{"project":{"acronym":"","projectId":90196,"title":"Compact Telescoping Array Design and Development","primaryTaxonomyNodes":[{"taxonomyNodeId":10865,"taxonomyRootId":8816,"parentNodeId":10864,"level":3,"code":"TX12.2.1","title":"Lightweight Concepts","definition":"Lightweight concepts are efficient structures and structural systems using new and innovative approaches to develop beyond-state-of-the-art mass reductions for affordable, enhanced performance, reliable, and environmentally responsible aerospace applications.","exampleTechnologies":"Components for space vehicles and surface habitats, in-space depots and landers, solar or antenna arrays, complex precision deployables, propulsion systems, and terrestrial airframes and engines which function either as primary load bearing or as secondary structures. The technologies used for these components may include either rigid construction (e.g., shell or truss structures) or expandable configurations (e.g., inflatable structures) having efficient structural geometries (e.g., hat-stiffened shells) constructed from advanced materials (e.g., polymer matrix composites) using advanced fabrication methods (e.g., additive manufacturing)","hasChildren":false,"hasInteriorContent":true}],"startTrl":3,"currentTrl":6,"endTrl":6,"benefits":"Potential CTA Phase II and Phase III SBIR contracts will build demonstration units representing 17 and 30 kW systems respectively. This will advance CTA technology to TRL 6. Increasing power level step by step advances CTA technology toward larger systems by taking advantage of the natural scalability of the CTA platform. This will bring SEP power class systems 50 kW and higher well within reach. NASA programs involving large solar arrays would be particularly interested in this technology development path as it directly supports mass-critical SEP mission requirements. The Asteroid Redirect Mission (ARM) is one relatively near term NASA mission that could benefit from CTA. Following Phase II and Phase III work, Angstrom Designs expects applications should be in the form of purchase contracts with our subcontractor and commercialization partner, Orbital ATK, to supply ARM or other NASA missions with efficient space power. Phase I results show that a CTA system could supply 50 kW for a potential ARM SEP mission delivering metrics of 190 W/kg specific power and 88 kW/m? power density. A future Mars cargo SEP mission could be fitted with 190 kW of CTA power with outstanding metrics: 187 W/kg and 98 kW/m?. Versatile packaging, exceptional performance and solid reliability over a wide range of power classes and g-loads all indicate that the CTA platform lends itself well to future NASA missions.
CTA is primarily the combination of flight-qualified components so the design is inherently lower risk than completely new arrays. After successful completion of the Phase II work, including building and testing a CTA wing, risk will be further reduced and the TRL of CTA will be significantly advanced. Phase II work will further reduce development costs and risks of future programs. CTA?s exceptional metrics and packaging versatility are also of great benefit to the non-NASA, commercial market. Phase II work will advance technology and lower risk to enable commercial infusion beyond NASA. Commercial satellite enterprises will be able to reap the benefits of reduced solar array mass in the form of increased payload capacity and/or reduced launch costs. CTA is also an excellent candidate for the advanced arrays needed for GEO-Comm satellites to take advantage of the cost benefits of using SEP and dual launch. The Phase II demonstrator CTA wing will be representative of a 17 kW system, a power level of interest to the suppliers in the GEO-Comm market. At least two suppliers of commercial satellites, Boeing and Orbital ATK, are currently seeking to replace rigid panel technology with flexible blanket systems in near term programs. Other high probability customers include the department of Defense, Air Force Research Laboratory and foreign governments all of whom have an interest in high power, low mass, low risk, low cost solar arrays.","description":"Solar arrays power the vast majority of space missions. Solar arrays with higher power, better mass efficiency and improved packaging are critical, especially given NASA interest in solar electric propulsion (SEP). The Phase I results shows that the Compact Telescoping Array (CTA) architecture, originally conceived by a NASA sponsored team, is a very promising new technology. Not only has CTA shown outstanding performance metrics, but it does so in a manner that is scalable, reliable and offers compact stowage. The proposed innovation is a solar array design consisting of a single central truss structure flanked by tensioned flexible photovoltaic blankets. This configuration has been shown in multiple analytical studies to be the most mass efficient for a cantilevered solar array. Phase I results confirm that CTA has very low structural mass which, with state-of-practice cell technology, allows the platform to deliver excellent specific power. For example, sub-200 kW systems show specific power approaching 190 W/kg and mega-Watt versions of CTA still produce better than 150 W/kg. The CTA stowed wing achieves the ?compact? attribute due to the fact that the two primary components of the system, the boom and the PV blankets, though by different methods, both stow into highly volume-efficient