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ATLAST-9.2m: a large-aperture deployable space telescope
Author(s) -
W. R. Oegerle,
Lee Feinberg,
Lloyd Purves,
Tupper Hyde,
Harley A. Thronson,
Jacqueline A. Townsend,
Marc Postman,
Matthew R. Bolcar,
Jason Budinoff,
Bruce H. Dean,
Mark Clampin,
Dennis Ebbets,
Qian Gong,
T. R. Gull,
Joseph M. Howard,
Andrew Jones,
Richard G. Lyon,
Bert A. Pasquale,
Charles M. Perrygo,
Jeffrey S. Smith,
Patrick L. Thompson,
B. E. Woodgate
Publication year - 2010
Publication title -
proceedings of spie, the international society for optical engineering/proceedings of spie
Language(s) - English
Resource type - Conference proceedings
SCImago Journal Rank - 0.192
H-Index - 176
eISSN - 1996-756X
pISSN - 0277-786X
DOI - 10.1117/12.857622
Subject(s) - telescope , aperture (computer memory) , spacecraft , james webb space telescope , wavefront , optics , observatory , upgrade , physics , reflecting telescope , spitzer space telescope , primary mirror , solar telescope , stray light , adaptive optics , aerospace engineering , computer science , astronomy , acoustics , engineering , operating system
We present results of a study of a deployable version of the Advanced Technology Large-Aperture Space Telescope (ATLAST), designed to operate in a Sun-Earth L2 orbit. The primary mirror of the segmented 9.2-meter aperture has 36 hexagonal 1.315 m (flat-to-flat) glass mirrors. The architecture and folding of the telescope is similar to JWST, allowing it to fit into the 6.5 m fairing of a modest upgrade to the Delta-IV Heavy version of the Evolved Expendable Launch Vehicle (EELV). We discuss the overall observatory design, optical design, instruments, stray light, wavefront sensing and control, pointing and thermal control, and in-space servicing options.

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