Vision and Voyages for Planetary Science in the - Solar System ...
Vision and Voyages for Planetary Science in the - Solar System ...
Vision and Voyages for Planetary Science in the - Solar System ...
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Near <strong>the</strong> end of <strong>the</strong> past decade, NASA <strong>in</strong>troduced a new acquisition vehicle called St<strong>and</strong> Alone<br />
Missions of Opportunity (SALMON). In addition to <strong>the</strong>ir science return, Missions of Opportunity provide<br />
a chance <strong>for</strong> new entrants to jo<strong>in</strong> <strong>the</strong> field, <strong>for</strong> technologies to be validated, <strong>and</strong> <strong>for</strong> future PIs to ga<strong>in</strong><br />
experience. The committee welcomes <strong>the</strong> <strong>in</strong>troduction of this highly flexible SALMON approach,<br />
<strong>and</strong> recommends that it be used wherever possible to facilitate Mission of Opportunity<br />
collaborations.<br />
An important special case of a small mission is <strong>the</strong> proposed jo<strong>in</strong>t European Space Agency<br />
(ESA)/NASA Mars Trace Gas Orbiter. The mission would launch <strong>in</strong> 2016, with NASA provid<strong>in</strong>g <strong>the</strong><br />
launch vehicle, ESA provid<strong>in</strong>g <strong>the</strong> orbiter, <strong>and</strong> a jo<strong>in</strong>t science payload that was recently selected. Based<br />
on its high science value <strong>and</strong> its relatively low cost to NASA, <strong>the</strong> committee supports flight of <strong>the</strong><br />
Mars Trace Gas Orbiter <strong>in</strong> 2016 as long as this division of responsibilities with ESA is preserved.<br />
Medium Missions<br />
The New Frontiers program allows <strong>for</strong> competitive selection of focused, strategic missions to<br />
conduct high-quality science. The current New Frontiers cost cap, <strong>in</strong>flated to FY2015 dollars, is $1.05<br />
billion, <strong>in</strong>clud<strong>in</strong>g launch vehicle costs. The committee recommends chang<strong>in</strong>g <strong>the</strong> New Frontiers cost<br />
cap to $1.0 billion FY2015, exclud<strong>in</strong>g launch vehicle costs. This change represents a modest <strong>in</strong>crease<br />
<strong>in</strong> <strong>the</strong> total cost of a New Frontiers mission provided that <strong>the</strong> cost of launch vehicles does not rise<br />
precipitously; <strong>the</strong> <strong>in</strong>crease is fully accounted <strong>for</strong> <strong>in</strong> <strong>the</strong> program recommendations below. This change<br />
will allow a scientifically rich <strong>and</strong> diverse set of New Frontiers missions to be carried out. Importantly, it<br />
will also help protect <strong>the</strong> science content of <strong>the</strong> New Frontiers program aga<strong>in</strong>st <strong>in</strong>creases <strong>and</strong> volatility <strong>in</strong><br />
launch vehicle costs.<br />
The New Frontiers program to date has resulted <strong>in</strong> <strong>the</strong> selection of <strong>the</strong> New Horizons mission to<br />
Pluto <strong>and</strong> <strong>the</strong> Juno mission to Jupiter. The <strong>for</strong>mer is <strong>in</strong> flight <strong>and</strong> <strong>the</strong> latter is <strong>in</strong> development. A<br />
competition to select a third New Frontiers mission is now underway, with selection scheduled <strong>for</strong> 2011.<br />
In this report <strong>the</strong> committee addresses subsequent New Frontiers missions, beg<strong>in</strong>n<strong>in</strong>g with <strong>the</strong> fourth, to<br />
be selected dur<strong>in</strong>g <strong>the</strong> decade 2013-2022.<br />
Based on <strong>the</strong>ir science value <strong>and</strong> projected costs, <strong>the</strong> committee has identified seven c<strong>and</strong>idate<br />
New Frontiers missions <strong>for</strong> <strong>the</strong> decade 2013-2022. All are judged to be plausibly achievable with<strong>in</strong> <strong>the</strong><br />
recommended New Frontiers cost cap (although, <strong>for</strong> some, not with<strong>in</strong> <strong>the</strong> previous cap). In alphabetical<br />
order, <strong>the</strong>y are:<br />
• Comet Surface Sample Return—The objective of this mission is to acquire <strong>and</strong> return to Earth<br />
a macroscopic sample from <strong>the</strong> surface of a comet nucleus us<strong>in</strong>g a sampl<strong>in</strong>g technique that preserves<br />
organic material <strong>in</strong> <strong>the</strong> sample.<br />
• Io Observer—The focus of this mission is to determ<strong>in</strong>e <strong>the</strong> <strong>in</strong>ternal structure of Io <strong>and</strong> to<br />
<strong>in</strong>vestigate <strong>the</strong> mechanisms that contribute to <strong>the</strong> satellite’s <strong>in</strong>tense volcanic activity from a highly<br />
elliptical orbit around Jupiter, mak<strong>in</strong>g multiple flybys of Io.<br />
• Lunar Geophysical Network—This mission consists of several identical l<strong>and</strong>ers distributed<br />
across <strong>the</strong> lunar surface, each carry<strong>in</strong>g geophysical <strong>in</strong>strumentation. The primary science objectives are<br />
to characterize <strong>the</strong> Moon’s <strong>in</strong>ternal structure, seismic activity, global heat flow budget, bulk composition,<br />
<strong>and</strong> magnetic field.<br />
• Lunar South Pole-Aitken Bas<strong>in</strong> Sample Return—The primary science objective of this<br />
mission is to return samples from this ancient <strong>and</strong> deeply excavated impact bas<strong>in</strong> to Earth <strong>for</strong><br />
characterization <strong>and</strong> study.<br />
• Saturn Probe—This mission would deploy a probe <strong>in</strong>to Saturn’s atmosphere to determ<strong>in</strong>e <strong>the</strong><br />
structure of <strong>the</strong> atmosphere as well as noble gas abundances <strong>and</strong> isotopic ratios of hydrogen, carbon,<br />
nitrogen, <strong>and</strong> oxygen.<br />
PREPUBLICATION COPY—SUBJECT TO FURTHER EDITORIAL CORRECTION<br />
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