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

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The projected need decreased from 2008 to 2010 largely due to dropp<strong>in</strong>g <strong>the</strong> lunar rovers<br />

associated with <strong>the</strong> Constellation program (56 kg of plutonium), but also due to a better underst<strong>and</strong><strong>in</strong>g of<br />

requirements. The current plan assumes an additional 10 kg of plutonium-238 will be purchased from<br />

Russia, <strong>and</strong> that an average of 1.5 kg/year of new domestic production can beg<strong>in</strong>, but no earlier than<br />

2015. The Russian purchase is subject to ongo<strong>in</strong>g negotiations, <strong>and</strong> monies <strong>for</strong> startup of domestic<br />

production were rejected <strong>in</strong> 2010 by <strong>the</strong> Congress. Hence, nei<strong>the</strong>r of <strong>the</strong>se sources is assured at this time,<br />

<strong>and</strong> without at least 5 kg of new material from Russia as well as renewed production, NASA’s current<br />

plans <strong>for</strong> future planetary missions cannot be carried out.<br />

This decadal survey recommends a variety of missions <strong>and</strong> mission c<strong>and</strong>idates (under <strong>the</strong> New<br />

Frontiers program) that require RPSs. As such, <strong>the</strong>se recommendations would modify NASA’s 2010<br />

requirements to some degree. The current supply of plutonium-238 is sufficient to fuel four MMRTGs<br />

plus three ASRGs, or 19 ASRGs, or cases <strong>in</strong> between.<br />

TABLE 9.5 Comparison of NASA Requirements <strong>for</strong> Plutonium-238 as Reported to DOE <strong>in</strong> 2008 <strong>and</strong><br />

2010<br />

Mission<br />

Projected<br />

Launch<br />

NASA Adm<strong>in</strong>istrator Letter<br />

of 29 Apr 2008<br />

Power<br />

(We)<br />

Pu-238<br />

Usage (kg)<br />

NASA Adm<strong>in</strong>istrator Letter<br />

of 25 Mar 2010<br />

Projected<br />

Launch<br />

Power<br />

(We)<br />

Mars <strong>Science</strong> Lab 2009 100 3.5 2011 100 3.5<br />

Lunar Precursor Not <strong>in</strong> plan 2015 280 1.8<br />

Mars (RPS <strong>and</strong> Heater Units) Not <strong>in</strong> plan 2018 280 1.8<br />

Outer Planets Flagship 1 2017 700-850 24.6 2020 612 21.3<br />

Discovery 12 2014 250 1.8 2015 280 1.8<br />

Discovery 14 2020 500 3.5 2021 280 1.8<br />

New Frontiers 4 2021 800 5.3 2022 280 1.8<br />

New Frontiers 5 2026 250-800 1.8-5.3 2027 280 1.8<br />

Discovery 16 2026 500 3.5 2027 280 1.8<br />

Outer Planets Flagship 2 2027 600-1000 5.3-6.2 Deleted from plan<br />

Pressurized Rover #1 2022 2000 14<br />

ATHLETE Rover 2024 2000 14<br />

Pressurized Rover #2 2026 2000 14<br />

Pressurized Rover #3 2028 2000 14<br />

Pu-238<br />

Usage<br />

(kg)<br />

Projected ESMD requirements deleted<br />

<strong>for</strong> human missions<br />

The largest user of plutonium-238 is any mission that basel<strong>in</strong>es MMRTGs ra<strong>the</strong>r than ASRGs.<br />

Currently this only applies to JEO, <strong>for</strong> which five MMRTGs are basel<strong>in</strong>ed—i.e., one more than can be<br />

supported by <strong>the</strong> current supply of Pu-238. The Titan Saturn <strong>System</strong> Mission is <strong>the</strong> only o<strong>the</strong>r mission<br />

that basel<strong>in</strong>es MMRTG use, <strong>and</strong> it is deferred until <strong>the</strong> decade subsequent to this study.<br />

None of <strong>the</strong> recommended Mars missions use an RPS. Of <strong>the</strong> potential New Frontiers missions<br />

requir<strong>in</strong>g RPSs, Io Observer requires two ASRGs, LGN four, Saturn Probe two, <strong>and</strong> Trojan Tour <strong>and</strong><br />

Rendezvous two. Hence, a maximum of six ASRGs <strong>for</strong> two New Frontiers missions brackets potential<br />

requirements. The Uranus Orbiter <strong>and</strong> Probe <strong>and</strong> <strong>the</strong> Enceladus Orbiter each require three ASRGs, <strong>and</strong><br />

cannot be carried out with MMRTGs due to <strong>the</strong> latter’s prohibitive mass. Discovery 12 is needed to<br />

qualify ASRGs, <strong>and</strong> Discovery 14 <strong>and</strong> 16 could potentially use <strong>the</strong>se as well—each is currently basel<strong>in</strong>ed<br />

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

9-25

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