Analytical theory of the spin-orbit state of a binary asteroid deflected by a kinetic impactor
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arXiv
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| Autori principali: | , , , , |
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| Natura: | Preprint |
| Pubblicazione: |
2024
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| _version_ | 1866929494656286720 |
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| author | Gaitanas, Michalis Efthymiopoulos, Christos Gkolias, Ioannis Voyatzis, George Tsiganis, Kleomenis |
| author_facet | Gaitanas, Michalis Efthymiopoulos, Christos Gkolias, Ioannis Voyatzis, George Tsiganis, Kleomenis |
| contents | 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 a linear and nonlinear (canonical) theory 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 $β$. |
| format | Preprint |
| id |
arxiv_https___arxiv_org_abs_2409_06534 |
| institution | arXiv |
| publishDate | 2024 |
| record_format | arxiv |
| spellingShingle | Analytical theory of the spin-orbit state of a binary asteroid deflected by a kinetic impactor Gaitanas, Michalis Efthymiopoulos, Christos Gkolias, Ioannis Voyatzis, George Tsiganis, Kleomenis Earth and Planetary Astrophysics 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 a linear and nonlinear (canonical) theory 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 $β$. |
| title | Analytical theory of the spin-orbit state of a binary asteroid deflected by a kinetic impactor |
| topic | Earth and Planetary Astrophysics |
| url | https://arxiv.org/abs/2409.06534 |