DOCSLIB.ORG

1994 Annual Report.Pdf

Total Page：16

File Type：pdf, Size：1020Kb

Download full-text PDF Read full-text
1994 Annual Report.Pdf Contents Craig Dickson Craig The Atlantis II A-frame lifts Alvin from the water following a dive off Mexico. Cover Photo: Foam from a passing wave frames a rosette water sampler and conductivity/temperature/depth instrument being recovered aboard R/V Knorr in the Antarctic in January 1994. Line handlers (back cover), top to bottom of photo, are Mike McCartney, Jason McKay, Marshall Swartz and Tom Whitworth (Texas A&M University). Photo by Craig Dickson Director’s Comments ....................................................... 2 Coastal Research Center .......................................... 24 Regular Support Staff ................................................... 39 Applied Ocean Physics & Engineering ...... 4 Center for Marine Exploration .......................... 25 1994 Degree Recipients ............................................ 42 Biology ............................................................................................. 7 Sea Grant Program .......................................................... 26 Fellows, Students, & Visitors ................................. 43 Geology & Geophysics ............................................... 11 Dean’s Comments ............................................................ 27 Trustees & Corporation Members ................. 46 Marine Chemistry & Geochemistry ............. 15 Ashore & Afloat ................................................................... 30 Voyage Statistics ................................................................. 49 Physical Oceanography ............................................ 19 Director’s Council ............................................................ 36 Publications ............................................................................ 51 Marine Policy Center .................................................... 23 Scientific & Technical Staff .................................... 37 Financial Statements .................................................... 64 1994 Annual Report Woods Hole Oceanographic Institution Woods Hole, MA 02543 • (508) 457-2000 Editor: Vicky Cullen • Designer: Jim Canavan Woods Hole Oceanographic Institution is an Equal Employment Opportunity and Affirmative Action Institution 1 Printed on Recycled Paper 1994 Annual Report Director’s Comments Looking back on my first year as Director, I must say there has been quite a share of challenges and accomplish- ments. Changes on both national and international levels require a more competitive and innovative Institution stance as we continue to build upon our strengths in basic ocean science research and education. With Jim Luyten’s new appointment as Associate Director for Research, the Institution, and, in particular, the science departments and centers, are well served not only by Jim’s vigorous and accom- plished scientific background, but also by his seasoned understanding of the Institution and its culture. Inc. Marine, Halter Courtesy of The year 1994 brought other new names and shapes: The keel laying of Bob Gagosian, immediately to the right of and other Japanese institutions. During the new AGOR 25 was accompanied by the sign, and Joe Coburn, fourth from a multi-phased expedition to the Mid- its official naming as Atlantis, continuing right, joined US Navy and Halter Marine Atlantic Ridge, many technologies were officials to celebrate the keel laying for the a WHOI tradition of seagoing excellence brought together to carry out controlled new Atlantis in Moss Point, Mississippi. that dates to our founding; Oceanus experiments on areas of the ocean floor returned from a mid-life refit that offers never before accessible. During this increased laboratory space and scien- project, Woods Hole was the occasion tific berthing, and the recently stretched for the visit of JAMSTEC’s R/V Yokosuka Bob Gagosian chats with Japan Marine Sci- Knorr and its 6,500-meter submersible Shinkai left in superb condition on a ence and Technology Center President Mitsusu remarkable 43,000-mile expedition to Ishizuka during the festivities surrounding 6500, an Institution event enjoyed by the the Indian Ocean. In addition, Atlantis II the July visit of the Japanese submersible more than 1,200 staff and family continues to maintain a Herculean Shinkai 6500 and its tender Yokosuka. members who came to tour the ship schedule with the and meet our international colleagues. submersible Alvin. This was a milestone in our relationship The US Navy in- with Japanese scientists, and it serves as creased Alvin’s a foundation for future collaboration. operating depth Over $10 million was raised in 1994, certification from bringing to $34 million the total secured 4,000 to 4,500 meters or committed toward the $50 million in 1994, allowing the Capital Campaign goal. The dedication submersible to and commitment of our Trustees and investigate 86 percent Corporation Members have really made of the world ocean a difference. Because of this success, we floor—25 percent were pleased to announce that the more than was Institution would, for the first time ever, previously accessible be able to provide some endowed to Alvin. salary support to Assistant Scientists in An international their second and third years, beginning research highlight of in 1995. Although the start is small (one 1994 was a very month’s support) it clearly marks a productive coopera- different way of doing research at WHOI tive project with the and is a major step toward a permanent Japan Marine Science underpinning for scientific innovation and Technology and flexibility. This is what the cam- Center (JAMSTEC), paign is primarily about: providing Tom Kleindinst