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Target Search and Selection for the DI/EPOXI SpacecraftUpon completion of the Hartley 2 flyby in November 2010, the Deep Impact (DI) spacecraft resided in a solar orbit without possibility for gravity assist with any large body. Conservative estimates of remaining fuel were enough to provide only an 18 m/s impulse on the spacecraft. We present our method and results of our systematic scan of potential small body encounters for DI, and our criteria to narrow the selection to the asteroid 2002 GT as the target flyby body. The mission profile has two deterministic maneuvers to achieve the encounter, the first of which executed on November 25, 2011.
Document ID
20130000418
Acquisition Source
Jet Propulsion Laboratory
Document Type
Conference Paper
External Source(s)
Authors
Grebow, Daniel J.
(Jet Propulsion Lab., California Inst. of Tech. Pasadena, CA, United States)
Bhaskaran, Shyam
(Jet Propulsion Lab., California Inst. of Tech. Pasadena, CA, United States)
Chesley, Steven R.
(Jet Propulsion Lab., California Inst. of Tech. Pasadena, CA, United States)
Date Acquired
August 27, 2013
Publication Date
August 13, 2012
Subject Category
Astronomy
Meeting Information
Meeting: AIAA/AAS Astrodynamics Specialist Conference
Location: Minneapolis, MN
Country: United States
Start Date: August 13, 2012
End Date: August 16, 2012
Sponsors: American Astronautical Society, American Inst. of Aeronautics and Astronautics
Distribution Limits
Public
Copyright
Other
Keywords
Deep Impact (DI)
Hartley 2
EPOXI2 (Deep Impact Extended Investigation and Extrasolar Planted Observation an

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