ROSALY M. C. LOPES Jet Propulsion Laboratory, California Institute Of
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Climate Disasters in the Philippines: a Case Study of the Immediate Causes and Root Drivers From
Zhzh ENVIRONMENT & NATURAL RESOURCES PROGRAM Climate Disasters in the Philippines: A Case Study of Immediate Causes and Root Drivers from Cagayan de Oro, Mindanao and Tropical Storm Sendong/Washi Benjamin Franta Hilly Ann Roa-Quiaoit Dexter Lo Gemma Narisma REPORT NOVEMBER 2016 Environment & Natural Resources Program Belfer Center for Science and International Affairs Harvard Kennedy School 79 JFK Street Cambridge, MA 02138 www.belfercenter.org/ENRP The authors of this report invites use of this information for educational purposes, requiring only that the reproduced material clearly cite the full source: Franta, Benjamin, et al, “Climate disasters in the Philippines: A case study of immediate causes and root drivers from Cagayan de Oro, Mindanao and Tropical Storm Sendong/Washi.” Belfer Center for Science and International Affairs, Cambridge, Mass: Harvard University, November 2016. Statements and views expressed in this report are solely those of the authors and do not imply endorsement by Harvard University, the Harvard Kennedy School, or the Belfer Center for Science and International Affairs. Design & Layout by Andrew Facini Cover photo: A destroyed church in Samar, Philippines, in the months following Typhoon Yolanda/ Haiyan. (Benjamin Franta) Copyright 2016, President and Fellows of Harvard College Printed in the United States of America ENVIRONMENT & NATURAL RESOURCES PROGRAM Climate Disasters in the Philippines: A Case Study of Immediate Causes and Root Drivers from Cagayan de Oro, Mindanao and Tropical Storm Sendong/Washi Benjamin Franta Hilly Ann Roa-Quiaoit Dexter Lo Gemma Narisma REPORT NOVEMBER 2016 The Environment and Natural Resources Program (ENRP) The Environment and Natural Resources Program at the Belfer Center for Science and International Affairs is at the center of the Harvard Kennedy School’s research and outreach on public policy that affects global environment quality and natural resource management. -
On the Ball! One of the Most Recognizable Stars on the U.S
TVhome The Daily Home June 7 - 13, 2015 On the Ball! One of the most recognizable stars on the U.S. Women’s World Cup roster, Hope Solo tends the goal as the U.S. 000208858R1 Women’s National Team takes on Sweden in the “2015 FIFA Women’s World Cup,” airing Friday at 7 p.m. on FOX. The Future of Banking? We’ve Got A 167 Year Head Start. You can now deposit checks directly from your smartphone by using FNB’s Mobile App for iPhones and Android devices. No more hurrying to the bank; handle your deposits from virtually anywhere with the Mobile Remote Deposit option available in our Mobile App today. (256) 362-2334 | www.fnbtalladega.com Some products or services have a fee or require enrollment and approval. Some restrictions may apply. Please visit your nearest branch for details. 000209980r1 2 THE DAILY HOME / TV HOME Sun., June 7, 2015 — Sat., June 13, 2015 DISH AT&T CABLE DIRECTV CHARTER CHARTER PELL CITY PELL ANNISTON CABLE ONE CABLE TALLADEGA SYLACAUGA SPORTS BIRMINGHAM BIRMINGHAM BIRMINGHAM CONVERSION CABLE COOSA WBRC 6 6 7 7 6 6 6 6 AUTO RACING 5 p.m. ESPN2 2015 NCAA Baseball WBIQ 10 4 10 10 10 10 Championship Super Regionals: Drag Racing Site 7, Game 2 (Live) WCIQ 7 10 4 WVTM 13 13 5 5 13 13 13 13 Sunday Monday WTTO 21 8 9 9 8 21 21 21 8 p.m. ESPN2 Toyota NHRA Sum- 12 p.m. ESPN2 2015 NCAA Baseball WUOA 23 14 6 6 23 23 23 mernationals from Old Bridge Championship Super Regionals Township Race. -
Planetary Report Report
The PLANETARYPLANETARY REPORT REPORT Volume XXV Number 5 September/October 2005 ATACAMA DESERT MarsMars AnalogsAnalogs VALLES MARINERIS Volume XXV Table of Number 5 Contents September/October 2005 A PUBLICATION OF Features From The Dry Earth, Wet Mars 6 Sometimes the best place to learn about Mars exploration is right here on Editor Earth. In Chile’s Atacama Desert, scientists have discovered an area so dry that organic material, and therefore evidence of life, is virtually undetectable. Study of he damage that Earth inflicts on her this parched Mars-like region on Earth may lead us to a better understanding of Tinhabitants—horribly demonstrated how to search for water and the elements of life in Martian soil. This year, The by Hurricane Katrina and the December Planetary Society cosponsored a field expedition to the Atacama Desert, sending tsunami—reminds us what fragile creatures graduate student Troy Hudson on a 1-week adventure with a team of scientists led we are, lucky to survive at all on this dynamic, by Society Board member Chris McKay. Here, Troy describes his experience. dispassionate ball of rock hurtling through space. 