bison, on 16 December 2012 - 12:26 AM, said:
On the particular issue of the supposed difficulty of moving a space probe about to different positions, in order to reach the gravitational focal points for various star systems: Using our own solar system as a model, the sphere defining the distance of the ideal focal points is about 186 billion miles in diameter.
If we assume that star systems of interest are one degree apart on this sphere, the distance between their focal points should, I believe, be about 162 million miles. At even the very modest speed of one percent that of light, it should take about 24 hours to move from one focal point to another.
It appears that here you assume that only a change in angle is required. However, is it not true that the star systems to be observed would need to be at least close to the same distance from the gravitational lens for that to be the case?
Obviously, signals can be corrected for variations, but my original point was that, in order to focus at any desired distance (and not just one distance) it would be necessary to alter the lens - in this case the gravitational field of the Sun.
If you were, for example, observing a star that was 25 LY away, then shifted to one that was 50 LY away, where is the adjustment for the change in distance (and not just degrees of arc?)
Telescopes would do a better job. How about radiotelescopes mounted on both the north and south poles of every planet in our system, and maybe on a few asteroids? That's be a nice-sized collector.
Harte
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