Odyssey Begins with Perfect Launch
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Planetary Science Division Status Report
Planetary Science Division Status Report Jim Green NASA, Planetary Science Division January 26, 2017 Astronomy and Astrophysics Advisory CommiBee Outline • Planetary Science ObjecFves • Missions and Events Overview • Flight Programs: – Discovery – New FronFers – Mars Programs – Outer Planets • Planetary Defense AcFviFes • R&A Overview • Educaon and Outreach AcFviFes • PSD Budget Overview New Horizons exploresPlanetary Science Pluto and the Kuiper Belt Ascertain the content, origin, and evoluFon of the Solar System and the potenFal for life elsewhere! 01/08/2016 As the highest resolution images continue to beam back from New Horizons, the mission is onto exploring Kuiper Belt Objects with the Long Range Reconnaissance Imager (LORRI) camera from unique viewing angles not visible from Earth. New Horizons is also beginning maneuvers to be able to swing close by a Kuiper Belt Object in the next year. Giant IcebergsObjecve 1.5.1 (water blocks) floatingObjecve 1.5.2 in glaciers of Objecve 1.5.3 Objecve 1.5.4 Objecve 1.5.5 hydrogen, mDemonstrate ethane, and other frozenDemonstrate progress gasses on the Demonstrate Sublimation pitsDemonstrate from the surface ofDemonstrate progress Pluto, potentially surface of Pluto.progress in in exploring and progress in showing a geologicallyprogress in improving active surface.in idenFfying and advancing the observing the objects exploring and understanding of the characterizing objects The Newunderstanding of Horizons missionin the Solar System to and the finding locaons origin and evoluFon in the Solar System explorationhow the chemical of Pluto wereunderstand how they voted the where life could of life on Earth to that pose threats to and physical formed and evolve have existed or guide the search for Earth or offer People’sprocesses in the Choice for Breakthrough of thecould exist today life elsewhere resources for human Year forSolar System 2015 by Science Magazine as exploraon operate, interact well as theand evolve top story of 2015 by Discover Magazine. -
Making It LOUD
Making it LOUD 2011 Annual Report WWW.USFIRST.ORG1 For over 20 years, FIRST® Founder Dean Kamen and everyone associated with FIRST have been on a mission to spread President Barack Obama, along with White House Technology Officer Aneesh Chopra, continued to feature FIRST teams as perfect examples of the president’s national White the word about the many educational, societal, economical, and House Science Fair initiative promoting STEM (science, technology, engineering, and Dean Kamen will.i.am planetary benefits of getting youth and adults alike involved in theFIRST math) education and celebrating science and math achievement in American schools. Morgan Freeman experience. Despite not having access to the millions of marketing Soledad O’Brien dollars required to make FIRST a household “brand,” the program has continued to grow each year at a blistering pace. …aND loudER Books, magazines, newspapers, cable TV, and the Web helped us create noise, too, with ongoing national coverage by Bloomberg, CNN, Popular Mechanics, In 2011, however, thanks to the fervent interest of major figures Popular Science, Wired, ESPN Magazine, WallStreetJournal.com, and more. Author Neal Bascomb brought the FIRST experience to life in his inspiring in government, the media, and mainstream entertainment, the book, The New Cool.Time Warner Cable incorporated “volume” of voices promoting FIRST... FIRST into its national “Connect A Million Minds™” initiative, featuring our FRC program in its TV show “It Ain’t Rocket Science.” The clamor of FIRST recognition continues to grow ...GOT TuRNED UP loud...VERY loud! louder every day. The continuing mainstream exposure is helping propel us toward our goal of making FIRST known and recognized around the globe. -
Genesis Radiation Environment
https://ntrs.nasa.gov/search.jsp?R=20070014073 2019-08-30T00:44:36+00:00Z 1 Source of Acquisition NASA Marshall Space Flight Center Genesis Radiation Environment Joseph I. Minow* NASA Marshull Space Flight Center, Huntsville, AL 35812 USA Richard L. Altstatt' and William C. Skipworth* Jacobs Engineering, Marshall Space Flight Center Group, Huntsville, AL 35812 USA The Genesis spacecraft launched on 8 August 2001 sampled solar wind environments at L1 from 2001 to 2004. After the Science Capsule door was opened, numerous foils and samples were exposed to the various solar wind environments during periods including slow solar wind from the streamer belts, fast solar wind flows from coronal holes, and coronal mass ejections. The Survey and Examination of Eroded Returned Surfaces (SEERS) program led by NASA's Space Environments and Effects program had initiated access for the space materials community to the remaining Science Capsule hardware after the science samples had been removed for evaluation of materials exposure to the space environment. This presentation will describe the process used to generate a reference radiation Genesis Radiation Environment developed for the SEERS program for use by the materials science community in their analyses of the Genesis hardware. I. Introduction ASA's Space Environments and Effects (SEE) Program initiated the Surveying and Examination of Eroded N Returned Surfaces (SEERS) Initiative in 2003. The goal of the Initiative was to provide leadership in the engineering analysis of returned flight hardware by supporting a comprehensive effort to understand environmental effects due to solar W, ionizing radiation, plasmas, neutral contamination, meteoroids, and other conditions experienced during the mission (not primary science mission objectives). -
