Zobrazeno 1 - 10
of 91
pro vyhledávání: '"V. Szebehely"'
Autor:
V. Szebehely
Publikováno v:
Modern Questions of Celestial Mechanics ISBN: 9783642110535
The problem under discussion is the restricted circular planar problem of three bodies (probleme restreint). Two bodies (assumed to be point masses and called primaries) revolve around their center of mass in circular orbits under the influence of th
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::0e015da2f5ba4570d1009c1520bd910d
https://doi.org/10.1007/978-3-642-11054-2_5
https://doi.org/10.1007/978-3-642-11054-2_5
Autor:
V. Szebehely
Publikováno v:
From Newton to Chaos ISBN: 9781489910875
In this paper a short and condensed biography of Henri Poincare is presented with detailed information concerning several biographical references. This is followed by a review of his publications emphasizing his work in celestial mechanics and on the
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::ea105f540b9da3b0c3f7055564ee3d3e
https://doi.org/10.1007/978-1-4899-1085-1_1
https://doi.org/10.1007/978-1-4899-1085-1_1
Autor:
V. Szebehely, K. Zare
Publikováno v:
From Newton to Chaos ISBN: 9781489910875
The dynamical behavior of the general three-body problem with equal masses is studied in the regions where the motion leads to triple close approaches (e.g., near equilateral triangular position with zero initial velocities). Due to the strong third
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::0812723b4697756ff5abe12fd91b8e82
https://doi.org/10.1007/978-1-4899-1085-1_30
https://doi.org/10.1007/978-1-4899-1085-1_30
Publikováno v:
Qualitative and Quantitative Behaviour of Planetary Systems ISBN: 9789401048989
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::ddb640d052eddf4307ad60398f8575d9
https://doi.org/10.1007/978-94-011-2030-2_5
https://doi.org/10.1007/978-94-011-2030-2_5
Autor:
R. H. Smith, V. Szebehely
Publikováno v:
Predictability, Stability, and Chaos in N-Body Dynamical Systems ISBN: 9781468459999
A complete qualitative understanding of the solutions of a set of nonlinear differential equations requires an investigation of the chaotic properties of the system. The circular restricted problem of three bodies has a long and rich history of quali
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::fa1e7d86917bb6faf498742257fb0440
https://doi.org/10.1007/978-1-4684-5997-5_38
https://doi.org/10.1007/978-1-4684-5997-5_38
Autor:
P. J. Message, V. Szebehely, E. P. Aksenov, V. A. Brumberg, M. S. Davis, A. Deprit, G. N. Duboshin, G. E. O. Giacaglia, G. Hori, Y. Kozai, B. Morando, L. Sehnal
Publikováno v:
Transactions of the International Astronomical Union. 16:9-17
Autor:
V. Szebehely
Publikováno v:
Transactions of the International Astronomical Union. 17:15-23
This report is organized according to twelve subjects of interest in modern celestial mechanics. Emphasis is placed on the results of an exhaustive literature search in which assistance was received from several members of Commission 7. The impetus o
Autor:
P. J. Message, Sylvio Ferraz-Mello, F. Nahon, J. Kovalevsky, E. P. Aksenov, J. Schubart, J. D. Hadjidemetriou, P. K. Seidelmann, Y Kozai, V. Szebehely, V. A. Brumberg
Publikováno v:
Transactions of the International Astronomical Union. 18:21-32
In the past three years progress of celestial mechanics research was as rapid as in the previous decade. In fact now new theories of planetary and lunar motions which have nearly the same accuracy as those of the most precise observations have become
Autor:
H. F. Henrichs, V. Szebehely, Cyril Ponnamperuma, C. de Jager, G. Pfotzer, J. Kovalevsky, H. J. Habing
Publikováno v:
Space Science Reviews. 25:83-86
Publikováno v:
Icarus. 58:169-177
Photographic evidence for a wide outer ring of Saturn, the E ring, was first introduced in 1967 and detailed observations were obtained in 1980. The brightness profile of the E ring indicates that the ring extends from three Saturn radii, the orbit o