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

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Conclusions<br />

Based on analyses of <strong>the</strong> mechanical, <strong>the</strong>rmal, power, avionics, <strong>and</strong> communication designs <strong>for</strong><br />

<strong>the</strong> probe <strong>and</strong> <strong>the</strong> carrier spacecraft, a Venus mission us<strong>in</strong>g <strong>the</strong> metallic bellows architecture <strong>for</strong> shortlived<br />

(~5 hrs) aerial mobility is technically feasible. The cost estimate <strong>for</strong> <strong>the</strong> nom<strong>in</strong>al basel<strong>in</strong>e mission<br />

was estimated to be <strong>in</strong> <strong>the</strong> flagship range. The cost is driven by <strong>the</strong> metallic bellows <strong>and</strong> support<strong>in</strong>g<br />

mechanisms <strong>for</strong> its operation. Technology development, accommodation, <strong>and</strong> complex <strong>in</strong>tegration also<br />

contribute to <strong>the</strong> high cost of <strong>the</strong> probe.<br />

VENUS INTREPID TESSERA LANDER<br />

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

Research Center.<br />

Overview<br />

The purpose of this enhanced rapid mission architecture study was to <strong>in</strong>vestigate a mission<br />

capable of safely l<strong>and</strong><strong>in</strong>g <strong>in</strong> one of <strong>the</strong> mounta<strong>in</strong>ous tessera regions of Venus. This mission concept<br />

provides key measurements of surface chemistry <strong>and</strong> m<strong>in</strong>eralogy <strong>and</strong> imag<strong>in</strong>g of a tessera region, as well<br />

as new measurements of important atmospheric species that can answer fundamental questions about <strong>the</strong><br />

evolution of Venus.<br />

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

• Characterize chemistry <strong>and</strong> m<strong>in</strong>eralogy of <strong>the</strong> Venus surface.<br />

• Place constra<strong>in</strong>ts on <strong>the</strong> size <strong>and</strong> temporal extent of a possible ocean <strong>in</strong> Venus’s past.<br />

• Characterize <strong>the</strong> morphology <strong>and</strong> relative stratigraphy of surface units.<br />

Mission Design<br />

The mission design elements <strong>in</strong>clude a carrier spacecraft to be used as a communications relay<br />

<strong>and</strong> a two-element probe. The probe elements are: <strong>the</strong> Venus l<strong>and</strong>er; <strong>and</strong> <strong>the</strong> entry <strong>and</strong> descent element<br />

<strong>in</strong>clud<strong>in</strong>g aeroshell <strong>and</strong> parachute systems. The l<strong>and</strong>er’s design focuses on enabl<strong>in</strong>g a safe l<strong>and</strong><strong>in</strong>g <strong>in</strong> <strong>the</strong><br />

rough tessera terra<strong>in</strong>. The launch opportunity considered was <strong>for</strong> 2021, with fly-by <strong>and</strong> descent/l<strong>and</strong><strong>in</strong>g<br />

mission elements <strong>in</strong> 2022.<br />

Mission Challenges<br />

The most significant challenges posed by this mission were related to <strong>the</strong> development of a high-<br />

TRL level Raman/laser-<strong>in</strong>duced breakdown spectroscopy (LIBS) system, safe l<strong>and</strong><strong>in</strong>g, <strong>and</strong> test<strong>in</strong>g at<br />

Venus environmental conditions. To reduce risk, advancements <strong>in</strong> two key technology areas are needed:<br />

first, verify<strong>in</strong>g <strong>the</strong> Raman/LIBS implementation, calibrated operation, <strong>and</strong> siz<strong>in</strong>g <strong>for</strong> <strong>the</strong> Venus surface<br />

environment, <strong>in</strong>clud<strong>in</strong>g high entry loads on <strong>the</strong> laser <strong>and</strong> second, additional analyses <strong>and</strong> test<strong>in</strong>g to ensure<br />

safe l<strong>and</strong><strong>in</strong>g <strong>in</strong> potentially rugged terra<strong>in</strong>s (at l<strong>and</strong>er scales).<br />

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

D-4

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