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

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impacts on Earth have played <strong>in</strong> mass ext<strong>in</strong>ction events, <strong>and</strong> <strong>the</strong>y still pose a modern day hazard. “How<br />

have <strong>the</strong> myriad chemical <strong>and</strong> physical properties that shaped <strong>the</strong> solar system operated, <strong>in</strong>teracted, <strong>and</strong><br />

evolved over time?” is a question that is directly addressed by <strong>the</strong> study of <strong>the</strong>ir role <strong>in</strong> accretion <strong>and</strong><br />

subsequent bombardment through time, <strong>in</strong> particular as <strong>the</strong>se bodies are believed to have served an<br />

important role <strong>in</strong> deliver<strong>in</strong>g organic materials <strong>and</strong> water to <strong>the</strong> <strong>in</strong>ner planets, particularly Earth.<br />

<strong>and</strong><br />

SCIENCE GOALS FOR THE STUDY OF PRIMITIVE BODIES<br />

The goals <strong>for</strong> research on primitive bodies <strong>for</strong> <strong>the</strong> next decade are twofold:<br />

• Decipher <strong>the</strong> record <strong>in</strong> primitive bodies of epochs <strong>and</strong> processes not obta<strong>in</strong>able elsewhere,<br />

• Underst<strong>and</strong> <strong>the</strong> role of primitive bodies as build<strong>in</strong>g blocks <strong>for</strong> planets <strong>and</strong> life.<br />

DECIPHER THE RECORD IN PRIMITIVE BODIES<br />

OF EPOCHS AND PROCESSES NOT OBTAINED ELSEWHERE<br />

Primitive bodies, be <strong>the</strong>y asteroids, comets, KBOs, possibly <strong>the</strong> martian moons, meteorites or<br />

IDPs—are thought to have <strong>for</strong>med earlier than <strong>the</strong> planets <strong>in</strong> <strong>the</strong> hierarchical assembly of solar system<br />

bodies. Because <strong>the</strong>y witnessed, or participated <strong>in</strong>, many of <strong>the</strong> <strong>for</strong>mative processes <strong>in</strong> <strong>the</strong> early solar<br />

nebula, <strong>the</strong>y can provide unique constra<strong>in</strong>ts on physical conditions <strong>and</strong> cosmochemical abundances. Such<br />

constra<strong>in</strong>ts come, <strong>in</strong> part, from observations <strong>and</strong> remote-sens<strong>in</strong>g measurements made from nearby<br />

spacecraft. Because we can visit only a small number of <strong>the</strong> myriad, highly diverse primitive bodies, we<br />

must also observe <strong>the</strong>m us<strong>in</strong>g Earth-based telescopes. Constra<strong>in</strong>ts on nebular processes, as well as<br />

absolute dat<strong>in</strong>g of events <strong>in</strong> <strong>the</strong> early solar system, also come from laboratory analyses of samples of<br />

<strong>the</strong>se bodies, whe<strong>the</strong>r collected <strong>and</strong> returned to Earth by spacecraft missions or obta<strong>in</strong>ed by <strong>the</strong> vagaries<br />

of celestial mechanics. The least-processed of <strong>the</strong>se samples conta<strong>in</strong> small amounts of t<strong>in</strong>y presolar<br />

gra<strong>in</strong>s, whose properties <strong>and</strong> compositions constra<strong>in</strong> astrophysical processes that predate <strong>the</strong> solar system.<br />

TABLE 4.1 Major Accomplishments by Telescopes <strong>and</strong> Space-based Studies of Primitive Bodies <strong>in</strong> <strong>the</strong><br />

Past Decade<br />

Major Accomplishment Mission <strong>and</strong>/or Technique<br />

Detailed orbital characterization of an asteroid, <strong>in</strong>clud<strong>in</strong>g successful l<strong>and</strong><strong>in</strong>g Near-Earth Asteroid Rendezvous<br />

Sampled a near-Earth asteroid <strong>and</strong> returned <strong>the</strong> sample to Earth; determ<strong>in</strong>ed Hayabusa<br />

that small asteroids can be rubble piles<br />

Determ<strong>in</strong>ed <strong>the</strong> density of a comet nucleus via <strong>the</strong> first controlled crater<strong>in</strong>g Deep Impact<br />

experiment on a primitive body<br />

Return of comet dust <strong>for</strong> analysis <strong>in</strong> terrestrial laboratories Stardust<br />

First reconnaissance of a possible <strong>for</strong>mer trans-Neptune object <strong>in</strong> <strong>the</strong> <strong>for</strong>m of Cass<strong>in</strong>i<br />

Saturn’s distant satellite, Phoebe<br />

Discovered that b<strong>in</strong>ary objects are common among near-Earth <strong>and</strong> ma<strong>in</strong> belt<br />

asteroids <strong>and</strong> Kuiper belt objects, <strong>and</strong> that comets occur with<strong>in</strong> <strong>the</strong> ma<strong>in</strong><br />

asteroid belt.<br />

Ground- <strong>and</strong> space-based<br />

telescopes <strong>and</strong> radar studies<br />

PREPUBLICATION COPY—SUBJECT TO FURTHER EDITORIAL CORRECTION<br />

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