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Smithsonian at the Poles: Contributions to International Polar

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392 SMITHSONIAN AT THE POLES / MCCOY, WELZENBACH, AND CORRIGAN<br />

FIGURE 4. Meteorite s<strong>to</strong>rage labor<strong>at</strong>ories <strong>at</strong> <strong>the</strong> <strong>Smithsonian</strong> Museum Support Center in Suitland, Maryland, modeled on <strong>the</strong> facility used for<br />

lunar rocks <strong>at</strong> NASA’s Johnson Space Center. The w<strong>at</strong>er- and oxygen-free nitrogen gas in <strong>the</strong> cabinets keeps meteorites from oxidizing and free<br />

from contamin<strong>at</strong>ion by environmental pollutants such as organic compounds, heavy metals, and salts, which could reduce <strong>the</strong> scientifi c value of<br />

<strong>the</strong> specimens. Pho<strong>to</strong> by Chip Clarke, SI.<br />

connected by a corridor of offi ces and labor<strong>at</strong>ories. Shortly<br />

after this facility opened, planning began for building wh<strong>at</strong><br />

became essentially a duplic<strong>at</strong>e of <strong>the</strong> dry nitrogen s<strong>to</strong>rage<br />

facility for Antarctic meteorites <strong>at</strong> Johnson Space Center in<br />

Hous<strong>to</strong>n, and <strong>the</strong> new museum s<strong>to</strong>rage facility opened in<br />

<strong>the</strong> fall of 1986. The fi rst signifi cant transfer (126 specimens)<br />

of Antarctic meteorites <strong>to</strong> <strong>the</strong> <strong>Smithsonian</strong> occurred<br />

in 1987. Regular annual transfers from Johnson Space Center<br />

<strong>to</strong> <strong>the</strong> museum began in 1992, and <strong>the</strong> fl ow of meteorites<br />

increased tremendously in 1998. At th<strong>at</strong> point, <strong>the</strong> Meteorite<br />

Processing Labor<strong>at</strong>ory <strong>at</strong> Johnson Space Center was<br />

essentially full, and <strong>the</strong> subsequent infl ux of newly recovered<br />

meteorites necessit<strong>at</strong>ed <strong>the</strong> transfer of large numbers of<br />

specimens <strong>to</strong> <strong>the</strong> SI. By <strong>the</strong> end of 2004, more than 11,300<br />

individual specimens had been transferred <strong>to</strong> <strong>the</strong> museum.<br />

When coupled with <strong>the</strong> chips and thin sections used for <strong>the</strong><br />

initial classifi c<strong>at</strong>ion, Antarctic meteorites now represent<br />

more than 80% of named meteorites in <strong>the</strong> <strong>Smithsonian</strong><br />

collection and more than 70% of all specimens. These percentages<br />

alone demonstr<strong>at</strong>e <strong>the</strong> spectacular impact of <strong>the</strong><br />

Antarctic Meteorite Program on <strong>the</strong> <strong>Smithsonian</strong>’s meteorite<br />

collection.<br />

During <strong>the</strong> 30 years of <strong>the</strong> U.S. Antarctic Meteorite<br />

Program, <strong>Smithsonian</strong> personnel have fulfi lled a number<br />

of o<strong>the</strong>r roles. The program is managed by a threemember<br />

Meteorite Steering Group with represent<strong>at</strong>ives<br />

from NASA, NSF, and <strong>the</strong> <strong>Smithsonian</strong>. Recommend<strong>at</strong>ions<br />

on sample alloc<strong>at</strong>ions are made by <strong>the</strong> Meteorite Working<br />

Group, a 10-member panel th<strong>at</strong> also includes members of<br />

<strong>the</strong> academic and research communities. <strong>Smithsonian</strong> personnel<br />

from both <strong>the</strong> N<strong>at</strong>ural His<strong>to</strong>ry Museum and <strong>the</strong><br />

Astrophysical Observ<strong>at</strong>ory have actively particip<strong>at</strong>ed or

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