Vision and Voyages for Planetary Science in the Decade 2013-2022
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Investigating Cosmic Snowballs
Investigating Cosmic Snowballs Professor David Jewitt CREDIT: NASA INVESTIGATING COSMIC SNOWBALLS Professor David Jewitt and his team at UCLA explore the nature of comets. These fleeting visitors to our cosmic shore are important sources of information, and can help to reveal the origin and evolution of the solar system. Most recently, Professor Jewitt’s team have explained the unusual activity of some of the most distant comets in the solar system. Comets play a vivid historical role in the orbital periods of less than 200 years), human psyche, often being interpreted and the other supplying long-period as portents of impending doom. In the objects (greater than 200 years). The era of modern science, we realise that nearest store of cometary precursors, comets are simply icy leftovers, frozen in containing billions of nuclei larger time since the solar system’s formation than a kilometre across, is called the about 4.6 billion years ago. Kuiper Belt. This is a fat disk of objects encircling the Sun with an inner edge Far from bringing us doom and disaster, at Neptune’s orbit – approximately 7.5 comets offer scientists unparalleled billion kilometres from the Sun, or 30 opportunities to learn about the earliest AU – and reaching out to at least several periods of the solar system’s evolution. thousand AU. Pluto resides in this region At the same time, they are some of and is now recognised as large Kuiper the most challenging objects to Belt object. study and remain some of the least well understood. The Kuiper belt was discovered by Professor David Jewitt and his former What Are Comets and Where Do student Jane Luu in 1992. -
Section 1: MIT Facts and History
1 MIT Facts and History Economic Information 9 Technology Licensing Office 9 People 9 Students 10 Undergraduate Students 11 Graduate Students 12 Degrees 13 Alumni 13 Postdoctoral Appointments 14 Faculty and Staff 15 Awards and Honors of Current Faculty and Staff 16 Awards Highlights 17 Fields of Study 18 Research Laboratories, Centers, and Programs 19 Academic and Research Affiliations 20 Education Highlights 23 Research Highlights 26 7 MIT Facts and History The Massachusetts Institute of Technology is one nologies for artificial limbs, and the magnetic core of the world’s preeminent research universities, memory that enabled the development of digital dedicated to advancing knowledge and educating computers. Exciting areas of research and education students in science, technology, and other areas of today include neuroscience and the study of the scholarship that will best serve the nation and the brain and mind, bioengineering, energy, the envi- world. It is known for rigorous academic programs, ronment and sustainable development, informa- cutting-edge research, a diverse campus commu- tion sciences and technology, new media, financial nity, and its long-standing commitment to working technology, and entrepreneurship. with the public and private sectors to bring new knowledge to bear on the world’s great challenges. University research is one of the mainsprings of growth in an economy that is increasingly defined William Barton Rogers, the Institute’s founding pres- by technology. A study released in February 2009 ident, believed that education should be both broad by the Kauffman Foundation estimates that MIT and useful, enabling students to participate in “the graduates had founded 25,800 active companies. -
Westminsterresearch the Astrobiology Primer V2.0 Domagal-Goldman, S.D., Wright, K.E., Adamala, K., De La Rubia Leigh, A., Bond
