This investigation into chemically altering, and thus geologically changing the nature of a planetary atmosphere and its surface provides new scientific predictions, insight, and numerical theories into the
feasibility of technologically inducing the habitability of other worlds. Innumerable permutations of potential planetary evolution pathways exist due to large variations in the astrophysical, atmospheric, and
geologic properties of a given world, dictated by unique planetary formation, dynamics, and evolution. Surface interactions that give rise to habitable climates are driven by geochemical reactions and
geomorphic processes that can act in feedbacks to either promote or decay the climactic habitability of a planetary atmosphere and surface. Using the TerraGenesis smartphone application created by Alexander
Winn, I simulate and track 21 different technologically induced planetary engineering scenarios. I present numerical-game simulation modeling of our solar system’s real terrestrial bodies: Mercury, Venus, Earth,
the Moon, and Mars, Jupiter’s moons: Io, Europa, Ganymede, Callisto, Saturn’s moons: Tethys, Dione, Rhea, Titan, and Iapetus, Uranus’s moon Oberon, and Pluto. I test a range of four hypothetical exoplanets
to colonize: Bacchus, Pontus, Ragnarok, and Boreas. I also use the model on the exoplanet TRAPPIST-1d, while considering this approach for other future exoplanet studies. Calculations in this application are taken
out with simple, coupled numerical rules, with model years into C.E., the Common Era. The user of this application 'controls' the terraformation process by manipulating the temperature, atmospheric pressure,
oxygen content, sea level, and biomass, limited by economic resources and population. Technologically induced terraforming in this numerical model produced all 21 tested habitable worlds, and reached stability
within 1,000–3,000 mission years. Through testing the efficacy of terraforming technologies to combat modern climate change on the Earth, this report additionally shows that it is at least feasible to achieve
stable habitability on Earth before (or after) a global climate catastrophe; reversing the effects of modern climate change may take on the order of 100–1,000 years. This paper also reviews and condenses the current literature in the year 2018 on terraforming as well as recent developments and advancements. This is the complete report and in this state has not been submitted for review.