scholarly journals Gravitational spin-orbit dynamics at the fifth-and-a-half post-Newtonian order

2021 ◽  
Vol 104 (12) ◽  
Author(s):  
Mohammed Khalil
Keyword(s):  
2020 ◽  
Vol 1412 ◽  
pp. 072018
Author(s):  
J Wragg ◽  
G Armstrong ◽  
D Clarke ◽  
C Ballance ◽  
A Brown ◽  
...  
Keyword(s):  

2011 ◽  
Vol 134 (20) ◽  
pp. 204311 ◽  
Author(s):  
Sarah M. Remmert ◽  
Simon T. Banks ◽  
Jeremy N. Harvey ◽  
Andrew J. Orr-Ewing ◽  
David C. Clary

2016 ◽  
Vol 747 ◽  
pp. 012069
Author(s):  
A. Ivanov ◽  
S. Andrianov ◽  
Yu. Senichev

2008 ◽  
Vol 101 (1-2) ◽  
pp. 159-170 ◽  
Author(s):  
Alessandra Celletti ◽  
Luigi Chierchia

2017 ◽  
Vol 8 (1) ◽  
Author(s):  
Takuya Satoh ◽  
Ryugo Iida ◽  
Takuya Higuchi ◽  
Yasuhiro Fujii ◽  
Akitoshi Koreeda ◽  
...  

2019 ◽  
Vol 123 (16) ◽  
Author(s):  
Jack Wragg ◽  
Daniel D. A. Clarke ◽  
Gregory S. J. Armstrong ◽  
Andrew C. Brown ◽  
Connor P. Ballance ◽  
...  
Keyword(s):  

2015 ◽  
Vol 10 (S318) ◽  
pp. 66-68
Author(s):  
Jean-Luc Margot ◽  
Shantanu P. Naidu

AbstractWe use radar images with decameter resolution to measure the sizes, shapes, spin states, mutual orbits, masses, and densities of components of asteroid binaries and triples. We simulate the spin-orbit dynamics of these systems and map the possible spin configurations of the satellites on surface of section plots. The presence of chaotic regions in the phase space has important consequences for the evolution of binary asteroids. It may substantially increase spin synchronization timescales, delay BYORP-type evolution, and extend the lifetime of binaries.


Sign in / Sign up

Export Citation Format

Share Document