Say, a hyperbolic orbit clear out of the solar system.

They intended to come within one mile of the surface in a hyperbolic orbit.

The two most general cases with these 6 degrees of freedom are the elliptic and the hyperbolic orbit.

"We're falling free, in a hyperbolic orbit around the pulsar.

It traveled by hyperbolic orbits, not the straight lines of a high-booster.

A majority of comets have either parabolic or hyperbolic orbits.

Objects in a hyperbolic orbit can escape from the solar system altogether."

Similar effects happen in closed and hyperbolic orbits.

Comets from interstellar distances would arrive on wide hyperbolic orbits.

Hyperbolic orbit, accelerating like they've got lots of power."

It is strictly defined for elliptic, parabolic, and hyperbolic orbits.

Others, such as time-of-flight are far more complicated, especially for near-circular and hyperbolic orbits.

Gabriel chose a long hyperbolic orbit that would take them nearly out to the orbit of the last planet.

'The best you can do is a hyperbolic orbit, and my guess is that it'll take full power to make that.

For a hyperbolic orbit, it is equal to the excess energy compared to that of a parabolic orbit.

"If he manages to knock our engines offline for even a few minutes, we'll be unable to escape this hyperbolic orbit.

The connection between the polar argument and time t is slightly different for elliptic and hyperbolic orbits.

"Setting up for hyperbolic orbit."

The hyperbolic Kepler equation is used for hyperbolic orbits (ε 1).

Furthermore, the equation was derived on the assumption of an elliptical orbit, and so it does not hold for parabolic or hyperbolic orbits.

Heavenly bodies such as comets with parabolic or even hyperbolic orbits are possible under the Newtonian theory and have been observed.

At first it was believed to be a natural body, moving on a hyperbolic orbit which would take it round the sun and on to the stars.

It's in a hyperbolic orbit."

Hope-fully, he thought, on a hyperbolic orbit that would give everyone a beautiful display, a bad fright, and then disappear, still shedding part of its mass.

An infinitesimal increase to ε results in a hyperbolic orbit with a turning angle of 180 degrees, and the orbit appears to be a ray.