164,96 €
183,29 €
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The elliptical restricted three body problem
The elliptical restricted three body problem
164,96
183,29 €
  • We will send in 10–14 business days.
Restricted three body problem is used to study the behavior of spacecraft, asteroids, and moons in systems like the Earth-Moon-Sun, Jupiter's moons etc. The present book deals with the problem of finding the existence and stability of the equilibrium points in the Elliptical restricted 3-body problem. It also helps in analyzing Lagrange points, which are positions in the orbital plane of the two massive bodies where the third body can maintain a stable position. Resonances play a critical role…
183.29
  • Publisher:
  • ISBN-10: 3639717783
  • ISBN-13: 9783639717785
  • Format: 15.2 x 22.9 x 1 cm, minkšti viršeliai
  • Language: English
  • SAVE -10% with code: EXTRA

The elliptical restricted three body problem (e-book) (used book) | bookbook.eu

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Restricted three body problem is used to study the behavior of spacecraft, asteroids, and moons in systems like the Earth-Moon-Sun, Jupiter's moons etc. The present book deals with the problem of finding the existence and stability of the equilibrium points in the Elliptical restricted 3-body problem. It also helps in analyzing Lagrange points, which are positions in the orbital plane of the two massive bodies where the third body can maintain a stable position. Resonances play a critical role in understanding the long-term evolution of orbits in celestial mechanics. The linear and non-linear stability has been studied for 3rd and 4th order resonance.

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  • Author: Shilpi Dewangan
  • Publisher:
  • ISBN-10: 3639717783
  • ISBN-13: 9783639717785
  • Format: 15.2 x 22.9 x 1 cm, minkšti viršeliai
  • Language: English English

Restricted three body problem is used to study the behavior of spacecraft, asteroids, and moons in systems like the Earth-Moon-Sun, Jupiter's moons etc. The present book deals with the problem of finding the existence and stability of the equilibrium points in the Elliptical restricted 3-body problem. It also helps in analyzing Lagrange points, which are positions in the orbital plane of the two massive bodies where the third body can maintain a stable position. Resonances play a critical role in understanding the long-term evolution of orbits in celestial mechanics. The linear and non-linear stability has been studied for 3rd and 4th order resonance.

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