The Mars 2001 Odyssey and the "Autogen" Process
View metadata, citation and similar papers at core.ac.uk brought to you by CORE provided by DigitalCommons@USU AUTOGEN: The Mars 2001 Odyssey and the "Autogen" Process By Roy Gladden June 6, 2002 Jet Propulsion Laboratory / California Institute of Technology Pasadena, California Abstract In many deep space and interplanetary missions, it is widely recognized that the scheduling of many commands to operate a spacecraft can follow very regular patterns. In these instances, it is greatly desired to convert the knowledge of how commands are scheduled into algorithms in order to automate the development of command sequences. In doing so, it is possible to dramatically reduce the number of people and work-hours that are required to develop a sequence. The development of the "autogen" process for the Mars 2001 Odyssey spacecraft is one implementation of this concept. It combines robust scheduling algorithms with software that is compatible with pre- existing "uplink" software, and literally reduced the duration of some sequence generation processes from weeks to minutes. This paper outlines the "autogen" tools and processes and describes how they have been implemented for the various phases of the Mars 2001 Odyssey mission. What is autogen? manually building the commands for lengthy and well- understood command sequences, efforts were made to The term "autogen" is applied in two different ways. develop software that would automatically schedule the First, "autogen," in its broadest sense, identifies a commands given certain input data. By taking the process that may be used to automatically generate knowledge for how commands were to be scheduled sequences for a spacecraft and, second, it is a Solaris and writing algorithms to replicate that knowledge, it script that has been used to facilitate this process. -
Bridge Linking Engineering and Society
Fall 2017 OPEN SOURCE HARDWARE The BRIDGE LINKING ENGINEERING AND SOCIETY Hardware: The Next Step toward Open Source Everything Alicia M. Gibb Freedom Reigns in Desktop 3D Printing Ben Malouf and Harris Kenny Reevaluating Intellectual Property Law in a 3D Printing Era Lucas S. Osborn Impacts of Open Source Hardware in Science and Engineering Joshua M. Pearce The Maker Movement and Engineering AnnMarie Thomas and Deb Besser 3D Printing for Low-Resource Settings Matthew P. Rogge, Melissa A. Menke, and William Hoyle The mission of the National Academy of Engineering is to advance the well-being of the nation by promoting a vibrant engineering profession and by marshalling the expertise and insights of eminent engineers to provide independent advice to the federal government on matters involving engineering and technology. The BRIDGE NATIONAL ACADEMY OF ENGINEERING Gordon R. England, Chair C. D. Mote, Jr., President Corale L. Brierley, Vice President Julia M. Phillips, Home Secretary Ruth A. David, Foreign Secretary Martin B. Sherwin, Treasurer Editor in Chief: Ronald M. Latanision Managing Editor: Cameron H. Fletcher Production Assistant: Penelope Gibbs The Bridge (ISSN 0737-6278) is published quarterly by the National Aca d emy of Engineering, 2101 Constitution Avenue NW, Washington, DC 20418. Periodicals postage paid at Washington, DC. Vol. 47, No. 3, Fall 2017 Postmaster: Send address changes to The Bridge, 2101 Constitution Avenue NW, Washington, DC 20418. Papers are presented in The Bridge on the basis of general interest and time- liness. They reflect the views of the authors and not necessarily the position of the National Academy of Engineering. -
Stardust Sample Return
National Aeronautics and Space Administration Stardust Sample Return Press Kit January 2006 www.nasa.gov Contacts Merrilee Fellows Policy/Program Management (818) 393-0754 NASA Headquarters, Washington DC Agle Stardust Mission (818) 393-9011 Jet Propulsion Laboratory, Pasadena, Calif. Vince Stricherz Science Investigation (206) 543-2580 University of Washington, Seattle, Wash. Contents General Release ............................................................................................................... 3 Media Services Information ……………………….................…………….................……. 5 Quick Facts …………………………………………..................………....…........…....….. 6 Mission Overview …………………………………….................……….....……............…… 7 Recovery Timeline ................................................................................................ 18 Spacecraft ………………………………………………..................…..……...........……… 20 Science Objectives …………………………………..................……………...…..........….. 28 Why Stardust?..................…………………………..................………….....………............... 31 Other Comet Missions .......................................................................................... 33 NASA's Discovery Program .................................................................................. 36 Program/Project Management …………………………........................…..…..………...... 40 1 2 GENERAL RELEASE: NASA PREPARES FOR RETURN OF INTERSTELLAR CARGO NASA’s Stardust mission is nearing Earth after a 2.88 billion mile round-trip journey -