packages. The individual boom segments all nest neatly inside one another while the PV blankets stow into compact Z-folded stacks. The result is a system that is capable of delivering compactness in excess of 100 kW/m?, far beyond expectations. The CTA system, although a new solar array configuration, is shown through Phase I research to have high reliability. This is achieved by leveraging heritage mechanical subsystems and by minimizing new mechanism design, thereby effectively delivering a higher TRL than would ordinarily be associated with a new system. The CTA design draws heavily from heritage designs of Angstrom Designs subcontractor Orbital ATK Goleta.","startYear":2016,"startMonth":4,"endYear":2018,"endMonth":5,"statusDescription":"Completed","principalInvestigators":[{"contactId":374449,"canUserEdit":false,"firstName":"Peter","lastName":"Sorensen","fullName":"Peter Sorensen","fullNameInverted":"Sorensen, Peter","primaryEmail":"Peter.Sorensen@Angstromdesigns.Com","publicEmail":true,"nacontact":false}],"programDirectors":[{"contactId":206378,"canUserEdit":false,"firstName":"Jason","lastName":"Kessler","fullName":"Jason L Kessler","fullNameInverted":"Kessler, Jason L","middleInitial":"L","primaryEmail":"jason.l.kessler@nasa.gov","publicEmail":true,"nacontact":false}],"programExecutives":[{"contactId":215154,"canUserEdit":false,"firstName":"Jennifer","lastName":"Gustetic","fullName":"Jennifer L Gustetic","fullNameInverted":"Gustetic, Jennifer L","middleInitial":"L","primaryEmail":"jennifer.l.gustetic@nasa.gov","publicEmail":true,"nacontact":false}],"programManagers":[{"contactId":62051,"canUserEdit":false,"firstName":"Carlos","lastName":"Torrez","fullName":"Carlos Torrez","fullNameInverted":"Torrez, Carlos","primaryEmail":"carlos.torrez@nasa.gov","publicEmail":true,"nacontact":false}],"projectManagers":[{"contactId":461333,"canUserEdit":false,"firstName":"Theresa","lastName":"Stanley","fullName":"Theresa M Stanley","fullNameInverted":"Stanley, Theresa M","middleInitial":"M","primaryEmail":"theresa.m.stanley@nasa.gov","publicEmail":true,"nacontact":false},{"contactId":3164660,"canUserEdit":false,"firstName":"Geoff","lastName":"Rose","fullName":"Geoff Rose","fullNameInverted":"Rose, Geoff","primaryEmail":"geoffrey.k.rose@nasa.gov","publicEmail":true,"nacontact":false}],"website":"","libraryItems":[{"file":{"fileExtension":"pdf","fileId":300639,"fileName":"SBIR_2015_2_BC_H5.01-9640","fileSize":32875,"objectId":297177,"objectType":{"lkuCodeId":889,"code":"LIBRARY_ITEMS","description":"Library Items","lkuCodeTypeId":182,"lkuCodeType":{"codeType":"OBJECT_TYPE","description":"Object Type"}},"objectTypeId":889,"fileSizeString":"32.1 KB"},"files":[{"fileExtension":"pdf","fileId":300639,"fileName":"SBIR_2015_2_BC_H5.01-9640","fileSize":32875,"objectId":297177,"objectType":{"lkuCodeId":889,"code":"LIBRARY_ITEMS","description":"Library Items","lkuCodeTypeId":182,"lkuCodeType":{"codeType":"OBJECT_TYPE","description":"Object Type"}},"objectTypeId":889,"fileSizeString":"32.1 KB"}],"id":297177,"title":"Briefing Chart","description":"Compact Telescoping Array Design and Development, Phase II Briefing Chart","libraryItemTypeId":1222,"projectId":90196,"primary":false,"publishedDateString":"","contentType":{"lkuCodeId":1222,"code":"DOCUMENT","description":"Document","lkuCodeTypeId":341,"lkuCodeType":{"codeType":"LIBRARY_ITEM_TYPE","description":"Library Item Type"}}},{"caption":"Compact Telescoping Array Design and Development, Phase II","file":{"fileExtension":"jpg","fileId":295600,"fileName":"SBIR_2015_2_BC_H5.01-9640","fileSize":13542,"objectId":292128,"objectType":{"lkuCodeId":889,"code":"LIBRARY_ITEMS","description":"Library Items","lkuCodeTypeId":182,"lkuCodeType":{"codeType":"OBJECT_TYPE","description":"Object Type"}},"objectTypeId":889,"fileSizeString":"13.2 KB"},"files":[{"fileExtension":"jpg","fileId":295600,"fileName":"SBIR_2015_2_BC_H5.01-9640","fileSize":13542,"objectId":292128,"objectType":{"lkuCodeId":889,"code":"LIBRARY_ITEMS","description":"Library Items","lkuCodeTypeId":182,"lkuCodeType":{"codeType":"OBJECT_TYPE","description":"Object Type"}},"objectTypeId":889,"fileSizeString":"13.2 KB"}],"id":292128,"title":"Briefing Chart Image","description":"Compact Telescoping Array Design and Development, Phase II","libraryItemTypeId":1095,"projectId":90196,"primary":true,"publishedDateString":"","contentType":{"lkuCodeId":1095,"code":"IMAGE","description":"Image","lkuCodeTypeId":341,"lkuCodeType":{"codeType":"LIBRARY_ITEM_TYPE","description":"Library Item Type"}}}],"transitions":[{"transitionId":67687,"projectId":90196,"partner":"Other","transitionDate":"2016-04-01","path":"Advanced From","relatedProjectId":33498,"relatedProject":{"acronym":"","projectId":33498,"title":"Compact Telescoping Array Design and Development","startTrl":2,"currentTrl":3,"endTrl":3,"benefits":"The path to commercialization is straightforward, via our commercialization partner ATK. ATK has significant interest in commercializing CTA technology and post-Phase II commercialization would be in the form of sales directly from ATK. The most direct commercialization would come in the form of a demo-wing for a NASA SEP mission such as ARM/ARRM or an earlier demonstration on ISS, where it could also function to provide supplemental power. NASA's interest in large arrays and SEP will not end with ARM, so larger, more powerful, follow-on missions will in interested in the capabilities of CTA, including manned and unmanned missions to Mars.
