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The Orbital Design of Alpha Centauri Exoplanet Satellite (ACESat)Exoplanet candidates discovered by Kepler are too distant for biomarkers to be detected with foreseeable technology. Alpha Centauri has high separation from other stars and is of close proximity to Earth, which makes the binary star system 'low hanging fruit' for scientists. Alpha Centauri Exoplanet Satellite (ACESat) is a mission proposed to Small Explorer Program (SMEX) that will use a coronagraph to search for an orbiting planet around one of the stars of Alpha Centauri. The trajectory design for this mission is presented here where three different trajectories are considered: Low Earth Orbit (LEO), Geosynchronous Orbit (GEO) and a Heliocentric Orbit. Uninterrupted stare time to Alpha Centauri is desirable for meeting science requirements, or an orbit that provides 90% stare time to the science target. The instrument thermal stability also has stringent requirements for proper function, influencing trajectory design.
Document ID
20160001280
Acquisition Source
Ames Research Center
Document Type
Conference Paper
Authors
Weston, Sasha
(SGT, Inc. Moffett Field, CA, United States)
Belikov, Rus
(NASA Ames Research Center Moffett Field, CA United States)
Bendek, Eduardo
(Bay Area Environmental Research Inst. Moffett Field, CA, United States)
Date Acquired
January 29, 2016
Publication Date
August 8, 2015
Subject Category
Instrumentation And Photography
Astronomy
Report/Patent Number
ARC-E-DAA-TN24327
SSC15-IX-5
Report Number: ARC-E-DAA-TN24327
Report Number: SSC15-IX-5
Meeting Information
Meeting: Annual AIAA/USU Conference on Small Satellites
Location: Logan, Utah
Country: United States
Start Date: August 8, 2015
End Date: August 13, 2015
Sponsors: American Inst. of Aeronautics and Astronautics
Funding Number(s)
CONTRACT_GRANT: NNA13AC87C
CONTRACT_GRANT: NNX14AR61A
Distribution Limits
Public
Copyright
Public Use Permitted.
Keywords
Alpha Centauri
orbit analysis
coronagraph
ACESAT
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