Planetary Science Advisory Committee February 21-23, 2018
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Mapping and Planetary Spatial Infrastructure Team
Mapping and Planetary Spatial Infrastructure Team INTRODUCTION SSB study on NASA PSD R&A Reorganization National Academy of Sciences, 13 May 2016 Jani Radebaugh, [email protected] Introducing the Mapping and Planetary Spatial Infrastructure Team • Mosaics, geologic maps, derived regional and global data products and associated geospatial infrastructure are integral to the success of the planetary science enterprise Introducing the Mapping and Planetary Spatial Infrastructure Team • Mosaics, geologic maps, derived regional and global data products and associated geospatial infrastructure are integral to the success of the planetary science enterprise Introducing the Mapping and Planetary Spatial Infrastructure Team • Mosaics, geologic maps, derived regional and global data products and associated geospatial infrastructure are integral to the success of the planetary science enterprise Introducing the Mapping and Planetary Spatial Infrastructure Team • Mosaics, geologic maps, derived regional and global data products and associated geospatial infrastructure are integral to the success of the planetary science enterprise Introducing the Mapping and Planetary Spatial Infrastructure Team • Mosaics, geologic maps, derived regional and global data products and associated geospatial infrastructure are integral to the success of the planetary science enterprise Introducing the Mapping and Planetary Spatial Infrastructure Team • Mosaics, geologic maps, derived regional and global data products and associated geospatial infrastructure are integral to the success of the planetary science enterprise Introducing the Mapping and Planetary Spatial Infrastructure Team • Mosaics, geologic maps, derived regional and global data products and associated geospatial infrastructure are integral to the success of the planetary science enterprise – Influence all phases of the mission lifecycle for science investigations and operations – Strategic needs must be anticipated and prioritized by the community – PSS recommended a “Cartography Research and Analysis Group” [CRAG] in Fall 2014. -
Mars Exploration: an Overview of Indian and International Mars Missions Nayamavalsa Scariah1, Dr
Taurian Innovative Journal/Volume 1/ Issue 1 Mars exploration: An overview of Indian and International Mars Missions NayamaValsa Scariah1, Dr. Mili Ghosh2, Dr.A.P.Krishna3 Birla Institute of Technology, Mesra, Ranchi Abstract- Mars is the fourth planet from the sun. It is 1. Introduction also known as red planet because of its iron oxide content. There are lots of missions have been launched to Mars is also known as red planet, because of the mars for better understanding of our neighboring planet. reddish iron oxide prevalent on its surface gives it a There are lots of unmanned spacecraft including reddish appearance. It is the fourth planet from sun. orbiters, landers and rovers have been launched into mars since early 1960. Sputnik was the first satellite The term sol is used to define duration of solar day on launched in 1957 by Soviet Union. After seven failure Mars. A mean Martian solar day or sol is 24 hours 39 missions to Mars, Mariner 4 was the first satellite which minutes and 34.244 seconds. Many space missions to reached the Martian orbiter successfully. The Viking 1 Mars have been planned and launched for Mars was the first lander reached on Mars on 1975. India exploration (Table:1) but most of them failed without successfully launched a spacecraft, Mangalyan (Mars completing the task specially in early attempts th Orbiter Mission) on 5 November, 2013, with five whereas some NASA missions were very payloads to Mars. India was the first nation to successful(such as the twin Mars Exploration Rovers, successfully reach Mars on its first attempt. -
Mapping and Planetary Spatial Infrastructure Team