WestminsterResearch http://www.westminster.ac.uk/westminsterresearch The Astrobiology Primer v2.0 Domagal-Goldman, S.D., Wright, K.E., Adamala, K., de la Rubia Leigh, A., Bond, J., Dartnell, L., Goldman, A.D., Lynch, K., Naud, M.-E., Paulino-Lima, I.G., Kelsi, S., Walter-Antonio, M., Abrevaya, X.C., Anderson, R., Arney, G., Atri, D., Azúa-Bustos, A., Bowman, J.S., Brazelton, W.J., Brennecka, G.A., Carns, R., Chopra, A., Colangelo-Lillis, J., Crockett, C.J., DeMarines, J., Frank, E.A., Frantz, C., de la Fuente, E., Galante, D., Glass, J., Gleeson, D., Glein, C.R., Goldblatt, C., Horak, R., Horodyskyj, L., Kaçar, B., Kereszturi, A., Knowles, E., Mayeur, P., McGlynn, S., Miguel, Y., Montgomery, M., Neish, C., Noack, L., Rugheimer, S., Stüeken, E.E., Tamez-Hidalgo, P., Walker, S.I. and Wong, T. This is a copy of the final version of an article published in Astrobiology. August 2016, 16(8): 561-653. doi:10.1089/ast.2015.1460. It is available from the publisher at: https://doi.org/10.1089/ast.2015.1460 © Shawn D. Domagal-Goldman and Katherine E. Wright, et al., 2016; Published by Mary Ann Liebert, Inc. This Open Access article is distributed under the terms of the Creative Commons Attribution Noncommercial License (http://creativecommons.org/licenses/by- nc/4.0/) which permits any noncommercial use, distribution, and reproduction in any medium, provided the original author(s) and the source are credited. The WestminsterResearch online digital archive at the University of Westminster aims to make the research output of the University available to a wider audience. -
Professor Peter Goldreich Member of the Board of Adjudicators Chairman of the Selection Committee for the Prize in Astronomy
The Shaw Prize The Shaw Prize is an international award to honour individuals who are currently active in their respective fields and who have recently achieved distinguished and significant advances, who have made outstanding contributions in academic and scientific research or applications, or who in other domains have achieved excellence. The award is dedicated to furthering societal progress, enhancing quality of life, and enriching humanity’s spiritual civilization. Preference is to be given to individuals whose significant work was recently achieved and who are currently active in their respective fields. Founder's Biographical Note The Shaw Prize was established under the auspices of Mr Run Run Shaw. Mr Shaw, born in China in 1907, was a native of Ningbo County, Zhejiang Province. He joined his brother’s film company in China in the 1920s. During the 1950s he founded the film company Shaw Brothers (HK) Limited in Hong Kong. He was one of the founding members of Television Broadcasts Limited launched in Hong Kong in 1967. Mr Shaw also founded two charities, The Shaw Foundation Hong Kong and The Sir Run Run Shaw Charitable Trust, both dedicated to the promotion of education, scientific and technological research, medical and welfare services, and culture and the arts. ~ 1 ~ Message from the Chief Executive I warmly congratulate the six Shaw Laureates of 2014. Established in 2002 under the auspices of Mr Run Run Shaw, the Shaw Prize is a highly prestigious recognition of the role that scientists play in shaping the development of a modern world. Since the first award in 2004, 54 leading international scientists have been honoured for their ground-breaking discoveries which have expanded the frontiers of human knowledge and made significant contributions to humankind. -
PDF Program Book
46th Meeting of the Division for Planetary Sciences with Historical Astronomy Division (HAD) 9-14 November 2014 | Tucson, AZ OFFICERS AND MEMBERS ........ 2 SPONSORS ............................... 2 EXHIBITORS .............................. 3 FLOOR PLANS ........................... 5 ATTENDEE SERVICES ................. 8 Session Numbering Key SCHEDULE AT-A-GLANCE ........ 10 100s Monday 200s Tuesday SUNDAY ................................. 20 300s Wednesday 400s Thursday MONDAY ................................ 23 500s Friday TUESDAY ................................ 44 Sessions are numbered in the program book by day and time. WEDNESDAY .......................... 75 All posters will be on display Monday - Friday THURSDAY.............................. 85 FRIDAY ................................. 119 Changes after 1 October are included only in the online program materials. AUTHORS INDEX .................. 137 1 DPS OFFICERS AND MEMBERS Current DPS Officers Heidi Hammel Chair Bonnie Buratti Vice-Chair Athena Coustenis Secretary Andrew Rivkin Treasurer Nick Schneider Education and Public Outreach Officer Vishnu Reddy Press Officer Current DPS Committee Members Rosaly Lopes Term Expires November 2014 Robert Pappalardo Term Expires November 2014 Ralph McNutt Term Expires November 2014 Ross Beyer Term Expires November 2015 Paul Withers Term Expires November 2015 Julie Castillo-Rogez Term Expires October 2016 Jani Radebaugh Term Expires October 2016 SPONSORS 2 EXHIBITORS Platinum Exhibitor Silver Exhibitors 3 EXHIBIT BOOTH ASSIGNMENTS 206 Applied -
