Astromaterials Research and Exploration Science at NASA Johnson Space Center
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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. -
USGS Open-File Report 2005-1190, Appendix A
USGS Open-File Report 2005-1190 APPENDIX B Detailed listing of personnel changes for the Branch of Astrogeology from 1960 through 1972. In the early 1960’s, the Branch of Astrogeology grew slowly. Growth was rapid during and after 1964 with a maximum of 250 employees being reached in 1970 when design and training for the Apollo missions were at their peaks. [Authors Note: The Branch of Astrogeology in 2006 consisted of approximately 80 employees.] Table 1. Number of Employee with the U.S. Geological Survey, Branch of Astrogeology from 1960 through 1987 [Author’s Note: Although Monthly Reports for Astrogeology were submitted to the USGS and NASA through 1977, new personnel and personnel changes were only documented in these reports through 1970.] Year Number of employees 1960 18 1961 26 1962 40 1963 59 1964 143 1965 154 1966 221 1967 239 1968 244 1969 234 1970 250 1960 The following personnel joined the Astrogeologic Studies Unit at Menlo Park during 1960 (see main text and Appendix A) (various sources): Henry J. Moore II (Geologist, September) Charles H. “Chuck” Marshall (Geologist/Lunar mapper; September) Richard E. Eggleton (Geologist, October) Richard V. Lugn (August) 1961 The following personnel came on duty with the Branch of Astrogeology at Menlo Park, California during 1961 (see main text and Appendix A) (various sources): David J. Roddy (Geologist; January/February) Martin L. Baker (Scientific Photographer; October) Jacquelyn H. Freeberg (Research Librarian and Bibliographer; December) Daniel J. Milton (Geologist; August) Carl H. Roach (Geophysicist; August) 1 Maxine Burgess (Secretary) 1962 The following was taken from the Branch of Astrogeology Monthly Report for April 1962 from Chief, Branch of Astrogeology to V.E. -
Bayesian Analysis of the Astrobiological Implications of Life's
Bayesian analysis of the astrobiological implications of life's early emergence on Earth David S. Spiegel ∗ y, Edwin L. Turner y z ∗Institute for Advanced Study, Princeton, NJ 08540,yDept. of Astrophysical Sciences, Princeton Univ., Princeton, NJ 08544, USA, and zInstitute for the Physics and Mathematics of the Universe, The Univ. of Tokyo, Kashiwa 227-8568, Japan Submitted to Proceedings of the National Academy of Sciences of the United States of America Life arose on Earth sometime in the first few hundred million years Any inferences about the probability of life arising (given after the young planet had cooled to the point that it could support the conditions present on the early Earth) must be informed water-based organisms on its surface. The early emergence of life by how long it took for the first living creatures to evolve. By on Earth has been taken as evidence that the probability of abiogen- definition, improbable events generally happen infrequently. esis is high, if starting from young-Earth-like conditions. We revisit It follows that the duration between events provides a metric this argument quantitatively in a Bayesian statistical framework. By (however imperfect) of the probability or rate of the events. constructing a simple model of the probability of abiogenesis, we calculate a Bayesian estimate of its posterior probability, given the The time-span between when Earth achieved pre-biotic condi- data that life emerged fairly early in Earth's history and that, billions tions suitable for abiogenesis plus generally habitable climatic of years later, curious creatures noted this fact and considered its conditions [5, 6, 7] and when life first arose, therefore, seems implications. -
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. -
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. -
51. Astrobiology: the Final Frontier of Science Education
www.astrosociety.org/uitc No. 51 - Summer 2000 © 2000, Astronomical Society of the Pacific, 390 Ashton Avenue, San Francisco, CA 94112. Astrobiology: The Final Frontier of Science Education by Jodi Asbell-Clarke and Jeff Lockwood What (or Whom) Are We Looking For? Where Do We Look? Lessons from Our Past The Search Is On What Does the Public Have to Learn from All This? A High School Curriculum in Astrobiology Astrobiology seems to be all the buzz these days. It was the focus of the ASP science symposium this summer; the University of Washington is offering it as a new Ph.D. program, and TERC (Technical Education Research Center) is developing a high school integrated science course based on it. So what is astrobiology? The NASA Astrobiology Institute defines this new discipline as the study of the origin, evolution, distribution, and destiny of life in the Universe. What this means for scientists is finding the means to blend research fields such as microbiology, geoscience, and astrophysics to collectively answer the largest looming questions of humankind. What it means for educators is an engaging and exciting discipline that is ripe for an integrated approach to science education. Virtually every topic that one deals with in high school science is embedded in astrobiology. What (or Whom) Are We Looking For? Movies and television shows such as Contact and Star Trek have teased viewers with the idea of life on other planets and even in other galaxies. Illustration courtesy of and © 2000 by These fictional accounts almost always deal with intelligent beings that have Kathleen L. -