Planetary Science Division Update Outline Administrative Changes
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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. -
Selection of the Insight Landing Site M. Golombek1, D. Kipp1, N
Manuscript Click here to download Manuscript InSight Landing Site Paper v9 Rev.docx Click here to view linked References Selection of the InSight Landing Site M. Golombek1, D. Kipp1, N. Warner1,2, I. J. Daubar1, R. Fergason3, R. Kirk3, R. Beyer4, A. Huertas1, S. Piqueux1, N. E. Putzig5, B. A. Campbell6, G. A. Morgan6, C. Charalambous7, W. T. Pike7, K. Gwinner8, F. Calef1, D. Kass1, M. Mischna1, J. Ashley1, C. Bloom1,9, N. Wigton1,10, T. Hare3, C. Schwartz1, H. Gengl1, L. Redmond1,11, M. Trautman1,12, J. Sweeney2, C. Grima11, I. B. Smith5, E. Sklyanskiy1, M. Lisano1, J. Benardino1, S. Smrekar1, P. Lognonné13, W. B. Banerdt1 1Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA 91109 2State University of New York at Geneseo, Department of Geological Sciences, 1 College Circle, Geneseo, NY 14454 3Astrogeology Science Center, U.S. Geological Survey, 2255 N. Gemini Dr., Flagstaff, AZ 86001 4Sagan Center at the SETI Institute and NASA Ames Research Center, Moffett Field, CA 94035 5Southwest Research Institute, Boulder, CO 80302; Now at Planetary Science Institute, Lakewood, CO 80401 6Smithsonian Institution, NASM CEPS, 6th at Independence SW, Washington, DC, 20560 7Department of Electrical and Electronic Engineering, Imperial College, South Kensington Campus, London 8German Aerospace Center (DLR), Institute of Planetary Research, 12489 Berlin, Germany 9Occidental College, Los Angeles, CA; Now at Central Washington University, Ellensburg, WA 98926 10Department of Earth and Planetary Sciences, University of Tennessee, Knoxville, TN 37996 11Institute for Geophysics, University of Texas, Austin, TX 78712 12MS GIS Program, University of Redlands, 1200 E. Colton Ave., Redlands, CA 92373-0999 13Institut Physique du Globe de Paris, Paris Cité, Université Paris Sorbonne, France Diderot Submitted to Space Science Reviews, Special InSight Issue v. -
Primitive Bodies Panel Planetary Science Decadal Survey Space Studies Board National Research Council
Space Studies Board Mailing Address: 500 Fifth Street, NW Washington, DC 20001 www.nationalacademies.org Primitive Bodies Panel Planetary Science Decadal Survey Space Studies Board National Research Council National Academy of Sciences Building 2101 Constitution Ave. NW, Washington, D.C. (Entrance at 2100 C Street NW) Conference Room 150 FINAL AGENDA1 September 9-11, 2009 Wednesday, September 9, 2009 CLOSED SESSION 7:30 a.m. Room Opens (Breakfast available in the meeting room) 8:30 a.m. Welcome and Agenda Review Joseph Veverka 8:45 a.m. Overview of NRC Study Process Dwayne Day 9:15 a.m. Balance and Composition Discussion Dwayne Day 10:00 a.m. Break OPEN SESSION2 10:15 a.m. Decadal Survey Overview Steven Squyres Cornell University 11:00 a.m. Lessons Learned from the 2003 Decadal Survey Dale Cruikshank NASA Ames Research Center 11:45 a.m. Committee Discussion (Lunch will be served in the meeting room, committee discussion will continue) 12:45 p.m. Charge to the Decadal Survey James Green/Lindley Johnson NASA Headquarters 1 Updated September 8, 2009 2 Webcast at http://nasa-nai.acrobat.com/primitive1/, Audio at 866-606-4717, Access Code 6686308. This meeting is being held to gather information to help the committee conduct its activities. The committee will examine the information and material obtained during open sessions in an effort to inform its work. Although opinions may be stated and lively discussion may ensue, no conclusions are being drawn at this time. Therefore, observers who draw conclusions about the committee's work based on today's discussions will be doing so prematurely. -
Rosetta Craft Makes Historic Comet Rendezvous European Space Agency's Comet-Chasing Mission Arrives After 10-Year Journey
