Precise modelling of spacecraft relative motion for formation flying spacecraft
Precise modelling of spacecraft relative motion for formation flying spacecraft
Relative spacecraft motion has long been a problem for mission analysts who plan rendezvous maneuvers. These planners look to the solution devised by Clohessy and Wiltshire as their primary analysis tool. The Clohessy-Wiltshire (CW) equations are usually sufficient for the rendezvous problem that is of short duration and has frequent thruster firings. Consequently, the long-term accuracy of the equations of motion is not as important in the rendezvous problem as in the formation-flying problem. The errors resulting from the assumptions made in the CW equations such as circular reference orbit, very close target orbit are unacceptable for the long-term prediction of relative motion needed for formation flying satellites. A precise analytic solution for the relative motion of and formation flying
satellites is needed to minimize fuel consumption and maximize lifetime. In this paper, we derive the relative coordinates of a deputy satellite with respect to a master satellite by a series of transformations and translations from the Earth-centered inertial frame to the spacecraftcentered rotating frame. The equations of relative coordinates derived in this paper are very precise and
can be used to analyze orbits of any eccentricity and of any initial separation with or without the inclusion of orbit perturbations.
Balaji, Shankar Kumar
938139e3-363c-42d8-a972-2f9e43c9c85c
Tatnall, Adrian
2c9224b6-4faa-4bfd-9026-84e37fa6bdf3
2003
Balaji, Shankar Kumar
938139e3-363c-42d8-a972-2f9e43c9c85c
Tatnall, Adrian
2c9224b6-4faa-4bfd-9026-84e37fa6bdf3
Balaji, Shankar Kumar and Tatnall, Adrian
(2003)
Precise modelling of spacecraft relative motion for formation flying spacecraft.
54th International Astronautical Congress of the International Astronautical Federation, the International Academy of Astronautics, and the International Institute of Space Law, Bremen, Germany.
28 Sep - 02 Oct 2003.
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Conference or Workshop Item
(Paper)
Abstract
Relative spacecraft motion has long been a problem for mission analysts who plan rendezvous maneuvers. These planners look to the solution devised by Clohessy and Wiltshire as their primary analysis tool. The Clohessy-Wiltshire (CW) equations are usually sufficient for the rendezvous problem that is of short duration and has frequent thruster firings. Consequently, the long-term accuracy of the equations of motion is not as important in the rendezvous problem as in the formation-flying problem. The errors resulting from the assumptions made in the CW equations such as circular reference orbit, very close target orbit are unacceptable for the long-term prediction of relative motion needed for formation flying satellites. A precise analytic solution for the relative motion of and formation flying
satellites is needed to minimize fuel consumption and maximize lifetime. In this paper, we derive the relative coordinates of a deputy satellite with respect to a master satellite by a series of transformations and translations from the Earth-centered inertial frame to the spacecraftcentered rotating frame. The equations of relative coordinates derived in this paper are very precise and
can be used to analyze orbits of any eccentricity and of any initial separation with or without the inclusion of orbit perturbations.
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Published date: 2003
Additional Information:
IAC-03-A.P.15
Venue - Dates:
54th International Astronautical Congress of the International Astronautical Federation, the International Academy of Astronautics, and the International Institute of Space Law, Bremen, Germany, 2003-09-28 - 2003-10-02
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Local EPrints ID: 22320
URI: http://eprints.soton.ac.uk/id/eprint/22320
PURE UUID: adb7e8cc-efa0-42d7-9d7b-4b7f37b6497e
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Date deposited: 05 Apr 2006
Last modified: 11 Dec 2021 14:37
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Author:
Shankar Kumar Balaji
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