transfer orbit for the next 8.6 months. Both the Polaris and Mars will rendezvous atAA2at that time. Because, like with all Hohmann transfers, the ship does not launch until the destination planet is in the proper position. That position being Mars 8.6 months prior in its orbit from point...
Hence, it would be worthwhile to examine the orbital evolution of EMRI in the presence of an accretion disc and, particularly, the detectability of eccentric orbits. Our goal is to study the orbital evolution of companion BH and the dependence of its detectability on the values of orbital ...
This work provides an outline of several results concerning topology, Lie algebra, orbits and dynamics of some integrable systems on them. All the results in this paper were obtained by the authors and the participants of the Seminar on Modern Geometry and Its Applications held in the Faculty ...
We conduct a comprehensive study on spherical orbits around two types of black holes: Kerr鈥揘ewman black holes, which are charged, and Ghosh black holes, which are nonsingular. In this work, we consider both null and timelike cases of orbits. Utilizing the Mino formalism, all analytical ...
This model has been studied extensively by numerical methods and qualitative techniques. However from the viewpoint of mathematics, the dynamics of the Lorenz equations has not been understood yet. Various methods have been proposed to simplify the Lorenz model without losing its physical meaning or ...
If the satellite orbit is very elliptical, the satellite will spend most of its time near apogee where it moves very slowly. This means that the satellite can be in view over its operational area for most of the time, and falling out of view when the satellite comes closer to the Earth...
Use Kepler's third law to relate the orbital period and the length of the semimajor axis of an orbit and predict the period of an orbit from its semimajor axis. About This Simulation Level: High School Higher Education Length: 16
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(2018) have questioned the use of the generalized potential and Legendre functions series to describe gravitation around spheroidal objects. A good example of such conceptual, mathematical and notational problems is provided by Earth's moment of inertia about its polar axis. Show abstract Debated ...
We show that our methods give reliable approximations of slow manifolds and canard orbits. As a second example, we consider the four-dimensional Hodgkin–Huxley model [8]. Its dynamics is very complex and features periodic MMOs with a series of action potentials separated by subthreshold ...