Mapping and Planetary Spatial Infrastructure Team Report to the Planetary Science Subcommittee March 2016 Introducing the Mapping and Planetary Spatial Infrastructure Team • Mosaics, geologic maps, derived regional and global data products, and associated geospatial infrastructure are integral to the success of the planetary science enterprise – Influences all phases of the mission lifecycle for science investigations and operations – Strategic needs must be anticipated and prioritized by the community – PSS recommended a “Cartography Research and Analysis Group” [CRAG] in Fall 2014. • A team fulfilling this role now exists in the form of MAPSIT – MAPSIT succeeds former PCGMWG and assumes strategic planning role But wait, I thought we did this already? • No, we didn’t (really!) • From 1974 to 2012: – 1974: Lunar Photography and Cartography Committee (LPACC) – 1977: Lunar and Planetary Photography and Cartography Committee (LPPACC) – 1979: Planetary Cartography Working Group (PCWG) – Produced two 10-year plans and a supplement (at right) – 1994-2012: Planetary Cartography & Geologic Mapping Working Group (PCGMWG) • PCGMWG ceased “advisory” role in ~2011 • PCGMWG disbanded 2015 with end of PGG • Looming gap for NASA long-term strategic planning and prioritization activities until addressed by MAPSIT formation 3/9/2016 3 Enabling Planetary Science • Planetary Spatial Infrastructure is the technology, policies, standards, human resources, software tools, and related activities necessary to Geographic Information Science and Technology acquire, -
LAURA KERBER Jet Propulsion Laboratory [email protected] 4800 Oak Grove Dr
LAURA KERBER Jet Propulsion Laboratory [email protected] 4800 Oak Grove Dr. Pasadena, CA __________________________________________________________________________________________ Education September 2006-May 2011 Brown University, Providence, RI PhD, Geological Sciences (May 2011) MS, Engineering, Fluid Mechanics (May 2011) MS, Geological Sciences (May 2008) August 2002-May 2006 Pomona College, Claremont, CA Major: Planetary Geology/Space Science Minor: Mathematics May 2002 Graduated Cherry Creek High School, Greenwood Village, Colorado, highest honors Research Experience and Roles September 2014- Present Jet Propulsion Laboratory, Research Scientist PI of Discovery Mission Concept Moon Diver Deputy Project Scientist, 2001 Mars Odyssey Yardang formation and distribution on Mars and Earth Ongoing development of end-to-end Martian sulfur cycle model, including microphysical processes, photochemistry, and interaction with the surface Measurement of wind over complex surfaces Microscale wind and erosion processes in cold polar deserts Science liaison to the Mars Program Office, Next Mars Orbiter (NeMO) Member of 2015 NeMO SAG Member of 2015 ICE-WG (In-situ resource utilization and civil engineering HEOMD working group) Science lead on several internal formulation studies, including a “Many MERs to Mars” concept study; “RSL Exploration with the Axel Extreme Terrain Robot” strategic initiative; “Autonomous Recognition of Signs of Life” spontaneous RTD; Moon Diver Instrument Trade Study; etc. Lead of Citizen Scientist “Planet Four: -
MEPAG Report to PSS 03-2016
Lisa Pratt, MEPAG Chair Report to PSS March 10-11, 2016 Mission Status Highlights • Curiosity is moving on from its several-month investigation of the Namib (part of Bagnold dunes) • MRO and ODY are stepping up observations as data rates increase – Both orbiters have started observing candidate sites (exploration zones) for humans on Mars • MER-B has survived winter and is exploring area where orbital data indicate clays • MAVEN has finished prime mission; special issue out with 59 papers reporting results • Foreign collaborations with ESA Mars Express and ExoMars MOMA continuing • 2020 Mars rover passed PDR review but has not gone through the Directorate or Agency Program Management Councils MEPAG Face-to-Face Meeting held March 2–3 • New MEPAG Chair: Jeff Johnson (JHU-APL) – Lisa Pratt moves to MEPAG Executive Committee – Nominations invited to fill vacancies on Goals Committee • Wide-Ranging Presentations and Discussion – Reports from PSD, MEP, and several space agencies • Including report from IMEWG iMARS coordination study – Overview of joint HEO-SMD activities • Successful first workshop for landing sites (Exploration Zones) for humans on Mars held October 2015 – MEPAG accepted two reports from its Science Analysis Groups • Science Objectives for Human Explorers on Mars (HSO-SAG) • Next Mars Orbiter (NEX-SAG) Next Mars Orbiter (1 of 3) MEPAG endorsed the NEX-SAG report which concluded: o z M’rs Prflitere utilizing Solar Electric Propulsion (SEP) and advanced telecom in a 5‑year mission in low Mars orbit, could provide exciting new science and resource identification A mission with SEP could have the capability for return of a cache of Mars samples to Earth vicinity as well as payload elements addressing high-priority resource and other science objectives o Return capability addresses the need to make progress on sample return, which is the Decadal Survey’s highest priority for flagship missions. -
