 Interim Director, School of Earth and Space Exploration, Arizona State University, 2005 The Dee and John Whiteman Dean’s Distinguished Professor, Department of Geological Sciences, 2001 – 2005; Assistant Professor, 1998 – 2001 Director, Center for Meteorite Studies, 2003 – 2005; Associate Director, 2000 – 2002 UNIVERSITY OF CALIFORNIA, LOS ANGELES, 1994-1998 W. W. Rubey Faculty Fellow, Department of Earth and Space Sciences, 1996 – 1998 University of California President's Postdoctoral Fellow, Dept. of Earth and Space Sci., 1994 – 1996 Education Ph.D. 1994 California Institute of Technology, Pasadena, CA, Geochemistry M. S. 1989 California Institute of Technology, Pasadena, CA, Geochemistry B. S. 1987 Arizona State University, Tempe, AZ, Chemistry, summa cum laude Selected Professional and Community Service Advisory Board, National Air & Space Museum (appointed by President Obama), 2013-present Advisory Board, US Merchant Marine Academy -
Space Biology Research and Biosensor Technologies: Past, Present, and Future †
biosensors Perspective Space Biology Research and Biosensor Technologies: Past, Present, and Future † Ada Kanapskyte 1,2, Elizabeth M. Hawkins 1,3,4, Lauren C. Liddell 5,6, Shilpa R. Bhardwaj 5,7, Diana Gentry 5 and Sergio R. Santa Maria 5,8,* 1 Space Life Sciences Training Program, NASA Ames Research Center, Moffett Field, CA 94035, USA; [email protected] (A.K.); [email protected] (E.M.H.) 2 Biomedical Engineering Department, The Ohio State University, Columbus, OH 43210, USA 3 KBR Wyle, Moffett Field, CA 94035, USA 4 Mammoth Biosciences, Inc., South San Francisco, CA 94080, USA 5 NASA Ames Research Center, Moffett Field, CA 94035, USA; [email protected] (L.C.L.); [email protected] (S.R.B.); [email protected] (D.G.) 6 Logyx, LLC, Mountain View, CA 94043, USA 7 The Bionetics Corporation, Yorktown, VA 23693, USA 8 COSMIAC Research Institute, University of New Mexico, Albuquerque, NM 87131, USA * Correspondence: [email protected]; Tel.: +1-650-604-1411 † Presented at the 1st International Electronic Conference on Biosensors, 2–17 November 2020; Available online: https://iecb2020.sciforum.net/. Abstract: In light of future missions beyond low Earth orbit (LEO) and the potential establishment of bases on the Moon and Mars, the effects of the deep space environment on biology need to be examined in order to develop protective countermeasures. Although many biological experiments have been performed in space since the 1960s, most have occurred in LEO and for only short periods of time. These LEO missions have studied many biological phenomena in a variety of model organisms, and have utilized a broad range of technologies. -
Uncorrected Proof
Planetary and Space Science xxx (xxxx) xxx-xxx Contents lists available at ScienceDirect Planetary and Space Science journal homepage: http://ees.elsevier.com Joint Europa Mission (JEM) a multi-scale study of Europa to characterize its habitability and search for extant life Michel Blanc a,∗, Nicolas André a, Olga Prieto-Ballesteros b, Javier Gomez-Elvira b, Geraint Jones c, Veerle Sterken d,e, William Desprats a,f, Leonid I. Gurvits g,p,ak, Krishan Khurana h, Aljona Blöcker i, Renaud Broquet j, Emma Bunce k, Cyril Cavel j, Gaël Choblet l, Geoffrey Colins m, Marcello Coradini n, John Cooper o, Dominic Dirkx p, Philippe Garnier a, David Gaudin f, Paul Hartogh q, Luciano Iess r, Adrian Jäggi d, Sascha Kempf s, Norbert Krupp q, Luisa Lara t, Jérémie LasuePROOFa, Valéry Lainey u, François Leblanc v, Jean-Pierre Lebreton w, Andrea Longobardo x, Ralph Lorenz y, Philippe Martins z, Zita Martins aa, Adam Masters ab,al, David Mimoun f, Ernesto Palumba x, Pascal Regnier j, Joachim Saur ac, Adriaan Schutte ad, Edward C. Sittler o, Tilman Spohn ae, Katrin Stephan ae, Károly Szegő af, Federico Tosi x, Steve Vance ag, Roland Wagner ae, Tim Van Hoolst ah, Martin Volwerk ai, Frances Westall aj a IRAP, France b INTA-CAB, Spain c MSSL/UCL, UK d University of Bern, Switzerland e ETH Zürich, Switzerland f ISAE, France g Joint Institute for VLBI ERIC, Dwingeloo, the Netherlands h UCLA, USA i Royal Institute of Technology KTH, Sweden j Airbus D&S, France k Univ. Leicester, UK l LPG, Univ. Nantes, France mWheaton College, USA n CSEO, USA o GSFC, USA p TU Delft, the Netherlands q MPS, Germany r Univ. -
Programme, (2016) 4Th International Workshop on Highly Siderophile Element Geochemistry
