Maintaining an Ecosystem under Critical Factor Constraint: The Worldhouse
Taylor (1998) presents a best-worst-case scenerio in which the possibility of human habitation of Mars is prohibited by the critical factor of the Martian nitrogen budget (more than 85% of the original inventory may have been lost). Under such a constraint, he argues, Mars may still be made habitable by the construction of a quasi-global “worldhouse,” consisting of a 1-3 km high “roof” spanning the equatorial- and mid-latitudes. The technology required for construction and maintenance of such a structure would not necessarily be far in advance of that currently available. The author goes into detail about everything from ethanal-based fuels to meteor strike prevention, underscoring the necessity of careful planning in an endeavor of this scale.

The table below gives the atmospheric mass savings of Taylor’s “paraterraforming” alternative. Given the likely insurmountable difficulty of full “open-skies habitability” on Mars, it is not so hard to see such a solution as a viable way around full terraformation.
Required Atmospheric Masses
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