NATURE | NEWS Rosetta craft makes historic comet rendezvous European Space Agency's comet-chasing mission arrives after 10-year journey. Elizabeth Gibney 06 August 2014 ESA/Rosetta/MPS for OSIRIS Team MPS/UPD/LAM/IAA/SSO/INTA/UPM/DASP/IDA Comet 67P/Churyumov–Gerasimenko, as seen by Rosetta from a distance of 285 kilometres. No one can deny that it was an epic trip. The European Space Agency's comet-chasing Rosetta spacecraft has arrived at its quarry, after launching more than a decade ago and travelling 6.4 billion kilometres through the Solar System. That makes it the first spacecraft to rendezvous with a comet, and takes the mission a step closer to its next, more ambitious goal of making the first ever soft landing on a comet. Speaking from mission control in Darmstadt, Germany, Matt Taylor, Rosetta project scientist for the European Space Agency (ESA), called the space mission “the sexiest there’s ever been”. Rosetta is now within 100 kilometres of its target, comet 67P/Churyumov–Gerasimenko (or 67P for short), which in July was discovered to be shaped like a rubber duck. After a six-minute thruster burn, at 11:29 a.m. local time on 6 August, ESA scientists confirmed that Rosetta had moved into the same orbit around the Sun as the comet. Rosetta is now moving at a walking pace relative to the motion of 67P — though both are hurtling through space at 15 kilometres per second. Unlike NASA’s Deep Impact and Stardust craft, and ESA’s Giotto mission, which flew by their target comets at high speed, Rosetta will now stay with the comet, taking a ring-side seat as 67P approaches the Sun, and eventually swings around it in August 2015. -
Solar System Exploration
Theme: Solar System Exploration Cassini, a robotic spacecraft launched in 1997 by NASA, is close enough now to resolve many rings and moons of its destination planet: Saturn. The spacecraft has now closed to within a single Earth-Sun separation from the ringed giant. In November 2003, Cassini snapped the contrast-enhanced color composite pictured above. Many features of Saturn's rings and cloud-tops now show considerable detail. When arriving at Saturn in July 2004, the Cassini orbiter will begin to circle and study the Saturnian system. Several months later, a probe named Huygens will separate and attempt to land on the surface of Titan. Solar System Exploration MAJOR EVENTS IN FY 2005 Deep Impact will launch in December 2004. The spacecraft will release a small (820 lbs.) Impactor directly into the path of comet Tempel 1 in July 2005. The resulting collision is expected to produce a small impact crater on the surface of the comet's nucleus, enabling scientists to investigate the composition of the comet's interior. Onboard the Cassini orbiter is a 703-pound scientific probe called Huygens that will be released in December 2004, beginning a 22-day coast phase toward Titan, Saturn's largest moon; Huygens will reach Titan's surface in January 2005. ESA 2-1 Theme: Solar System Exploration OVERVIEW The exploration of the solar system is a major component of the President's vision of NASA's future. Our cosmic "neighborhood" will first be scouted by robotic trailblazers pursuing answers to key questions about the diverse environments of the planets, comets, asteroids, and other bodies in our solar system. -
OSIRIS-Rex, Returning the Asteroid Sample
OSIRIS-REx, Returning the Asteroid Sample Thomas Ajluni Timothy Linn William Willcockson ASRC Federal Space & Defense Lockheed Martin Space Systems Lockheed Martin Space Systems 7000 Muirkirk Meadows Drive Company, P.O. Box 179 Company, P.O. Box 179 Suite 100, Beltsville, MD 20705 Denver, CO 80201 Denver, CO 80201 301.286.1831 303-977-0659 303-977-5094 [email protected] [email protected] [email protected] David Everett Ronald Mink Joshua Wood NASA Goddard Space Flight NASA Goddard Space Flight Lockheed Martin Space Systems Center, 8800 Greenbelt Road Center, 8800 Greenbelt Road Company, P.O. Box 179 Greenbelt, MD 20771 Greenbelt, MD 20771 Denver, CO 80201 301.286.1596 301.286.3524 303-977-3199 [email protected] [email protected] [email protected] Abstract—This paper addresses the technical aspects of the sample return system for the upcoming Origins, Spectral x attitude control Interpretation, Resource Identification, and Security-Regolith x propulsion Explorer (OSIRIS-REx) asteroid sample return mission. The x power overall mission design and current implementation are presented as an overview to establish a context for the x thermal control technical description of the reentry and landing segment of the x telecommunications mission. x command and data handling x structural support to ensure successful rendezvous The prime objective of the OSIRIS-REx mission is to sample a with Bennu primitive, carbonaceous asteroid and to return that sample to Earth in pristine condition for detailed laboratory analysis. x characterization of Bennu’s properties Targeting the near-Earth asteroid Bennu, the mission launches x delivery of the sampler to the surface, and return of in September 2016 with an Earth reentry date of September the spacecraft to the vicinity of the Earth 24, 2023. -
The Planetary Report
