Literature DB >> 32699805

Technology gap assessment for a future large-aperture ultraviolet-optical-infrared space telescope.

Matthew R Bolcar1, Kunjithapatham Balasubramanian2, Julie Crooke1, Lee Feinberg1, Manuel Quijada1, Bernard J Rauscher1, David Redding2, Norman Rioux1, Stuart Shaklan2, H Philip Stahl3, Carl M Stahle1, Harley Thronson1.   

Abstract

The Advanced Technology Large Aperture Space Telescope (ATLAST) team identified five key technology areas to enable candidate architectures for a future large-aperture ultraviolet/optical/infrared (LUVOIR) space observatory envisioned by the NASA Astrophysics 30-year roadmap, "Enduring Quests, Daring Visions." The science goals of ATLAST address a broad range of astrophysical questions from early galaxy and star formation to the processes that contributed to the formation of life on Earth, combining general astrophysics with direct-imaging and spectroscopy of habitable exoplanets. The key technology areas are internal coronagraphs, starshades (or external occulters), ultra-stable large-aperture telescope systems, detectors, and mirror coatings. For each technology area, we define best estimates of required capabilities, current state-of-the-art performance, and current technology readiness level (TRL), thus identifying the current technology gap. We also report on current, planned, or recommended efforts to develop each technology to TRL 5.

Keywords:  coronagraph; lightweight mirrors; space telescopes; starshade; technology development; ultra-stable systems

Year:  2016        PMID: 32699805      PMCID: PMC7375264          DOI: 10.1117/1.jatis.2.4.041209

Source DB:  PubMed          Journal:  J Astron Telesc Instrum Syst        ISSN: 2329-4124            Impact factor:   1.436


  4 in total

1.  Reflectivity and optical surface height requirements in a broadband coronagraph. 1. Contrast floor due to controllable spatial frequencies.

Authors:  Stuart B Shaklan; Joseph J Green
Journal:  Appl Opt       Date:  2006-07-20       Impact factor: 1.980

2.  Measurement of large cryogenic structures using a spatially phase-shifted digital speckle pattern interferometer.

Authors:  Babak Saif; Marcel Bluth; Perry Greenfield; Warren Hack; Bente Hoffmann Eegholm; Peter Blake; Ritva Keski-Kuha; Lee Feinberg; Jonathan W Arenberg
Journal:  Appl Opt       Date:  2008-02-20       Impact factor: 1.980

3.  Monochromatic verification of high-contrast imaging with an occulter.

Authors:  Dan Sirbu; N Jeremy Kasdin; Robert J Vanderbei
Journal:  Opt Express       Date:  2013-12-30       Impact factor: 3.894

4.  IDENTIFYING PLANETARY BIOSIGNATURE IMPOSTORS: SPECTRAL FEATURES OF CO AND O4 RESULTING FROM ABIOTIC O2/O3 PRODUCTION.

Authors:  Edward W Schwieterman; Victoria S Meadows; Shawn D Domagal-Goldman; Drake Deming; Giada N Arney; Rodrigo Luger; Chester E Harman; Amit Misra; Rory Barnes
Journal:  Astrophys J Lett       Date:  2016-02-25       Impact factor: 7.413

  4 in total
  1 in total

1.  Highly Reflective Silver-Enhanced Coating with High Adhesion and Sulfurization Resistance for Telescopes.

Authors:  Hsing-Yu Wu; Shao-Rong Huang; Chih-Hsuan Shih; Li-Jen Hsiao; Hong-Wei Chen; Ming-Chung Cheng; Jin-Cherng Hsu
Journal:  Nanomaterials (Basel)       Date:  2022-03-23       Impact factor: 5.076

  1 in total

北京卡尤迪生物科技股份有限公司 © 2022-2023.