logging in or signing up science Mattia Download Post to : URL : Related Presentations : Share Add to Flag Embed Email Send to Blogs and Networks Add to Channel Uploaded from authorPOINTLite Insert YouTube videos in PowerPont slides with aS Desktop Copy embed code: (To copy code, click on the text box) Embed: URL: Thumbnail: WordPress Embed Customize Embed The presentation is successfully added In Your Favorites. Views: 58 Category: Entertainment License: All Rights Reserved Like it (0) Dislike it (0) Added: January 16, 2008 This Presentation is Public Favorites: 0 Presentation Description No description available. Comments Posting comment... Premium member Presentation Transcript STARDUST CRR: STARDUST CRR SCIENCE REQUIREMENTS June 11 , 1996Slide2: BRIEF MISSION SYNOPSIS 3 axis stabilized s/c with Return Capsule 7 yr, 3 loop trajectory with 1 EGA Flyby of Wild 2 - 6 km/s - 100 km distance Comet sample collection by intact capture In-situ dust analysis & detection Nucleus and coma imaging IS collection & detection on cruise Samples returned via direct entrySlide3: STARDUST Trajectory LAUNCH 2/15/99 EGA 3 OUTBOUND LEGS IS Dust Analysis (CIDA) 3 INBOUND LEGS IS Dust collection WILD 2 Flyby 1/02/04 (4yr 10 mos) SAMPLE RETURN Jan 13, 2006 (6 yr 11 mos)Slide4: Primary Objective Comet Particle Collection and Return to Earth Secondary Objectives IS Particle Collection and Return to Earth Comet Imaging (Nucleus and Coma) In-situ Particle Analysis for Coma Flythrough Tertiary Objectives In-situ Analysis for Interstellar/Interplanetary Dust Comet Gas Collection and Return to Earth Dynamics Science Dust Shield MonitorsScience Requirements: Science Requirements Primary Requirement: Secondary Requirements: Tertiary Requirement: Collect 1000 comet particles >15µm at encounter velocity <6.5 km/s and return to Earth Collect 100 interstellar particles >0.1µm and return to Earth; Provide >65 images of Wild 2, having a resolution of at least 67µrad/pixel, taken within 2000 km of the comet nucleus through selected filters; Provide in-situ particle analysis for comet coma flythrough capable of resolving abundant elements in cometary solids Provide in-situ particle analysis for interstellar and interplanetary dust; Collect comet coma molecules and return to Earth; Measure dust mass fluence, large particles and comet mass upper limit; Provide dust flux measurement of 10-9g to 1g particles Cometary Particle Collection: Cometary Particle Collection Collect >1000 Particles >15µm diameter Wholly intact or retain unmelted fragments Collect in Silica Aerogel Thickness >3 cm Total collection area > 1000 cm2, 1200 cm2 goal IS Particle Collection >100 particles >0.1µm diameter Area >1000cm2, 1200cm2 goal thickness >1cmCometary Gas Collection: Cometary Gas Collection Collection on aerogel - minimize contamination Best-effort use of other exposed materials Optical Nav. Cam. Imaging Capability for <100m/pixel resolution at 1500km >64 images total, 67 µrad/pixel >56 during encounter period Dynamic range of 12 bits 8 filter positions 0.8 Gbit storage >5% photometric accuracy - all imagesDust Flux Monitor: Dust Flux Monitor 10-9g to 1g sensitivity CIDA Mass range 1-330 AMU Mass Resolution >150, >300 goal Detection sensitivity 2 x 10-16 to 3 x 10-9 g Area > 50cm2 0.1 Gbits storage during flyby You do not have the permission to view this presentation. In order to view it, please contact the author of the presentation.
science Mattia Download Post to : URL : Related Presentations : Share Add to Flag Embed Email Send to Blogs and Networks Add to Channel Uploaded from authorPOINTLite Insert YouTube videos in PowerPont slides with aS Desktop Copy embed code: (To copy code, click on the text box) Embed: URL: Thumbnail: WordPress Embed Customize Embed The presentation is successfully added In Your Favorites. Views: 58 Category: Entertainment License: All Rights Reserved Like it (0) Dislike it (0) Added: January 16, 2008 This Presentation is Public Favorites: 0 Presentation Description No description available. Comments Posting comment... Premium member Presentation Transcript STARDUST CRR: STARDUST CRR SCIENCE REQUIREMENTS June 11 , 1996Slide2: BRIEF MISSION SYNOPSIS 3 axis stabilized s/c with Return Capsule 7 yr, 3 loop trajectory with 1 EGA Flyby of Wild 2 - 6 km/s - 100 km distance Comet sample collection by intact capture In-situ dust analysis & detection Nucleus and coma imaging IS collection & detection on cruise Samples returned via direct entrySlide3: STARDUST Trajectory LAUNCH 2/15/99 EGA 3 OUTBOUND LEGS IS Dust Analysis (CIDA) 3 INBOUND LEGS IS Dust collection WILD 2 Flyby 1/02/04 (4yr 10 mos) SAMPLE RETURN Jan 13, 2006 (6 yr 11 mos)Slide4: Primary Objective Comet Particle Collection and Return to Earth Secondary Objectives IS Particle Collection and Return to Earth Comet Imaging (Nucleus and Coma) In-situ Particle Analysis for Coma Flythrough Tertiary Objectives In-situ Analysis for Interstellar/Interplanetary Dust Comet Gas Collection and Return to Earth Dynamics Science Dust Shield MonitorsScience Requirements: Science Requirements Primary Requirement: Secondary Requirements: Tertiary Requirement: Collect 1000 comet particles >15µm at encounter velocity <6.5 km/s and return to Earth Collect 100 interstellar particles >0.1µm and return to Earth; Provide >65 images of Wild 2, having a resolution of at least 67µrad/pixel, taken within 2000 km of the comet nucleus through selected filters; Provide in-situ particle analysis for comet coma flythrough capable of resolving abundant elements in cometary solids Provide in-situ particle analysis for interstellar and interplanetary dust; Collect comet coma molecules and return to Earth; Measure dust mass fluence, large particles and comet mass upper limit; Provide dust flux measurement of 10-9g to 1g particles Cometary Particle Collection: Cometary Particle Collection Collect >1000 Particles >15µm diameter Wholly intact or retain unmelted fragments Collect in Silica Aerogel Thickness >3 cm Total collection area > 1000 cm2, 1200 cm2 goal IS Particle Collection >100 particles >0.1µm diameter Area >1000cm2, 1200cm2 goal thickness >1cmCometary Gas Collection: Cometary Gas Collection Collection on aerogel - minimize contamination Best-effort use of other exposed materials Optical Nav. Cam. Imaging Capability for <100m/pixel resolution at 1500km >64 images total, 67 µrad/pixel >56 during encounter period Dynamic range of 12 bits 8 filter positions 0.8 Gbit storage >5% photometric accuracy - all imagesDust Flux Monitor: Dust Flux Monitor 10-9g to 1g sensitivity CIDA Mass range 1-330 AMU Mass Resolution >150, >300 goal Detection sensitivity 2 x 10-16 to 3 x 10-9 g Area > 50cm2 0.1 Gbits storage during flyby