The Messenger Sept. 8Th GENESIS SUNDAY
WHAT’S INSIDE: Stewardship and Finance……...pg. 2 Congregational News…………... pg. 3 Celebrating Lohmen……………..pg. 4 Adult Education…………………...pg. 5 Faith Through the Generations….pgs. 6-7 Community Events…………..pgs. 8-9 WPC Food Pantry………………..pg. 10 The Messenger Prayer Ministry & Groups…….pg. 11 Environmental Stewardship...pg. 12 VOLUME 89, ISSUE 8 Confirmation Class……………...pg. 12 AUGUST 2019 Sept. 8th GENESIS SUNDAY Bring the whole family and invite a friend for a day full of food, games, live music, and lots of wild surprises! 2 CONGREGATIONAL NEWS The Pastor Nominating Committee Report (PNC) Nine members of the congregation were nominated and elected to serve on the Pastor Nominating Committee (PNC). They are: Andrew Finkner, Michael Gregg, Steve Hughes, Jim Kinkennon, Sandi Larson, Deb Schorr, Alisha Stokes, Allen Wachter and Joyce Douglas, Moderator. These members represent the whole congregation and have the responsibility for nominating an individual to present to the congregation to serve as our Head of Staff. In the future months, the PNC will journey through the search process seeking to hear the call of Christ. The first step will be to review the documentation from our group meetings held last Fall which represents the needs of Westminster and then complete the Ministry Information Form. The PNC has received reading materials already and will begin meeting together in early August. The PNC plans to keep the congregation informed on the status of this search. Our journey begins……… Joyce Douglas, Moderator LOOKING AHEAD Sun. August 4th—Celebrating Lohmen, our sister church in Germany (after worship, meet in chancel) Tues., Aug. -
Titan and Enceladus $1 B Mission
JPL D-37401 B January 30, 2007 Titan and Enceladus $1B Mission Feasibility Study Report Prepared for NASA’s Planetary Science Division Prepared By: Kim Reh Contributing Authors: John Elliott Tom Spilker Ed Jorgensen John Spencer (Southwest Research Institute) Ralph Lorenz (The Johns Hopkins University, Applied Physics Laboratory) KSC GSFC ARC Approved By: _________________________________ Kim Reh Dr. Ralph Lorenz Jet Propulsion Laboratory The Johns Hopkins University, Applied Study Manager Physics Laboratory Titan Science Lead _________________________________ Dr. John Spencer Southwest Research Institute Enceladus Science Lead Pre-decisional — For Planning and Discussion Purposes Only Titan and Enceladus Feasibility Study Report Table of Contents JPL D-37401 B The following members of an Expert Advisory and Review Board contributed to ensuring the consistency and quality of the study results through a comprehensive review and advisory process and concur with the results herein. Name Title/Organization Concurrence Chief Engineer/JPL Planetary Flight Projects Gentry Lee Office Duncan MacPherson JPL Review Fellow Glen Fountain NH Project Manager/JHU-APL John Niehoff Sr. Research Engineer/SAIC Bob Pappalardo Planetary Scientist/JPL Torrence Johnson Chief Scientist/JPL i Pre-decisional — For Planning and Discussion Purposes Only Titan and Enceladus Feasibility Study Report Table of Contents JPL D-37401 B This page intentionally left blank ii Pre-decisional — For Planning and Discussion Purposes Only Titan and Enceladus Feasibility Study Report Table of Contents JPL D-37401 B Table of Contents 1. EXECUTIVE SUMMARY.................................................................................................. 1-1 1.1 Study Objectives and Guidelines............................................................................ 1-1 1.2 Relation to Cassini-Huygens, New Horizons and Juno.......................................... 1-1 1.3 Technical Approach............................................................................................... -
Genesis Sample Return
NATIONAL AERONAUTICS AND SPACE ADMINISTRATION Genesis Sample Return Press Kit September 2004 Media Contacts Donald Savage Policy/program management 202/358-1727 Headquarters, [email protected] Washington, D.C. DC Agle Genesis mission 818/393-9011 Jet Propulsion Laboratory, [email protected] Pasadena, Calif. Robert Tindol Principal investigator 626/395-3631 California Institute of Technology [email protected] Pasadena, Calif. Contents General Release ……................……………………………….........................………..……....… 3 Media Services Information …………………………….........................................………..…….... 5 Quick Facts…………………………………………………….......................................………....…. 6 Mysteries of the Solar Nebula ........………...…………………………......................................……7 Solar Studies Past and Present ...................................................................................... 8 NASA's Discovery Program .......................................................................................... 10 Mission Overview….………...…………...…………………………....................................…….... 12 Mid-Air Retrievals........................................................................................................... 14 Sample Return Missions ................................................................................................ 15 Spacecraft ………………………………………………………………......................................…. 26 Science Objectives ………………………………………………………....................................…. 33 The Solar Corona and -
