Vision and Voyages for Planetary Science in the - Solar System ...

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A Guide to Reading this Report There are many ways that individuals can and will read this report. Ideally, every reader will begin at the beginning and work their way through to the end. But, this is not essential. Indeed, the desires of most readers will be satisfied by the selective reading of different parts of this report. The remainder of this section and the adjacent chart (Figure 1.16) serves a reader’s guide. The fundamental principle used to frame this report derives from a hierarchy of science priorities. The core of the report (Chapters 4-9) is devoted to working from major, foundational topics that drive the overall planetary program—the origins of the solar system, the workings of planets, and the conditions that promote the emergence of life (the themes and priority questions discussed in Chapter 3)—to the science missions that the committee has identified as the top planetary science spacecraft activities for the coming decade (Chapter 9). The major questions forming the foundations of planetary science deal with topics that will almost certainly not be fully addressed in a single decade. Rather, many generations of scientists have already labored over them and additional generations will likely follow suit. The topics discussed in Chapter 3 are too broad and too fundamental to be fully addressed in the period 2013-2022. However, a general reader interested in the current scope of, and key motivations for undertaking, activities in the planetary sciences need only read Chapters 1, 2, and 3. Those general readers interested in a preview of the spacecraft missions recommended for implementation in the decade to come should jump to Chapter 9. A decadal plan must be based on the identification and exploitation of those components or subcomponents of the big, foundational topics showing the most promise of resolution in the coming 10 years. Chapters 4-8 contain the most basic breakdown of these foundational topics, divided largely in terms of locations in the solar system—i.e., the inner planets (Chapter 5), Mars (Chapter 6), the giant planets (Chapter 7) and their satellites (Chapter 8), and the myriad small bodies that are scattered throughout the solar system (Chapter 4). Thus, Chapters 4-8 are devoted to the identification of the particular aspects of Chapter 3’s crosscutting themes and questions showing the greatest promise for resolution in the next 10 years. Chapters 4-8 all follow the same general outline, starting with a link to key science questions in Chapter 3, outlining the science goals, identifying important questions and future directions, addressing any necessary technology development, and finally discussing potential missions. Some of the big questions can be better addressed at some specific destinations in the solar system rather than others. Chapter 4-8 lay out questions best addressed by visits to the inner planets, to Mars, to the giant planets and their satellites, and to primitive bodies like asteroids and comets, and begin to define the missions that can gather the data that can answer specific aspects of important questions. Thus, readers with a deeper interest in current planetary science research activities should concentrate on Chapters 4-8 and then move on to discussion of high priority spacecraft missions in Chapter 9. If more details are required on the research, infrastructure, and technology required to support these missions, turn to Chapters 10 and 11. Readers who are most interested in near-term matters of public policy will naturally turn to Chapters 9, 10 and 11 to understand what programs the committee has recommended to initiate or continue to fund, but they will gain a full understanding of why the committee has reached these conclusions by starting with the big questions. PREPUBLICATION COPY—SUBJECT TO FURTHER EDITORIAL CORRECTION 1-16
FIGURE 1.14 Schematic showing the flow from one chapter to the next. PREPUBLICATION COPY—SUBJECT TO FURTHER EDITORIAL CORRECTION 1-17
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PREPUBLICATION COPY Subject to Furt
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The National Academy of Sciences is
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COMMITTEE ON THE PLANETARY SCIENCE
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STAFF DAVID H. SMITH, Senior Progra
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Preface Strategic planning activiti
Page 11 and 12: statement of task’s call for “i
Page 13 and 14: Understand the Processes That Contr
Page 15 and 16: Executive Summary In recent years,
Page 17 and 18: however, that the Discovery program
Page 19 and 20: • Jupiter Europa Orbiter (descope
Page 21 and 22: TABLE ES.2 Medium Class Missions—
Page 23 and 24: Summary This report was requested b
Page 25 and 26: • Recent volcanic activity on Ven
Page 27 and 28: Mission Study Process and Technical
Page 29 and 30: Near the end of the past decade, NA
Page 31 and 32: • Mars Astrobiology Explorer-Cach
Page 33 and 34: development, and descoped or cancel
Page 35 and 36: Plausible circumstances could impro
Page 37 and 38: Data Distribution and Archiving Dat
Page 39 and 40: Sample curation facilities are crit
Page 41 and 42: consider making equivalent systems
Page 43 and 44: committee concluded that for the mo
Page 45 and 46: alanced ground-based solar astronom
Page 47 and 48: 1 Introduction to Planetary Science
Page 49 and 50: THE 2002 SOLAR SYSTEM EXPLORATION D
Page 51 and 52: Medium The first decadal survey ide
Page 53 and 54: FIGURE 1.6 Victoria crater as image
Page 55 and 56: FIGURE 1.8 The mirror for the Large
Page 57 and 58: FIGURE 1.10 From a comet, to the de
Page 59 and 60: • The committee’s programmatic
Page 61: • Opportunities for joint venture
Page 65 and 66: 2 National and International Progra
Page 67 and 68: FIGURE 2.3 Sand dunes on Mars photo
Page 69 and 70: NASA’s Earth Science Division Pla
Page 71 and 72: More recently, among the goals of t
Page 73 and 74: FIGURE 2.6 A natural bridge on the
Page 75 and 76: investigations should still be deve
Page 77 and 78: FIGURE 2.10 The surface of Titan as
Page 79 and 80: 3 Shared objectives that incorporat
Page 81 and 82: 3 Priority Questions in Planetary S
Page 83 and 84: • How have the myriad chemical an
Page 85 and 86: How Did the Giant Planets and Their
Page 87 and 88: heavy bombardment? Clues to address
Page 89 and 90: Did Mars or Venus Host Ancient Aque
Page 91 and 92: We lack critical geophysical data a
Page 93 and 94: detected in time. The report conclu
