29 September 1995 Sun-synchronous orbit mission for passively cooled reconnaissance of the interstellar medium
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Abstract
The Marshall Space Flight Center, Alabama, in a teaming arrangement with the University of Florida, Gainesville, and the Joint Astronomy Center, Hawaii, has completed a comprehensive investigation into the feasibility of a low-cost infrared space astronomy mission. This mission would map the emission of molecular hydrogen in our galaxy at two or three previously inaccessible mid-IR wavelengths, and provide information on the temperatures. The feasibility of the low-cost mission hinged on whether a thermal design could be found which would allow sufficient passive cooling of the telescope to elimiate the need for a large, expensive dewar. An approach has been found which can provide telescope temperatures on the order of 50 K, which makes the mission feasible at low cost in low-Earth orbit.
© (1995) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Jonathan W. Campbell, Jonathan W. Campbell, John Fikes, John Fikes, Mark Gerry, Mark Gerry, Jim McCarter, Jim McCarter, Harold Blevins, Harold Blevins, William D. Jones, William D. Jones, Donald E. Williams, Donald E. Williams, Holly Chandler, Holly Chandler, Allen Green, Allen Green, Terry Schmitt, Terry Schmitt, Linda Vestal, Linda Vestal, Belinda Wright, Belinda Wright, John Larkin Jackson, John Larkin Jackson, R. Greg Schunk, R. Greg Schunk, Ken Swaim, Ken Swaim, Susan Spencer, Susan Spencer, Charles M. Telesco, Charles M. Telesco, Seppo Laine, Seppo Laine, Timothy G. Hawarden, Timothy G. Hawarden, Charles R. Taylor, Charles R. Taylor, Russell A. Chipman, Russell A. Chipman, Richard T. Parmley, Richard T. Parmley, "Sun-synchronous orbit mission for passively cooled reconnaissance of the interstellar medium", Proc. SPIE 2553, Infrared Spaceborne Remote Sensing III, (29 September 1995); doi: 10.1117/12.221356; https://doi.org/10.1117/12.221356
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