A Publication of THEPLANETA SOCIETY o o o • o -e o o Board of Directors CARL SAGAN NORMAN R. AUGUSTI NE President Chairman and CEO, Director, Martin Marietta Corporation Laboratory for Planetary Studies, Cornelf University JOHN E. BRYSON Chairman and CEO, BRUCE MURRAY Southern California Edison Vice President Professor of Planetary Science, JOSEPH RYAN California Institute of Technology O'Melveny & Myers LOU IS FRIEDMAN STEVEN SPI ELBERG A WARNING FROM YOUR EDITOR Bringing People Together Through Executive Director director and producer You may soon be getting a phone call Planetary Science-Page 13-Education Board of Advisors from me. No, I won't be asking you for has always been close to the hearts of DIANE ACKERMAN JOHN M. LOGSDON donations or nagging you about a missed Planetary Society members, and we have poet and author Director, Space Policy Institute, George Washington University deadline (a common fear among planetary sponsored many programs to promote sci BUZZ ALDRIN Apollo 11 astronaut HANS MARK scientists). Instead, I will be asking for ence education around the world. We've The University of Texas at Austin RICHARD BERENDZEN your opinion about The Planetary Report. gathered together reports on three projects educator and astrophysicist JAMES MICHENER author JACQUES BLAMONT Each month our computer will randomly now completed and one just beginning. Chief Scientist, Centre MARVIN MINSKY Nationa! d'Etudes Spatia/es, Toshiba Professor of Media Arts select several members whom I will call to A Planetary Readers' Service-Page 16- France and Sciences, Massachusetts Institute of Technology discuss the contents of our latest issue-or For most of its history, the science we call RAY BRADBURY poet and author PHILIP MORRISON any other topic related to our publications. -
Chondrule-Like Material in Wild 2: a New Insight from Impact Experiments of Chondrule Fragments on Stardust Analogue Al Foil
52nd Lunar and Planetary Science Conference 2021 (LPI Contrib. No. 2548) 1925.pdf CHONDRULE-LIKE MATERIAL IN WILD 2: A NEW INSIGHT FROM IMPACT EXPERIMENTS OF CHONDRULE FRAGMENTS ON STARDUST ANALOGUE AL FOIL. M. Van Ginneken1 and P. J. Wozniakiewicz1, 1Centre for Astrophysics and Planetary Science, School of Physical Sciences, University of Kent, United Kingdom ([email protected]; [email protected]) Introduction: NASA’s Stardust mission was the shape of craters depends mainly on the physical first mission to bring back to Earth material from a properties of the impactor [19]. Solid grains or dense celestial body, i.e. the Jupiter Family Comet (JFC) consolidated aggregates similar to chondrule fragments 81P/Wild 2 (hereafter Wild 2) [1]. Cometary dust was will result in bowl-shaped craters, the depth of which captured via impact into a collector that was deployed depending on the density of the material, whereas loose during a fly-by through the coma of Wild 2 at a relative aggregates of submicron particles result in complex speed of 6 km s-1. The collector consisted of silica features. Simulation of Stardust impacts using silicate aerogel secured into a metal frame by aluminum 1100 grains have shown that about 50% of silicate dominated foil (hereafter Al foil). A major result of the mission was impactors are retained as residue, which can be analysed the discovery that, contrary to expectations, Wild 2 was and provide precious chemical information [20]. not predominantly composed of presolar grains and low Studies of residues in a small (ø < 10 µm) or large temperature outer solar nebula material, but rather high (ø > 10 µm) craters on Stardust foil have shown that temperature (>>1000 °C) material typical of primitive these can give information on the bulk chemistry of the meteorites [1 - 3]. -
IMPLEMENTATION of TRIDENT: a DISCOVERY-CLASS MISSION to TRITON. K. L. Mitchell1 , L. M. Prockter2, W. E. Frazier1, W. D. Smythe1, B