See discussions, stats, and author profiles for this publication at: https://www.researchgate.net/publication/324759584 Per request - Programme, (2016) 4th International Workshop on Highly Siderophile Element Geochemistry Research · July 2016 CITATIONS 0 1 author: Amy Riches 72 PUBLICATIONS 384 CITATIONS SEE PROFILE Some of the authors of this publication are also working on these related projects: 4th International Workshop on Highly Siderophile Element Geochemistry View project All content following this page was uploaded by Amy Riches on 25 April 2018. The user has requested enhancement of the downloaded file. Durham Geochemistry Centre Thank you to our sponsors who have made this workshop possible: 1 Welcome The event organisers are delighted to welcome, to the 4th International Workshop on Highly Siderophile Element Geochemistry, scientists of all career levels from academic institutions and government organisations from all over the globe. Durham University’s Department of Earth Sciences and its Geochemistry Group are thrilled to have brought together a large and diverse set of experts in HSE sciences, and we look forward to hosting a very productive meeting. Overview This specialist workshop is a 4 day event timed to occur between the 2016 Annual Goldschmidt Conference and the 79th Annual Meeting of the Meteoritical Society. It builds on the legacy of three highly-successful preceding meetings, the last of which took place in Durham in 2006 (then Chair, Dr. Ambre Luguet). This event also complements the short course on highly siderophile and strongly chalcophile elements in high temperature geochemistry and cosmochemistry held 7 months prior and linked to RiMG volume #81. The 4th International Workshop on Highly Siderophile Element Geochemistry is of cross-disciplinary appeal in covering analytical advances, as well as low-temperature and high-temperature geo- and cosmochemistry topics pertaining to HSEs and allied elements. -
The Meteoritical Society Newsletter 2001
SUPPLEMENT TO METEORITICS & PLANETARY SCIENCE, VOL. 36, 11 The Meteoritical Society Newsletter (November 2001) A report of the business carried out by the Society over the past year, edited by Edward Scott, Secretary. PRESIDENT'S EDITORIAL Nomenclature President's Editorial Gero Kurat There are some indications that SNC meteorites could originate from Mars, there are others that relate them to carbonaceous Things usually turn out somewhat different from what one expects chondrites. Among the advocates for a martian origin is also the them to be and this was exactly so also with my first few months in foremost expert on these meteorites, Hap McSween. Some colleagues office. I was positively surprised by the amount of activities initiated neglect the possibility that SNC meteorites could not come from Mars by members of our Society. The overwhelmingly constructive and call them "martian meteorites". Others prefer to call them contributions make investing time for the Society a joy. There are, "SNICs", for obvious reasons. Hap has this year been honored for however, also some unsolved problems which do not create instant his work on "martian meteorites". As the possibility for a non-martian joy but whose solution eventually could lead to improvements origin of SNC meteorites still exists, a curious conundrum emerges: beneficial for all of us. So joy is awaiting us afterwards. Us means how could Hap have done this wonderful work on something that the Council and in particular the Secretary of the Society who does possibly does not exist? Please help us to solve that riddle—the best an excellent job in spite of the bumpy communication between our three solutions will receive prizes. -
Figure 1 (Left) SOLID Instrument Block Diagram Showing 3 Main Modules. Power Is Provided by ICU, Which Collects Internal Senso
Eighth International Conference on Mars (2014) 1069.pdf THE SIGNS OF LIFE DETECTOR (SOLID): AN INSTRUMENT TO DETECT MOLECULAR BIOSIGNATURES ON MARS. V. Parro1, C. Stoker2, A.F. Davila3, R. Quinn4., Javier Gomez-Elvira1 1Centro de Astrobiología ([email protected]), 2NASA Ames Research Center ([email protected]), 3Carl Sagan Center at the SETI Institiute ([email protected]), 4Carl Sagan Center at the SETI Institiute ([email protected]). Introduction: The case for life on Mars grows fluorescence images with the results of the immunoas- stronger. Investigations at Gale Crater by Curiosity say. have revealed fine-grained sedimentary rocks inferred Conceptually, immunoassays mimic our immune to represent an ancient lake environment suited to sup- system in that a fleet of antibodies (Ab) is designed to port life [1]. In addition, Curiosity tentatively found a chemically capture desired organic compounds termed heterogeneous distribution of organic carbon within antigens (Ag) in solution. Antibodies possess high these sediments [2], consistent with the detection of specificity and affinity for their respective Ag, making native organic C in Mars meteorites. Futhermore, immunoassays both reliable and sensitive, with con- modern potentially habitable environments have been firmed detection limits of a few ppb for specific com- recognized on Mars including the N. Polar region vis- pounds. For analysis, the liquid extract obtained in the ited by Phoenix [3], gully featuers suggesting modern SPU is exposed to a fleet of Ab’s designed to anchor to water flows [4], and RSLs that occur seasonally sug- a specific region of the target organic compound. Spe- gest liquid processes[5]. -
The Meteoritical Society Newsletter
