Escape velocity - Won't the orbital path just become larger with higher initial velocity? Escape velocity is the minimum speed needed for an object to escape from the gravitational influence of a massive body. However, gravity has infinite range. Object $A$ is always getting pulled by the gravity of object $B$ no matter the distance between object A and B. (Maybe the force becomes extremely small with increasing distance, but still not zero)
So, how can an object possibly “escape the gravitational influence of another object”? Is there a more accurate definition of escape velocity? Won't the orbital path just become infinitely large with increasing initial velocity?
 A: The important part here is the speed of the orbiting object.
Every distance of the orbiting object has its own orbiting speed (orbiting along the circle). If you increase the speed, the orbiting path changes to an ellipse; if you increase the speed more, the ellipse becomes more and more prolonged.
If you continue to increase speed, there will be the moment in which the path becomes parabolic — and parabola is not closed curve anymore, so the object escapes — not from the gravitational force, but from the orbiting around the object.
A: 
Is there a more accurate definition of escape velocity?

First, consider an object with a radial orbit (zero angular momentum orbit) in a $1/r^2$ central force field. The total energy $E$ of the object (which is constant) is the sum of the (negative) potential energy $U(r)$ due to the force field and the kinetic energy $T(v)$ due to the radial speed.
There are three cases to consider:


*

*$E \lt 0$:  The orbit is bounded, i.e., there is a maximum, finite distance $r = r_{max}$ where the speed (and thus kinetic energy) is zero, and the object has maximum (least negative) potential energy

*$E \ge 0$:  The orbit is unbounded, i.e., the object never has zero speed. As $r \rightarrow \infty$, the kinetic energy $T$ asymptotically approaches $E$ from above.

*$E = 0$:  A special case of the unbounded orbit in that $T \rightarrow 0$ as $r\rightarrow\infty$.
It is this special case that is relevant to the definition of escape velocity. At any radius $r_0$ in the central force field, there is a speed $v_e$ such that
$$T(v_e) = |U(r_0)|$$
Thus, an object starting at $r = r_0$ with outward radial velocity $\vec{v}_e$ has just enough kinetic energy to, ahem, 'coast to a stop at $r = \infty$'.
More precisely, the object will coast arbitrarily far away with speed arbitrarily close to zero. In this sense, the object 'escapes' the central force field, but just so.  
A: Yes, what you have really discovered is that the phenomenon under consideration has been mislabeled as "escape". At least as far as a layman's likely understanding. Or perhaps the problem is the layman's understanding of "from what". Where you are thinking of "from gravity", what the scientist means is "from a closed orbital path" (elliptical), or in short "from orbit" itself, "orbit" implying a return. As to how an object can possibly evade the persistent force of gravity trying to return it, maybe this will help: an object moving away from a gravitational body is experiencing a decrease in the body's gravitational pull as distance increases. It is possible for an object to have sufficient speed that the decreasing pull always remains below the object's ability to "outrun" that pull. The object's speed never decreases below what would allow the body to pull it back in from whatever distance it has currently managed to obtain. It "wins" the energy race.
A: You are right. The notion of "escape" from a gravitational field is something that only exists in an idealized mathematical model of the situation. In that idealized model, we have only one gravitator, in a space-time of infinite extent. With that, we can state the idea of the escape velocity as thus:

It is the minimum speed that an object must be thrown away from the gravitator, in order that it will reach infinite distance, after an infinite lapse of time.

If you throw the object with less speed than this, it will come back: either it will strike the gravitator's surface, or it will go into a repeating orbit around it that nonetheless stays within some maximum distance from the object. But if you throw it outward with speed at least the escape velocity or higher, then the orbital path "becomes infinitely large" - it goes out to, and intersects (in a sense) infinity.
In formal language, if $\mathbf{r}(t)$ is a vector pointing from the gravitator toward the thrown object and which traces its trajectory, and at $t = 0$ we throw the object, the escape velocity is the minimum speed $v_\mathrm{esc}$ such that if
$$|\mathbf{r}'(0)| \ge v_\mathrm{esc}$$
i.e. the speeed at time of throw is larger, then
$$\lim_{t \rightarrow \infty} |\mathbf{r}(t)| = \infty$$
, that is, the distance from the planet grows forever. In reality, of course, there are two limitations: for one, we can never have an infinite time go by, which means that the object will, at all times, still be theoretically under the influence of the gravitator, even if that influence is extremely small. The other limitation is that in reality, there will be other gravity sources present at distance, which will then change the trajectory in other ways once their influence begins to dominate control over the motion of the thrown object and this, in turn, will also prevent reaching that infinite distance. For example, if we are talking about the Solar System, and we are "escaping" the Earth, if we launch a craft away with no more than Earth's escape velocity, then it will only "escape" until the Sun's gravity begins to dominate it, at which point it will now follow a more complicated trajectory based on mutual influence between the Earth and Sun (mostly, it will orbit the Sun, since the Earth will move away in the interim, but it may encounter the Earth again), and also, to some extent, the other planets.
Nonetheless, it is useful because we can take it as a ballpark for the minimum speed, and hence minimum effort which our engine must expend, to "get away" from the gravity source and get to a more remote destination like, say, Mars. Of course, actually travelling there will require more speed change (so-called "delta vee"), because we will also need to navigate to intercept that destination and then settle onto its surface safely.
A: Throw a stone up, and it will fall back on Earth. But if you give it very, very large speed, it will go away, into space. Surely, it's always under the gravitational influence of the planet but it has speed great enough that it never returns back. 
The minimum speed needed for this is called escape velocity. And at that speed (or greater) the path of the object is an open curve; this means the curve extends to infinity and the object, hence, has no bounds on how far it can go.
A: 
How can an object possibly “escape the gravitational influence of another object”? Is there a more accurate definition of escape velocity? Won't the orbital path just become infinitely large with increasing initial velocity?

