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Welcome to Terraforming Wiki. We are currently editing over 457 articles, and you can help About this wiki| New pages| New files| Active users| Categories| Wiki tutorial| Help pages Terraforming Wiki Terraforming is nothing more -
Pluto Simulation
This is a simulation of what one would expect to find on a terraformed Pluto, using formulas from Math And Terraforming. Please note that not even the supercomputers at NASA can provide us with a -
Mars
Mars is the fourth planet from the Sun and the second-smallest planet in the Solar System, being larger than only Mercury. In English, Mars carries the name of the Roman god of war and -
Time, Day And Year On Other Planets
On Earth, we have time measured in time units that are useful only on Earth. Each planet has its own day length and its own year length. We measure time using units that are made -
Greenhouse Calculator
Back to Math And Terraforming. In order to terraform a planet, most important is to change its atmospheric temperature. This is done in different ways: for an Inner Planet you need Anti Greenhouse Technology, including -
Tidal Locked Planet
If a planet is too close to its hosting star, it will be tidally- locked. Such planets should be found around M - type stars, White dwarfs and Brown Dwarfs. The climate pattern around a tidally -
Venus
These goals are closely related, since Venus' extreme temperature is due to the greenhouse effect caused by its dense atmosphere. The construction of a solar shade is impractical and thus will be overlooked in this -
Bioforming
Bioforming is a concept related to terraforming. Bioforming aims to transform life to improve its capability to survive, including on another celestial body (planet or moon), or other places. Life has evolved to be very -
Jupiter Simulation
This is a simulation of what one would expect to find on a terraformed Jupiter, using formulas from Math And Terraforming. Please note that not even the supercomputers at NASA can provide us with a -
Brown Dwarfs
For a classification of stars see The H-R Diagram. See also Main Sequence M Type Objects - Habitable Simulation and Brown Dwarfs - Habitability Simulation. A brown dwarf is a failed star. It is a celestial -
Io Simulation
This is a simulation of what one would expect to find on a terraformed Io, using formulas from Math And Terraforming. Please note that not even the supercomputers at NASA can provide us with a -
Callisto Simulation
This is a simulation of what one would expect to find on a terraformed Callisto, using formulas from Math And Terraforming. Please note that not even the supercomputers at NASA can provide us with a -
Titan Simulation
This is a simulation of what one would expect to find on a terraformed Titan, using formulas from Math And Terraforming. Please note that not even the supercomputers at NASA can provide us with a -
B-Type Stars
For a classification of stars see The H-R Diagram. See*Main Sequence B Type Stars - Habitable Simulation and Main Sequence Stars for more details. B - type stars (blue-white) are very rare, but because -
Europa Simulation
This is a simulation of what one would expect to find on a terraformed Europa, using formulas from Math And Terraforming. Please note that not even the supercomputers at NASA can provide us with a -
Creating An Atmosphere
Back to Planetary Terraforming And Colonization An Atmosphere is vital for any terraformed planet. Unfortunately, there are many planets who lack it. Creating it is possible in two ways: by adding it from other sources -
Terraforming
300px Terraforming (literally: Earth-shaping) is the proces of turning lifeless, uninhabitable planets, dwarf planets and other objects into Earth-like objects that can support human life. This can supposedly be done by modifying the -
M-Type Stars
For a classification of stars see The H-R Diagram. Additional information can be found on Main Sequence Stars and Main Sequence M Type Objects - Habitable Simulation. M-type stars are the most common stars -
Habitable Zone
A habitable zone is an approximated distance to a star where life would theoretically exist. This distance varies up to high levels, because of 3 categories of factors: hosting star, hosted planet and additional technologies -
Phobos
Phobos is the largest and the closest of the two Martian moons. It orbits above the Martian surface at an altitude of 9,377 km (5,823 mi). Phobos is one of the least-reflective -
Mountain Planet
A mountain planet is a theoretical planet whose geography includes extreme altitude changes. The weather conditions included in this article are largely based off that of Mercury, since Mercury is the closest thing to a -
Red Giants
For a classification of stars see The H-R Diagram. Red Giants are big stars that have left main sequence. They change fast and will, at some point, go supernova or will decay into White -
K-Type Stars
For a classification of stars see The H-R Diagram. See Main Sequence Stars and Main Sequence K Type Stars - Habitable Simulation K - type stars are the second most common main sequence stars after M -
A-Type Stars
For a classification of stars see The H-R Diagram. Additional information can be found at Main Sequence A Type Stars - Habitable Simulation and Main Sequence Stars. A - type stars are more rare than K -
High Gravity Rocky Planet
A high gravity rocky planet is a planet with breathable atmosphere (after terraforming), with accessible ground and with a gravity over 1.75 times stronger then Earth. In majority of cases, the planet is a
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