Page 95 and 96: How Have the Myriad of Chemical and
Page 97 and 98: 13. P.R. Estrada, I. Mosqueira, J.J
Page 99 and 100: 51. M.J. Mumma, G.L. Villanueva, R.
Page 101 and 102: 4 The Primitive Bodies: Building Bl
Page 103 and 104: FIGURE 4.1 Asteroids and comet nucl
Page 105 and 106: • How do the compositions of pres
Page 107 and 108: Future Directions for Investigation
Page 109 and 110: Astrobiology is the study of the or
Page 111 and 112: Important Questions Some important
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observations of the outer parts of
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Sample Curation and Laboratory Faci
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In the previous decadal survey, CCS
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asteroid (either ice-rock or metal-
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hazard. Asteroid 433 Eros, one of t
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BOX 4.1 The Discovery Program, Vita
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ody exploration can be achieved by
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34. H.H. Hsieh and D. Jewitt. 2006.
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FIGURE 5.1 Mercury, Venus, and the
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Constrain the Bulk Composition of t
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from Venus Express and Galileo may
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• Understand the composition and
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• Is there evidence of environmen
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Important Questions Some important
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timescales, including the possible
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that may have fostered life, there
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• Venus In Situ Explorer • Sout
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FIGURE 5.3 Venus’s climate is con
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Important scientific objectives tha
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BOX 5.1 Planetary Roadmaps Roadmaps
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4. D.J. Lawrence, W.C. Feldman, J.O
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6 Mars: Evolution of an Earth-like
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BOX 6.1 Mars Science Laboratory Sch
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live there now?”—both key compo
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characteristics (water, gradients i
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availability, physicochemical facto
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UNDERSTAND THE PROCESSES AND HISTOR
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FIGURE 6.4 Examples of recent clima
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particularly the polar-layered depo
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FIGURE 6.6 Geologic time sequence o
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Future Directions for Investigation
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planets and for understanding subse
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experiments, compounded by the unce
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Curation Martian samples require sc
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particle sizes, wavelength ranges,
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environmental conditions including
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Mars Polar Climate Mission As a fol
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R.E. Arvidson, C.C. Allen, D.J. Des
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27. J. Grotzinger, J.F. Bell III, W
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B.M. Jakosky and R.J. Phillips. 200
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72. White papers received by decada
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(MRR-SAG). Posted by the Mars Explo
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the solar system formed. Understand
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FIGURE 7.2 Left: This Hubble image
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temperatures, helium is enhanced in
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FIGURE 7.4 The intrinsic specific l
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Investigate the Chemistry of Giant
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Jupiters seen around other stars in
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• What causes the enormous differ
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FIGURE 7.5 Top: This composite comp
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EXPLORING THE GIANT PLANET’S ROLE
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destroy areas of land equivalent to
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• Assess tidal evolution within g
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• What processes drive the visibl
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esolution visible and near-infrared
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INTERCONNECTIONS Links to Other Par
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SUPPORTING RESEARCH AND RELATED ACT
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FIGURE 7.10 Our atmosphere blocks l
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Cassini Solstice Mission ADVANCING
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8. Determine the composition, struc
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Summary To achieve the primary goal
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Outer Solar System; William B. McKi
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TABLE 8.1 Characteristics of the La
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organisms live there now?” Titan
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• Why are Titan and Callisto appa
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Callisto but unlike Ganymede. This
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valuable window into solar system h
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FIGURE 8.6 Multiple jets, dominated
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FIGURE 8.8 Schematic of the complex
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orbits of Io and Europa), and poten
