The vertical components would be canceled out in any case. If you have two stars, there will be a hemisphere above the plane and below the plane for both of them. Treating things as point masses is only an approximation; there's not a magical distance or gradient where the properties of gravity suddenly change.
I'm not saying there is. Think of this in terms of vectors. For two stars 6LY apart the horizontal component is very large and the vertical one is basically negligible in comparison. When a nebula is 10LY across the vertical component is almost as big as horizontal one. That means a lot of the gravity is being cancelled out and the overall gravitational attraction felt by the remaining star is consequently much smaller.
Ahh, okay. Then the site I linked to earlier may actually be right.
The horizontal component will also move closer to the second sun too. And based on my last set of calculations, we know(?) that that will affect the second sun much more so than the particles moving vertically only and the particles on the other side of the original sun. It looks like the two might actually cancel each other out.
Moving vertically:Before:
P1x = (G*dM/6^2)*cos0
P1y = (G*dM/6^2)*sin0
P2x = (G*dM/6^2)*cos0
P2y = (G*dM/6^2)*sin0
Px = P1x + P2x = .0556G*dM
After:
P1x = (G*dM/7.8102^2)*cos(atan2(5,6))
P1y = (G*dM/7.8102^2)*sin(atan2(5,6))
P2x = (G*dM/7.8102^2)*cos(atan2(-5,6))
P2y = (G*dM/7.8102^2)*sin(atan2(-5,6))
Px = P1x + P2x = .0252*G*dM
Moving towards the other sun:P1 = G*dM/6^2
P2 = G*dM/6^2
P1+P2 = .0556G*dM
P1 = G*dM/1^2
P2 = G*dM/11^2
P1+P2 = 1.0083*G*dM
There's also particles in the x axis which will behave much more like the vertical particles. I think you'd need to do the full integration to know for sure.
My point is that its hard to say whether that's important or not. Depends on whether subspace nodes are simply dependant on the gravitational field of the local star or whether its dependant on all the stars in the vicinity too.
That's not even what I was saying in the first place. I'm not talking about subspace nodes at all, nor am I talking about more than one sun. Quit bringing up new topics into this discussion; it's hard enough when neither of us have a very good grasp of the physics involved.
We know that intrasystem subspace drives depend on a gravitational field.
Assumption: There is a threshold to the gravitational field beyond which it is too weak for intrasystem subspace drives to work.
Question: Would destroying the Capellan sun increase the distance from the system's center that the required field strength exists?
Experiment: Does expanding the mass of the Capellan sun cause the gravitational force at a constant point outside both the nebula and the sun to increase or decrease?
It wouldn't be exactly the same, that's what I'm getting at above. How big a difference it would make depends on how much mass Capella has ejected during the supernova and how big the nebula has become. My point is that I can't give numbers for that since I don't remember the maths any more.
Remember I'm not talking about effects within the Capella system only. I'm talking about the Capella explosion possibly having gravitational effects on other star systems.
Fine, then go start your own thread instead of trying to derail my reasoning
We know that intrasystem jump drives will not reach to other systems under ordinary circumstances. If the answer to the question for my experiment is "Yes", then it's possible that intrasystem jump drives could reach there. If the answer is "no", then we know that they still wouldn't.
IIRC it would take years for the effects to reach other solar systems anyway, so what it would actually do would be irrelevant as subspace travel is generally conducted on the order of hours or minutes.