The apparent paradox can be resolved by considering the kinetic and potential energy of an 'object' projected from a planet's surface at some initial velocity. 

Imagine an object travelling outwards from the centre of gravity of a planet at uniform speed and calculating the potential energy being gained. If the force on the object due to gravity was uniform with distance then the potential energy would increase linearly with distance.  If the object was released from a given height it would fall and impact with a velocity V (assuming no atmosphere).  
Energy = mgh = 1/2mv^2
So V from a given height = (2gh)^0.5
However, with increasing distance from the 'planet's" center of gravity the inverse square gravitational effects means that the energy needed to reach that altitude increases more slowly with distance. The integration of required energy with increasing distance has a finite value at infinity. |
Conversely, an object "falling" from an infinite distance has non-infinite potential energy and so non-infinite impact velocity. This is the escape velocity. 
An object projected from the planet at escape velocity will lose kinetic energy as it "rises" but the rate of loss will decrease with distance due to the inverse square gravitational effect. It will ultimately come to a stop at infinite distance.
An object projected at lower than escape velocity will "stop rising" at some distance less than infinity.   
An object projected at above escape velocity will still have net kinetic energy and "outward" motion both at infinity and at all lesser distances. 
A: You know the old saying, "What goes up, must come down"? If you go up at escape velocity or faster, it's not true. 
You'll keep slowing down, but never come down, because the gravitational influence of the body you're "escaping" falls off (by the inverse square rule) as you get further away. It never goes away, but it's never strong enough to reverse your velocity.
A: This notion confused me too, but a simple way to explain it would be to compare the gravitational pull on the object at each given moment to the sum of an infinite series of numbers, say the series (1/2)+(1/4)+(1/8)+(1/16)…  It's easy to see that this series goes on forever, as you can simply cut each new term in half to create the next term.  However, while this series is always getting bigger, it will never approach infinity.  If you could sum up all the infinite terms of this series, it would ultimately add up to 1.  
Think of a empty box with a volume of 1 cubic meter.  Fill in half the volume with water, then fill in half the remaining volume with water, then half the remaining volume again... you will get closer and closer to filling the box exactly, which is a finite volume, despite the fact that you are adding water an infinite number of times.  If you place the box on a scale opposite an identical box that is completely filled with water, the box you are adding water to will never tip the scale in its favor.
In the same way, if you were to add up the pull of gravity on an object traveling at escape velocity over an infinite time frame, you would find that the pull of gravity on that object is ultimately adds up to a specific number - escape velocity.  Therefore, going at or faster than escape velocity means that the object will never be pulled back, similar to how the partially-filled water box in the previous paragraph will never outweigh the completely-filled one.
A: The object doesn't escape the gravitational influence; as you have noted, $1/r^2$ is never equal to $0$. However, what we mean by "escape velocity"is that the object has enough energy (large enough velocity) so that its path would have to "turn around at infinity". In other words, the object's velocity is high enough and decreasing slow enough to where the object will never turn around.
A: You are right. To talk of escaping the Earth’s gravitational field is nonsense, and confusing nonsense, and therefore immoral. 
A particle at rest at the distance of Sirius and free of all other gravitational influences will fall towards the Earth. The acceleration is 56 microns per century per century. 
If you imagine an object projected up from the Earth at high speed, the Earth’s gravity will slow it down and carry on slowing it down for ever. Because gravity is governed by an inverse square law, the total slowing down adds up to a finite figure. (If gravity had been $1/r$ rather than $1/r^2$ the sum would have been infinite, not finite).
“Escape velocity” is thus defined as “the speed at which you have to start if you want to get all the way to infinity without falling back”. Or rather, since that is impossible, it is the speed greater than all those that do fall back eventually. 
Talking about escaping the Earth’s gravitational field is a lie, but at least an understandable one, since if you are next to Sirius you will be subject to gravitational accelerations much greater than 56 microns per century per century. 
A: If you fell from infinity to the body you would go splat on it with a given amount of energy, energy you picked up gradually as you fell. However if instead you set off from the body with slightly more kinetic energy than that which you went splat with, then you would reach infinity and beond! The speed you need to have that amount of kinetic energy is the escape velocity.
A: 
Won't the orbital path just become infinitely large with
  increasing initial velocity?

