Paper
25 October 2007 System models used to support a space-based telescope design for discovery of near Earth objects
Mike Lieber, Jeffrey Van Cleve, Robert Arentz, Harold Reitsema, Roger Linfield, Chuck Hardesty
Author Affiliations +
Abstract
In this paper we investigate the effects of several key system parameters related to development of a space-based observatory for discovering near-earth objects (NEOs). The space-based mission is seen as complementary to ground-based observations for identifying objects with the potential to impact the Earth. A system model is developed from an articial data set of 1218 NEOs with initial orbital elements generated from a probability distribution model similar to that incorporated in the NASA NEO Science Definition Team Report. By running the model over a 7 year period, the statistics of NEO detection can be investigated as a function of changes to telescope parameters. This paper discusses the system model development of orbital models, radiometric calculations and some initial results from parameter studies on the engineering design.
© (2007) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Mike Lieber, Jeffrey Van Cleve, Robert Arentz, Harold Reitsema, Roger Linfield, and Chuck Hardesty "System models used to support a space-based telescope design for discovery of near Earth objects", Proc. SPIE 6675, Optical Modeling and Performance Predictions III, 66750A (25 October 2007); https://doi.org/10.1117/12.734324
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KEYWORDS
Systems modeling

Space telescopes

Data modeling

Optical instrument design

K band

Observatories

Performance modeling

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