NAI Icy Satellites Environments Focus Group
Discussion with NAI Icy Satellites Environments Focus Group NASA Outer Planets Assessment Group William B McKinnon, Chair Washington University Sept 8, 2010 1 What is OPAG? The Outer Planets Assessment Group (OPAG) was established by NASA in late 2004 to identify scientific priorities and pathways for solar system exploration beyond the asteroid belt. The group consists of an ~15-person steering committee which actively solicits input from the scientific community and reports its findings to NASAʼs Planetary Science Division and the Planetary Science Subcommittee of NASAʼs Advisory Council." !It is OPAG's goal that its findings represent the broad consensus of the scientific community. OPAG holds meeting semiannually, each attended by ~100 scientists. The meetings consist of a broad range of presentations from NASA HQ representatives, mission PIs, individual scientists, and technology researchers. Meetings often include breakout sessions where scientists work in small groups to prioritize scientific questions and mission requirements at specific destinations (e.g., Europa, Titan, giant planets, midsize icy satellites such as Enceladus). Community input is solicited at the meetings and through the OPAG email list containing over 500 members." 2 Outer Planets Assessement Group Steering Committee William McKinnon, Washington University (Chair, 2009- )" Torrence Johnson*, Jet Propulsion Laboratory" Fran Bagenal, University of Colorado (Chair, 2004-2009)" Bill Kurth, University of Iowa" Sushil Atreya, University of Michigan" Ralph Lorenz, JHU/APL" -
Gordon Woodcock Space Architecture Award 2020 Candidate: a Scott Howe
Gordon Woodcock Space Architecture Award 2020 Candidate: A Scott Howe To the AIAA Space Architecture Technical Committee, thank you very much for nominating me for this award. I feel humbled, and I’m sure there are many worthy candidates. I feel as though I have been busy in some distant corner of the field, but I am very pleased that Space Architecture has grown to what it is today. The following are my statements and comments as requested – please let me know if further information is needed. 1. Statement confirming you’ve been involved in the field for at least 10 years: I was at the impressionable age of 9 years old when Neil and Buzz walked on the moon and was interested in space ever since. However, the idea of working for NASA seemed way beyond my reach, and didn’t seem compatible with my desire to become an architect so I went straight into architecture. I worked in terrestrial architecture since 1978. A turning point came when I began working in Japan in 1988, and got involved with the folks doing robotic construction. I began considering the issue of large-scale construction using entirely autonomous, mechanized means, and in the late 1990’s was introduced to early AIAA Design Engineering Space Architecture WG efforts by Marc Cohen and Ted Hall. I submitted my first Space Architecture paper, discussing a robotic outpost construction system in 2000 and increased my involvement in AIAA after that. I became a full-time Space Architect in 2007 when I joined the NASA Jet Propulsion Laboratory and have been working on robotic construction for planetary surfaces, the design of outposts and habitats, and pressurized vehicles ever since that time. -
Lava Lakes in the Solar System Rosaly LOPES , Jani RADEBAUGH
