Keith_w wrote:This style of weapon couldn't do it? You still have not said how you think this style of weapon would work, never mind why it wouldn't do what I suggested. "Dropping" a KEV onto a planet won't work work for reasons I have already mentioned, unless you don't care where it lands, Ghaba-style.
The usual design for a weapon like this is to decelerate the weapon from orbital speed so that it falls into the planet. The deceleration could be done by a launcher in orbit or by rockets on the weapon itself. The weapon may or may not have guidance rockets to assist in final targeting. David has hinted that the weapons on the Rakurai may have guidance systems.
But, in general the purpose of the weapon is to use the gravitational potential energy of the planet to produce the energy released by the impacting weapon. If the gravitational potential energy is the primary source of energy for the impactor, the launcher or rockets only need to provide enough energy to decelerate the weapon from orbit. In that case, it would not have enough energy to boost the weapon out of orbit away from the planet.
It is certainly possible to design an orbital ballistic system with more energy. That would mean that a significant amount of the energy of the impactor would come from the launcher or rocket, in addition to the gravitational potential energy. I have not every said that it is impossible for the OBS to be designed this way. I have only said that I doubt that it is.
As for showing that gravity assist won't work, I am pretty sure that you simply paraphrased the Wikipedia entry and waved your hands, declaring it to be a non-starter.
Actually, I paraphrased the textbooks sitting next to me. And I did not wave my hands. I showed you the equation which demonstrates that the final velocity with respect to the planet is unchanged. You have not disputed that--you just don't seem to believe that this is important.
I have used the term escape velocity up to this point, because that's the term most people are comfortable with. Escape velocity is more complicated than most people realize. It is not a fixed speed--it is dependent on your altitude above the planet. The escape velocity at the Earth's surface is 11.2 km/s. If you launch a rocket at 12 km/s, it will escape the earth's gravity and fly away in interplanetary space. But as the rocket rises, it's velocity slows. At 500,000 km, it's speed with respect to the Earth will be far below 11.2 km/s. In fact, it's relative speed will approach 0.8 km/s as it gets further away from the Earth (12 km/s - 11.2 km/s). But escape velocity depends on the altitude; the rocket is still moving 0.8 km/s faster than escape velocity
at that altitude.
So a more complete way of analyzing it is by examining the mechanical energy E of the rocket (or KEW, in this case). The mechanical energy is the sum of the kinetic energy K(with respect to the planet) and the gravitational potential energy U (with respect to the planet). E = K + U.
The kinetic energy is the familiar K = 1/2 mv^2. The gravitational potential energy is U = -GMm/r. Notice that the gravitational potential energy is negative! The full equation then becomes E = (1/2 mv^2) - (GMm/r).
This equation is critically important. This total mechanical energy is a
constant, unless energy is added or subtracted to the system by some other source. In other words, you could change the total mechanical energy if you used a rocket, or a launcher, or some other method of transferring energy to the KEW. But if you don't use transfer energy to or from the KEW, the total mechanical energy stays the same.
Notice that the gravitational potential energy is dependent on r, the distance from the planet. Imagine a KEW in an elliptical orbit, or falling toward the planet. As the KEW gets closer to the planet, the gravitational potential energy decreases (becoming more negative). Since E is a constant, the potential energy U is transferred to K. K increases, which means it moves faster. Similarly, as the KEW moves away from the planet, the kinetic energy K is transferred to the potential energy U. An object which is in free-fall (whether rising, falling, in orbit or not) transfers energy between K and U as the altitude changes. An object in an elliptical orbit goes through a cycle, with maximum K at perigee (or periapse), and minimum K at apogee (or apoapse). But the energy E stays the same the entire time.
If the total energy E is negative, then the object is in orbit. (If the orbit intersects the planet, we would call it falling.) An astronomer would say that the object is bound. If the total energy E is positive, it is not in orbit--it will escape the planet (assuming it doesn't hit something). It is unbound. In common speech, the object has escape velocity. If the total energy is exactly E, then it has barely enough energy to escape the planet. In technical terms, the speed of the object would approach zero as the object approaches infinite distance.
Let me emphasize once again that this equation applies whether you are in orbit or not. In particular, it will still apply even when you are using a gravity assist. If the total mechanical energy E with respect to the planet is less than zero, it is trapped in orbit. You would need some
other source of energy to get the object out of orbit. That energy might be rockets, or electromagnetic launcher, or solar sails, or manipulating the planet's magnetic field, or whatever. But if you do that, it is that energy source which is getting the object out of orbit, not gravity assist.