50th Lunar and Planetary Science Conference 2019 (LPI Contrib. No. 2132) 3200.pdf IMPLEMENTATION OF TRIDENT: A DISCOVERY-CLASS MISSION TO TRITON. K. L. Mitchell1 , L. M. Prockter2, W. E. Frazier1, W. D. Smythe1, B. M. Sutin1, D. A. Bearden1, and the Trident Team. 1Jet Propulsion Laboratory ([email protected]), Pasadena, CA 91109-8099, United States, 2Lunar and Planetary Insti- tute/USRA, Houston, TX, United States. Overview: Trident is an exciting mission concept to Why Now?: By launching during 2026, Trident investigate Neptune’s large moon Triton, an exotic can- takes advantage of a rare, efficient gravity-assist align- didate ocean world at 30 AU (Prockter et al., this meet- ment, to capitalize on a narrow – but closing – observa- ing). The concept is responsive to recommendations of tional window that enables assessment of changes in the recent NASA Roadmap to Ocean Worlds study Triton’s plume activity and surface characteristics since (Hendrix et al., 2019), and to the 2013 Planetary Deca- Voyager 2’s encounter one Neptune-Triton season ago. dal Survey’s habitability and workings themes (Squyres Conclusion: This mission design allows Trident to et al., 2011). A rare, low Δv trajectory (Fig. 1) enables accomplish a scientifically rich yet radically cost-effec- an MMRTG-powered spacecraft fitting under the Dis- tive investigation of an unusual icy world, dramatically covery cost cap. The spacecraft has a robust design and expanding the horizons of NASA’s Discovery Program. uses high heritage instruments (table 1) with minimal References: [1] Prockter L. M. et al. (2019) LPS L, development costs. -
The MESSENGER Mission to Mercury: Some Lessons Learned
The MESSENGER Mission to Mercury: Some Lessons Learned Sean C. Solomon Lamont-Doherty Earth Observatory Columbia University PI Forum #5 16 March 2016 40th LPSC The Woodlands, Texas 25 March 2009 Mission Milestones Selection as a Discovery Mission July 1999 Phase B (detailed design) January 2000 – June 2001 Phase C/D (fabrication, assembly, & test) July 2001 – July 2004 Launch August 2004 Earth flyby August 2005 Venus flybys October 2006, June 2007 Mercury flybys January 2008, October 2008, September 2009 Mercury orbital operations March 2011 – April 2015 Managed by The Johns Hopkins University Applied Physics Laboratory and the Carnegie Institution of Washington 2 Faced Broad Challenges • Demanding limits to mass growth • Hazardous thermal and radiation environment • Complex mission design with limited launch opportunities and a long cruise phase 3 Some Obvious Advice for PIs • Budget ample reserves: cost, schedule, mass, power • Learn project management and systems engineering • Assemble the best possible team • Accomplish as much in Phase B as possible 4 Anticipate Technical Challenges A challenge anticipated: Solar arrays • Multiple vendors engaged • Thorough testing program • Final vendor selection after all prototype testing A challenge not anticipated: Inertial Measurement Unit (IMU) MESSENGER Solar Array •Expertise resided with a single vendor •That vendor was bought out by a new vendor, who closed a key facility and had to reinvent expertise MESSENGER IMU 5 …and More Technical Challenges • Manufacturer applied excess epoxy • Delamination -
Space Sector Brochure
SPACE SPACE REVOLUTIONIZING THE WAY TO SPACE SPACECRAFT TECHNOLOGIES PROPULSION Moog provides components and subsystems for cold gas, chemical, and electric Moog is a proven leader in components, subsystems, and systems propulsion and designs, develops, and manufactures complete chemical propulsion for spacecraft of all sizes, from smallsats to GEO spacecraft. systems, including tanks, to accelerate the spacecraft for orbit-insertion, station Moog has been successfully providing spacecraft controls, in- keeping, or attitude control. Moog makes thrusters from <1N to 500N to support the space propulsion, and major subsystems for science, military, propulsion requirements for small to large spacecraft. and commercial operations for more than 60 years. AVIONICS Moog is a proven provider of high performance and reliable space-rated avionics hardware and software for command and data handling, power distribution, payload processing, memory, GPS receivers, motor controllers, and onboard computing. POWER SYSTEMS Moog leverages its proven spacecraft avionics and high-power control systems to supply hardware for telemetry, as well as solar array and battery power management and switching. Applications include bus line power to valves, motors, torque rods, and other end effectors. Moog has developed products for Power Management and Distribution (PMAD) Systems, such as high power DC converters, switching, and power stabilization. MECHANISMS Moog has produced spacecraft motion control products for more than 50 years, dating back to the historic Apollo and Pioneer programs. Today, we offer rotary, linear, and specialized mechanisms for spacecraft motion control needs. Moog is a world-class manufacturer of solar array drives, propulsion positioning gimbals, electric propulsion gimbals, antenna positioner mechanisms, docking and release mechanisms, and specialty payload positioners. -
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