DOCSLIB.ORG

The Comet Astrobiology Exploration Sample Return (CAESAR)

Total Page：16

File Type：pdf, Size：1020Kb

Download full-text PDF Read full-text
The Comet Astrobiology Exploration Sample Return (CAESAR) Project Overview Michael Amato NASA GSFC CAESAR Project and GSFC, Cornell, and other partner proprietary and copyright Information CAESAR The CAESAR (Comet Astrobiology Exploration SAmple Return) mission is one of two New Frontiers missions selected for Phase A. CAESAR will acquire a sample from the nucleus of comet Churyumov-Gerasimenko, returning it safely to Earth. Comets are made up of materials from ancient stars, interstellar clouds, and the birth of our solar system. The CAESAR sample will reveal how these materials contributed to the early Earth, including the origins of the Earth's oceans, and of life The CAESAR mission seeks to return this sample from 67P/Churyumov-Gerasimenko, a comet that was successfully explored by the European Space Agency’s Rosetta spacecraft, to determine its origin and history. • PI Steve Squyres of Cornell University • CAESAR would be managed by NASA’s Goddard Space Flight Center CAESAR Project and GSFC, Cornell, and other partner proprietary and copyright Information CAESAR Sample Science CAESAR Project and GSFC, Cornell, and other partner proprietary and copyright Information Churyumov-Gerasimenko CAESAR Project and GSFC, Cornell, and other partner proprietary and copyright Information The CAESAR Spacecraft GSFC Restore-L EDU arm NEXT-C Ion Thruster CAESAR Project and GSFC, Cornell, and other partner proprietary and copyright Information Mission Timeline 2024 2026 2028 2030 2032 2034 2036 2038 Comet Ops SEP Cruise to 67P SEP Return to Earth Launch August 2024 Launch Arrive at Comet March 2029 Depart Comet November 2033 Earth Return November 2038 CAESAR Project and GSFC, Cornell, and other partner proprietary and copyright Information CAESAR Trajectory Outbound Inbound Launch 8/15/24 Earth Return 67P Arrival 67P Departure 11/20/38 Earth Flyby 3/26/29 11/6/33 Earth Flyby 11/26/25 11/23/37 CAESAR Project and GSFC, Cornell, and other partner proprietary and copyright Information CAESAR Mission Operations Phases Initial Survey Detailed Survey Light Touch Operations CAESAR Project and GSFC, Cornell, and other partner proprietary and copyright Information CAESAR Preliminary Touch Site Selection CAESAR Project and GSFC, Cornell, and other partner proprietary and copyright Information CAESAR Sample Touch Operations Slew to TAG Attitude Traj. Interface Point Altitude TIP, CP, and MP Δv’s 300m updated based on current nav state Checkpoint 150m Range coridor monitored by LRF after TIP Matchpoint 50m Onboard navigation solution running continuously based on image data (1 image/minute, TBD) 0m 10 km De-Orbit Maneuver TAG Timeline T–5 hrs T–30 mins T–20 mins T–10 mins T–0 mins Δt=4.5 hrs Δt=10 mins Δt=10 mins Δt=10 mins DOI TIP CP MP TAG CAESAR Project and GSFC, Cornell, and other partner proprietary and copyright Information CAESAR Sample Acquisition System CAESAR Project and GSFC, Cornell, and other partner proprietary and copyright Information CAESAR Sample Containment System CAESAR CAESAR Project and GSFC, Cornell, and other partner proprietary and copyright Information CAESAR Gas Containment System GSFC CAESAR Project and GSFC, Cornell, and other partner proprietary and copyright Information CAESAR Sample Return Capsule Stowed Sample Container CAESAR Project and GSFC, Cornell, and other partner proprietary and copyright Information CAESAR Sample Return Capsule CAESAR Project and GSFC, Cornell, and other partner proprietary and copyright Information CAESAR Sample Touch Operations CAESAR Project and GSFC, Cornell, and other partner proprietary and copyright Information BACK Up CAESAR Project and GSFC, Cornell, and other partner proprietary and copyright Information SRC Recovery CAESAR Project and GSFC, Cornell, and other partner proprietary and copyright Information .
