Dynamic Problems of the Planets and Asteroids, and Their Discussion

2016

AdAp

Self Cite

Abstract. In light of the latest research developments, this paper describes the fundamental principles of the astronomic theory of climate change. It comprises three problems: the evolution of the orbital motion, the evolution of the Earth's rotational motion and the evolution of the insolation controlled by the evolutions of those motions. All the problems have been solved in a new way and other methods. The paper demonstrates geometric parameters of the Earth's insolation by the Sun, and explains a new insolation theory. Its results are identical to the results of the previous theory. The equations of orbital movement are established, is told about their solution and the results for the different periods of time are submitted. These results improve the results of the previous theories: the planets' and the Moon's orbits are stable and the Solar system is stable. In much the same way, the problem of the Earth's rotation is described. Unlike the previous papers, this problem is solved here without simplification. The calculations demonstrate significant oscillation of the Earth's axis. These results were confirmed with other three independent solutions of the Earth's rotation problem. The oscillations of the Earth's axis result in such oscillations of insolation that explain the paleoclimate changes. The material in this paper is presented in a format intelligible for a broad audience.

“…8 [31]. Similar studies were carried out for all other planets and the Moon [28][32] [33]. The parameters of their orbits change steadily, like the parameters of the Earth's orbit.…”

Section: Evolution Of Orbital Motionmentioning

confidence: 86%

“…A high-precision method was developed to solve these equations, and it was later used to develop the Galactica system [22], which is free for access [23]. Viability of this method is confirmed by the solution of a number of problems in the contemporary celestial and space dynamics [24] - [28].…”

Section: Evolution Of Orbital Motionmentioning

confidence: 99%

Fundamental Principles and Results of a New Astronomic Theory of Climate Change

2016

AdAp

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“…For creation of a new earth, mankind has to gain sufficient experience in managing with cosmic objects. In 2008, we have suggested turning asteroid Apophis into an earth satellite [23] - [24]. On April 13, 2029, the asteroid will approach the Earth to a distance of six Earth radii (see Fig.…”

Section: Formation Of the Future Habitat For Mankindmentioning

confidence: 99%

“…11) [23] - [24]. For making that asteroid to round the Earth orbit, we have to accelerate the asteroid at its aphelion point (A a ) and, then, decelerate it at the point of its closest approach to the Earth (that is, at the point A b ).…”

Section: Formation Of the Future Habitat For Mankindmentioning

confidence: 99%

Advances in Mechanics and Outlook for Future Mankind Progress

2017

IJMECS

Abstract-Three problems for the interaction between N bodies to which exact solutions were obtained are discussed. In the first problem, the bodies are located axisymmetrically in a plane. Possible trajectories of the bodies here are ellipses, parabolas, hyperbolas, or straight lines. Results of solving this problem are further used for solving problems about Earth's rotation and Mercury's perihelion. In the second problem, the body system consists of several layers, and it rotates as an entity. In the third problem, the bodies are uniformly distributed over a sphere, and they move experiencing no mutual collisions. The latter problem allows the formation of several planets, for instance, one hundred planets resembling the Earth and moving under identical conditions with respect to the Sun. The latter possibility opens a way toward unrestricted mankind progress.

“…We used this option while investigating into the approach of asteroids to planets and Moon [9][10]. Figure 1 and Figure 7 in [10] show data obtained on the basis of file dice.dat.…”

Section: Close-approach File Dicedatmentioning

confidence: 99%

The System of Free Access Galactica to Compute Interactions of N-Bodies

2012

IJMECS

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Abstract-The Galactica System is intended for resolving N-body interaction problems. It is based on a high-precision method for solving differential equations of motion of bodies whose interaction forces are inversely proportional to the squared distance. The differential equations of motion and their solution method are given in paper. The structure of the input file, the files of initial conditions and output files are described. The examples of these files for different solved tasks are presented. The actions of executable files are explained. The paper describes all the theoretical and practical issues so that even a novice researcher could use Galactica System in his/her works.