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Inmathematics, specifically in the study ofdynamical systems, anorbit is a collection of points related by theevolution function of the dynamical system. It can be understood as the subset ofphase space covered by the trajectory of the dynamical system under a particular set ofinitial conditions, as the system evolves. As a phase space trajectory is uniquely determined for any given set of phase space coordinates, it is not possible for different orbits to intersect in phase space, therefore the set of all orbits of a dynamical system is apartition of the phase space. Understanding the properties of orbits by usingtopological methods is one of the objectives of the modern theory of dynamical systems.
Fordiscrete-time dynamical systems, the orbits aresequences; forreal dynamical systems, the orbits arecurves; and forholomorphic dynamical systems, the orbits areRiemann surfaces.

Given a dynamical system (T,M, Φ) withT agroup,M aset and Φ the evolution function
we define
then the set
is called theorbit throughx. An orbit which consists of a single point is calledconstant orbit. A non-constant orbit is calledclosed orperiodic if there exists a in such that
Given a real dynamical system (R,M, Φ),I(x) is an open interval in thereal numbers, that is. For anyx inM
is calledpositive semi-orbit throughx and
is callednegative semi-orbit throughx.
For a discrete time dynamical system with a time-invariant evolution function:
Theforward orbit of x is the set :
If the function is invertible, thebackward orbit of x is the set :
andorbit of x is the set :
where :
For a general dynamical system, especially in homogeneous dynamics, when one has a "nice" group acting on a probability space in a measure-preserving way, an orbit will be called periodic (or equivalently, closed) if the stabilizer is a lattice inside.
In addition, a related term is a bounded orbit, when the set is pre-compact inside.
The classification of orbits can lead to interesting questions with relations to other mathematical areas, for example the Oppenheim conjecture (proved by Margulis) and the Littlewood conjecture (partially proved by Lindenstrauss) are dealing with the question whether every bounded orbit of some natural action on the homogeneous space is indeed periodic one, this observation is due to Raghunathan and in different language due to Cassels and Swinnerton-Dyer . Such questions are intimately related to deep measure-classification theorems.
It is often the case that the evolution function can be understood to compose the elements of agroup, in which case thegroup-theoretic orbits of thegroup action are the same thing as the dynamical orbits.
A basic classification of orbits is
An orbit can fail to be closed in two ways. It could be anasymptotically periodic orbit if itconverges to a periodic orbit. Such orbits are not closed because they never truly repeat, but they become arbitrarily close to a repeating orbit.An orbit can also bechaotic. These orbits come arbitrarily close to the initial point, but fail to ever converge to a periodic orbit. They exhibitsensitive dependence on initial conditions, meaning that small differences in the initial value will cause large differences in future points of the orbit.
There are other properties of orbits that allow for different classifications. An orbit can behyperbolic if nearby points approach or diverge from the orbit exponentially fast.