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NASA Scientific and Technical Aerospace Reports

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The <strong>NASA</strong> supported project ‘Modeling of Cometary Atmospheres’ has been quite successful in broadening our<br />

underst<strong>and</strong>ing of the cometary environment. We list peer reviewed publications <strong>and</strong> conference presentation that have been<br />

made as a result of studies performed under this project. Following the list we present details of a selection of the results.<br />

Author<br />

Cometary Atmospheres; Ion Distribution; Magnetohydrodynamics<br />

20040111967 <strong>NASA</strong> Johnson Space Center, Houston, TX, USA<br />

The LEO Particulate Environment as Determined by LDEF<br />

See, Thomas H.; Zolensky, Michael E.; Hoerz, Friedrick; Bernhard, P.; Leago, Kimberly S.; Warren, Jack L.; Sapp, Clyde A.;<br />

Foster, Tammy R.; Kinard, William H.; [1993]; 11 pp.; In English; Original contains color <strong>and</strong> black <strong>and</strong> white illustrations;<br />

No Copyright; Avail: CASI; A03, Hardcopy<br />

The Meteoroid & Debris Special Investigation Group has been studying the low-Earth orbit particulate environment by<br />

examining <strong>and</strong> documenting impact craters that occurred on the Long Duration Exposure Facility (LDEF) during its 5.7 year<br />

stay in orbit.<br />

Author<br />

Debris; Long Duration Exposure Facility; Low Earth Orbits; Meteoroids; Particulates<br />

20040120953 Computer Sciences Corp., Huntsville, AL, USA<br />

Atmospheric Models for Aerocapture Systems Studies<br />

Justus, C. G.; Duvall, Aleta; Keller, Vernon W.; December 19, 2003; 5 pp.; In English; AIAA Atmospheric Flight Mechanics<br />

Symposium, 16-19 Aug. 2004, Providence, RI, USA<br />

Contract(s)/Grant(s): NAS8-60000; No Copyright; Avail: Other Sources<br />

Aerocapture uses atmospheric drag to decelerate into captured orbit from interplanetary transfer orbit. This includes<br />

capture into Earth orbit from, for example, Lunar-return or Mars-return orbit. Eight Solar System destinations have sufficient<br />

atmosphere for aerocapture to be applicable - three of the rocky planets (Venus, Earth, <strong>and</strong> Mars), four gas giants (Jupiter,<br />

Saturn, Uranus, <strong>and</strong> Neptune), <strong>and</strong> Saturn’s moon Titan. These destinations fall into two groups: (1) The rocky planets, which<br />

have warm surface temperatures (approx. 200 to 750 K) <strong>and</strong> rapid decrease of density with altitude, <strong>and</strong> (2) the gas giants <strong>and</strong><br />

Titan, which have cold temperatures (approx. 70 to 170 K) at the surface or 1-bar pressure level, <strong>and</strong> slow rate of decrease<br />

of density with altitude. The height variation of average density with altitude above 1-bar pressure level for the gas giant<br />

planets is shown. The periapsis density required for aerocapture of spacecraft having typical values of ballistic coefficient (a<br />

measure of mass per unit cross-sectional area) is also shown. The aerocapture altitudes at the gas giants would typically range<br />

from approx. 150 to 300 km. Density profiles are compared for the rocky planets with those for Titan <strong>and</strong> Neptune.<br />

Aerocapture at the rocky planets would occur at heights of approx. 50 to 100 km. For comparison, typical density <strong>and</strong> altitudes<br />

for aerobraking operations (circularizing a highly elliptical capture orbit, using multiple atmospheric passes) are also indicated.<br />

Author (revised)<br />

Atmospheric Models; Aerocapture; Aerobraking; Planetary Atmospheres<br />

20040121084 <strong>NASA</strong> Marshall Space Flight Center, Huntsville, AL, USA<br />

Computed Tomography <strong>and</strong> its Application for the 3D Characterization of Coarse Grained Meteorites<br />

Gillies, Donald C.; Engel, H. P.; Carpenter, P. K.; [2004]; 1 pp.; In English; Microscopy <strong>and</strong> Microanalysis 2004 Conference,<br />

1-5 Aug. 2004, Savannah, GA, USA; No Copyright; Avail: Other Sources; Abstract Only<br />

With judicious selection of parameters, computed tomography can provide high precision density data. Such data can lead<br />

to a non-destructive determination of the phases <strong>and</strong> phase distribution within large solid objects. Of particular interest is the<br />

structure of the Mundrabilla meteorite, which has 25 volumes, percent of a sulfide within a metallic meteorite. 3D digital<br />

imaging has enabled a quantitative evaluation of the distribution <strong>and</strong> contiguity of the phases to be determined.<br />

Author<br />

Meteorites; Tomography; Three Dimensional Models; Microscopy<br />

20040121128 Aviation Week <strong>and</strong> Space Technology, USA<br />

Making Tracks at JPL<br />

Covault, Craig; Aviation Week <strong>and</strong> Space Technology; June 21, 2004; Volume 160, No. 25, pp. 66-67; In English; Original<br />

contains black <strong>and</strong> white illustrations; Copyright; Avail: Other Sources<br />

The President’s commission on manned <strong>and</strong> unmanned lunar <strong>and</strong> Mars exploration is calling for redefinition of the U.S.<br />

322

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