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Proceedings Article

Science with the James Webb space telescope

[+] Author Affiliations
Jonathan P. Gardner, John C. Mather, Mark Clampin, Matthew A. Greenhouse, George Sonneborn

NASA Goddard Space Flight Ctr.

Rene Doyon

Univ. de Montréal (Canada)

Heidi B. Hammel

Space Science Institute

John B. Hutchings

Herzberg Institute of Astrophysics (Canada)

Peter Jakobsen

European Space Agency - ESTEC (Netherlands)

Simon J. Lilly

Swiss Federal Institute of Technology, ETH Zürich (Switzerland)

Knox S. Long, Matt Mountain, Massimo Stiavelli, H. S. Stockman

Space Telescope Science Institute

Jonathan I. Lunine

Lunar and Planetary Lab.

Mark J. McCaughrean

Univ. of Exeter (United Kingdom)

John Nella

Northrop Grumman Space Technology

George H. Rieke, Marcia J. Rieke

Univ. of Arizona

Hans-Walter Rix

Max-Planck-Institut für Astronomie (Germany)

Eric P. Smith

NASA

Rogier A. Windhorst

Arizona State Univ.

Gillian S. Wright

United Kingdom Astronomy Technology Ctr. (United Kingdom)

Proc. SPIE 6265, Space Telescopes and Instrumentation I: Optical, Infrared, and Millimeter, 62650N (June 10, 2006); doi:10.1117/12.670492
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From Conference Volume 6265

  • Space Telescopes and Instrumentation I: Optical, Infrared, and Millimeter
  • John C. Mather; Howard A. MacEwen; Mattheus W. M. de Graauw
  • Orlando, Florida , USA | May 24, 2006

abstract

The scientific capabilities of the James Webb Space Telescope (JWST) fall into four themes. The End of the Dark Ages: First Light and Reionization theme seeks to identify the first luminous sources to form and to determine the ionization history of the universe. The Assembly of Galaxies theme seeks to determine how galaxies and the dark matter, gas, stars, metals, morphological structures, and active nuclei within them evolved from the epoch of reionization to the present. The Birth of Stars and Protoplanetary Systems theme seeks to unravel the birth and early evolution of stars, from infall onto dust-enshrouded protostars, to the genesis of planetary systems. Planetary Systems and the Origins of Life theme seeks to determine the physical and chemical properties of planetary systems around nearby stars and of our own, and investigate the potential for life in those systems. To enable these for science themes, JWST will be a large (6.5m) cold (50K) telescope with four instruments, capable of imaging and spectroscopy from 0.6 to 29 microns wavelength.

© (2006) COPYRIGHT SPIE--The International Society for Optical Engineering. Downloading of the abstract is permitted for personal use only.
Citation

Jonathan P. Gardner ; John C. Mather ; Mark Clampin ; Rene Doyon ; Matthew A. Greenhouse, et al.
"Science with the James Webb space telescope", Proc. SPIE 6265, Space Telescopes and Instrumentation I: Optical, Infrared, and Millimeter, 62650N (June 10, 2006); doi:10.1117/12.670492; http://dx.doi.org/10.1117/12.670492


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