Load more

Recommended publications
  • From Hayabusa to Hayabusa2: Present Status and Plans for Sample Curations of Asteroidal Sample Return Missions by Jaxa
    81st Annual Meeting of The Meteoritical Society 2018 (LPI Contrib. No. 2067) 6117.pdf FROM HAYABUSA TO HAYABUSA2: PRESENT STATUS AND PLANS FOR SAMPLE CURATIONS OF ASTEROIDAL SAMPLE RETURN MISSIONS BY JAXA. T. Yada1, K. Sakamoto1, M. Yoshitake1, K. Kumagai2, M. Nishimura2, Y. Nakano1, S. Furuya1, M. Abe1, T. Okada1, S. Tachibana3, H. Yurimoto1,4, and M. Fujimoto1,5, 1Astromat. Sci. Res. Group, Inst. Space Astronaut. Sci., Japan Aerosp. Explor. Agnecy, 3-1-1 Yoshinodai, Chuo, Sagamihara, Kanagawa 252-5210, Japan ([email protected]), 2 Marine Works Japan Ltd., 3-54-1 Oppamahigashi, Yokosuka 237-0063 Japan, 3Dept. Earth Planet. Sci., Grad. Sch. Science, Univ. Tokyo, 7-3-1 Hongo, Bunkyo, Tokyo 113-0033, Japan, 4Dept. Earth Science, Grad. Sch. Science, Hokkaido Univ., Kita 8, Nishi 5, Kita, Sapporo, Hokkaido 060-0808, Japan, 5Earth-Life Sci. Inst., Tokyo Inst. Tech., 2-12-1-1E-1 Ookayama, Meguro, Tokyo 152-8550, Japan. Introduction: The new era of sample return missions had started since the Stardust returned samples from com- et 81P/Wild 2 in 2006 [1], followed by the Hayabusa spacecraft from the near-Earth S-type asteroid 25143 Itokawa in 2010 [2,3]. In this year, Hayabusa2 will reach its target body, the near-Earth C-type asteroid 162173 Ryugu [4], and also OSIRIS-REx toward the near-Earth B-type asteroid 101955 Bennu [5]. Additionally, several other sample return missions have been planned recently, such as the Martian Moons eXplorer (MMX) for the Phobos and/or Deimos [6], the CAESAR for 67P/Churyumov-Gerasimenko [7], and the HELACLES for the the Moon [8].
    [Show full text]
  • Planetary Science Update
    Planetary Science Division Status Report Jim Green NASA, Planetary Science Division October 11, 2017 Presentation at LEAG Planetary Science Missions Events 2016 March – Launch of ESA’s ExoMars Trace Gas Orbiter July 4 – Juno inserted in Jupiter orbit * Completed September 8 – Launch of Asteroid mission OSIRIS – REx to asteroid Bennu September 30 – Landing Rosetta on comet CG October 19 – ExoMars EDM landing and TGO orbit insertion 2017 January 4 – Discovery Mission selection announced February 9-20 - OSIRIS-REx began Earth-Trojan search April 22 – Cassini begins plane change maneuver for the “Grand Finale” August 22 – Solar Eclipse across America September 15 – Cassini end of mission at Saturn September 22 – OSIRIS-REx Earth flyby October 28 – International Observe the Moon night (1st quarter) 2018 May 5 - Launch InSight mission to Mars August – OSIRIS-REx arrival at Bennu October – Launch of ESA’s BepiColombo to Mercury November 26 – InSight landing on Mars 2019 January 1 – New Horizons flyby of Kuiper Belt object 2014MU69 Formulation Implementation Primary Ops BepiColombo Lunar Extended Ops (ESA) Reconnaissance Orbiter Lucy New Horizons Psyche Juno Dawn JUICE (ESA) ExoMars 2016 MMX MAVEN MRO (ESA) (JAXA) Mars Express Mars (ESA) Odyssey OSIRIS-REx ExoMars 2020 (ESA) Mars Rover Opportunity Curiosity InSight 2020 Rover Rover NEOWISE Europa Clipper Discovery Program Discovery Program NEO characteristics: Mars evolution: Lunar formation: Nature of dust/coma: Solar wind sampling: NEAR (1996-1999) Mars Pathfinder (1996-1997) Lunar Prospector
    [Show full text]
  • The Magellan Spacecraft at Venus by Andrew Fraknoi, Astronomical Society of the Pacific