12 The Pioneer Anomaly: A Deep Space Mystery Our exploration of other worlds has As Pioneer 10 and 11 head toward the farthest reaches of our solar system, taught us that the potential for planetary something strange is happening—they are mysteriously slowing down. Scientists catastrophe is always with us. On Mars, do not yet know why the spacecraft aren’t acting as expected; however, The we’ve seen planet-rending gouges cut by Planetary Society has stepped in to help fund the effort to analyze roughly 25 years catastrophic floods. -
2009-06-19.Pdf2013-02-12 15:4710.7 MB
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(Preprint) AAS 18-416 PRELIMINARY INTERPLANETARY MISSION
(Preprint) AAS 18-416 PRELIMINARY INTERPLANETARY MISSION DESIGN AND NAVIGATION FOR THE DRAGONFLY NEW FRONTIERS MISSION CONCEPT Christopher J. Scott,∗ Martin T. Ozimek,∗ Douglas S. Adams,y Ralph D. Lorenz,z Shyam Bhaskaran,x Rodica Ionasescu,{ Mark Jesick,{ and Frank E. Laipert{ Dragonfly is one of two mission concepts selected in December 2017 to advance into Phase A of NASA’s New Frontiers competition. Dragonfly would address the Ocean Worlds mis- sion theme by investigating Titan’s habitability and prebiotic chemistry and searching for evidence of chemical biosignatures of past (or extant) life. A rotorcraft lander, Dragonfly would capitalize on Titan’s dense atmosphere to enable mobility and sample materials from a variety of geologic settings. This paper describes Dragonfly’s baseline mission design giv- ing a complete picture of the inherent tradespace and outlines the design process from launch to atmospheric entry. INTRODUCTION Hosting the moons Titan and Enceladus, the Saturnian system contains at least two unique destinations that have been classified as ocean worlds. Titan, the second largest moon in the solar system behind Ganymede and the only planetary satellite with a significant atmosphere, is larger than the planet Mercury at 5,150 km (3,200 miles) in diameter. Its atmosphere, approximately 10 times the column mass of Earth’s, is composed of 95% nitrogen, 5% methane, 0.1% hydrogen along with trace amounts of organics.1 Titan’s atmosphere may resemble that of the Earth before biological processes began modifying its composition. Similar to the hydrological cycle on Earth, Titan’s methane evaporates into clouds, rains, and flows over the surface to fill lakes and seas, and subsequently evaporates back into the atmosphere. -
NEWSLETTER Comets: Visitors from The
P LANETARY S CIENCE I NSTITUTE NEWSLETTER SPRING 2006 Vol. 7, No. 1 Comets: Visitors from the Early Solar System by Beatrice Mueller This is a great time to be a cometary scientist. We have had three successful spacecraft encounters in the past few years: Deep Space 1 flew by comet 19P/Borrelly in September 2001; Stardust flew through the dust coma of comet 81P/Wild 2 col- lecting samples in January, 2004, and delivering them success- fully to Earth in January, 2006; and, most recently, Deep Impact (the mission, not the movie) hit comet 9P/Tempel 1 in July, 2005. We have also had two “naked-eye” comets in the middle of the nineties: comets Hale-Bopp and Hyakutake, both discov- ered by amateurs. Although I am not on the science teams of these spacecraft mis- sions, I was, and still am, involved with ground-based support observations doing additional scientific research. Only a few specific, but important, science questions can be answered at the time of the actual short-lived spacecraft flybys and much impor- tant research is accomplished long after these exciting events. I am working currently on the rotation state of comet 10P/ Tempel 2. Ignacio Ferrin and I (Mueller & Ferrin 1996, Icarus) observed this comet in 1994 and compared the derived rotation period with a previous pass and found a small change in the rota- Raw CCD R-filter image of the main component of comet tion period. Numerical simulations by Nalin Samarasinha (PSI & 73P/Schwassmann-Wachmann 3 (small white object). Note the National Optical Astronomy Observatory [NOAO]) show the extension and fuzziness of the comet and the narrow tail. -
