First, you have the gravity well of the planet that you are departing, then you have the gravity well of the star around which that planet is orbiting, which is sufficiently strong so as to keep that planet in orbit around said star, then you have the gravity well of the galaxy which is keeping all of the stars orbiting the Galactic Core, and you finally have the Universal Gravitation constant.
Also, by 1-G acceleration, it means that you are supplying sufficient force to a mass to accelerate it at the rate of 9.81 meters per second per second or 32.174 feet per second per second. It has nothing to do with the gravitation field that you are in.
What do you mean that T5 says that beyond 10 Diameters the efficiency of a gravitic drive would drop to 1%? The Earth's Moon is about 30 Earth diameters away from the Earth. The Earth possesses a sufficiently strong gravitational field to retain the Moon in orbit against the gravitation pull of the Sun at that distance. Also see the discussion of the Lagrange Points here, where the interaction of the Earth's, Moon's, and Sun's gravitational fields creates a stable volume in space for orbit:
http://en.wikipedia.org/wiki/Lagrangian_point
Also, in accelerating to that 10D distance, you build up a considerable velocity, which does not go away simply because you stop exerting a acceleration force. Assume that, based on Starter Traveller, you boost for 1-G for 2000 seconds to reach a distance of 10,000 kilometers from a planet's surface. That 2000 seconds of 1-G boost gives you a velocity of 19.62 kilometers
PER SECOND, or 70,632 kilometers
PER HOUR. If all you do is coast from that point, supplying just enough force to counteract the slowing of the ship by the planetary and stellar gravitational fields, you will reach your safe Jump Point at 1,280,000 kilometers distance from the planet in about 18 hours, 7 minutes, 20 seconds. That does assume no turnover and deceleration to have essentially zero relative velocity at the jump point (you do not really have zero velocity, but explaining that gets a bit complicated).
However, if your gravitic drive does become basically ineffective at a distance of 10 diameters from the departure planet, and you have to arrive at the target planet 100 diameters distance,
HOW DO YOU GET TO THE ARRIVAL PLANET? According to your statement of the rules,
YOUR DRIVE DOES NOT WORK. For that matter, how do you decelerate at all once you are halfway to the jump point?
Accelerating at 1-G to your 10 diameter distance from the Earth, when you reach that point 128,000 kilometers from the surface, you have been boosting at 1-G for 7,224 seconds, or a fraction over 2 hours. You are traveling at over 70 kilometers
PER SECOND, or over 250,000 kilometers
PER HOUR. Your drive no longer works effectively.
HOW DO YOU SLOW DOWN?
If, in fact, the T5 rules really state that beyond 10 diameters from a planet, your drive works at 1% efficiency, then there is a
MASSIVE problem with how the gravitics drive is described at working, which needs to be either fixed or simply dropped from further consideration.