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Cassini has revealed that most of t
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satellite interiors should include
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hardened technology for Io and Gany
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FIGURE 8.11 After a comprehensive t
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FIGURE 8.12 Galileo color image of
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Titan Saturn System Mission Many Ti
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1. What is the nature of Enceladus
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the majority of the Jupiter Europa
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7. O. Mousis, J.I. Lunine, M. Pasek
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45. K.K. Khurana, M.G. Kivelson, K.
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9 Recommended Flight Investigations
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All of the recommendations below ar
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As discussed in more detail below,
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• Ensure that there are adequate
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TABLE 9.2 Discovery Program Mission
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overarching questions in Chapter 3.
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These five were selected from the s
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The Mars community, in their inputs
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should immediately undertake an eff
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(a) (b) FIGURE 9.1 Notional funding
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As noted, the recommended and cost-
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described above are the existing De
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The projected need decreased from 2
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partnership with the Department of
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10 Planetary Science Research and I
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Through the direct involvement of s
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Theoretical development and numeric
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Defining the Need Jon Miller, in hi
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efforts, can help assure compatibil
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history. And telescopic observation
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Hubble Space Telescope Hubble obser
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Although Ka-band downlink has a cle
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and Planetary Institute. Currently,
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the Green Bank Telescope (GBT), and
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up observations. Likewise, monitori
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11 The Role of Technology Developme
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particular technology item. In gene
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The Requirement for Power Of all th
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proposals and populated by technolo
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TABLE 11.1 Summary of Types of Miss
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Solar System Access and Other Core
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influence on the planetary science
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A Letter of Request and Statement o
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latter topics are treated in the NR
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main findings and recommendations s
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TABLE B.1 Institutional Distributio
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M. Gudipati, Laboratory Studies for
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Scott A. Sandford, The Comet Coma R
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C Cost and Technical Evaluation of
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were all full mission studies selec
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Schedule To aid in the assessment o
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FIGURE C.3 Complexity Based Risk As
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Lunar Lander Network⎯Four Landers
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Caching Mars Rover Mars Astrobiolog
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Mars Sample Return Lander and Mars
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Flagship‐class Europa Orbiter SOU
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Saturn Atmospheric Entry Probe SOUR
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Enceladus Orbiter Spacecraft SOURCE
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Uranus Orbiter with Entry Probe SOU
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SUMMARY Linked technical, cost, and
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Overview The purpose of this rapid
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Conclusions Based on analyses of th
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Technology development was found to
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• Characterize the local meteorol
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• Characterize Ganymede’s uniqu
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landing in the small southern lakes
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atmospheric probe and another a sep
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FIGURE E.1 Projected budget for the
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Biosphere: The life zone of Earth o
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EPOXI: The name of the extended mis
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Late heavy bombardment: A postulate
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Nili Fossae region: A fracture in t
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Protoplanet: A planet in the proces
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Stardust: A spacecraft launched in
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G Mission and Technology Study Repo
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