Resonant perturbations with the earth's gravity field

Jérôme Daquin; Florent Deleflie; Pierre Mercier; Jérôme Pérez

Resonant perturbations with the earth's gravity field

Jérôme Daquin, Florent Deleflie, Pierre Mercier, Jérôme Pérez

Research output: Contribution in Book/Catalog/Report/Conference proceeding › Conference contribution

Abstract

We confront stability results coming from the mean motion theory and the osculating theory in orbital mechanics. The dynamical area studied correspond to the (2:1) tesseral resonance. We present Fast Lyapunov Indicator stability maps, based on the integration of the variational equations, realized in various dynamical configurations and in particular for eccentric orbits. Our main conclusions supports the idea that the tesseral chaos is not sensitive to the averaging process and validate, on a stability point of view, the minimal model implemented in our mean orbit propagator.

Original language	English
Title of host publication	Advances In The Astronautical Sciences
Editors	Donald L. Mackison, Ossama Abdelkhalik, Roby S. Wilson, Renato Zanetti
Publisher	Univelt Inc.
Pages	2873-2890
Number of pages	18
ISBN (Electronic)	9780877036111
Publication status	Published - 1 Jan 2014
Externally published	Yes
Event	24th AAS/AIAA Space Flight Mechanics Meeting, 2014 - Mexico, United States Duration: 26 Jan 2014 → 30 Jan 2014

Publication series

Name	Advances in the Astronautical Sciences
Volume	152
ISSN (Print)	0065-3438

Conference

Conference	24th AAS/AIAA Space Flight Mechanics Meeting, 2014
Country/Territory	United States
City	Mexico
Period	26/01/14 → 30/01/14

Cite this

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title = "Resonant perturbations with the earth's gravity field",

abstract = "We confront stability results coming from the mean motion theory and the osculating theory in orbital mechanics. The dynamical area studied correspond to the (2:1) tesseral resonance. We present Fast Lyapunov Indicator stability maps, based on the integration of the variational equations, realized in various dynamical configurations and in particular for eccentric orbits. Our main conclusions supports the idea that the tesseral chaos is not sensitive to the averaging process and validate, on a stability point of view, the minimal model implemented in our mean orbit propagator.",

author = "J{\'e}r{\^o}me Daquin and Florent Deleflie and Pierre Mercier and J{\'e}r{\^o}me P{\'e}rez",

year = "2014",

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language = "English",

series = "Advances in the Astronautical Sciences",

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editor = "Mackison, {Donald L.} and Ossama Abdelkhalik and Wilson, {Roby S.} and Renato Zanetti",

booktitle = "Advances In The Astronautical Sciences",

note = "24th AAS/AIAA Space Flight Mechanics Meeting, 2014 ; Conference date: 26-01-2014 Through 30-01-2014",

}

Daquin, J, Deleflie, F, Mercier, P & Pérez, J 2014, Resonant perturbations with the earth's gravity field. in DL Mackison, O Abdelkhalik, RS Wilson & R Zanetti (eds), Advances In The Astronautical Sciences. Advances in the Astronautical Sciences, vol. 152, Univelt Inc., pp. 2873-2890, 24th AAS/AIAA Space Flight Mechanics Meeting, 2014, Mexico, United States, 26/01/14.

Resonant perturbations with the earth's gravity field. / Daquin, Jérôme; Deleflie, Florent; Mercier, Pierre et al.
Advances In The Astronautical Sciences. ed. / Donald L. Mackison; Ossama Abdelkhalik; Roby S. Wilson; Renato Zanetti. Univelt Inc., 2014. p. 2873-2890 (Advances in the Astronautical Sciences; Vol. 152).

Research output: Contribution in Book/Catalog/Report/Conference proceeding › Conference contribution

TY - GEN

T1 - Resonant perturbations with the earth's gravity field

AU - Daquin, Jérôme

AU - Deleflie, Florent

AU - Mercier, Pierre

AU - Pérez, Jérôme

PY - 2014/1/1

Y1 - 2014/1/1

N2 - We confront stability results coming from the mean motion theory and the osculating theory in orbital mechanics. The dynamical area studied correspond to the (2:1) tesseral resonance. We present Fast Lyapunov Indicator stability maps, based on the integration of the variational equations, realized in various dynamical configurations and in particular for eccentric orbits. Our main conclusions supports the idea that the tesseral chaos is not sensitive to the averaging process and validate, on a stability point of view, the minimal model implemented in our mean orbit propagator.

AB - We confront stability results coming from the mean motion theory and the osculating theory in orbital mechanics. The dynamical area studied correspond to the (2:1) tesseral resonance. We present Fast Lyapunov Indicator stability maps, based on the integration of the variational equations, realized in various dynamical configurations and in particular for eccentric orbits. Our main conclusions supports the idea that the tesseral chaos is not sensitive to the averaging process and validate, on a stability point of view, the minimal model implemented in our mean orbit propagator.

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M3 - Conference contribution

AN - SCOPUS:84940749155

T3 - Advances in the Astronautical Sciences

SP - 2873

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BT - Advances In The Astronautical Sciences

A2 - Mackison, Donald L.

A2 - Abdelkhalik, Ossama

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PB - Univelt Inc.

T2 - 24th AAS/AIAA Space Flight Mechanics Meeting, 2014

Y2 - 26 January 2014 through 30 January 2014

ER -

Resonant perturbations with the earth's gravity field

Abstract

Publication series

Conference

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