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Title: Space hands-on universe telescope and orbiting wide-angle light-collector telescope to be built on the Japanese experiment module exposure facility of the international space station

Journal Article · · AIP Conference Proceedings
DOI:https://doi.org/10.1063/1.57685· OSTI ID:341320
 [1];  [2];  [3]
  1. Department of Physics, University of Alabama in Huntsville, Huntsville, Alabama 35899 (United States)
  2. The Institute of the Physical and Chemical Research (RIKEN) 2-1 Hirosawa, Wako, 351-0198 (Japan)
  3. Lawrence Berkeley Laboratory, University of California, Berkeley, California 94720 (United States)

A concept study to build great observatories on, and deploy from, the ISS is presented. Use of the ISS infra-structure including robotic arms and astronauts{close_quote} EVA would permit a construction of very large optical telescopes. We envisage that the second phase of the ISS after its initial construction can landmark a new era for both ISS and Space Sciences. Ultimately, this study would plan a 10-or 20-meter class space telescope. For its first step, we envisioned an immediate extension of the Exposed Facility of ISS for building a {open_quotes}Work-bench{close_quotes} for this purpose. Initial activities can begin with two modest-sized telescopes soon after the ISS construction. These early missions being studied are space Hands-On Universe Telescope (SHOUT) and Orbiting Wide-angle Light-collector (OWL). SHOUT is a 1-m telescope for science education. It will be built and adjusted on the exposure module of the Japanese Experiment Module (JEM) of the International Space Station by using a robotic arm and the EVA of astronauts. We also seek the possibility to release it from ISS after its perfection on orbit, so that it is free from the vibrations and gas contaminations on and around the ISS. SHOUT is an engineering prototype of 10-m Space Telescope (Space SUBARU Telescope). It would be scaled from the Space-SUBARU telescope so that the testing with the SHOUT would warrant the required specifications for the 10-meter Space-SUBARU construction on the ISS. The goal of the test with the SHOUT is to warrant a spatial resolution of 0.01 arc-seconds using the active/adaptive optics. It will test the following three major engineering challenges: (1) active/adaptive optics in space; (2) building of large structures by astronauts; and (3) release of a spacecraft from ISS to a free-flying orbit. The present feasibility study for the next generation great observatories that are to be built on the JEM Exposure Facility (EF) has been already funded by the Japan Space Forum, under the auspices of the National Space Development Agency (NASDA) of Japan. Included in this study are SHOUT, Space SUBARU telescope as well as OWL, Large Area gamma-ray Telescope (LAGT), and Space Submilimeter and Infrared Telescope (S-SIT). {copyright} {ital 1999 American Institute of Physics.}

Sponsoring Organization:
USDOE
OSTI ID:
341320
Report Number(s):
CONF-990103-; ISSN 0094-243X; TRN: 9911M0014
Journal Information:
AIP Conference Proceedings, Vol. 458, Issue 1; Conference: 1999 space technology and applications international forum, Albuquerque, NM (United States), 31 Jan - 4 Feb 1999; Other Information: PBD: Jan 1999
Country of Publication:
United States
Language:
English

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