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Dynamical performance for science-mode stationkeeping with an external occulter

  • Dan Sirbu
  • , Christian Vad Karsten
  • , N Jeremy Kasdin
    • Princeton University

    Research output: Contribution to journalConference articleResearchpeer-review

    759 Downloads (Orbit)

    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 languageEnglish
    JournalProceedings of SPIE - The International Society for Optical Engineering
    Volume7731
    ISSN0277-786X
    DOIs
    Publication statusPublished - 2010
    EventSpace Telescopes and Instrumentation 2010: Optical, Infrared, and Millimeter Wave - San Diego, United States
    Duration: 27 Jun 20102 Jul 2010

    Conference

    ConferenceSpace Telescopes and Instrumentation 2010: Optical, Infrared, and Millimeter Wave
    Country/TerritoryUnited States
    CitySan Diego
    Period27/06/201002/07/2010

    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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