VITA David Jewitt Address Dept. Earth, Planetary and Space
VITA David Jewitt Address Dept. Earth, Planetary and Space Sciences, UCLA 595 Charles Young Drive East, Box 951567 Los Angeles, CA 90095-1567 [email protected], http://www2.ess.ucla.edu/~jewitt/ Education B. Sc. University College London 1979 M. S. California Institute of Technology 1980 Ph. D. California Institute of Technology 1983 Professional Experience Summer Student Royal Greenwich Observatory 1978 Anthony Fellowship California Institute of Technology 1979-1980 Research Assistant California Institute of Technology 1980-1983 Assistant Professor Massachusetts Institute of Technology 1983-1988 Associate Professor and Astronomer University of Hawaii 1988-1993 Professor and Astronomer University of Hawaii 1993-2009 Professor Dept. Earth, Planetary & Space Sciences, UCLA 2009- Inst. of Geophys & Planetary Physics, UCLA 2009-2011 Dept. Physics & Astronomy, UCLA 2010- Director Institute for Planets & Exoplanets, UCLA, 2011- Honors Regent's Medal, University of Hawaii 1994 Scientist of the Year, ARCS 1996 Exceptional Scientific Achievement Award, NASA 1996 Fellow of University College London 1998 Fellow of the American Academy of Arts and Sciences 2005 Fellow of the American Association for the Advancement of Science 2005 Member of the National Academy of Sciences 2005 National Observatory, Chinese Academy of Sciences, Honorary Professor 2006-2011 National Central University, Taiwan, Adjunct Professor 2007 The Shaw Prize for Astronomy 2012 The Kavli Prize for Astrophysics 2012 Foreign Member, Norwegian Academy of Sciences & Letters 2012 Research -
NASA Astrobiology Institute 2018 Annual Science Report
A National Aeronautics and Space Administration 2018 Annual Science Report Table of Contents 2018 at the NAI 1 NAI 2018 Teams 2 2018 Team Reports The Evolution of Prebiotic Chemical Complexity and the Organic Inventory 6 of Protoplanetary Disk and Primordial Planets Lead Institution: NASA Ames Research Center Reliving the Past: Experimental Evolution of Major Transitions 18 Lead Institution: Georgia Institute of Technology Origin and Evolution of Organics and Water in Planetary Systems 34 Lead Institution: NASA Goddard Space Flight Center Icy Worlds: Astrobiology at the Water-Rock Interface and Beyond 46 Lead Institution: NASA Jet Propulsion Laboratory Habitability of Hydrocarbon Worlds: Titan and Beyond 60 Lead Institution: NASA Jet Propulsion Laboratory The Origins of Molecules in Diverse Space and Planetary Environments 72 and Their Intramolecular Isotope Signatures Lead Institution: Pennsylvania State University ENIGMA: Evolution of Nanomachines in Geospheres and Microbial Ancestors 80 Lead Institution: Rutgers University Changing Planetary Environments and the Fingerprints of Life 88 Lead Institution: SETI Institute Alternative Earths 100 Lead Institution: University of California, Riverside Rock Powered Life 120 Lead Institution: University of Colorado Boulder NASA Astrobiology Institute iii Annual Report 2018 2018 at the NAI In 2018, the NASA Astrobiology Program announced a plan to transition to a new structure of Research Coordination Networks, RCNs, and simultaneously planned the termination of the NASA Astrobiology Institute -
Astrobiology on Habitable Worlds