No, is the short answer (more on that in a moment). 
But firstly, your basic confusion appears to arise from mixing up two separate concepts:
a. For the orbital path to be infinitely large implies an infinite initial velocity (which obviously is not possible in any realistic scenario: nothing in the universe travels with infinite velocity).
b. For an orbital path to be possible at all implies a finite initial velocity -- and we're back to "no is the short answer" -- because:
i) If it was possible to have infinite initial velocity, by definition that must exceed the escape velocity, which is a defined, finite, velocity. The moment it does exceed that (finite) velocity, which would be long before reaching infinite velocity, any type of orbit becomes impossible: the rocket must go shooting off into space.
Orbit is an equilibrium state, where the force pushing the orbiting object away from the planet (basically, its momentum) is exactly equal to the force pulling it toward the planet (basically, gravity). If the outward impetus is in exact balance with the inward impetus, the equilibrium thus achieved causes the orbiting object to maintain a constant distance from the planet: an orbit.
ii) A slight imbalance in those forces will cause the orbiting object to orbit out to a greater radius distance, or to orbit in to a lesser radius distance; but a large (positive) imbalance will result in the object leaving orbit: it will cease to follow a curved path about the planet: the larger imbalance will cause it to follow, increasingly, a less curved path, until the path has largely ceased to curve at all: the object is now going in a straight line (approximately), so has ceased to orbit.
iii) Having once attained escape velocity, whether or not this follows upon an orbiting stage, if the rocket does no more than maintain its constant velocity it can never be recaptured by the planet's gravity, because the gravitational strength falls off with distance: under the inverse-square law, when the distance from the planet doubles the gravitational strength is not constant, but reduces to one-quarter. With merely constant speed, the rocket can never be captured by the falling gravitational force (because the latter is falling).
Only by decelerating could the rocket reduce its momentum such as to be travelling with less velocity than the critical threshold needed for equilibrium, i.e. an orbit, at its new radius distance from the planet (a very large deceleration would be involved, once the rocket has travelled even a short distance, because in real life, at a very short distance from the planet its gravity gives way to the Sun's far greater gravity, with the planet becoming thereafter a negligible influence).
So a further misunderstanding in your question now emerges: by treating the planet as if it was the only source of gravity in near-space, you have misled yourself into neglecting nearby stronger gravitational forces! Those forces overwhelm the planetary effects at quite short distances, such that your orbital-path assumptions break down, once the rocket has moved only quite a short distance from the planet.
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ADDENDUM -
The very small differences in orbital altitude associated with an eliptical orbit are irrelevent to my answer. The only relevent issue is whether the orbit is stable: if it is, minor altitude differences won't clarify the position any. I am addressing only the main issue: is the satellite-cum-rocket able to accelerate (taking it out of orbit), and is it able to decelerate (taking it out of orbit).
Like it or not, in reality all rockets burn fuel at a constant rate, and the only reason they go faster is that gravitational resistance to their motion decreases as altitude increases, obeying the inverse-square law.
Burning fuel at a constant rate, the amount of fuel it is possible to carry sets a real limit on its initial velocity (if it is going further than Earth orbit), and there are practical restrictions on the weight of fuel it is possible to lift (every extra ton of fuel in the tanks increases the mass which must be lifted into space). So increasing the payload of fuel has negative consequences also, not purely positive ones.
And a high enough initial velocity will prevent the rocket going into orbit: it will do what planetary probes do, and depart for Mars or beyond. If it never completes even a single orbit, it is not reasonable to describe it as having an orbit. If it will also depart the solar system, as some do, it will not even be orbiting the Sun, in any meaningful sense.
The gravitational influence of a single quark is tiny, for an individual quark, so it is only logical to conclude that its radius is also tiny. It is therefore not logical to conclude that its influence is infinite. The inverse-square law demonstrates that even with objects of stellar mass, the influence declines rapidly. Doubling the distance, the strength declines to a quarter, i.e. 25 percent (1 over 2 squared, i.e. 1/4). At 8 times the distance, the strength is only one percent (1 over 8 squared, i.e. 1/64th).
