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  • Instrumentation and Photography  (17)
  • Economics and Cost Analysis  (10)
  • 1
    Publication Date: 2019-07-12
    Description: At 2015 SPIE O&P we presented "Preliminary Analysis of Random Segment Errors on Coronagraph Performance" Key Findings: Contrast Leakage for 4thorder Sinc2(X) coronagraph is 10X more sensitive to random segment piston than random tip/tilt, Fewer segments (i.e. 1 ring) or very many segments (〉 16 rings) has less contrast leakage as a function of piston or tip/tilt than an aperture with 2 to 4 rings of segments. Revised Findings: Piston is only 2.5X more sensitive than Tip/Tilt
    Keywords: Instrumentation and Photography
    Type: MSFC-E-DAA-TN32194
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  • 2
    Publication Date: 2018-06-12
    Description: Scheduled to begin its 10 year mission no sooner than 2013, the James Webb Space Telescope (JWST) will search for the first luminous objects of the Universe to help answer fundamental questions about how the Universe came to look like it does today. At 6.5 meters in diameter, JWST will be the world's largest space telescope. This talk reviews science objectives for JWST and how they drive the JWST architecture, e.g. aperture, wavelength range and operating temperature. Additionally, the talk provides an overview of the JWST primary mirror technology development and fabrication status.
    Keywords: Instrumentation and Photography
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  • 3
    Publication Date: 2019-07-18
    Description: A parametric cost model for ground-based telescopes is developed using multi-variable statistical analysis, The model includes both engineering and performance parameters. While diameter continues to be the dominant cost driver, other significant factors include primary mirror radius of curvature and diffraction limited wavelength. The model includes an explicit factor for primary mirror segmentation and/or duplication (i.e.. multi-telescope phased-array systems). Additionally, single variable models based on aperture diameter are derived. This analysis indicates that recent mirror technology advances have indeed reduced the historical telescope cost curve.
    Keywords: Economics and Cost Analysis
    Type: Astronomical Telescopes and Instrumentation 2004; Jun 21, 2004 - Jun 25, 2004; Glasgow, Scotland; United Kingdom
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  • 4
    Publication Date: 2019-07-13
    Description: Technology advancement is required to enable NASA's high priority missions of the future. To prepare for those missions requires a roadmap of how to get from the current state of the art to where technology needs to be in 5, 10, 15 and 20 years. SIOSS identifies where substantial enhancements in mission capabilities are needed and provides strategic guidance for the agency's budget formulation and prioritization process.
    Keywords: Instrumentation and Photography
    Type: M11-1090 , NASA Cosmic Origins Program Analysis Group (COPAG) Meeting; Sep 22, 2011 - Sep 23, 2011; Baltimore, MD; United States
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  • 5
    Publication Date: 2019-07-13
    Description: Parametric cost models can be used by designers and project managers to perform relative cost comparisons between major architectural cost drivers and allow high-level design trades; enable cost-benefit analysis for technology development investment; and, provide a basis for estimating total project cost between related concepts. This paper reports on recent revisions and improvements to our ground telescope cost model and refinements of our understanding of space telescope cost models. One interesting observation is that while space telescopes are 50X to 100X more expensive than ground telescopes, their respective scaling relationships are similar. Another interesting speculation is that the role of technology development may be different between ground and space telescopes. For ground telescopes, the data indicates that technology development tends to reduce cost by approximately 50% every 20 years. But for space telescopes, there appears to be no such cost reduction because we do not tend to re-fly similar systems. Thus, instead of reducing cost, 20 years of technology development may be required to enable a doubling of space telescope capability. Other findings include: mass should not be used to estimate cost; spacecraft and science instrument costs account for approximately 50% of total mission cost; and, integration and testing accounts for only about 10% of total mission cost.
    Keywords: Economics and Cost Analysis
    Type: M12-1983 , Proceedings of SPIE; 8442|Space Telescopes and Instrumentation 2012: Optical, Infrared, and Millimeter Wave; Jul 01, 2012 - Jul 06, 2012; Amsterdam; Netherlands
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  • 6
    Publication Date: 2019-07-13
    Description: No abstract available
    Keywords: Economics and Cost Analysis
    Type: M12-1842 , SPIE Astronomical Telescopes and Instrumentation Symposia Space Telescopes and Instrumentation 2012: Optical, Infrared, and Millimeter Wave Conference; Jul 01, 2012 - Jul 06, 2012
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  • 7
    Publication Date: 2019-07-13
    Description: Parametric cost models are used to plan missions, compare concepts and justify technology investments. This paper reviews an on-going effort to develop cost modes for space telescopes. This paper summarizes the methodology used to develop cost models and documents how changes to the database have changed previously published preliminary cost models. While the cost models are evolving, the previously published findings remain valid: it costs less per square meter of collecting aperture to build a large telescope than a small telescope; technology development as a function of time reduces cost; and lower areal density telescopes cost more than more massive telescopes.
    Keywords: Economics and Cost Analysis
    Type: M11-0599 , M11-0930 , ICO-22: 22nd General Congress of the International Commission for Optics (ICO); Aug 15, 2011 - Aug 19, 2011; Puebla; Mexico
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  • 8
    Publication Date: 2019-07-13
    Description: Since the June 2010 Astronomy Conference, an independent review of our cost data base discovered some inaccuracies and inconsistencies which can modify our previously reported results. This paper will review changes to the data base, our confidence in those changes and their effect on various parametric cost models
    Keywords: Economics and Cost Analysis
    Type: M11-0318 , M11-0929 , M11-1016 , 2011 SPIE Opitcs and Photonics; Aug 21, 2011 - Aug 25, 2011; San Diego, CA; United States
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  • 9
    Publication Date: 2019-07-12
    Description: The Advanced Technology Large-Aperture Space Telescope (ATLAST) is a concept for an 8-meter to 16-meter UVOIR space observatory for launch in the 2025-2030 era. ATLAST will allow astronomers to answer fundamental questions at the forefront of modern astrophysics, including "Is there life elsewhere in the Galaxy?" We present a range of science drivers that define the main performance requirements for ATLAST (8 to 16 milliarcsec angular resolution, diffraction limited imaging at 0.5 m wavelength, minimum collecting area of 45 square meters, high sensitivity to light wavelengths from 0.1 m to 2.4 m, high stability in wavefront sensing and control). We will also discuss the synergy between ATLAST and other anticipated future facilities (e.g., TMT, EELT, ALMA) and the priorities for technology development that will enable the construction for a cost that is comparable to current generation observatory-class space missions.
    Keywords: Instrumentation and Photography
    Type: GSFC.JA.5210.2011
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  • 10
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    In:  CASI
    Publication Date: 2019-07-19
    Description: Parametric cost models are an important tool for planning missions, compare concepts and justify technology investments. This paper presents on-going efforts to develop single variable and multi-variable cost models for space telescope optical telescope assembly (OTA). These models are based on data collected from historical space telescope missions. Standard statistical methods are used to derive CERs for OTA cost versus aperture diameter and mass. The results are compared with previously published models.
    Keywords: Instrumentation and Photography
    Type: M11-0380 , International Commission for Optics: (ICO) 22 General Congress; Aug 15, 2011 - Aug 19, 2011; Puebla; Mexico
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