    www.astrosociety.org/uitc No. 18 - Fall 1991 © 1991, Astronomical Society of the Pacific, 390 Ashton Avenue, San Francisco, CA 94112. The Magellan Spacecraft at Venus by Andrew Fraknoi, Astronomical Society of the Pacific "Having finally penetrated below the clouds of Venus, we find its surface to be naked [not hidden], revealing the history of hundreds of millions of years of geological activity. Venus is a geologist's dream planet.'' —Astronomer David Morrison This fall, the brightest star-like object you can see in the eastern skies before dawn isn't a star at all — it's Venus, the second closest planet to the Sun. Because Venus is so similar in diameter and mass to our world, and also has a gaseous atmosphere, it has been called the Earth's "sister planet''. Many years ago, scientists expected its surface, which is perpetually hidden beneath a thick cloud layer, to look like Earth's as well. Earlier this century, some people even imagined that Venus was a hot, humid, swampy world populated by prehistoric creatures! But we now know Venus is very, very different. New radar images of Venus, just returned from NASA's Magellan spacecraft orbiting the planet, have provided astronomers the clearest view ever of its surface, revealing unique geological features, meteor impact craters, and evidence of volcanic eruptions different from any others found in the solar system. This issue of The Universe in the Classroom is devoted to what Magellan is teaching us today about our nearest neighbor, Venus. Where is Venus, and what is it like? Spacecraft exploration of Venus's surface Magellan — a "recycled'' spacecraft How does Magellan take pictures through the clouds? What has Magellan revealed about Venus? How does Venus' surface compare with Earth's? What is the next step in Magellan's mission? If Venus is such an uninviting place, why are we interested in it? Reading List Why is it so hot on Venus? Where is Venus, and what is it like? Venus orbits the Sun in a nearly circular path between Mercury and the Earth, about 3/4 as far from our star as the Earth is.
    [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]
  • Scientific Goals for Exploration of the Outer Solar System
    Scientific Goals for Exploration of the Outer Solar System Explore Outer Planet Systems and Ocean Worlds OPAG Report v. 28 August 2019 This is a living document and new revisions will be posted with the appropriate date stamp. Outline August 2019 Letter of Response to Dr. Glaze Request for Pre Decadal Big Questions............i, ii EXECUTIVE SUMMARY ......................................................................................................... 3 1.0 INTRODUCTION ................................................................................................................ 4 1.1 The Outer Solar System in Vision and Voyages ................................................................ 5 1.2 New Emphasis since the Decadal Survey: Exploring Ocean Worlds .................................. 8 2.0 GIANT PLANETS ............................................................................................................... 9 2.1 Jupiter and Saturn ........................................................................................................... 11 2.2 Uranus and Neptune ……………………………………………………………………… 15 3.0 GIANT PLANET MAGNETOSPHERES ........................................................................... 18 4.0 GIANT PLANET RING SYSTEMS ................................................................................... 22 5.0 GIANT PLANETS’ MOONS ............................................................................................. 25 5.1 Pristine/Primitive (Less Evolved?) Satellites’ Objectives ...............................................