Astrobiology on habitable worlds: The case for considering prebiotic chemistry in mission design Aaron Engelhart, Jennifer Blank, Christopher Carr, Zachary Adam, Ariel Anbar, Steven Benner, Donald Burke-Aguero, Aaron Burton, Andrew Ellington, Michael Gaylor, et al. To cite this version: Aaron Engelhart, Jennifer Blank, Christopher Carr, Zachary Adam, Ariel Anbar, et al.. Astrobiology on habitable worlds: The case for considering prebiotic chemistry in mission design. 2020. hal- 03161833 HAL Id: hal-03161833 https://hal.archives-ouvertes.fr/hal-03161833 Submitted on 8 Mar 2021 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. Astrobiology on habitable worlds: The case for considering prebiotic chemistry in mission design Lead author: Aaron E. Engelhart, University of Minnesota. Phone: 612-625-1950 E-mail: [email protected] Co-authors: Jennifer G Blank, NASA Ames Research Center/Blue Marble Space Institute of Science Christopher Carr, Georgia Institute of Technology Henderson James Cleaves, Earth-Life Science Institute Kennda Lynch, Lunar and Planetary Institute/USRA Co-signatories: Zachary Adam, University of Arizona Katarzyna P. Adamala, University of Minnesota Ariel D. Anbar, Arizona State University Laura M. Barge, Jet Propulsion Laboratory David A. Baum, University of Wisconsin-Madison Steven A. -
Bulletin Issue 29 Spring 2018 New Series by Paul Haley Begins in This Issue: 19Th Century Observatories 2018 Sha Spring Conference
BULLETIN ISSUE 29 SPRING 2018 NEW SERIES BY PAUL HALEY BEGINS IN THIS ISSUE: 19TH CENTURY OBSERVATORIES 2018 SHA SPRING CONFERENCE The first talk is at 1015 and the Saturday 21st April 2018 The conference registraon is morning session ends at 1215 Instute of Astronomy, between 0930 and 1000 at which for lunch. The lunch break is University of Cambridge me refreshments are available unl 1330. An on-site lunch Madingley Road, Cambridge in the lecture theatre. The will be available (£5.00) BUT CB3 0HA conference starts at 1000 with a MUST BE PRE-ORDERED. There welcome by the SHA Chairman are no nearby eang places. Bob Bower introduces the There is a break for refreshments Aer the break there is the aernoon session at 1330 then from 1530 to 1600 when Tea/ final talk. The aernoon there are two one-hour talks. Coffee and biscuits will be session will end at 5 p.m. and provided. the conference will then close. 10 00 - 1015 10 15 - 1115 1115 - 1215 SHA Chairman Bob Bower Carolyn Kennett and Brian Sheen Kevin Kilburn Welcomes delegates to Ancient Skies and the Megaliths Forgotten Star Atlas the Instute of of Cornwall Astronomy for the SHA 2018 Archeoastronomy in Cornwall The 18th Century unpublished Spring Conference Past and Present Uranographia Britannica by Dr John Bevis 13 30 - 1430 14 30 - 1530 16 00 – 17 00 Nik Szymanek Kenelm England Jonathan Maxwell The Road to Modern Berkshire Astronomers 5000 BC Some lesser known aspects Astrophotography to AD 2018 regarding the evolution of The pioneering days of Some topics on astronomers and refracting telescopes: from early astrophotographers, observations made from Lippershey's spectacle lens to the up to modern times Berkshire since pre-historic Apochromats times until last week An insight into the development of 2 the refracting telescope In this Issue BOOK SALE AT THE 2017 AGM Digital Bulletin The Digital Bulletin provides extra content and links when viewing the 4 Bulletin as a PDF. -
Conference Program
Conference Program 2018 Conference Chair George K. Tan 2018 Organizing Committee Aaron Pital Jonny Tan Adriana Lozoya Julia McGonigle Becky Rapf Justin Lawrence Ben Intoy Kennda Lynch Bradley Burcar Kimberly Chen Brandon Carroll Marcus Bray Brett McGuire Marshall Seaton Chase Chivers Micha Schaible Chloe Stanton Nadia Szeinbaum Chris Parsons Rio Febrian David Fiahlo Santi Mestre Fos Dedra Eichstedt Scot Sutton Elizabeth Spiers Sheri Motamedi Jay Kroll Zach Duca Jennifer Farrar Proposal Writing Retreat Organizing Committee Becky Rapf (Chair) Julia McGonigle Dedra Eichstedt Zach Duca 2 Sponsors 3 Schedule Monday Tuesday Wednesday Thursday Friday 6/4/18 6/5/18 6/6/18 6/7/18 6/8/18 Breakfast Breakfast Breakfast 8:00AM 8:00-9:00AM 8:00-9:00AM 8:00-9:00AM Talks Talks 9:00AM 1 Warm-up + 3 Talks 1 Warm-up + 3 Talks 9:00AM-10:10AM 9:00AM-10:10AM Coffee Break Coffee Break 10:00AM 10:10AM-10:30AM 10:10AM-10:30AM Talks Talks 4 Talks 4 Talks Field Trip 10:30AM-11:50AM 10:30AM-11:50AM 10:00AM-2:00PM 11:00AM Lunch Lunch 11:50AM-1:00PM 11:50AM-1:00PM 12:00PM Arrival 1:00PM Talks Talks 1 Warm-up + 3 Talks 1 Warm-up + 3 Talks 1:00PM-2:10PM 1:00PM-2:10PM Break 2:00PM Break Break Departure 2:00PM-3:00PM 2:10PM-2:30PM 2:10PM-2:30PM Talks Career Panel Primer 3.0 Info. 3 Talks 2:30PM-3:30PM Session 2:30PM-3:30PM 3:00PM-3:30PM 3:00PM Early Career Town Hall 3:30-4:00PM Posters Posters AGC 2019 Planning 4:00PM 3:30PM-5:30PM 3:30PM-5:30PM 4:00-5:00PM Reception 5:00PM 5:00PM-6:00PM Opening Dinner Dinner On Your Own 6:00PM 5:00PM - 7:00PM 5:30PM - 7:30PM Outreach -
