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Spitzer Operations: Scheduling the Out YearsSpitzer Warm Mission operations have remained robust and exceptionally efficient since the cryogenic mission ended in mid-2009. The distance to the now exceeds 1 AU, making telecommunications increasingly difficult; however, analysis has shown that two-way communication could be maintained through at least 2017 with minimal loss in observing efficiency. The science program continues to emphasize the characterization of exoplanets, time domain studies, and deep surveys, all of which can impose interesting scheduling constraints. Recent changes have significantly improved on-board data compression, which both enables certain high volume observations and reduces Spitzer's demand for competitive Deep Space Network resources.
Document ID
20130009352
Acquisition Source
Jet Propulsion Laboratory
Document Type
Conference Paper
External Source(s)
Authors
Mahoney, William A.
(California Inst. of Tech. Pasadena, CA, United States)
Effertz, Mark J.
(Lockheed Martin Space Systems Co. Littleton, CO, United States)
Fisher, Mark E.
(Lockheed Martin Space Systems Co. Littleton, CO, United States)
Garcia, Lisa J.
(California Inst. of Tech. Pasadena, CA, United States)
Hunt, Joseph C. Jr.
(Jet Propulsion Lab., California Inst. of Tech. Pasadena, CA, United States)
Mannings, Vincent
(California Inst. of Tech. Pasadena, CA, United States)
McElroy, Douglas B.
(California Inst. of Tech. Pasadena, CA, United States)
Scire, Elena
(California Inst. of Tech. Pasadena, CA, United States)
Date Acquired
August 27, 2013
Publication Date
July 1, 2012
Subject Category
Astronomy
Meeting Information
Meeting: SPIE Astronomical Telescopes+Instrumentation
Location: Amsterdam
Country: Netherlands
Start Date: July 1, 2012
End Date: July 6, 2012
Distribution Limits
Public
Copyright
Other
Keywords
Spitzer
spacecraft operations
observation scheduling
scheduling

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