2008 - Communication Across the Curriculum (CAC)
2008 - Communication Across the Curriculum (CAC)
2008 - Communication Across the Curriculum (CAC)
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E s s a y<br />
site effort. And that will take an incredible degree of precision in<br />
planning. But this is all in <strong>the</strong> future. Right now, <strong>the</strong> work is far<br />
more simplistic, though it will affect future surveyors to a large<br />
degree. There are fundamental questions being debated right<br />
now:<br />
* Do we use <strong>the</strong> Earth-style systems of longitude using two<br />
sets of 180-degree hemispheres, or do we use a full sphere of<br />
360 degrees Or do we realize that Mars will not just be settled<br />
by Americans, and use international metric units<br />
* Does <strong>the</strong> smaller diameter of Mars (less than 3400 km)<br />
indicate that <strong>the</strong> octomatic base-8 number system may be more<br />
appropriate as a standard instead of <strong>the</strong> Roman base-10 or<br />
surveying’s traditional base-60 systems<br />
* What physical monuments will be required to resist <strong>the</strong><br />
Martian climate and be easily found after a few dozen giant<br />
sandstorms blow over it Or should physical monuments be<br />
avoided altoge<strong>the</strong>r, replaced by detailed records of boundaries<br />
supported by major landmarks and GPS<br />
* How will all this affect land and development laws Certainly<br />
our modern Machiavellian legal code has it’s limitations, and <strong>the</strong><br />
opportunity to build a new simplified and dynamic legal code is<br />
undeniable. But what directions will <strong>the</strong>se laws take<br />
* It is estimated that Mars needs to have at least 25% liquid<br />
surface water before it becomes fully habitable (no spacesuits<br />
required), and much of this will come from frozen sub-surface<br />
ice or imported from nearby sources. What will this do to Martian<br />
topography, and how do we plan for those changes<br />
* Martian colonization will be heavily computer dependent.<br />
However, <strong>the</strong> space shuttle currently runs on <strong>the</strong> equivalent of<br />
<strong>the</strong> old 386 desktop computers because more modern systems<br />
have great difficulty working in low-gravity environments.<br />
Someday this barrier will be broken, and how will we apply this<br />
new generation of electronics to surveying<br />
V o l u m e I V : F a l l 2 0 0 8<br />
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