    [Show full text]
  • Samuel Patrick Dennis Birch Email: [email protected] Current Address: Webpage: 426 Space Sciences Bldg
    Samuel Patrick Dennis Birch Email: [email protected] Current Address: Webpage: https://geomorph-sbirch.com 426 Space Sciences Bldg. Phone: 510-712-0270 Ithaca, NY 14853-6801 PROFESSIONAL HIGHLIGHTS Published 8 first author papers, co-authored 17 more. NESSF Fellow (2015). 51 Pegasi b Fellow (2020). Cassini RADAR Associate Team Member. Rosetta OSIRIS Graduate Student Collaborator. CAESAR Co-Investigator. AGU Planetary Sciences Section Early Career Representative (2019-2021). Advisor for 14 graduate, undergraduate and high school students (6 presently). CURRENT AFFILIATION Cornell Center for Astrophysics and Planetary Science, Cornell University EDUCATION - Ph.D. – Cornell University, Ithaca NY May 2018 - Concentration: Planetary Science (Minors: Geophysics/Astronomy) - B.A. (High Honors) – University of California Berkeley, Berkeley, CA May 2014 - Concentration: Geophysics ACADEMIC AWARDS AND FELLOWSHIPS - Heising-Simons Foundation 51 Pegasi b Postdoctoral Fellowship 2020 - Department of Earth and Atmospheric Sciences Excellence in Research Award 2018 - NASA Earth and Space Science Fellowship 2015 - Berkeley Distinguished Honors in Geophysics 2014 - Berkeley International Undergraduate Student Tuition Grant 2013 PROFESSIONAL APPOINTMENTS - Massachusetts Institute of Technology – 51 Pegasi b Postdoctoral Fellow 2020 – 2023 - Cornell University – Research Associate 2018 – 2020 - Cornell University – Ph.D. Student 2014 – 2018 - Cornell University – REU Summer Intern 2013 - University of California Berkeley – Geological Fluid Dynamics Lab Manager 2013 – 2014 CURRENT RESEARCH INTERESTS - Titan Geomorphology & Surface Processes - Cometary (and Small Body) Geology & Surface Processes - Numerical Landscape Evolution Modeling - Sublimation Erosion & Surface Processes in the Outer Solar System JOURNAL PUBLICATIONS (*Indicates paper was led by a student advisee) h-index: 11 i10-index: 12 Citations: 261 Researcher ID: L-1249-2017 [25] S.P.D.
    [Show full text]
  • Aerospace-America-June-2019.Pdf
    Q&A 10 URBAN AIR MOBILITY 14 NASA’S NEW FRONTIERS 28 NASA’s Bridenstine on lunar planning Coping with complexity Next probe goes to Titan or to comet In 1921, an Army pilot dropped insecticide on crops, starting a dashing new profession that might or might not survive the age of drones. PAGE 20 TOMORROW’s Crop dustERS JUNE 2019 | A publication of the American Institute of Aeronautics and Astronautics | aerospaceamerica.aiaa.org NEWAWARDS$500K UP TO ,1129$7( 75$16)250285)8785( R&D FUNDING PROGRAM 7KH1DWLRQDO5HFRQQDLVVDQFH2IÀFH'LUHFWRU·V,QQRYDWLRQ,QLWLDWLYH ',, 3URJUDPIXQGVFXWWLQJHGJHVFLHQWLÀFUHVHDUFKLQDKLJKULVNKLJKSD\RII environment to discover innovative concepts and creative ideas that transform RYHUKHDGLQWHOOLJHQFHFDSDELOLWLHVDQGV\VWHPVIRUIXWXUHQDWLRQDOVHFXULW\LQWHOOLJHQFH QHHGV7KHSURJUDPVHHNVWKHEULJKWHVWPLQGVDQGEUHDNWKURXJKWHFKQRORJLHVIURP LQGXVWU\DFDGHPLDQDWLRQDOODERUDWRULHVDQG86JRYHUQPHQWDJHQFLHV 9LVLWWKHZHEVLWHIRU%URDG$JHQF\$QQRXQFHPHQWDQG *RYHUQPHQW6RXUFHV6RXJKW$QQRXQFHPHQWUHTXLUHPHQWV 703.808.2769 www.nro.gov/About-the-NRO/Business-Opportunities FEATURES | June 2019 MORE AT aerospaceamerica.aiaa.org 14 28 36 20 Designing for the NASA managers Pitching urban commuter face “agonizing” innovative ideas Crop dusting market choice to government into the future Lithium ion batteries Those in charge of Aerospace give engineers the agency’s entrepreneurs can Pilots in the daring profession face fl exibility but also New Frontiers series avoid common pitfalls challenges from drones as aerial present a modeling must decide between by practicing their application enters its second century. challenge. Here’s how exploring a comet or technique. Vahana’s designers Saturn’s Titan moon. By Jan Tegler coped. By Amanda Miller By Adam Hadhazy By Keith Button aerospaceamerica.aiaa.org | JUNE 2019 | 1 19–22 AUGUST 2019 INDIANAPOLIS, IN EXPOSITION AND SPONSORSHIP Promote and grow your business at the world’s only conference event to showcase both aeronautics and space propulsion and energy technologies in a single venue that is unmatched by any competitive event.
