Transport of Mars-crossing asteroids from the quasi-Hilda region

Publikation: Beiträge in ZeitschriftenZeitschriftenaufsätzeForschungbegutachtet

Standard

Transport of Mars-crossing asteroids from the quasi-Hilda region. / Dellnitz, Michael; Junge, Oliver; Lo, Martin W. et al.
in: Physical Review Letters, Jahrgang 94, Nr. 23, 231102, 17.06.2005.

Publikation: Beiträge in ZeitschriftenZeitschriftenaufsätzeForschungbegutachtet

Harvard

Dellnitz, M, Junge, O, Lo, MW, Marsden, JE, Padberg, K, Preis, R, Ross, SD & Thiere, B 2005, 'Transport of Mars-crossing asteroids from the quasi-Hilda region', Physical Review Letters, Jg. 94, Nr. 23, 231102. https://doi.org/10.1103/PhysRevLett.94.231102

APA

Dellnitz, M., Junge, O., Lo, M. W., Marsden, J. E., Padberg, K., Preis, R., Ross, S. D., & Thiere, B. (2005). Transport of Mars-crossing asteroids from the quasi-Hilda region. Physical Review Letters, 94(23), Artikel 231102. https://doi.org/10.1103/PhysRevLett.94.231102

Vancouver

Dellnitz M, Junge O, Lo MW, Marsden JE, Padberg K, Preis R et al. Transport of Mars-crossing asteroids from the quasi-Hilda region. Physical Review Letters. 2005 Jun 17;94(23):231102. doi: 10.1103/PhysRevLett.94.231102

Bibtex

@article{0b3523450f254ea381e5695cf763befd,
title = "Transport of Mars-crossing asteroids from the quasi-Hilda region",
abstract = "We employ set oriented methods in combination with graph partitioning algorithms to identify key dynamical regions in the Sun-Jupiter-particle three-body system. Transport rates from a region near the 32 Hilda resonance into the realm of orbits crossing Mars' orbit are computed. In contrast to common numerical approaches, our technique does not depend on single long term simulations of the underlying model. Thus, our statistical results are particularly reliable since they are not affected by a dynamical behavior which is almost nonergodic (i.e., dominated by strongly almost invariant sets).",
keywords = "Mathematics",
author = "Michael Dellnitz and Oliver Junge and Lo, {Martin W.} and Marsden, {Jerrold E.} and Kathrin Padberg and Robert Preis and Ross, {Shane D.} and Bianca Thiere",
note = "{\textcopyright}2005 The American Physical Society (Received 30 September 2004; published 16 June 2005) This research was partly supported by the DAAD, the DFG Priority Program 1095, the NSF-ITR Grant No. ACI-0204932, Grant No. NSF-DMS 0402842, the Max Planck Society, and the California Institute of Technology President's Fund. This work was carried out in part at the Jet Propulsion Laboratory and California Institute of Technology under a contract with National Aeronautics and Space Administration.",
year = "2005",
month = jun,
day = "17",
doi = "10.1103/PhysRevLett.94.231102",
language = "English",
volume = "94",
journal = "Physical Review Letters",
issn = "0031-9007",
publisher = "American Physical Society",
number = "23",

}

RIS

TY - JOUR

T1 - Transport of Mars-crossing asteroids from the quasi-Hilda region

AU - Dellnitz, Michael

AU - Junge, Oliver

AU - Lo, Martin W.

AU - Marsden, Jerrold E.

AU - Padberg, Kathrin

AU - Preis, Robert

AU - Ross, Shane D.

AU - Thiere, Bianca

N1 - ©2005 The American Physical Society (Received 30 September 2004; published 16 June 2005) This research was partly supported by the DAAD, the DFG Priority Program 1095, the NSF-ITR Grant No. ACI-0204932, Grant No. NSF-DMS 0402842, the Max Planck Society, and the California Institute of Technology President's Fund. This work was carried out in part at the Jet Propulsion Laboratory and California Institute of Technology under a contract with National Aeronautics and Space Administration.

PY - 2005/6/17

Y1 - 2005/6/17

N2 - We employ set oriented methods in combination with graph partitioning algorithms to identify key dynamical regions in the Sun-Jupiter-particle three-body system. Transport rates from a region near the 32 Hilda resonance into the realm of orbits crossing Mars' orbit are computed. In contrast to common numerical approaches, our technique does not depend on single long term simulations of the underlying model. Thus, our statistical results are particularly reliable since they are not affected by a dynamical behavior which is almost nonergodic (i.e., dominated by strongly almost invariant sets).

AB - We employ set oriented methods in combination with graph partitioning algorithms to identify key dynamical regions in the Sun-Jupiter-particle three-body system. Transport rates from a region near the 32 Hilda resonance into the realm of orbits crossing Mars' orbit are computed. In contrast to common numerical approaches, our technique does not depend on single long term simulations of the underlying model. Thus, our statistical results are particularly reliable since they are not affected by a dynamical behavior which is almost nonergodic (i.e., dominated by strongly almost invariant sets).

KW - Mathematics

UR - http://www.scopus.com/inward/record.url?scp=27744479494&partnerID=8YFLogxK

UR - https://www.mendeley.com/catalogue/9e1e8d0b-51c8-3da0-9c96-173d61d4cd18/

U2 - 10.1103/PhysRevLett.94.231102

DO - 10.1103/PhysRevLett.94.231102

M3 - Journal articles

C2 - 16090456

AN - SCOPUS:27744479494

VL - 94

JO - Physical Review Letters

JF - Physical Review Letters

SN - 0031-9007

IS - 23

M1 - 231102

ER -

DOI