Standard

Dynamical environments of MU69 and similar objects. / Rollin, Guillaume; Shevchenko, Ivan I.; Lages, José.

в: Icarus, Том 357, 114178, 15.03.2021.

Результаты исследований: Научные публикации в периодических изданиях › статья › Рецензирование

Harvard

Rollin, G, Shevchenko, II & Lages, J 2021, 'Dynamical environments of MU69 and similar objects', Icarus, Том. 357, 114178. https://doi.org/10.1016/j.icarus.2020.114178, https://doi.org/10.1016/j.icarus.2020.114178

APA

Rollin, G., Shevchenko, I. I., & Lages, J. (2021). Dynamical environments of MU69 and similar objects. Icarus, 357, [114178]. https://doi.org/10.1016/j.icarus.2020.114178, https://doi.org/10.1016/j.icarus.2020.114178

Vancouver

Rollin G, Shevchenko II, Lages J. Dynamical environments of MU69 and similar objects. Icarus. 2021 Март 15;357. 114178. https://doi.org/10.1016/j.icarus.2020.114178, https://doi.org/10.1016/j.icarus.2020.114178

Author

Rollin, Guillaume ; Shevchenko, Ivan I. ; Lages, José. / Dynamical environments of MU69 and similar objects. в: Icarus. 2021 ; Том 357.

BibTeX

@article{882a8d82eb3c4bd7b338576f5b16c701,
title = "Dynamical environments of MU69 and similar objects",
abstract = "We explore properties of the long-term dynamics of particles (moonlets, fragments, debris etc.) around KBO 2014 MU69 (Arrokoth), as well as around similar contact-binary objects potentially present in the Kuiper belt. The chaotic diffusion of particles inside the Hill sphere of MU69 (or, generally, a similar object) is studied by means of construction of appropriate stability diagrams and by application of analytical approaches generally based on the Kepler map theory. The formation and evolution of the particle clouds, due to the chaotic diffusion inside the Hill sphere, are studied and the cloud lifetimes are estimated.",
keywords = "2014 MU69, Arrokoth, Celestial mechanics, Contact binaries, Dynamical chaos, Kuiper belt objects",
author = "Guillaume Rollin and Shevchenko, {Ivan I.} and Jos{\'e} Lages",
note = "Funding Information: The authors are grateful to Beno{\^i}t Noyelles for helpful remarks. I.I.S. was supported in part by the grant 13.1902.21.0039 of the Ministry of Science and Higher Education of the Russian Federation . Publisher Copyright: {\textcopyright} 2020 Copyright: Copyright 2020 Elsevier B.V., All rights reserved.",
year = "2021",
month = mar,
day = "15",
doi = "10.1016/j.icarus.2020.114178",
language = "English",
volume = "357",
journal = "Icarus",
issn = "0019-1035",
publisher = "Elsevier",

}

RIS

TY - JOUR

T1 - Dynamical environments of MU69 and similar objects

AU - Rollin, Guillaume

AU - Shevchenko, Ivan I.

AU - Lages, José

N1 - Funding Information: The authors are grateful to Benoît Noyelles for helpful remarks. I.I.S. was supported in part by the grant 13.1902.21.0039 of the Ministry of Science and Higher Education of the Russian Federation . Publisher Copyright: © 2020 Copyright: Copyright 2020 Elsevier B.V., All rights reserved.

PY - 2021/3/15

Y1 - 2021/3/15

N2 - We explore properties of the long-term dynamics of particles (moonlets, fragments, debris etc.) around KBO 2014 MU69 (Arrokoth), as well as around similar contact-binary objects potentially present in the Kuiper belt. The chaotic diffusion of particles inside the Hill sphere of MU69 (or, generally, a similar object) is studied by means of construction of appropriate stability diagrams and by application of analytical approaches generally based on the Kepler map theory. The formation and evolution of the particle clouds, due to the chaotic diffusion inside the Hill sphere, are studied and the cloud lifetimes are estimated.

AB - We explore properties of the long-term dynamics of particles (moonlets, fragments, debris etc.) around KBO 2014 MU69 (Arrokoth), as well as around similar contact-binary objects potentially present in the Kuiper belt. The chaotic diffusion of particles inside the Hill sphere of MU69 (or, generally, a similar object) is studied by means of construction of appropriate stability diagrams and by application of analytical approaches generally based on the Kepler map theory. The formation and evolution of the particle clouds, due to the chaotic diffusion inside the Hill sphere, are studied and the cloud lifetimes are estimated.

KW - 2014 MU69

KW - Arrokoth

KW - Celestial mechanics

KW - Contact binaries

KW - Dynamical chaos

KW - Kuiper belt objects

UR - http://www.scopus.com/inward/record.url?scp=85093102739&partnerID=8YFLogxK

UR - https://www.mendeley.com/catalogue/4e34791b-595a-3c50-a211-0b8150a4717f/

U2 - 10.1016/j.icarus.2020.114178

DO - 10.1016/j.icarus.2020.114178

M3 - Article

AN - SCOPUS:85093102739

VL - 357

JO - Icarus

JF - Icarus

SN - 0019-1035

M1 - 114178

ER -

ID: 70633971