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For the Dragon Eye DTO, \u201cSTS-133 FRD, Dragon Eye will replace TriDAR DTO on OV-103,\u201d notes the LSFR presentation \u2013 available for download on L2.<\/p>\n
The Dragon Eye DTO will mount to the same location on the external Airlock truss of Discovery as the TriDAR DTO did on STS-128 and STS-131.<\/p>\n
The installation tech order is scheduled to be \u201cmanifested on STS-133 MECSLSI.\u201d The hardware for the Dragon Eye will be Government Flown Equipment (GFE) with a \u201cgo\u201d for installation date by July 14.<\/p>\n
STS-133 Specific Articles: http:\/\/www.nasaspaceflight.com\/tag\/sts-133\/<\/p>\n
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Additionally, PRSD tank set 5 is scheduled to be removed for Ascent Performance Margin (APM) requirements. Originally, this removal included the inadvertent inclusion of the removal of an air duct that is used to support tank sets 3 and 5.<\/p>\n
This inadvertent demanifestation of the air duct for tank set 3 (which is still installed on Discovery) was immediately reversed and will be left installed to \u201csupport tank set 3 LH purge.\u201d<\/p>\n
Moreover, the LSFR notes several (5 total) potential modifications to Discovery that could be implemented pending approval and processing flow time constraints.<\/p>\n
![\"\"](\"https:\/\/www.nasaspaceflight.com\/wp-content\/uploads\/2010\/06\/A34.jpg\" "\\"A3\\"")
The first potential modification includes an increase to the Boundary Layer Transition (BLT) DTO (Detailed Test Objective) protuberance tile.<\/p>\n\u201cRe-flight of protuberance tile and associated thermocouple installation with likely protuberance height increase to 0.50-inches,\u201d notes the LSFR document.<\/p>\n
A thermal analysis conducted on May 10 found no issues with a protuberance tile height of 0.50-inches.<\/p>\n
Nonetheless, \u201cProtuberance tiles with height options of 0.35\u2033, 0.45\u2033 and 0.50\u2033 are being fabricated \u2013 engineering release for chosen option to be released by June 11 in support of GO implementation schedule,\u201d notes the LSFR presentation.<\/p>\n
A baseline of the BLT DTO tile height is scheduled for the Program Requirements Control Board (PRCB)\/Delta PRCB on June 10.<\/p>\n
![\"\"](\"https:\/\/www.nasaspaceflight.com\/wp-content\/uploads\/2010\/06\/A44.jpg\" "\\"A4\\"")
In line with the BLT DTO, consideration is also being given to a re-flight of the catalytic coating DTO (3rd flight total) on a downstream BLT DTO TPS (Thermal Protection System) tile.<\/p>\n\u201cShelf life extension testing of existing lot of catalytic coating completed with no issues. Thermal analysis shows no concern with heating from larger 0.50-inch protuberance.\u201d<\/p>\n
If a re-flight is approved, there would be no configuration change to the catalytic coating DTO from Discovery\u2019s previous flight; therefore, no modification would need to be baselined.<\/p>\n
The only forward work necessary would be the removal and replacement of the STS-131 catalytic coating tile.<\/p>\n
![\"\"](\"https:\/\/www.nasaspaceflight.com\/wp-content\/uploads\/2010\/06\/A47.jpg\" "\\"A47\\"")
Switching gears, the third potential modification relates to the Ceramic Insert Plugs what have been seen to liberate on recent missions.<\/p>\n\u201cTPS PRT recommendation for corrective actions related to ceramic insert plug loss \/ protrusion as seen on STS-131,\u201d notes the presentation.<\/p>\n
The modification would change the \u201cplug braided cord\u201d in order to \u201creduce configuration variability and provide plug installation running torque consistency to improve plug retention.\u201d<\/p>\n
This modification would be fleet wide.<\/p>\n
Also on tap for potential implementation on Discovery for STS-133 is the inclusion of Port and Starboard WLE (Wing Leading Edge) reference marks.<\/p>\n
\u201cImagery has determined the docked OBSS (Orbiter Boom Sensor System) LDRI (Laser Dynamic Range Imager) inspection involves different trajectories from the nominal OBSS survey, due to ISS hardware considerations.<\/p>\n
\u201cPan and tilt unit (PTU) adjustments for proper LDRI sensor pointing made during survey auto-sequences are based on visual cues from the LDRI imagery.\u201d<\/p>\n
The LSFR presentation notes that the flight-specific pause points for the various views of the WLE surfaces are \u201cfairly nondescript.\u201d As a result, a recommendation has been brought forward to add \u201cposition identifying symbols\u201d on both the port and starboard WLE RCC (Reinforced Carbon-Carbon) panels.<\/p>\n
