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

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l<strong>and</strong><strong>in</strong>g <strong>in</strong> <strong>the</strong> small sou<strong>the</strong>rn lakes challeng<strong>in</strong>g; all architectures thus assumed l<strong>and</strong><strong>in</strong>gs on <strong>the</strong> much<br />

larger Kraken Mare <strong>in</strong> <strong>the</strong> north. A requirement to target Kraken Mare constra<strong>in</strong>ed <strong>the</strong> trajectory of <strong>the</strong><br />

DTE mission s<strong>in</strong>ce <strong>the</strong> likely launch opportunity left little time be<strong>for</strong>e Earth would no longer be <strong>in</strong> view<br />

from <strong>the</strong> lake surface. Consequently, a high C3 trajectory was required <strong>for</strong> this architecture to reduce<br />

travel time to Titan, <strong>in</strong>creas<strong>in</strong>g launch mass <strong>and</strong> launch costs.<br />

Conclusions<br />

The exploration of Titan’s hydrocarbon lakes has high scientific potential <strong>and</strong> <strong>the</strong> Titan lake<br />

l<strong>and</strong>er concepts appear feasible. However, based on <strong>the</strong> costs <strong>and</strong> <strong>the</strong> relatively limited science scope of a<br />

st<strong>and</strong>-alone lake probe without <strong>the</strong> orbiter <strong>and</strong> balloon elements, <strong>the</strong> st<strong>and</strong>-alone lake probe concepts were<br />

judged to be lower priority than a lake probe which was an element of a flagship mission, or some of <strong>the</strong><br />

o<strong>the</strong>r mission concepts studied. The cryogenic environment <strong>and</strong> lack of heritage <strong>in</strong> lake probe design<br />

necessitates strategic <strong>in</strong>vestment <strong>in</strong> technology development, <strong>in</strong>clud<strong>in</strong>g cryogenic sample acquisition <strong>and</strong><br />

h<strong>and</strong>l<strong>in</strong>g.<br />

CHIRON ORBITER<br />

A mission concept study per<strong>for</strong>med by NASA’s Goddard Space Flight Center.<br />

Overview<br />

The purpose of this rapid mission architecture study was to determ<strong>in</strong>e several options <strong>for</strong><br />

deliver<strong>in</strong>g a useful payload <strong>in</strong>to orbit around Chiron. The five options discussed focused ma<strong>in</strong>ly on <strong>the</strong><br />

propulsion <strong>and</strong> trajectories needed to place a satellite, with a given science package, <strong>in</strong>to orbit around<br />

Chiron.<br />

<strong>Science</strong> Objectives<br />

• Observe current geologic state <strong>and</strong> composition of surface <strong>and</strong> <strong>in</strong>fer past evolution <strong>and</strong><br />

relative importance of surface processes.<br />

• Observe <strong>and</strong> measure <strong>the</strong> sporadic outgass<strong>in</strong>g activity <strong>and</strong> determ<strong>in</strong>e <strong>the</strong> composition of<br />

outgassed volatiles.<br />

• Characterize bulk properties <strong>and</strong> <strong>in</strong>terior structure.<br />

Mission Design<br />

The majority of <strong>the</strong> eng<strong>in</strong>eer<strong>in</strong>g work <strong>for</strong> this study was spent on propulsion, power, <strong>and</strong><br />

trajectory trades to def<strong>in</strong>e how <strong>the</strong> science payload could be delivered to Chiron with<strong>in</strong> <strong>the</strong> given<br />

constra<strong>in</strong>ts, leav<strong>in</strong>g less resource <strong>for</strong> <strong>the</strong> def<strong>in</strong>ition of <strong>the</strong> science package. Several trajectories <strong>for</strong> flights<br />

between Earth <strong>and</strong> Chiron <strong>in</strong>clud<strong>in</strong>g both direct <strong>and</strong> flyby orbital trajectories were exam<strong>in</strong>ed. Launch was<br />

determ<strong>in</strong>ed to occur between 2019 <strong>and</strong> 2025 depend<strong>in</strong>g on propulsion option, with a cruise phase duration<br />

between 11 <strong>and</strong> 13 years.<br />

None of <strong>the</strong> prelim<strong>in</strong>ary propulsion solutions deliver an acceptable mass to Chiron with an 11year<br />

transit time; however, five propulsion options were determ<strong>in</strong>ed that could deliver acceptable masses<br />

<strong>in</strong>to Chiron Orbit with a 13-year transit time as <strong>the</strong> basel<strong>in</strong>e.<br />

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

D-12

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