Tom 2 Woods Hole Oceanographic Institution Director’s Comments Tom Kleindinst Tom More than 1,200 WHOI people visited R/V Yokosuka during the ship’s July visit to Woods Hole. resources to our researchers so that they Developing a trusting and respectful and strength as well as unique individu- can devote more time to creativity and relationship with the new leaders will alism. All will be called upon more and innovative ideas. We continue working require careful planning; it is our biggest more as we optimize the challenges and very hard to complete or exceed the task for the year ahead. We must opportunities ahead and progress, with campaign goal in the next two years, formulate a Washington, DC, strategy as clear vision, towards our goals. securing the kind of support that is well as guidelines for internal decisions Robert B. Gagosian critical for the continuing excellence of aimed toward continuing excellence in Director the Institution. a cost-competitive manner. We must Changes in the National Science develop an Institution goal-setting Foundation (NSF) and the Office of process that includes, perhaps for the Naval Research (ONR), our two major first time in recent history, specific federal research sponsors, are directly implementation plans related to the urgency of raising private to ensure that the funds for the advancement of ocean goals are met. This science research. With increased will be a complex national proposal competition, the exercise, one which demand for cost competitiveness, and will involve new roles federal emphasis on “vertical integra- for scientific staff, tion” at ONR and “relevance” at NSF, we senior management, must ensure that we are knowledgeable and others so that an about the needs of the country and integrated and articulate about how our research formidable presence applies to those needs. As Director, I in both the scientific will continue to conduct straightforward and political arenas dialogue with federal agency leaders to can be secured for ensure that our research and scientific the future. resources are well known and stay With the benefit of highly placed in the national agenda’s 1994’s challenges and priority list. accomplishments, we In addition to altered climates at NSF at the Woods Hole and ONR, the new Congress’s commit- Oceanographic tee overhauls and the Contract with Institution look America’s initial recommendations also forward to opportu- present changes and challenges. It is nity and change that imperative that we effectively communi- will enhance our cate the value and importance of ocean mission and establish science to the country and the world. our firm footing in Only through dialogue with the new national and inter- leaders can we hope to ensure that national agendas. Kleindinst Tom useful information gets to policy makers This Institution has A cheering crowd welcomes R/V Knorr home from a summer and influences their decisions. tremendous vitality research voyage. 3 1994 Annual Report Applied Ocean Physics & Engineering Ken Prada displays the “PC in a Can,” which brings the computer power of a desktop computer to a variety of oceanographic instruments. Tom Kleindinst Tom “PC in a Can” Supports The Applied Ocean Physics and Design and Engineering Award for their Extensive Computing Engineering (AOP&E) Department, with work on ABE. W. Kenneth Stewart 145 staff members and 36 graduate received a Certificate of Recognition as In Ocean Instruments students, had a very productive year in part of the Computerworld Smithsonian Modern scientific needs require ever 1994. Forty-two principal investigators Awards for his contributions to real-time more capable tools for gathering led 130 basic and applied research visualization of oceanographic data. information. Most oceanographic projects in ocean acoustics, coastal and Robert Ballard received honorary degrees ocean fluid dynamics, ocean systems
Load more

Recommended publications
  • THE PLANETARY REPORT FAREWELL, SEPTEMBER EQUINOX 2017 VOLUME 37, NUMBER 3 CASSINI Planetary.Org CELEBRATING a LEGACY of DISCOVERIES
    THE PLANETARY REPORT FAREWELL, SEPTEMBER EQUINOX 2017 VOLUME 37, NUMBER 3 CASSINI planetary.org CELEBRATING A LEGACY OF DISCOVERIES ATMOSPHERIC CHANGES C DYNAMIC RINGS C COMPLICATED TITAN C ACTIVE ENCELADUS ABOUT THIS ISSUE LINDA J. SPILKER is Cassini project scientist at the Jet Propulsion Laboratory. IN 2004, Cassini, the most distant planetary seafloor. As a bonus, it has revealed jets of orbiter ever launched by humanity, arrived at water vapor and ice particles shooting out of Saturn. For 13 years, through its primary and fractures at the moon’s south pole. two extended missions, this spacecraft has These discoveries have fundamentally been making astonishing discoveries, reshap- altered many of our concepts of where life ing and changing our understanding of this may be found in our solar system. Cassini’s unique planetary system within our larger observations at Enceladus and Titan have made system of unique worlds. A few months ater exploring these ocean worlds a major focus for arrival, Cassini released Huygens, European planetary science. New insights from these dis- Space Agency’s parachuted probe built to coveries also have implications for potentially study the atmosphere and surface of Titan habitable worlds beyond our solar system. and image its surface for the very first time. In this special issue of The Planetary Report, a handful of Cassini scientists share some results from their studies of Saturn and its moons. Because there’s no way to fit every- thing into this slim volume, they’ve focused on a few highlights. Meanwhile, Cassini continues performing its Grand Finale orbits between the rings and the top of Saturn’s atmosphere, circling the planet once every 6.5 days.