Global Humanitarian Assistance Report 2013
GLOBAL HUMANITARIAN ASSISTANCE REPORT 2013 GLOBAL HUMANITARIAN ASSISTANCE Report 2013 Acknowledgements Thank you The Global Humanitarian Assistance (GHA) team would like to thank the many people who have been involved in helping us put the GHA report 2013 together: our colleagues at Development Initiatives; Diane Broadley of Broadley Design; Jon Lewis at Essential Print Management for his role in production; Lydia Poole for peer reviewing; Lisa Walmsley for research on the 'How technology can improve response' section; Velina Stoianova for research and analysis into private humanitarian funding. We would like to thank the programme’s funders for their continued support: the Canadian International Development Agency (CIDA); the Human Rights, Good Governance and Humanitarian Aid Department of the Ministry of Foreign Affairs, the Netherlands; the Swedish International Development Cooperation Agency (Sida), Sweden; and the Department for International Development (DFID), the United Kingdom. The GHA report 2013 was co-authored by Oliver Buston (Consultant) and Kerry Smith (Programme Manager) with extensive data analysis and research from GHA team members: Chloe Stirk, Dan Sparks, Daniele Malerba (Data Lead) and Hannah Sweeney, while Jenny Claydon coordinated editorial production. Editorial guidance was provided by Executive Directors, Judith Randel and Tony German, and Director of Research, Analysis and Evidence, Dan Coppard. Contents Foreword 2 Executive summary 3 Part 1: Humanitarian response to crisis 9 1. How much humanitarian assistance was given? 11 How much was needed? 12 Was enough given? 14 2. Where does humanitarian assistance come from? 19 Government donors 20 In focus: Gulf States 28 Individual and private donors 30 Domestic government response 34 In focus: Turkey 36 3. -
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 -
Leveraging Public Data to Reconstruct the Cost History of Planetary Exploration
Leveraging Public Data to Reconstruct the Cost History of Planetary Exploration Casey Dreier Senior Space Policy Adviser The Planetary Society Motivations MSL Curiosity Press Kit: • Publicly-reported mission costs are inconsistent and lack detail • Comparisons are difficult between missions and over time Perseverance Press Kit: • A problem for both public education and advocates: • Press kit numbers are what gets reported! • How much “should” a mission cost? Voyager Press Kit: • How to interpret the total cost—is a $1B mission “expensive” or “a good deal”? • How much is a mission in the context of all planetary spending? Or all of NASA spending? Juno Press Kit: • How much of a mission cost are development, launch, and operations? What does it cost to explore the planets? Project Goals vs • Compile a complete record of mission and program costs for NASA’s robotic planetary program using public data. • Useful for public and public policy discourse: • Normalized to include accounting changes • Include all mission costs: development, launch, and all operations • Inflation-adjusted values • Provide costs by year • Easily and freely accessible Method • Primary source: NASA budget estimates provided by NASA HQ History Office • Used “actual” reported obligations • Augmented by a variety of secondary sources, in order of preference: • Official NASA statements (press releases, public briefings) • Projected values in PBRs • Reporting from high-quality news agencies • Normalizations (“gap fill” strategy): • Include all LV costs, except STS • Removed -
PAC March 9 10 2020 Report
NASA ADVISORY COUNCIL PLANETARY SCIENCE ADVISORY COMMITTEE March 9-10, 2020 NASA Headquarters Washington, DC MEETING REPORT _____________________________________________________________ Anne Verbiscer, Chair ____________________________________________________________ Stephen Rinehart, Executive Secretary Table of Contents Opening and Announcements, Introductions 3 PSD Update and Status 3 PSD R&A Status 5 Planetary Protection 7 Discussion 8 Mars Exploration Program 8 Lunar Exploration Program 9 PDCO 11 Planetary Data System 12 PDS at Headquarters 13 Findings and Discussion 13 General Comments 13 Exoplanets in Our Backyard 14 AP Assets for Solar System Observations 15 Solar System Science with JWST 16 Mercury Group 17 VEXAG 17 SBAG 18 OPAG 19 MEPAG 19 MAPSIT 20 LEAG 