Lava Lakes in the Solar System Rosaly LOPES1#+, Jani RADEBAUGH2, Tracy GREGG3, Robert HOWELL4, Andrew HARRIS5 1 Jet Propulsion Laboratory, California Institute of Technology, United States, 2 Brigham Young University , United States, 3 SUNY Buffalo, United States, 4 University of Wyoming, United States, 5 Universite Blaise Pascal, Clermont-Ferrand, France #Corresponding author: [email protected] +Presenter Lava lakes are rare on Earth but common on Jupiter’s moon Io and likely occurred on other bodies such as Venus and Mars. Data from the Galileo spacecraft revealed that many Ionian paterae (calderas) are active, and several showed greater thermal emission around their edges (Lopes et al., 2004), which can be explained by the crust of a lava lake breaking up against the patera walls. Observations from both Galileo and ground-based telescopes reveal that several paterae, including Pele and Janus, have persistently high thermal output with regions of exposed, high-temperature lavas, indicative of large, vigorously active lava lakes similar to the Marum/Mbwelesu lava lake on Ambrym, Vanuatu. The volcano on Io that is the largest and has the greatest thermal output, Loki, has semi-periodic cycles of intense activity, interpreted as the foundering crust of a lava lake (Rathbun et al., Geophys. Res. Lett. 29; de Kleer et al., DPS, 2016), similar to the crusted, active lava lakes in Erta Ale, Ethiopia and Halemaumau, Hawaii. Alternatively, Loki Patera could be underlain by a thin, persistent magma “lens” that feeds thin, temporary lava lakes within the patera (Gregg and Lopes, 2008, Icarus 194). One significant and yet unexplained difference between Ionian and terrestrial paterae is the existence of cold “islands” in Ionian paterae that persist for decades (e.g., observed by both Voyagerand Galileo) despite intense and likely continuous activity. -
Mapping and Planetary Spatial Infrastructure Team
The Ol Doinyo Lengai volcano, Tanzania, as an analogue for Carbon Planets Jani Radebaugh, Rory Barnes, Jeff Keith Department of Geological Sciences, Brigham Young University, Department of Physics, University of Washington Field Analogues are Valuable • Knowledge of landforms on other planets is incomplete • Similar physics, materials can be found on Earth • Earth landscapes can yield important information about other planets MEDUSA FOSSE FORMATION, MARS DUNHUANG, CHINA, 40 N 93 E Field Analogues are Valuable • Knowledge of landforms on other planets is incomplete • Similar physics, materials can be found on Earth • Earth landscapes can yield important information about other planets TITAN Field Analogues are Valuable • Knowledge of landforms on other planets is incomplete • Similar physics, materials can be found on Earth • Earth landscapes can yield important information about other planets DUNHUANG, CHINA, 40 N 93 E Field Analogues are Valuable • Yardangs: Wind important, but also bedrock, rainfall, gravels LUT DESERT, IRAN Field Analogues of exoplanets?? • We’ve yet to even “see” an exoplanet • They are planetary surfaces worth studying as we do for our solar system TRAPPIST-1 Carbon Planets • Postulated to form in carbon-rich nebular environments (Seager and Kuchner 2005) • When C/O>0.8 in the disk (Bond et al. 2010) • May reach >75% carbon in the habitable zone! ARTIST LUYTEN Carbon Planets • Even in our solar system, carbon is enriched in certain locations • Mercury may have had graphite crust on magma ocean (Peplowski et al. 2016) Mercury MESSENGER M-dwarf Carbon Planets • Carbon planets orbiting M-dwarf stars could spend millions/billions of years closer than the habitable zone during pre-main-sequence (e.g. -
Lineations and Structural Mapping of Io's Paterae and Mountains
1 Lineations and structural mapping of Io’s paterae and mountains: Implications for internal stresses Alexandra A. Ahern, Jani Radebaugh, Eric H. Christiansen, Ronald A. Harris Brigham Young University Department of Geological Sciences, S-389 ESC, Provo, UT 84606 Abstract Io is the most volcanically active and tidally influenced body in the solar system. Its paterae and mountains are among its most distinguishing features. Paterae, similar to calderas, are volcano- tectonic collapse features, often with active lava flows on their floors. Io’s mountains are some of the highest in the solar system and contain many linear features that reveal global and regional stresses. This study investigates the relationship of linear features associated with paterae and mountains to stress fields associated with proposed mechanisms of formation: tidal forces, crustal loading, and local tectonics. 1. Introduction global scale processes. Paterae and Io, the innermost of the Galilean mountains are widely distributed and satellites, experiences great amounts of among Io’s most important volcanic and tidal stress as it orbits between Jupiter tectonic features. As such, they can and the other Galilean moons Europa, provide valuable insight into the Ganymede, and Callisto. This has volcanic and tectonic processes enabled accumulation of vast stores of operating on Io. internal heat (Peale et al., 1979) and has made Io the most volcanically active object in the solar system (Davies, 2001), evidenced by abundant lava flows and lava fountains (Radebaugh et al., 2001). Io also contains some of the largest mountains in the solar system, supported by a silicate-rich crust interlayered with sulfurous frosts (Schenk et al., 2001). -