    [Show full text]
  • Returning Samples from Enceladus for Life Detection
    Returning Samples from Enceladus for Life Detection 1 Marc Neveu*1,2, Ariel Anbar3,4, Alfonso Davila5, Daniel P. Glavin1, Shannon M. MacKenzie6, 2 Charity Phillips-Lander7, Brent Sherwood8, Yoshinori Takano9, Peter Williams4, Hajime 3 Yano10. 4 1Solar System Exploration Division, NASA Goddard Space Flight Center, Greenbelt, MD, USA 5 2Department of Astronomy, University of Maryland, College Park, MD, USA 6 3School of Earth & Space Exploration, Arizona State University, Tempe, AZ, USA 7 4School of Molecular Sciences, Arizona State University, Tempe, AZ, USA 8 5NASA Ames Research Center, Moffett Field, CA, USA 9 6Johns Hopkins Applied Physics Laboratory, Laurel, MD, USA 10 7Southwest Research Institute, San Antonio, TX, USA 11 8Blue Origin, Seattle, WA, USA 12 9Japan Agency for Marine-Earth Science & Technology, Yokosuka, Japan 13 10Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency, Sagamihara, 14 Japan 15 * Correspondence: 16 Marc Neveu 17 [email protected] 18 Keywords: Enceladus, astrobiology, sample return, life detection, ocean worlds, icy satellites 19 Number of words: 12683 20 Number of figures: 6 + 4 Tables 21 Abstract 22 Evidence suggests that Saturn’s icy moon Enceladus has a subsurface ocean that sources plumes of 23 water vapor and ice vented to space from its south pole. In situ analyses of this material by the 24 Cassini spacecraft have shown that the ocean contains key ingredients for life (elements H, C, N, O 25 and possibly S; simple and complex organic compounds; chemical disequilibria at water-rock 26 interfaces; clement temperature, pressure, and pH). The Cassini discoveries make Enceladus’ interior 27 a prime locale for life detection beyond Earth.
    [Show full text]
  • Organic Matter in Cometary Environments
    life Review Organic Matter in Cometary Environments Adam J. McKay 1,2,* and Nathan X. Roth 3,4 1 Department of Physics, American University, Washington, DC 20016, USA 2 Planetary Systems Laboratory Code 693, Solar System Exploration Division, NASA Goddard Space Flight Center, Greenbelt, MD 20771, USA 3 Astrochemistry Laboratory Code 691, Solar System Exploration Division, NASA Goddard Space Flight Center, Greenbelt, MD 20771, USA; [email protected] 4 Universities Space Research Association, Columbia, MD 21046, USA * Correspondence: [email protected] Abstract: Comets contain primitive material leftover from the formation of the Solar System, making studies of their composition important for understanding the formation of volatile material in the early Solar System. This includes organic molecules, which, for the purpose of this review, we define as compounds with C–H and/or C–C bonds. In this review, we discuss the history and recent breakthroughs of the study of organic matter in comets, from simple organic molecules and photodissociation fragments to large macromolecular structures. We summarize results both from Earth-based studies as well as spacecraft missions to comets, highlighted by the Rosetta mission, which orbited comet 67P/Churyumov–Gerasimenko for two years, providing unprecedented insights into the nature of comets. We conclude with future prospects for the study of organic matter in comets. Keywords: comet; organics; volatiles; astrobiology 1. Introduction Comets are primitive leftovers from the formation of the Solar System. As such, their composition provides clues to physics and chemistry operating during the protoplane- Citation: McKay, A.J.; Roth, N.X. tary disk phase (Figure1), as well as the preceding phases of star formation (e.g., [ 1,2]).
