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NASA Scientific and Technical Aerospace Reports

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20040070922 <strong>NASA</strong> Marshall Space Flight Center, Huntsville, AL, USA<br />

Crystallization of a Li2O2SiO2 Glass under High Hydrostatic Pressures<br />

Fuss, T.; Day, D. E.; Lesher, C. E.; Ray, C. S.; [2004]; 1 pp.; In English; 106th Annual Meeting of the American Ceramic<br />

Society, 18-21 Apr. 2004, Indianapolis, IN, USA<br />

Contract(s)/Grant(s): NAG8-1465; No Copyright; Avail: Other Sources; Abstract Only<br />

The crystallization behavior of a Li2O.2SiO2 (LS2) glass subjected to a uniform hydrostatic pressure of 4.5 or 6 GPa was<br />

investigated between 550 <strong>and</strong> 800 C using XRD, IR, Raman, TEM, NMR, <strong>and</strong> DTA. The density of the glass subjected to 6<br />

GPa was between 2.52 plus or minus 0.01 <strong>and</strong> 2.57 plus or minus 0.01 grams per cubic centimeters, depending upon the<br />

processing temperatures, <strong>and</strong> was higher than that of the stoichiometric LS2 crystals, 2.46 plus or minus 0.01 grams per cubic<br />

centimeter. Thus, crystallization in 6 GPa glass occurred in a condition of negative volume dilatation, deltaV = V(sub glass)<br />

- V(sub crystal), while that for the 4.5 GPa glass occurred in the condition deltaV greater than 0. For deltaV greater than 0,<br />

which also includes the control glass at ambient (one atmosphere) pressure, the glasses always crystallize Li2Si2O5<br />

(orthorhombic, Ccc2) crystals, but for deltaV less than 0 (6 GPa), the glasses crystallize Li2SiO3 crystals with a slightly<br />

deformed structure. The crystal growth rate vs. temperature curve moved to higher temperature with increasing pressure, <strong>and</strong><br />

was independent of the sign of deltaV. These results for the effect of hydrostatic pressure on the crystallization of LS2 glass<br />

were discussed from thermodynamic considerations.<br />

Author<br />

Crystallization; Hydrostatic Pressure; Lithium Compounds; Silicon Dioxide; Glass; High Pressure<br />

20040070958 Planetary Science Inst., Tucson, AZ, USA<br />

Observing the Sky <strong>and</strong> Lunar Photo of the Day: Two New Astronomy Education Web Sites<br />

Wood, C. A.; Brausch, J.; Kramer, R.; Ayiomamitis, A.; Lunar <strong>and</strong> Planetary Science XXXV: Engaging K-12 Educators,<br />

Students <strong>and</strong> the General Public in Space Science Exploration; 2004; 1 pp.; In English; Lunar <strong>and</strong> Planetary Science XXXV,<br />

15-19 Mar. 2004, Houston, TX, USA; No Copyright; Avail: CASI; C01, CD-ROM; A01, Hardcopy<br />

The Internet provides the most direct way for scientists to communicate with large numbers of people around the world,<br />

without the distortions often introduced by traditional media. Thus, the Internet is the ideal medium for large-scale scientific<br />

public outreach. Having previously reached as many as 4,000,000 unique visitors per year with VolcanoWorld (http://<br />

volcano.und.edu), a <strong>NASA</strong>-funded web site that provided information direct from PhD volcanologists, we have developed two<br />

new astronomy-related web sites to provide accurate <strong>and</strong> interesting information to teachers, students <strong>and</strong> the public.<br />

Derived from text<br />

Education; Websites; Lunar Photographs; <strong>NASA</strong> Space Programs; Astronomy; Volcanology<br />

20040071004 Agnes Scott Coll., Decatur, GA, USA<br />

Public Enthusiasm Generated by the 2003 Mars Opposition <strong>and</strong> L<strong>and</strong>ing of the Exploration Rovers<br />

Crane, A. N.; Albin, E. F.; Lunar <strong>and</strong> Planetary Science XXXV: Engaging K-12 Educators, Students <strong>and</strong> the General Public<br />

in Space Science Exploration; 2004; 1 pp.; In English; Lunar <strong>and</strong> Planetary Science XXXV, 15-19 Mar. 2004, Houston, TX,<br />

USA; Copyright; Avail: CASI; C01, CD-ROM; A01, Hardcopy<br />

Interest in Mars is at an all time high. For many weeks leading up to <strong>and</strong> after August 27th or, the date of opposition,<br />

record crowds flocked to observatories for a look at Mars. Public enthusiasm was just as high upon the l<strong>and</strong>ing on the two<br />

exploration rovers in January 2004. Even after the media &quot;dropped&quot; the event <strong>and</strong> moved on to other stories, the<br />

public response was still strong. It is suggested that such overwhelming public enthusiasm can be taken as good reason to seek<br />

a higher level of government funding for the exploration of the Red Planet. Observations <strong>and</strong> impressions of the public<br />

response to the 2003 close approach <strong>and</strong> exploration rover l<strong>and</strong>ings on Mars were taken from our affiliation with the Fernbank<br />

Science Center in Atlanta, Georgia -- a museum which houses a well equipped planetarium <strong>and</strong> observatory. Fernbank staff<br />

produced an original planetarium presentation entitled &quot;Visions of Mars.&quot; Due to overflow crowds, special<br />

extended showings were offered. After the planetarium program, members of the public were invited to the observatory for<br />

a look at Mars. On many evenings, centered around opposition, the observatory remained open from 9:00 p.m. until 5:30 a.m.<br />

the following morning. On each of these nights, we estimate that at least 950 people saw Mars through our telescope. An<br />

important tool, the CCD video camera, proved invaluable in preparing observers for their actual observation of Mars. The<br />

Mars mania continues. Two Mars Exploration Rovers were launched toward the Red Planet in the summer of 2003. These<br />

probes, Spirit <strong>and</strong> Opportunity, l<strong>and</strong>ed on Mars in January 2004 .<br />

Derived from text<br />

Mars Exploration; Mars Roving Vehicles; Mars L<strong>and</strong>ing<br />

326

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