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This leads to a "tail disconnection event".
The longer the period the more elongated the ellipse. List of numbered comets and List of Halley-type comets Periodic comets or short-period comets are generally defined as those having orbital periods of less than years.
Comets whose aphelia are near a major planet's orbit are called its "family". Short-period comets with orbital periods less than 20 years and low inclinations up to 30 degrees to the ecliptic are called traditional Jupiter-family comets JFCs. Jupiter is the source of the greatest perturbations, being more than twice as massive as all the other planets combined.
These perturbations can deflect long-period comets into shorter orbital periods. Occasionally the gravitational influence of the outer planets in the case of Kuiper belt objects or nearby stars in the case of Oort cloud objects may throw one of these bodies into an elliptical orbit that takes it inwards toward the Sun to form a visible comet.
Unlike the return of periodic comets, whose orbits have been established by previous observations, the appearance of new comets by this mechanism is unpredictable. List of long-period cometsList of near-parabolic cometsand List of hyperbolic comets Orbits of Comet Kohoutek red and the Earth blueillustrating the high eccentricity of its orbit and its rapid motion when close to the Sun.
Long-period comets have highly eccentric orbits and periods ranging from years to thousands of years. The future orbit of a long-period comet is properly obtained when the osculating orbit is computed at an epoch after leaving the planetary region and is calculated with respect to the center of mass of the Solar System. By definition long-period comets remain gravitationally bound to the Sun; those comets that are ejected from the Solar System due to close passes by major planets are no longer properly considered as having "periods".
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The orbits of long-period comets take them far beyond the outer planets at aphelia, and the plane of their orbits need not lie near the ecliptic. Single-apparition or non-periodic comets are similar to long-period comets because they also have parabolic or slightly hyperbolic trajectories  when near perihelion in the inner Solar System. However, gravitational perturbations from giant planets cause their orbits to change. Single-apparition comets have a hyperbolic or parabolic osculating orbit which allows them to permanently exit the Solar System after a single pass of the Sun.
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Some authorities use the term "periodic comet" to refer to any comet with a periodic orbit that is, all short-period comets plus all long-period comets whereas others use it to mean exclusively short-period comets. Early observations have revealed a few genuinely hyperbolic i. If comets pervaded interstellar spacethey would be moving with velocities of the same order as the relative velocities of stars near the Sun a few tens of km per second.