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Exploring the Unknown: Selected Documents in ... - The Black Vault

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746<br />

Project Apollo: Americans to <strong>the</strong> Moon<br />

Lunar “Garden<strong>in</strong>g”<br />

Geological evidence of lunar surface turnover as this applies to Apollo 11<br />

and 12 sites persuades us aga<strong>in</strong>st <strong>the</strong> existence at <strong>the</strong>se places of a protected region<br />

conta<strong>in</strong><strong>in</strong>g at least some water and organic matter, and <strong>the</strong>refore a possible abode<br />

for lunar organisms. F<strong>in</strong>ally, m<strong>in</strong>eralogical f<strong>in</strong>d<strong>in</strong>gs and evidence from isotope<br />

dat<strong>in</strong>g <strong>in</strong>dicate a k<strong>in</strong>d of sample heterogeneity which could best be expla<strong>in</strong>ed by<br />

assum<strong>in</strong>g transport of substantial amounts of material onto <strong>the</strong> mare, presumably<br />

from <strong>the</strong> neighbor<strong>in</strong>g highlands. It seems quite possible or even likely that <strong>in</strong> <strong>the</strong><br />

Apollo 11 and 12 samples, several percent may represent highland material. Even<br />

so, it would hardly be permissible to generalize from knowledge of <strong>the</strong>se two sites<br />

to <strong>the</strong> many particular local environments to be found on <strong>the</strong> moon. Much of <strong>the</strong><br />

moon is as yet unknown and thus predictions of biological significance about <strong>the</strong><br />

land<strong>in</strong>g site of Apollo 13 may be <strong>in</strong> error.<br />

Lunar Quarant<strong>in</strong>e Program<br />

We note that <strong>the</strong> Apollo 11 and 12 samples were <strong>in</strong> all likelihood from<br />

<strong>the</strong> upper surfaces of lava beds. It is <strong>the</strong>refore not surpris<strong>in</strong>g that <strong>the</strong> samples<br />

from both areas appear sterile. Any possible pre-exist<strong>in</strong>g life would have been<br />

destroyed by processes which created <strong>the</strong>se formations, and <strong>the</strong> likelihood of<br />

re<strong>in</strong>oculation from o<strong>the</strong>r (highland?) areas might have been negligible. On or<br />

near <strong>the</strong> surface, radiation and temperature extremes probably preclude growth<br />

and perhaps even survival of live organisms. In any case, o<strong>the</strong>r Apollo land<strong>in</strong>g<br />

sites are apt to have quite different and new chemical characteristics. Even <strong>the</strong><br />

two mare sites, orig<strong>in</strong>ally expected to be much <strong>the</strong> same, have turned out to be<br />

surpris<strong>in</strong>gly different. It is surely unwise to generalize from this limited Apollo<br />

sampl<strong>in</strong>g and it seems to most of us that <strong>the</strong> new <strong>in</strong>formation ga<strong>in</strong>ed from past<br />

Apollo missions is <strong>in</strong>sufficient to justify a substantial change <strong>in</strong> lunar quarant<strong>in</strong>e<br />

policy applicable to <strong>the</strong> Apollo 13 mission which is targeted for a highland land<strong>in</strong>g<br />

site. We <strong>the</strong>refore endorse <strong>the</strong> policy established by <strong>the</strong> ICBC which asserts that<br />

each time a substantially new type of lunar environment is visited or sampled a<br />

maximum back-contam<strong>in</strong>ation hazard obta<strong>in</strong>s and whatever quarant<strong>in</strong>e measures<br />

have been agreed upon for that circumstances become fully applicable.<br />

Quarant<strong>in</strong>e of Lunar Samples<br />

<strong>The</strong> overrid<strong>in</strong>g reason for cont<strong>in</strong>u<strong>in</strong>g <strong>the</strong> quarant<strong>in</strong>e of <strong>the</strong> astronauts<br />

and <strong>the</strong> lunar samples returned from <strong>the</strong> Apollo 13 mission is <strong>the</strong> possibility that<br />

materials that have not been exposed on <strong>the</strong> lunar surface for long periods will be<br />

returned <strong>in</strong> <strong>the</strong> lower portion of a drill core sample. An additional but secondary<br />

reason for cont<strong>in</strong>u<strong>in</strong>g <strong>the</strong> quarant<strong>in</strong>e is <strong>the</strong> planned return of materials that differ<br />

significantly <strong>in</strong> composition, age and orig<strong>in</strong> from <strong>the</strong> Apollo 11 and 12 samples. In<br />

previous missions <strong>the</strong> sample chosen for <strong>the</strong> biological protocol was selected to be<br />

representative of all <strong>the</strong> returned rocks and soil. Detailed study of <strong>the</strong>se rock and<br />

soil samples have not shown us that <strong>the</strong>re is little variation among <strong>the</strong> rock types.<br />

<strong>The</strong> requirement of pooled test samples has resulted <strong>in</strong> severe time constra<strong>in</strong>ts <strong>in</strong><br />

<strong>the</strong> prelim<strong>in</strong>ary exam<strong>in</strong>ations of <strong>the</strong> lunar samples. Handl<strong>in</strong>g lunar samples <strong>in</strong> <strong>the</strong><br />

LRL under quarant<strong>in</strong>e restrictions precludes some desirable operations, <strong>in</strong>troduces<br />

chemical contam<strong>in</strong>ation of <strong>the</strong> samples, and is responsible for harm<strong>in</strong>g delicate

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