Abstract
An external occulter flown in precise formation with a telescope is being considered for high-contrast direct
imaging of exoplanets as a viable mission scenario. In this paper, the dynamics about the Sun-Earth L2 region for
an occulter-telescope constellation are considered in conjunction with fourth-body and solar radiation pressure
acting as disturbing forces. An optimal observation window is defined in terms of both thrust required and
the Sun-constellation geometry. By simulation, the effects of the stellar latitude and distance, the spacecraft
separation, the magnitude of the disturbing forces, and
| Original language | English |
|---|---|
| Journal | Proceedings of SPIE - The International Society for Optical Engineering |
| Volume | 7731 |
| ISSN | 0277-786X |
| DOIs | |
| Publication status | Published - 2010 |
| Event | Space Telescopes and Instrumentation 2010: Optical, Infrared, and Millimeter Wave - San Diego, United States Duration: 27 Jun 2010 → 2 Jul 2010 |
Conference
| Conference | Space Telescopes and Instrumentation 2010: Optical, Infrared, and Millimeter Wave |
|---|---|
| Country/Territory | United States |
| City | San Diego |
| Period | 27/06/2010 → 02/07/2010 |
Bibliographical note
Copyright 2010 Society of Photo-Optical Instrumentation Engineers. One print or electronic copy may be made for personal use only. Systematic reproduction and distribution, duplication of any material in this paper for a fee or for commercial purposes, or modification of the content of the paper are prohibited.Keywords
- External Occulter
- Stationkeeping
- Circularly Restricted Three Body Problem
- High Contrast Imaging
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