The Meteoritical Society Newsletter November, 2000 A report of Society activities during the past year compiled by Ed Scott, Secretary Sections: President's address New Council Meteoritics & Planetary Science Geochimica et Cosmochimica Acta Society Awards and Honors Planetary Sciences Best Student Paper Award Annual Meetings Finances Other committees and activities Constitutional changes PRESIDENT'S EDITORIAL Michael J. Drake It's been another great year for the Meteoritical Society! Mini Wadhwa, Andy Davis, and colleagues did a wonderful job of organizing and running the Chicago meeting and associated functions. Chicago was revealed as a vibrant, elegant city. As always, there are special people and families who provide generous help to the Society. The Barringer family has continued its support of graduate student travel, the Barringer Medal, and the Barringer lecture, which was given by Torrence Johnson. The Society is extremely grateful for this generous support. Speaking of medals, this year's medallists were Guenter Lugmair (Leonard Medal), Ralph Baldwin (Barringer Medal), and Meenakshi Wadhwa (Nier Prize - and chocolate medallions!) Congratulations to Guenter, Ralph, and Mini! In Rome, the awardees will be Harry McSween (Leonard Medal), Sasha Basilevsky (Barringer Medal), and Larry Nittler (Nier Prize), again well-deserved recipients of our prestigious awards. There will be further changes in Officers of the Society. It is my great pleasure to announce that Gero Kurat assumes the office of President, Gary Huss Vice President, and Tim Swindle Treasurer of the Meteoritical Society. David Kring has graciously agreed to serve as Deputy Treasurer. As you are aware, this year was the first since the 1970s that we had a contested Presidential election. -
It's Life… Isn't
It’s life… isn’t it? Scientists find it hard enough to pin down evidence of early life on our own planet. How on Earth do we plan to determine whether life exists elsewhere? John Whitfield finds out. e can, it’s fair to say, be confident their research agendas towards looking for As a control,the landers did the same tests on that there’s life on Earth — but life,says chemist Richard Mathies of the Uni- a heat-sterilized sample of martian soil. ASA/SPL Wproving it is a different matter. In versity of California,Berkeley.“Exobiology is Remarkably, every test gave a positive N December 1990, the Galileo spacecraft becoming more prominent,” he says. NASA result. The soil samples released oxygen and pointed its sensors back at Earth before and the European Space Agency (ESA) are compounds made from ingredients in the setting off for Jupiter. The probe reported moving from rock and mineral experiments nutrient solution, and carbon in the experi- an atmosphere abundant in oxygen and to biological ones, he explains. In 2009, both ment seemed to be incorporated into unusually rich in methane. It also detected a agencies will send landers to Mars that, organic molecules. Unfortunately, most of mysterious pigment that was unlikely to be unlike the Spirit and Opportunity rovers the controls — except the experiments of mineral origin: something earthlings call now on the planet, will be designed to look designed to detect nutrient uptake — also chlorophyll. Yet the astrophysicist Carl for the chemistry of life. gave positive results. At the same time, two Sagan and his colleagues were still cautious Astrobiologists are currently working out instruments designed to analyse the planet’s in their conclusions based on these results. -
Planetary & Solar System Sciences
EGU General Assembly 2012 EGU General Assembly 2012 Programme Group Programme PS – Planetary & Solar System Sciences Monday, 23 April ........................................................................................................................................................................ 2 PS1.1 ........................................................................................................................................................................................ 2 PS2.2 ........................................................................................................................................................................................ 2 GD1.1/PS2.7 .............................................................................................................................................................................. 3 PS3.3 ........................................................................................................................................................................................ 4 PS5.3/ST6.4 ............................................................................................................................................................................... 4 ST2.4/PS5.4 ............................................................................................................................................................................... 6 Tuesday, 24 April ......................................................................................................................................................................