Mars-Base-Camp-2028.Pdf
Mars Base Camp An Architecture for Sending Humans to Mars by 2028 A Technical Paper Presented by: Timothy Cichan Stephen A. Bailey Lockheed Martin Space Deep Space Systems, Inc. [email protected] [email protected] Scott D. Norris Robert P. Chambers Lockheed Martin Space Lockheed Martin Space [email protected] [email protected] Robert P. Chambers Joshua W. Ehrlich Lockheed Martin Space Lockheed Martin Space [email protected] [email protected] October 2016 978-1-5090-1613-6/17/$31.00 ©2017 IEEE Abstract—Orion, the Multi-Purpose Crew Vehicle, near term Mars mission is compelling and feasible, is a key piece of the NASA human exploration and will highlight the required key systems. architecture for beyond earth orbit (BEO). Lockheed Martin was awarded the contracts for TABLE OF CONTENTS the design, development, test, and production for Orion up through the Exploration Mission 2 (EM- 1. INTRODUCTION ..................................................... 2 2). Additionally, Lockheed Martin is working on 2. ARCHITECTURE PURPOSE AND TENETS ....................... 3 defining the cis-lunar Proving Ground mission 3. MISSION CAMPAIGN, INCLUDING PROVING GROUND architecture, in partnership with NASA, and MISSIONS ................................................................ 5 exploring the definition of Mars missions as the 4. MISSION DESCRIPTION AND CONCEPT OF OPERATIONS . 7 horizon goal to provide input to the plans for 5. ELEMENT DESCRIPTIONS ....................................... 13 human exploration of the solar system. This paper 6. TRAJECTORY DESIGN ............................................ 16 describes an architecture to determine the 7. SCIENCE ............................................................. 19 feasibility of a Mars Base Camp architecture 8. MARS SURFACE ACCESS FOR CREW ......................... 14 within about a decade. -
NASA ADVISORY COUNCIL Planetary Sciences Subcommittee
Planetary Sciences Subcommittee September 29-30, 2016 NASA ADVISORY COUNCIL Planetary Sciences Subcommittee September 29-30, 2016 NASA Headquarters Washington, D.C. MEETING MINUTES _____________________________________________________________ Clive Neal, Acting Chair _____________________________________________________________ Jonathan Rall, Executive Secretary 1 Planetary Sciences Subcommittee September 29-30, 2016 Table of Contents Welcome, Agenda, Announcements 3 PSD & R&A Status and Findings Update 3 Report on Senior Review 2016 6 GPRAMA 7 Mars Updates 8 Europa and Icy Worlds 11 Discussion 13 Adjourn First Day 13 Agenda Updates and Announcements 14 Analysis Groups Quick Update and Discussions 14 Planetary Protection 18 Synergies Between PSS and PPS 19 Discussion 19 Participating Scientists 21 DSN Updated 22 Extended Missions Report 23 Findings and Recommendations Discussions 24 Adjourn 26 Appendix A-Attendees Appendix B-Membership roster Appendix C-Presentations Appendix D-Agenda Prepared by Elizabeth Sheley Ingenicomm, Inc. 2 Planetary Sciences Subcommittee September 29-30, 2016 Thursday, September 29, 2016 Welcome, Agenda, Announcements Dr. Jonathan Rall, Executive Secretary of the Planetary Sciences Subcommittee (PSS) of the NASA Advisory Committee (NAC), welcomed the meeting participants. After asking the PSS members to introduce themselves, Dr. Clive Neal, Acting Chair of PSS, reviewed the PSS terms of reference. He made the point that biological planetary protection is outside the scope of the PSS charge, instead falling to the Planetary Protection Subcommittee (PPS). However, there are overlapping issues, and the PPS Chair, along with NASA’s Planetary Protection Officer, would make presentations at this meeting. PSD & R&A Status and Findings Update Dr. Rall presented the Planetary Science Division (PSD) update on behalf of the Division Director, Dr.