Chapters 1-10 As a Single File (Pdf)
Boldrin & Levine: Against Intellectual Monopoly, Chapter 1 Chapter 1: Introduction In late 1764, while repairing a small Newcomen steam engine, the idea of allowing steam to expand and condense in separate containers sprang into the mind of James Watt. He spent the next few months in unceasing labor building a model of the new engine. In 1768, after a series of improvements and substantial borrowing, he applied for a patent on the idea. August found Watt in London about the patent and he spent another six months working hard to obtain it. The patent was finally awarded in January of the following year. Nothing much happened by way of production until 1775. Then, with a major effort supported by his business partner, the rich industrialist Matthew Boulton, Watt secured an Act of Parliament extending his patent until the year 1800. The great statesman Edmund Burke spoke eloquently in Parliament in the name of economic freedom and against the creation of unnecessary monopoly – but to no avail. The connections of Watt’s partner Boulton were too solid to be defeated by simple principle. Once Watt’s patents were secured and production started, a substantial portion of his energy was devoted to fending off rival inventors. In 1782, Watt secured an additional patent, made “necessary in consequence of ... having been so unfairly anticipated, by [Matthew] Wasborough in the crank motion.” More dramatically, in the 1790s, when the superior Hornblower engine was put into production, Boulton and Watt went after him with the full force of the legal system. During the period of Watt’s patents the U.K. -
The Dean of Engineering: Interview with Dean Kamen
Maker www.makezine.com/04/interview INTERVIEW BY WILLIAM LIDWELL PHOTOGRAPHY BY GERRY MANACSA >> 25 Make: Volume 04 Make: 26 Maker Caption TK 27 Make: Volume 04 Dean Kamen holds more than 150 patents on revolutionary inventions ranging from portable dialysis machines to qualify it as a sort of technology museum. sophisticated mobility devices to highly effi- Dressed in his customary cotton work shirt cient and compact Stirling engines.In addition and Levi’s, Kamen wasted little time in getting to numerous honorary degrees, Kamen has things started: “You know how a slide rule received such honors as the Lemelson-MIT works?” he asked without context or warning. Prize, Heinz Award, Kilby Award, and the Na- I sheepishly confessed that I didn’t. “Slide tional Medal of Technology. A tireless advocate rules were a bit before my time,” I said. Clearly for science and technology education, Kamen dissatisfied with my response, Kamen sprang founded FIRST (For Inspiration and Recogni- from his chair and quickly located a six-foot tion of Science and Technology) to encour- slide rule lying against a wall in his office. He age kids to pursue careers as scientists and then proceeded to show me how to use this engineers, as well as to reset societal values giant slide rule to perform all manner of cal- so that people aspire to be thinkers and inven- culations, simple and complex, and frequently tors. “Our culture celebrates one thing: sports inserted commentary on the design elements heroes,” he says. “You have teenagers thinking that made the slide rule work. -
NASA Sets Sights on Asteroid Exploration : Nature News & Comment
NASA sets sights on asteroid exploration Agency plans to launch a mission to visit the Trojan asteroids in 2021, and one to the metallic asteroid Psyche in 2023. Alexandra Witze 04 January 2017 NASA/JPL-Caltech An artist’s conception of the Psyche spacecraft, which will explore a metallic asteroid. NASA will send two spacecraft to explore asteroids in the hopes of revealing new information about the Solar System’s origins. Psyche will journey to what could be the metallic heart of a failed planet and Lucy will investigate the Trojan asteroids near Jupiter. The missions, announced on 4 January, are part of NASA’s Discovery Program for planetary exploration. They were shortlisted by NASA in September 2015 and have survived a final cut that eliminated two proposed missions to Venus — which has not seen a US planetary mission since Magellan launched in 1989. “What can I say? It’s deeply disappointing,” says Robert Grimm, a planetary scientist at the Southwest Research Institute in Boulder, Colorado, and chairman of a group that analyses Venus issues for NASA. “We want to make sure NASA continues to support high-level Venus activities.” Scheduled to launch in October 2021 and arrive at its first major target in 2027, Lucy will explore six of Jupiter’s Trojan asteroids, which are trapped in orbits ahead of and behind the giant planet. Named after the famous hominid fossil, the spacecraft will investigate the origins of the giant planets by looking at the fragments left over from their formation. “These small bodies really are the fossils of planet formation,” said Lucy principal investigator Hal Levison of the Southwest Research Institute, at a media teleconference.