Rotational Characterization of Hayabusa II Target Asteroid (162173)
Rotational Characterization of Hayabusa II Target Asteroid (162173) 1999 JU3 Nicholas A. Moskovitz a;b;1 Shinsuke Abe c Kang-Shian Pan c David J. Osip d Dimitra Pefkou a Mario D. Melita e Mauro Elias e Kohei Kitazato f Schelte J. Bus g Francesca E. DeMeo a Richard P. Binzel a Paul A. Abell h aMassachusetts Institute of Technology, Department of Earth, Atmospheric and Planetary Sciences, 77 Massachusetts Avenue, Cambridge, MA 02139 (U.S.A.) bCarnegie Institution of Washington, Department of Terrestrial Magnetism, 5241 Broad Branch Road, Washington, DC 20008 (U.S.A.) cNational Central University, Institute of Astronomy, 300 Jhongda Road, Jhongli, Taoyuan 32001 (Taiwan) dCarnegie Institution of Washington, Las Campanas Observatory, Colina El Pino, Casilla 601 La Serena (Chile) eUniversidad de Buenos Aires, Instituto de Astronomica y Fisica del Espacio, Buenos Aires (Argentina) f The University of Aizu, Research Center for Advanced Information Science and arXiv:1302.1199v1 [astro-ph.EP] 5 Feb 2013 Technology, Ikki-machi, Aizu-Wakamatsu, Fukushima 965-8580 (Japan) gUniversity of Hawaii, Institute for Astronomy, 640 N. A'ohoku Place, Hilo, HI 96720 (U.S.A.) hNASA Johnson Space Center, Astromaterials Research and Exploration Science Directorate, Houston, TX 77058 (U.S.A.) Copyright c 2012 Nicholas A. Moskovitz Preprint submitted to Icarus 12 October 2018 Number of pages: 24 Number of tables: 3 Number of figures: 6 1 Observations conducted while at Carnegie DTM, current address is MIT. 2 Proposed Running Head: Rotational characterization of 1999 JU3 Please send Editorial Correspondence to: Nicholas A. Moskovitz Department of Earth, Atmospheric and Planetary Sciences Massachusetts Institute of Technology 77 Massachusetts Avenue Cambridge, MA 02139, USA. -
The Formation of the Martian Moons Rosenblatt P., Hyodo R
The Final Manuscript to Oxford Science Encyclopedia: The formation of the Martian moons Rosenblatt P., Hyodo R., Pignatale F., Trinh A., Charnoz S., Dunseath K.M., Dunseath-Terao M., & Genda H. Summary Almost all the planets of our solar system have moons. Each planetary system has however unique characteristics. The Martian system has not one single big moon like the Earth, not tens of moons of various sizes like for the giant planets, but two small moons: Phobos and Deimos. How did form such a system? This question is still being investigated on the basis of the Earth-based and space-borne observations of the Martian moons and of the more modern theories proposed to account for the formation of other moon systems. The most recent scenario of formation of the Martian moons relies on a giant impact occurring at early Mars history and having also formed the so-called hemispheric crustal dichotomy. This scenario accounts for the current orbits of both moons unlike the scenario of capture of small size asteroids. It also predicts a composition of disk material as a mixture of Mars and impactor materials that is in agreement with remote sensing observations of both moon surfaces, which suggests a composition different from Mars. The composition of the Martian moons is however unclear, given the ambiguity on the interpretation of the remote sensing observations. The study of the formation of the Martian moon system has improved our understanding of moon formation of terrestrial planets: The giant collision scenario can have various outcomes and not only a big moon as for the Earth.