21 CAPTEM 21 Discussion 22 Findings and Recommendations Discussion 23 Appendix A- Attendees Appendix B- Membership roster Appendix C- Agenda Appendix D- Presentations Prepared by Joan M. Zimmermann Zantech, Inc. 2 Opening, Announcements, Around the Table Identification Executive Secretary of the Planetary Science Advisory Committee (PAC), Dr. Stephen Rinehart, opened the meeting and made administrative announcements. PAC Chair, Dr. Anne Verbiscer, welcomed everyone to the virtual meeting. Announcements were made around the table and on Webex. PSD Status Report Dr. Lori Glaze, Director of the Planetary Science Division, gave a status report. First addressing the President’s Budget Request (PBR) for Fiscal Year 2021 (FY21) for the Science Mission Directorate (SMD), Dr. Glaze noted that it was one of the strongest science budgets in NASA history, representing a 12% increase over the enacted FY20 budget. The total PBR keeps NASA on track to land on the Moon by 2024; and to help prepare for human exploration at Mars. -
The Planetary Report
!-' Volume XIX Number 6 November/December 1999 Volume XIX On the Cover: The spring eq uinox for Mars' sou thern hemisphere arrived Table of Number 6 August 2, 1999, br in gi ng in the warm seasons of the yea r. The frosts of the southern polar cap began to retreat. As summer Contents Novem ber/December 1999 approached, so did the Mars Polar Lander (MPL), scheduled to touch down near the edge of the frost cap on December 3. What will MPL fi nd? We don't know yet, but the lander may encounter dust storms, which freque ntly blow in th is regio n. In this image, take n in late July, we see grayish-orange du st Features clouds just above the frost cap at the lower left. Image: Malin Space Science Systems/NASA 4 An Intervievv With Tim Ferris Does life exist on other worlds? How do we find it? Ifwe find it, how do we study or communicate with it? Science writer Tim Ferris addresses these questions in a new Public Broadcasting System television series about the possibility of extraterrestrial life, He shares some of hi s thoughts with The Planetary Report. Froln Over One Million Served: The 5 SETI@home Passes the Million Mark SETI@home is definitely the biggest research project The Planetary Society has ever been Editor involved with-and it just keeps getting bigger. Have you joined yet? t's hard to explore planets, really hard. 6 Assessing the Hazard: Those of us of a certain age remember The Development of the Torino Scale I How do you convey the approximate degree of danger posed by a passing asteroid to someone John F. -
Active Volcanism on Io: Global Distribution and Variations in Activity
Icarus 140, 243–264 (1999) Article ID icar.1999.6129, available online at http://www.idealibrary.com on Active Volcanism on Io: Global Distribution and Variations in Activity Rosaly Lopes-Gautier Jet Propulsion Laboratory, California Institute of Technology, Pasadena, California 91109 E-mail: [email protected] Alfred S. McEwen Department of Planetary Sciences, Lunar and Planetary Laboratory, University of Arizona, P. O. Box 210092, Tucson, Arizona 85721-0092 William B. Smythe Jet Propulsion Laboratory, California Institute of Technology, Pasadena, California 91109 P. E. Geissler Department of Planetary Sciences, Lunar and Planetary Laboratory, University of Arizona, P. O. Box 210092, Tucson, Arizona 85721-0092 L. Kamp and A. G. Davies Jet Propulsion Laboratory, California Institute of Technology, Pasadena, California 91109 J. R. Spencer Lowell Observatory, Flagstaff, Arizona 86001 L. Keszthelyi Department of Planetary Sciences, Lunar and Planetary Laboratory, University of Arizona, P. O. Box 210092, Tucson, Arizona 85721-0092 R. Carlson Jet Propulsion Laboratory, California Institute of Technology, Pasadena, California 91109 F. E. Leader and R. Mehlman Institute of Geophysics and Planetary Physics, University of California—Los Angeles, Los Angeles, California 90095 L. Soderblom Branch of Astrogeologic Studies, U.S. Geological Survey, Flagstaff, Arizona 86001 and The Galileo NIMS and SSI Teams Received June 23, 1998; revised February 10, 1999 in 1979. A total of 61 active volcanic centers have been identified Io’s volcanic activity has been monitored by instruments aboard from Voyager, groundbased, and Galileo observations. Of these, 41 the Galileo spacecraft since June 28, 1996. We present results from are hot spots detected by NIMS and/or SSI.