Re: FT Taskforce and Fleet Actions
From: Ryan M Gill <rmgill@m...>
Date: Tue, 7 Aug 2001 12:20:06 -0400
Subject: Re: FT Taskforce and Fleet Actions
At 10:16 AM -0400 8/7/01, Jerry Acord wrote:
>
>Consider two scenarios: 1) the Earth orbiting the Sun at 1 AU; 2) the
Earth
>orbiting a 1-solar mass black hole at 1 AU. The orbit is the same in
both
>scenarios. Replacing the Sun with a b.h. will not magically suck all
the
>planets into it. 1 solar mass is 1 solar mass. However, close in you
Course getting the Sun to become a black hole when it isn't over the
Chandrakar (sp?)
limit is of course impossible. Thats the nice thing about a main
sequence dwarf.
>_will_ get weird effects and spacetime _is_ warped much more severely
close
>to the b.h. than it is near the Sun. It's just further out that the
severe
>warping smooths out. That's why a b.h. will have an event horizon, but
the
>Sun obviously doesn't...
Ok, I see, the slope is sooner for the gravity well in the case of
the larger star. But is the well as deep since it's spread out?
>(SImilar argument, but in the opposite direction, for G2V vs. red
giant)
>
>So as far as FTL / hyperspace travel is concerned, you could say the
"higher
>order spacetime perturbations" of the denser object lead to a
relatively
>further stand-off distance for safe hyperspace entry etc. etc. etc.
(hands
>waving vigorously...)
Yeah, it'd be easier in my mind to base it off of total mass of the
star/system. The safe region of a Moderate to distant binary system
(or even a trinary with a 2 dwarfs and a compact main sequence) would
be nasty.
--
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