![\"\"](\"https:\/\/www.nasaspaceflight.com\/wp-content\/uploads\/2010\/06\/A66.jpg\" "\\"A66\\"")
This will \u201cfacilitate the survey and help diminish the likelihood of missed coverage during a contingency docked late inspection.\u201d<\/p>\nThese reference marks, if approved, will be applied to the WLE RCC panels with an \u201capproved black Sharpie\u201d in a manner similar to the already sharpie-applied reference marks on the nose cap RCC of all three orbiters.<\/p>\n
A Change Request for this modification will be processed \u201cat a later date\u201d and will be similar to the Change Request processed for STS-134 on Endeavour.<\/p>\n
The fifth and final potential modification gained relatively little note in the LSFR. \u201cMEI Instrumentation Filter Tech Order Configuration: Tech order M072-755113-004 update to be picked up in STS-133 MECSLSI (post STS-133 LSFR change). -004 documents acoustic sensor filters added late in the STS-131 flow.\u201d<\/p>\n
With the potential modifications to Discovery reviewed, the LSFR document goes on to discuss three (3) opportunity modifications that have already been presented to and approved by the PRCB and are simply waiting for enough time in an OPF flow to be brought to completion.<\/p>\n
The first opportunity modification is a WLE Spar \u201cSneak Flow\u201d protection installation that would increase the damage tolerance of the WLE RCC panels by \u201cadding a flow restrictor to limit allowable plume flow to 50% across the flow restrictor.\u201d<\/p>\n
![\"\"](\"https:\/\/www.nasaspaceflight.com\/wp-content\/uploads\/2010\/06\/A324.jpg\" "\\"A324\\"")
This modification is nearly complete thanks to work done on previous OPF flows. Currently, only LH RCC panels 2-4 (3 out of 44 RCC panels total) have not had this modification applied.<\/p>\nThe second opportunity modification is a redesign of the lower WLE Carrier Panel Horse Collar Gap Filler.<\/p>\n
\u201cRedesigns the lower WLE access carrier panel horse collar gap fillers with an enhanced design with additional sleeving,\u201d notes the LSFR presentation.<\/p>\n
As with the WLE Spar \u201cSneak Flow\u201d protection, this modification is nearly complete save LH RCC panels 2-4.<\/p>\n
The final opportunity modification is a Connector Saver (ME414-0630) Redesign for the LH OMS Pod and Ku Band antenna.<\/p>\n
\u201cConnector Saver mod provides proper interfacial seal and wavy washer engagement retention force to reduce risk of inadvertent demate during use.\u201d<\/p>\n
Again this work is nearly complete thanks to previous OPF flows and only the Left OMS Pod and Ku Band locations remain.<\/p>\n","protected":false},"excerpt":{"rendered":"
While Shuttle Program managers continue their review of potential launch dates for the final two shuttle missions, preparations on Discovery for what is currently her final flight are well underway at the Kennedy Space Center, with the Launch Site Flow Review (LSFR) for the STS-133\/ULF5 mission outlining the modifications to be made to Discovery during […]<\/p>\n","protected":false},"author":1,"featured_media":0,"comment_status":"","ping_status":"","sticky":false,"template":"","format":"standard","meta":{"_acf_changed":false,"inline_featured_image":false,"footnotes":"","_links_to":"","_links_to_target":""},"categories":[2],"tags":[9051],"class_list":["post-40758","post","type-post","status-publish","format-standard","hentry","category-news","tag-sts-133"],"acf":[],"_links":{"self":[{"href":"https:\/\/starpath.global\/blog\/wp-json\/wp\/v2\/posts\/40758"}],"collection":[{"href":"https:\/\/starpath.global\/blog\/wp-json\/wp\/v2\/posts"}],"about":[{"href":"https:\/\/starpath.global\/blog\/wp-json\/wp\/v2\/types\/post"}],"author":[{"embeddable":true,"href":"https:\/\/starpath.global\/blog\/wp-json\/wp\/v2\/users\/1"}],"replies":[{"embeddable":true,"href":"https:\/\/starpath.global\/blog\/wp-json\/wp\/v2\/comments?post=40758"}],"version-history":[{"count":0,"href":"https:\/\/starpath.global\/blog\/wp-json\/wp\/v2\/posts\/40758\/revisions"}],"wp:attachment":[{"href":"https:\/\/starpath.global\/blog\/wp-json\/wp\/v2\/media?parent=40758"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/starpath.global\/blog\/wp-json\/wp\/v2\/categories?post=40758"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/starpath.global\/blog\/wp-json\/wp\/v2\/tags?post=40758"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}