[meteorite-list] New Report on Hubble Space Telescope Impact Damage
From: Ron Baalke <baalke_at_meteoritecentral.com>
Date: Thu Apr 22 09:54:03 2004 Message-ID: <200202121552.HAA02560_at_zagami.jpl.nasa.gov> New Report on Hubble Space Telescope Impact Damage Orbital Debris Quarterly Johnson Space Center January 2002 The Image Science and Analysis Group at the NASA Johnson Space Center has just released its latest assessment of small particle damage to the HST in Survey of the Hubble Space Telescope Micrometeoroid and Orbital Debris Impacts From Space Shuttle Service Mission 3A Imagery (JSC-29539). Prepared primarily by David Bretz and the late Leif Anenson, the report characterizes the results of a special investigation of HST photographs from the December 1999 mission of STS-103 to identify high velocity impact features. A similar analysis was performed following the second HST servicing mission by STS-82 (see Survey of the Hubble Space Telescope Micrometeoroid and Orbital Debris Impacts from Service Mission 2 Imagery, JSC-28472, 1998). During the STS-103 mission the Electronic Still Camera (ESC) was used from inside the Space Shuttle crew cabin to map all visible areas of the body of HST using a 80-200 mm lens at full zoom (200 mm) and to image selected areas with the 400 mm telephoto lens. Astronaut Scott Kelly was the primary survey photographer, who underwent preflight training for this mission task. A total of 99 images (50 with the 200 mm lens and 49 with the 400 mm lens) were taken from the aft flight deck. Many of these images were selected for special particle impact analysis. In all, 571 impact features (strikes) were selected for characterization and measurement: 398 in the 200 mm lens images and 173 in the 400 mm lens images. Where possible, the dimensions of both the central hole and the outer delamination ring were measured. The most prevalent hole size seen in the 200 mm lens images was 2-3 mm, but the higher resolution 400 mm lens images yielded a majority of hole diameters in the 1-2 mm range. The delamination ring diameters typically are twice the size of the associated hole. One of the most important metrics for determining the flux of the particle environment is the density (number per square meter) of impacts. Average impact densities of about 45/m2 were found on the -V3 quadrant of HST. This is a cumulative effect over almost 10 years in Earth orbit. Unfortunately, micrometeoroid and orbital debris impacts cannot be differentiated in the images. Therefore, statistical techniques, taking into account the mean densities of micrometeoroids and orbital debris and their effects on hypervelocity impact morphology, will need to be applied to distinguish the probable populations. IMGE CAPTION: [http://www.orbitaldebris.jsc.nasa.gov/newsletter/v7i1/hubble_fig1.jpg] Five HST impact sites photographed with 400 mm lens. Received on Tue 12 Feb 2002 10:52:48 AM PST |
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