    [Show full text]
  • Chang'e 5 Samples (Mexag) (Head-Final)
    Chang’E 5 Lunar Sample Return Mission Update James w. Head Department of Earth, Environmental and Planetary Sciences Brown University Providence, RI 02912 USA Extraterrestrial Materials Analysis Group (ExMAG) Spring Meeting: April 7 - 8, 2021. Extraterrestrial Materials Analysis Group (ExMAG) Spring Meeting Barbara Cohen, ExMAG Chair. 2/10/21 • 1. Please provide an update on the Chang'e 5 Sample Return Mission. • 2. What is known of the collection so far? • 3. Please provide an overview of allocation procedures. • 4. Since US federally-funded researchers cannot work directly with China - Who outside of China is working with the mission team? • 5. We'd also appreciate your thoughts on: What NASA might be able to do to enable the US analysis community to collaborate on this sample collection? Extraterrestrial Materials Analysis Group (ExMAG) Spring Meeting Barbara Cohen, ExMAG Chair. 2/10/21 • 1. Some Myths and Realities. • 2. Organization of the Chinese Space Program. • 3. Chinese Lunar Exploration Program (CLEP) context for Chang’e 5. • 4. Chang’e 5 Landing Site Selection, Global Context, Key Questions, Mission Operations and Sample Return. • 5. Returned Sample Location, Storage, Preliminary Analysis and Distribution. • 6. Opportunities for International Cooperation. Extraterrestrial Materials Analysis Group (ExMAG) Spring Meeting Barbara Cohen, ExMAG Chair. 2/10/21 • 1. Some Myths and Realities. • 2. Organization of the Chinese Space Program. • 3. Chinese Lunar Exploration Program (CLEP) context for Chang’e 5. • 4. Chang’e 5 Landing Site Selection, Global Context, Key Questions, Mission Operations and Sample Return. • 5. Returned Sample Location, Storage, Preliminary Analysis and Distribution. • 6. Opportunities for International Cooperation.
    [Show full text]
  • Cubex: a Compact X-Ray Telescope Enables Both X-Ray Fluorescence Imaging Spectroscopy and Pulsar Timing Based Navigation
    SSC18-V-05 CubeX: A compact X-Ray Telescope Enables both X-Ray Fluorescence Imaging Spectroscopy and Pulsar Timing Based Navigation Jan Stupl, Monica Ebert, David Mauro SGT / NASA Ames NASA Ames Research Center, Moffett Field, CA; 650-604-4032 [email protected] JaeSub Hong Harvard University Cambridge, MA Suzanne Romaine, Almus Kenter, Janet Evans, Ralph Kraft Smithsonian Astrophysical Observatory Cambridge, MA Larry Nittler Carnegie Institution of Washington Washington, DC Ian Crawford Birkbeck College London, UK David Kring Lunar and Planetary Institute Houston, TX Noah Petro, Keith. Gendreau, Jason Mitchell, Luke Winternitz NASA Goddard Space Flight Center Greenbelt, MD Rebecca. Masterson, Gregory Prigozhin Massachusetts Institute of Technology Cambridge, MA Brittany Wickizer NASA Ames Research Center Moffett Field, CA Kellen Bonner, Ashley Clark, Arwen Dave, Andres Dono-Perez, Ali Kashani, Daniel Larrabee, Samuel Montez, Karolyn Ronzano, Tim Snyder MEI / NASA Ames Research Center Joel Mueting, Laura Plice Metis / NASA Ames Research Center NASA Ames Research Center, Moffett Field, CA Yueh-Liang Shen, Duy Nguyen Booz Allen Hamilton / NASA Ames NASA Ames Research Center, Moffett Field, CA Stupl 1 32nd Annual AIAA/USU Conference on Small Satellites ABSTRACT This paper describes the miniaturized X-ray telescope payload, CubeX, in the context of a lunar mission. The first part describes the payload in detail, the second part summarizes a small satellite mission concept that utilizes its compact form factor and performance. This instrument can be used for both X-ray fluorescence (XRF) imaging spectroscopy and X-ray pulsar timing-based navigation (XNAV). It combines high angular resolution (<1 arcminutes) Miniature Wolter-I X-ray optics (MiXO) with a common focal plane consisting of high spectral resolution (<150 eV at 1 keV) CMOS X-ray sensors and a high timing resolution (< 1 µsec) SDD X-ray sensor.
