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

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Protoplanet: A planet <strong>in</strong> <strong>the</strong> process of accretion from material <strong>in</strong> a protoplanetary disk.<br />

Protoplanetary disk: A circumstellar disk of matter, <strong>in</strong>clud<strong>in</strong>g gas <strong>and</strong> dust, from which planets may<br />

eventually <strong>for</strong>m or be <strong>in</strong> <strong>the</strong> process of <strong>for</strong>m<strong>in</strong>g.<br />

238 Pu: An isotope of plutonium whose physical properties make it ideally suited <strong>for</strong> use as a heat source<br />

<strong>in</strong> radioisotope power systems.<br />

Pyroclastic: Rocks composed solely or primarily of fragments of volcanic materials.<br />

Pyrrhotite: An unusual iron sulfide m<strong>in</strong>eral with a variable iron content.<br />

Q factor: A parameter which describes how under-damped an oscillatory system is; <strong>the</strong> higher <strong>the</strong> Q, <strong>the</strong><br />

more slowly oscillations die out after be<strong>in</strong>g excited.<br />

R&A: Research <strong>and</strong> Analysis.<br />

Radiative balance: Account<strong>in</strong>g <strong>for</strong> all sources of <strong>in</strong>go<strong>in</strong>g <strong>and</strong> outgo<strong>in</strong>g sources of radiation <strong>in</strong> a system.<br />

Radiogenic heat<strong>in</strong>g: The <strong>the</strong>rmal energy released by <strong>the</strong> decay of naturally occurr<strong>in</strong>g radioactive<br />

materials.<br />

Radiolysis: The dissociation of molecules by ioniz<strong>in</strong>g radiation.<br />

Radionuclides: A radioactive nuclide.<br />

Redox reaction: Any of a large class of chemical reactions characterized by <strong>the</strong> reduction of one<br />

reactant <strong>and</strong> <strong>the</strong> simultaneous oxidation of ano<strong>the</strong>r.<br />

Regolith: The layer of dust <strong>and</strong> fragmented rocky debris which <strong>for</strong>ms <strong>the</strong> uppermost surface on many<br />

planets, satellites, <strong>and</strong> asteroids. It is <strong>for</strong>med by a variety of process <strong>in</strong>clud<strong>in</strong>g meteoritic impact,<br />

REP: Radioisotope Electric Propulsion.<br />

Retrograde: Orbital motion or rotation <strong>in</strong> a clockwise direction as viewed from <strong>the</strong> north pole of <strong>the</strong><br />

ecliptic or of <strong>the</strong> rotat<strong>in</strong>g object; i.e., <strong>in</strong> <strong>the</strong> opposite sense to <strong>the</strong> rotation of Earth <strong>and</strong> most of <strong>the</strong> o<strong>the</strong>r<br />

planetary bodies <strong>in</strong> <strong>the</strong> solar system.<br />

REU: Research Experience <strong>for</strong> Undergraduates program.<br />

ROSES: Research Opportunities <strong>in</strong> Space <strong>and</strong> Earth <strong>Science</strong>s.<br />

Rosetta: A European Space Agency spacecraft, launched <strong>in</strong> 2004, that will rendezvous with Comet<br />

67P/Churyumov-Gerasimenko <strong>in</strong> 2014, fly<strong>in</strong>g past two asteroids on <strong>the</strong> way.<br />

RPS: Radioisotope Power <strong>System</strong>s.<br />

SALMON: NASA’s St<strong>and</strong>-Alone Mission of Opportunity program.<br />

SDT: <strong>Science</strong> Def<strong>in</strong>ition Team.<br />

SED: Spectral Energy Distribution.<br />

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

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