Príklady orbit

• Qualitatively similar orbits are obtained in the many par ticle calculations.

• In opposition to this, chaos is effective for causing rapid desynchronization, because of its characteristic exponential divergence of nearby orbits.

• Dynamically we find most orbits to be stable over long time scales and typically this happens in a wider parameter area than in co-rotating systems.

• The bar will hence be able to relocate stars, and stars with low or high metallicity could be found far away from their original orbits.

• We only need that the return maps at periodic orbits are diagonal on the stable and unstable manifolds.

• In most cases, those planets follow orbits with significant eccentricity, leading to substantial seasonal temperature excursions.

• In most cases, those planets follow orbits with significant eccentricity, leading to substantial temperature excursions.

• Indeed, nebular drag and collisions would ensure that orbits with zero eccentricity were preferred.

• The steady-state solution of the equation of motion is then derived in cartesian coordinates and two groups of electron orbits are defined.

• Here, a planetary system consisting of one star and two identical-mass planets in circular but mutually inclined orbits is considered.

• Quasiperiodic orbits can look quite complicated, especially if there exist many incommensurable frequencies.

• The velocity of the planet orbiting at this distance satisfies the relation vn=w/n.

• The project mission was to locate intelligent signals coming from hypothetical planets orbiting the stars.

• A caustic is formed by the envelope of these orbits.

• Note that the orbits are almost per fectly laminar and there is no sign of filamentation.