    [Show full text]
  • OCEANUS (Organisms and Compounds of Europa – an Analysis Under the Surface) – Concept Mission De- Sign
    49th Lunar and Planetary Science Conference 2018 (LPI Contrib. No. 2083) 1871.pdf OCEANUS (Organisms and Compounds of Europa – an Analysis Under the Surface) – Concept Mission De- sign. M.V. Heemskerk1, G. de Zeeuw1, W. van Westrenen1, B. H. Foing1,2. 1VU University Amsterdam, de Boelelaan 1105, 1081 HZ Amsterdam, The Netherlands, ([email protected], [email protected], [email protected]) 2ESA ESTEC, Keplerlaan 1, 2201 AZ Noordwijk, The Netherlands ([email protected]) Introduction: 1. Buildup of the ice crust and its ocean; Un- In 2022, ESA (European Space Agency) will launch derstanding how recent and/or current tidal an orbiter – JUICE (JUpiter ICy moon Explorer) – and geological processes are formed. which will collect atmospheric data of Jupiter and 2. Chemical composition; Characterizing the three of its Galilean moons; Ganymede, Europa and properties of the ocean and its crust to de- Callisto [1]. As this is but an orbiter, further explora- scry the origin of organic compounds. tion of the (sub)surface remains out of reach. As of 3. Geomorphology; Understanding the for- today, the most suitable prospect for the occurrence of extra-terrestrial life forms appears to be Europa. mation of surface features Europa contains liquid water [2], simple organic B. Model Instrument Payload: The lander payload compounds [3], a subsurface power source [4] and a consists of two high-definition reconnaissance camer- lot of ice. Convection and tidal flexure could also as, a magnetometer, an altimeter, a short-wave infra- give way to a possible zone for the emergence of life, red spectrometer, a gamma and X-ray detector, a ra- for the bottom of this subsurface ocean may house diation shielding, the ESS, and the ECMD.
    [Show full text]
  • Mars= Oceanus Borealis, Ancient Glaciers, and the Megaoutflo Hypothesis
    Lunar and Planetary Science XXXI 1863.pdf MARS= OCEANUS BOREALIS, ANCIENT GLACIERS, AND THE MEGAOUTFLO HYPOTHESIS. V.R. Baker1, 2, R.G. Strom2, J.M. Dohm1, V.C. Gulick3, J.S. Kargel4, G. Komatsu5, G.G. Ori5, and J.W. Rice, Jr.2; 1Dept. Of Hydrology and Water Res., Univ. of Arizona, Tucson, AZ 85721-0011, 2Lunar and Planetary Laboratory, Univ. of Arizona, Tucson, AZ 85721-0092, 3NASA-Ames Research Center, MS 245-3, Moffett Field, CA 94035, 4U.S. Geological Survey, 2255 N. Gemini Drive, Flagstaff, AZ 86001; 5Dipartimento di Scienze, Universitad d=Annunzio, Viale Pindaro 42, 65127 Pescara, Italy. ([email protected]) Introduction: Recent results from the Mars Orbiter (~108+ years), during which the Mars surface had ex- Laser Altimeter (MOLA) instrument of Mars Global tremely cold, dry conditions similar to those prevailing Surveyor [1, 2] corroborate the existence of a vast today, terminated by short-duration (~104 to 105 years) ocean on the northern plains of Mars. Named Oceanus episodes of much warmer, wetter conditions associated Borealis [3], this great ponding of water, documented with a transient greenhouse climate. These quasi-stable by several investigators over the past 15 years [4, 5, 6, episodes resulted in glaciation [21, 22] and valley net- 7, 8], formed and reformed episodically during later work formation [8, 23] late in Martian history, coinci- Mars history, after cessation of the late heavy bom- dent with the great outflow channel discharges that bardment [3]. Among the many geological indicators formed Oceanus Borealis. The processes are cyclic of this ocean, several interpreted shoreline features [7, with the long epochs of cold-dry conditions alternating 9] are disputed by one study of a small number of Mars with very short episodes of cool-wet conditions associ- Orbiter Camera (MOC) images [10].