The entire space community is interested in high performance solar arrays. CTA offers great promise for mass efficiency, compact stowage, scalability to high power, and variability to fit different spacecraft busses and fairings. Benefits over the current state of practice will be most significant for large wings, so early commercialization efforts will focus on the needs of larger satellites in higher orbits, such as MEO-orbit GPS satellites and GEO-orbit communications satellites. These applications are equally relevant for non-NASA customers such as Air Force and private, commercial prime contractors.","description":"NASA has significant interest in developing solar electric propulsion technology (SEP) and has identified SEP as enabling for many of NASA's near-term and long-term missions, including the asteroid redirect mission (ARM). Large, scalable solar arrays are critical to enabling SEP missions, and could also serve many other sub-sections of the civil, commercial, and defense space markets. A recently published paper by NIA and NASA shows the Compact Telescoping Array (CTA) concept, which possesses the potential for 60 kW/m3 at 1 MW of power with an elegantly simple design concept derived in part from the international space station (ISS) solar array. The potential performance of CTA, including packing density, scalability and structural efficiency, is excellent. This array technology appears to be an excellent path forward for many current mission needs. Since the vast majority of CTA's subsystems can be implemented with elements that possess significant flight heritage, it is expected that significant progress can be made under SBIR funding to prepare CTA for infusion in the market. The proposed work advances the conceptual work begun by Mikulas, Pappa, Warren and Rose. Angstrom Designs, partnered with ATK space, proposes to explore combining flight-heritage sub-systems to progress the CTA concept, increase the TRL of the overall design, and establish the path for successful commercial infusion.","startYear":2015,"startMonth":6,"endYear":2015,"endMonth":12,"statusDescription":"Completed","website":"","program":{"acronym":"SBIR/STTR","active":true,"description":"
The NASA SBIR and STTR programs fund the research, development, and demonstration of innovative technologies that fulfill NASA needs as described in the annual Solicitations and have significant potential for successful commercialization. If you are a small business concern (SBC) with 500 or fewer employees or a non-profit RI such as a university or a research laboratory with ties to an SBC, then NASA encourages you to learn more about the SBIR and STTR programs as a potential source of seed funding for the development of your innovations.
The SBIR and STTR programs have 3 phases:
The SBIR and STTR Phase I contracts last for 6 months with a maximum funding of $125,000, and Phase II contracts last for 24 months with a maximum funding of $750,000 - $1.5 million.
Opportunity for Continued Technology Development Post-Phase II:
The NASA SBIR/STTR Program currently has in place two initiatives for supporting its small business partners past the basic Phase I and Phase II elements of the program that emphasize opportunities for commercialization. Specifically, the NASA SBIR/STTR Program has the Phase II Enhancement (Phase II-E) and Phase II eXpanded (Phase II-X) contract options.
Please review the links below to obtain more information on the SBIR/STTR programs.
Provides an overview of the SBIR and STTR programs as implemented by NASA
Provides access to the annual SBIR/STTR Solicitations containing detailed information on the program eligibility requirements, proposal instructions and research topics and subtopics
Schedule and links for the SBIR/STTR solicitations and selection announcements
Federal and non-Federal sources of assistance for small business
Search our complete archive of awarded project abstracts to learn about what NASA has funded
Still have questions? Visit the program FAQs
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The SBIR and STTR programs have 3 phases:
The SBIR and STTR Phase I contracts last for 6 months with a maximum funding of $125,000, and Phase II contracts last for 24 months with a maximum funding of $750,000 - $1.5 million.
Opportunity for Continued Technology Development Post-Phase II:
The NASA SBIR/STTR Program currently has in place two initiatives for supporting its small business partners past the basic Phase I and Phase II elements of the program that emphasize opportunities for commercialization. Specifically, the NASA SBIR/STTR Program has the Phase II Enhancement (Phase II-E) and Phase II eXpanded (Phase II-X) contract options.
Please review the links below to obtain more information on the SBIR/STTR programs.
Provides an overview of the SBIR and STTR programs as implemented by NASA
Provides access to the annual SBIR/STTR Solicitations containing detailed information on the program eligibility requirements, proposal instructions and research topics and subtopics
Schedule and links for the SBIR/STTR solicitations and selection announcements
Federal and non-Federal sources of assistance for small business
Search our complete archive of awarded project abstracts to learn about what NASA has funded
Still have questions? Visit the program FAQs
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