    [Show full text]
  • 20190206 Ver8 En3
    Asteroid explorer, Hayabusa2, reporter briefing February 6, 2019 JAXA Hayabusa2 Project Topics Regarding Hayabusa2: Touchdown operation plan Touchdown related information 2019/02/06 Hayabusa2 reporter briefing 2 Contents 0. Hayabusa2 and mission flow outline 1. Current status and overall schedule of the project 2. Touchdown operation plan 3. Projectile firing experiment 4. Scientific importance of the touchdown 5. Future plans Amendment Reference material 2019/02/06 Hayabusa2 reporter briefing 3 Overview of Hayabusa2 Objective We will explore and sample the C-type asteroid Ryugu, which is a more primitive type than the S-type asteroid Itokawa that Hayabusa explored, and elucidate interactions between minerals, water, and organic matter in the primitive solar system. By doing so, we will learn about the origin and evolution of Earth, the oceans, and life, and maintain and develop the technologies for deep-space return exploration (as demonstrated with Hayabusa), a field in which Japan leads the world. Expected results and effects By exploring a C-type asteroid, which is rich in water and organic materials, we will clarify interactions between the building blocks of Earth and the evolution of its oceans and life, thereby developing solar system science. Japan will further its worldwide lead in this field by taking on the new challenge of obtaining samples from a crater produced by an impacting device. We will establish stable technologies for return exploration of solar-system bodies. Features: World’s first sample return mission to a C-type asteroid. World’s first attempt at a rendezvous with an asteroid and performance of observation before and after projectile Hayabusa 2 primary specifications(Illustration: Akihiro Ikeshita) impact from an impactor.
    [Show full text]
  • Bringing It Back
    editorial Bringing it back NASA’s spacecraft OSIRIS-REx is planning to bring back a sample from a near-Earth asteroid in 2023, and it has just delivered its frst scientifc results. It is only one of the projects from various space agencies that will put small bodies and sample return into the spotlight in the upcoming decade. ample return of extraterrestrial This Nature Astronomy issue features is roughly double the size) will allow us to materials from the Moon was quite OSIRIS-REx, a NASA mission that aims perform in-depth comparative planetology, Scommon towards the end of space race. to bring back a sample from near-Earth which will only be strengthened when both In total, the American Apollo programme asteroid Bennu in 2023, after spending samples hit the laboratory. brought a whopping 382 kg of lunar samples a couple of years orbiting the asteroid Small bodies have been enjoying some to Earth. The corresponding Soviet Luna in order to characterize it. OSIRIS-REx special attention in space exploration for programme acquired only ~300 g, but with arrived at Bennu at the end of last year, and quite some time, but the next decade will fully robotic procedures. In contrast, the the relevant papers of this issue cover the exhibit a string of missions from a variety of amount of extraterrestrial material brought Approach and Preliminary Survey phases, actors. JAXA has built a full vision behind back since the end of the Luna 24 mission in between August and December 2018, which its small-bodies programme, as described 1976 sums up to a handful of microparticles are crucial to get a first impression of the by Masaki Fujimoto and Elizabeth Tasker, from the Stardust and Hayabusa missions.
    [Show full text]
  • National Rabies Management Program Report 2004
    COOPERATIVE RABIES MANAGEMENT PROGRAM NATIONAL REPORT 2004 United States Department of Agriculture Animal and Plant Health Inspection Service Wildlife Services 0 COOPERATIVE RABIES MANAGEMENT PROGRAM NATIONAL REPORT 2004 COMPILED and EDITED BY: Craig D. Kostrzewski Rabies Program Assistant Kathleen Nelson Staff Rabies Biologist REVIEWED BY: Dennis Slate National Rabies Management Program Coordinator USDA-APHIS-Wildlife Services 59 Chenell Drive, Suite 2 Concord, NH 03301 1 TABLE OF CONTENTS COOPERATIVE RABIES MANAGEMENT PROGRAM EXECUTIVE SUMMARY .........................................................................................................................................................3 ALABAMA......................................................................................................................................................................................7 ARIZONA......................................................................................................................................................................................11 CALIFORNIA ..............................................................................................................................................................................16 FLORIDA......................................................................................................................................................................................18 GEORGIA .....................................................................................................................................................................................23
    [Show full text]