    [Show full text]
  • 2015 October
    TTSIQ #13 page 1 OCTOBER 2015 www.nasa.gov/press-release/nasa-confirms-evidence-that-liquid-water-flows-on-today-s-mars Flash! Sept. 28, 2015: www.space.com/30674-flowing-water-on-mars-discovery-pictures.html www.space.com/30673-water-flows-on-mars-discovery.html - “boosting odds for life!” These dark, narrow, 100 meter~yards long streaks called “recurring slope lineae” flowing downhill on Mars are inferred to have been formed by contemporary flowing water www.space.com/30683-mars-liquid-water-astronaut-exploration.html INDEX 2 Co-sponsoring Organizations NEWS SECTION pp. 3-56 3-13 Earth Orbit and Mission to Planet Earth 13-14 Space Tourism 15-20 Cislunar Space and the Moon 20-28 Mars 29-33 Asteroids & Comets 34-47 Other Planets & their moons 48-56 Starbound ARTICLES & ESSAY SECTION pp 56-84 56 Replace "Pluto the Dwarf Planet" with "Pluto-Charon Binary Planet" 61 Kepler Shipyards: an Innovative force that could reshape the future 64 Moon Fans + Mars Fans => Collaboration on Joint Project Areas 65 Editor’s List of Needed Science Missions 66 Skyfields 68 Alan Bean: from “Moonwalker” to Artist 69 Economic Assessment and Systems Analysis of an Evolvable Lunar Architecture that Leverages Commercial Space Capabilities and Public-Private-Partnerships 71 An Evolved Commercialized International Space Station 74 Remembrance of Dr. APJ Abdul Kalam 75 The Problem of Rational Investment of Capital in Sustainable Futures on Earth and in Space 75 Recommendations to Overcome Non-Technical Challenges to Cleaning Up Orbital Debris STUDENTS & TEACHERS pp 85-96 Past TTSIQ issues are online at: www.moonsociety.org/international/ttsiq/ and at: www.nss.org/tothestarsOO TTSIQ #13 page 2 OCTOBER 2015 TTSIQ Sponsor Organizations 1.
    [Show full text]
  • 03-074 Oceanus DOEI 8 12.Indd
    http://oceanusmag.whoi.edu/v42n2/sohn.html Unique Vehicles for a Unique Environment New autonomous robots will pierce an ice-covered ocean and explore the Arctic abyss By Robert Reves-Sohn, Associate Scientist, Geology and Geophysics Department, Woods Hole Oceanographic Institution magine you have inherited a magnificent medieval cas- Itle. You wander its corridors, climbing spiral staircases to hidden towers, delving purposefully into subterranean caverns, and delighting in the details of its architecture, history, and artistic treasures. Over time you come to realize there is a great North Wing Puma and Jaguar are autonomous that has long been sealed off from the rest of the castle. underwater vehicles (AUVs) designed You’ve found old documents in the library describ- to overcome the technical challenges ing construction of the North Wing, and it appears as that now preclude under-ice operations though it was built using rare materials that are not in the Arctic Ocean. They will home in found anywhere else in the castle. As best as you can to an acoustic beacon and latch onto a tell the castle’s main thermostat is inside the North Puma wire suspended from a hole in the ice. Wing, which adds some urgency because lately Puma has sonars and sensors to search the castle seems to be getting inexplicably wide areas and detect temperature, warmer. And, perhaps most intriguing, chemical, or turbidity signals from recent evidence suggests that some- hydrothermal vent plumes (the green thing—perhaps even something lasers detect particulates in the water). unusual—might actually be Puma can track the plume back to its living in there.
