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Opening
the Next Frontier
by Anthony Tate
Part 4: So, why aren't we going?
The mood of the country has changed, at last. The mass swell of
the 60's counterculture is passing through its lifecycle, and slowly
clearing the way for new, younger, more aggressive leaders and thinkers.
Slowly but steadily America is looking for those new frontiers. We are
tired of resting on the laurels won for us by our grandfathers.
But one huge hurdle remains. While America's mood is looking for
adventure, and our technology has emphatically progressed to the point
that we can tackle hurdles of this size with less than a Herculean
effort, science has not altered its rules one little bit.
And that is why the Space Shuttle uses fuels that are not even as
good as the ones the moon Rocket used. We are stuck.
Sure, there is research into high energy metastable fuels. Liquid
Ozone has been investigated as a possibly better oxidizer, but even with
our better technology we can't make it stable enough to use.
Metallic hydrogen also has great potential, but we can't even make
it last a few seconds, never mind make rocket fuel out of it.
Spin-stabilized triplet helium also has huge potential, but it's even
harder to make than metallic hydrogen. Sadly, it looks like chemistry is
just not going to be amenable to our desires, at least not anytime soon.
By anytime soon, I mean 'this century.' Metastable fuels are HARD.
So, it looks like we are stuck, despite our newly adventurous
mood.
Well, not quite, but getting past the stubbornness of chemistry
requires that we cheat. Or maybe make a little deal with the Devil.
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Contents:
1: The Frontier Spirit
2: What went wrong.
3: Where do we go next?
4: So, why
aren't we going?
5: Dealing with the Devil
6: A brief technical interlude
7: So how good is Nuclear, anyway?
8: Heat, temperature, and cooling.
9: But isn't this dangerous?
10: Prometheus would be proud of
us.
11: Ok, that all sounds nice, but
this is just fantasy, right?
12: But isn't this just too big?
13: But doesn't this thing make
nuclear waste?
14: Conclusions
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