Analytical theory of the spin-orbit state of a binary asteroid deflected by a kinetic impactor
We study the perturbed-from-synchronous librational state of a double asteroid, modeled by the Full Two Rigid Body Problem (F2RBP), with primary emphasis on deriving analytical formulas which describe the system’s evolution after deflection by a kinetic impactor. To this end, both linear and nonline...
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Published in | Celestial mechanics and dynamical astronomy Vol. 136; no. 4; p. 32 |
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Main Authors | , , , , |
Format | Journal Article |
Language | English |
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Springer Netherlands
01.08.2024
Springer Nature B.V |
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ISSN | 0923-2958 1572-9478 |
DOI | 10.1007/s10569-024-10204-4 |
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Abstract | We study the perturbed-from-synchronous librational state of a double asteroid, modeled by the Full Two Rigid Body Problem (F2RBP), with primary emphasis on deriving analytical formulas which describe the system’s evolution after deflection by a kinetic impactor. To this end, both linear and nonlinear (canonical) theories are developed. We make the simplifying approximations (to be relaxed in a forthcoming paper) of planar binary orbit and axisymmetric shape of the primary body. To study the effect of a DART-like hit on the secondary body, the momentum transfer enhancement parameter
β
is introduced and retained as a symbolic variable throughout all formulas derived, either by linear or nonlinear theory. Our approach can be of use in the context of the analysis of the post-impact data from kinetic impactor missions, by providing a precise modeling of the impactor’s effect on the seconadry’s librational state as a function of
β
. |
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AbstractList | We study the perturbed-from-synchronous librational state of a double asteroid, modeled by the Full Two Rigid Body Problem (F2RBP), with primary emphasis on deriving analytical formulas which describe the system’s evolution after deflection by a kinetic impactor. To this end, both linear and nonlinear (canonical) theories are developed. We make the simplifying approximations (to be relaxed in a forthcoming paper) of planar binary orbit and axisymmetric shape of the primary body. To study the effect of a DART-like hit on the secondary body, the momentum transfer enhancement parameter
β
is introduced and retained as a symbolic variable throughout all formulas derived, either by linear or nonlinear theory. Our approach can be of use in the context of the analysis of the post-impact data from kinetic impactor missions, by providing a precise modeling of the impactor’s effect on the seconadry’s librational state as a function of
β
. We study the perturbed-from-synchronous librational state of a double asteroid, modeled by the Full Two Rigid Body Problem (F2RBP), with primary emphasis on deriving analytical formulas which describe the system’s evolution after deflection by a kinetic impactor. To this end, both linear and nonlinear (canonical) theories are developed. We make the simplifying approximations (to be relaxed in a forthcoming paper) of planar binary orbit and axisymmetric shape of the primary body. To study the effect of a DART-like hit on the secondary body, the momentum transfer enhancement parameter β is introduced and retained as a symbolic variable throughout all formulas derived, either by linear or nonlinear theory. Our approach can be of use in the context of the analysis of the post-impact data from kinetic impactor missions, by providing a precise modeling of the impactor’s effect on the seconadry’s librational state as a function of β. |
ArticleNumber | 32 |
Author | Efthymiopoulos, Christos Voyatzis, George Tsiganis, Kleomenis Gaitanas, Michalis Gkolias, Ioannis |
Author_xml | – sequence: 1 givenname: Michalis surname: Gaitanas fullname: Gaitanas, Michalis email: mgaitana@physics.auth.gr organization: Department of Physics, Aristotle University of Thessaloniki – sequence: 2 givenname: Christos surname: Efthymiopoulos fullname: Efthymiopoulos, Christos organization: Department of Mathematics, Università degli Studi di Padova – sequence: 3 givenname: Ioannis surname: Gkolias fullname: Gkolias, Ioannis organization: Department of Physics, Aristotle University of Thessaloniki – sequence: 4 givenname: George surname: Voyatzis fullname: Voyatzis, George organization: Department of Physics, Aristotle University of Thessaloniki – sequence: 5 givenname: Kleomenis surname: Tsiganis fullname: Tsiganis, Kleomenis organization: Department of Physics, Aristotle University of Thessaloniki |
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Cites_doi | 10.1038/s41550-024-02200-3 10.3847/PSJ/ac063e 10.3847/PSJ/ac3bd1 10.1007/BF00691912 10.1007/s10569-012-9469-0 10.1038/s41586-023-05805-2 10.1016/j.icarus.2021.114624 10.1016/j.icarus.2019.113439 10.1007/s10569-009-9184-7 10.3847/PSJ/acebc7 10.3847/PSJ/ac76c9 10.1007/BF01230629 10.1007/s10569-016-9731-y 10.1016/j.icarus.2009.02.001 10.1038/s41586-023-05878-z 10.1038/s41586-023-05810-5 10.1016/0167-2789(92)90028-L |
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Keywords | Kinetic impactor Canonical perturbation theory Dynamical evolution Binary asteroid |
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SubjectTerms | Aerospace Technology and Astronautics Asteroids Astrophysics and Astroparticles Axisymmetric bodies Classical Mechanics Deflection Dynamical Systems and Ergodic Theory Geophysics/Geodesy Impact analysis Mathematical analysis Momentum transfer Orbits Original Article Physics Physics and Astronomy Rigid structures Shape effects |
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Title | Analytical theory of the spin-orbit state of a binary asteroid deflected by a kinetic impactor |
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