    [Show full text]
  • 2018 Workshop on Autonomy for Future NASA Science Missions
    NOTE: This document was prepared by a team that participated in the 2018 Workshop on Autonomy for Future NASA Science Missions. It is for informational purposes to inform discussions regarding the use of autonomy in notional science missions and does not specify Agency plans or directives. 2018 Workshop on Autonomy for Future NASA Science Missions: Output and Results Table of Contents Introduction .................................................................................................................................... 2 Summary: Post-Workshop Findings ................................................................................................ 3 The Astrophysics Design Reference Mission Report ...................................................................... 5 The Earth Design Reference Mission Report ................................................................................ 16 The Heliophysics Design Reference Mission Report ..................................................................... 30 The Mars Design Reference Mission Report ................................................................................ 43 The Moon Design Reference Missions Report ............................................................................. 57 The Ocean Worlds Design Reference Mission Report .................................................................. 74 Small Bodies Design Reference Mission Report ........................................................................... 91 Venus Design Reference Mission Report
    [Show full text]
  • OSIRIS-Rex Goes Asteroid Collecting
    OSIRIS-REx Goes Asteroid Collecting — Scott Messenger, NASA Johnson Space Center OSIRIS-REx is NASA’s third New Frontiers mission, following the New Horizons mission, which completed a flyby of Pluto in 2015, and the Juno mission to orbit Jupiter, which has just begun science operations. The OSIRIS-REx mission’s primary objective is to collect pristine surface samples of a carbonaceous asteroid and return them to Earth for analysis. Carbonaceous asteroids and comets are considered to be L “primitive” bodies that have preserved remnants of the solar system starting materials. By studying them, scientists can learn about the origin and earliest evolution of the solar system. The OSIRIS-REx spacecraft was launched on September 8, 2016, beginning its two- year journey to asteroid 101955 Bennu (formerly designated 1999 RQ36). After more than one year of detailed remote observations, OSIRIS-REx will obtain surface samples and return them to Earth in September 2023. The OSIRIS-REx proposal, led by the late Dr. Michael J. Drake, was selected during the 2011 New Frontiers competition, and is now led by Dr. Dante Lauretta of the University of Arizona. The Pmission name OSIRIS-REx (an acronym for Origins, Spectral Interpretation, Resource Identification, Security, Regolith Explorer) embodies five objectives: (1) Origins: Return and analyze a sample of a carbonaceous asteroid; (2) Spectral Interpretation: Provide ground truth for remote observations of asteroids; (3) Resource Identification: Determine the mineral and chemical makeup of a near-Earth asteroid; (4) Security: Directly measure the non-gravitational force known as the Yarkovsky effect, which changes asteroidal orbits through its Iinteraction with sunlight; and (5) Regolith Explorer: Determine the properties of unconsolidated material that covers the asteroid surface.
    [Show full text]
  • 98-031 Oceanus F/W 97 Final
    A hotspot created the island of Iceland and its characteristic volcanic landscape. Hitting the Hotspots Hotspots are rela- tively small regions on the earth where New Studies Reveal Critical Interactions unusually hot rocks rise from deep inside Between Hotspots and Mid-Ocean Ridges the mantle layer. Jian Lin Associate Scientist, Geology & Geophysics Department he great volcanic mid-ocean ridge system hotspots may play a critical role in shaping the stretches continuously around the globe for seafloor—acting in some cases as strategically T 60,000 kilometers, nearly all of it hidden positioned supply stations that fuel the lengthy beneath the world’s oceans. In some places, how- mid-ocean ridges with magma. ever, mid-ocean ridge volcanoes are so massive that Studies of ridge-hotspot interactions received a they emerge above sea level to create some of the major boost in 1995 when the US Navy declassified most spectacular islands on our planet. Iceland, the gravity data from its Geosat satellite, which flew Azores, and the Galápagos are examples of these from 1985 to 1990. The satellite recorded in unprec- “hotspot” islands—so named because they are edented detail the height of the ocean surface. With believed to form above small regions scattered accuracy within 5 centimeters, it revealed small around the earth where unusually hot rocks rise bumps and dips created by the gravitational pull of from deep inside the mantle layer. dense underwater mountains and valleys. Research- But hotspots may not be such isolated phenom- ers often use precise gravity measurements to probe ena. Exciting advances in satellite oceanography, unseen materials below the ocean floor.
    [Show full text]
  • Strategic Investments in Instrumentation and Facilities for Extraterrestrial Sample Curation and Analysis
    PREPUBLICATION COPY—SUBJECT TO FURTHER EDITORIAL CORRECTION Strategic Investments in Instrumentation and Facilities for Extraterrestrial Sample Curation and Analysis ADVANCE COPY NOT FOR PUBLIC RELEASE BEFORE Thursday, December 20, 2018 at 11:00 a.m. ___________________________________________________________________________________ PLEASE CITE AS A REPORT OF THE NATIONAL ACADEMIES OF SCIENCES, ENGINEERING, AND MEDICINE Committee on Extraterrestrial Sample Analysis Facilities Space Studies Board Division on Engineering and Physical Sciences A Consensus Study Report of PREPUBLICATION COPY—SUBJECT TO FURTHER EDITORIAL CORRECTION THE NATIONAL ACADEMIES PRESS 500 Fifth Street, NW Washington, DC 20001 This activity was supported by Grant/Contract No. XXXX with XXXXX. Any opinions, findings, conclusions, or recommendations expressed in this publication do not necessarily reflect the views of any organization or agency that provided support for the project. International Standard Book Number-13: 978-0-309-XXXXX-X International Standard Book Number-10: 0-309-XXXXX-X Digital Object Identifier: https://doi.org/10.17226/25312 Additional copies of this publication are available for sale from the National Academies Press, 500 Fifth Street, NW, Keck 360, Washington, DC 20001; (800) 624-6242 or (202) 334-3313; http://www.nap.edu. Copyright 2018 by the National Academy of Sciences. All rights reserved. Printed in the United States of America Suggested citation: National Academies of Sciences, Engineering, and Medicine. 2018. Strategic Investments in Instrumentation and Facilities for Extraterrestrial Sample Curation and Analysis. Washington, DC: The National Academies Press. https://doi.org/10.17226/25312. PREPUBLICATION COPY—SUBJECT TO FURTHER EDITORIAL CORRECTION The National Academy of Sciences was established in 1863 by an Act of Congress, signed by President Lincoln, as a private, nongovernmental institution to advise the nation on issues related to science and technology.
    [Show full text]
  • Impact Excitation of a Seismic Pulse and Vibrational Normal Modes on Asteroid Bennu and Associated Slumping of Regolith
    Impact Excitation of a Seismic Pulse and Vibrational Normal Modes on Asteroid Bennu and Associated Slumping of Regolith Alice C. Quillena,1,∗, Yuhui Zhaob, YuanYuan Chenb, Paul Sánchezc, Randal C. Nelsond, Stephen R. Schwartze;f aDepartment of Physics and Astronomy, University of Rochester, Rochester, NY 14627, USA bKey Laboratory of Planetary Sciences, Purple Mountain Observatory, Chinese Academy of Sciences, Nanjing 210008, China cColorado Center for Astrodynamics Research, The University of Colorado Boulder, UCB 431, Boulder, CO 80309-0431, United States dDepartment of Computer Science, University of Rochester, Rochester, NY 14627, USA eLunar and Planetary Laboratory, University of Arizona, Tucson, AZ, USA fLaboratoire Lagrange, Université Côte d’Azur, Observatoire de la Côte d’Azur, CNRS, C.S. 34229, 06304 Nice Cedex 4, France Abstract We consider an impact on an asteroid that is energetic enough to cause resurfacing by seismic reverberation and just below the catastrophic disrup- tion threshold, assuming that seismic waves are not rapidly attenuated. In asteroids with diameter less than 1 km we identify a regime where rare en- ergetic impactors can excite seismic waves with frequencies near those of the asteroid’s slowest normal modes. In this regime, the distribution of seismic reverberation is not evenly distributed across the body surface. With mass- spring model elastic simulations, we model impact excitation of seismic waves with a force pulse exerted on the surface and using three different asteroid shape models. The simulations exhibit antipodal focusing and normal mode excitation. If the impulse excited vibrational energy is long lasting, vibrations arXiv:1804.02058v2 [astro-ph.EP] 23 Sep 2018 are highest at impact point, its antipode and at high surface elevations such as an equatorial ridge.
    [Show full text]