Colonizing Outer Space/Colonization/Space/Generalities/Celestial Bodies

Colonizing Mars edit

Mars seen by the Hubble Space Telescope, Realistic Colors

Mars is a frequent topic of discussion regarding colonization possibilities. A project for the colonization of Mars provides an opportunity to examine how we live here on Earth and what aspects of our own planet and its effects on our lives we value and would wish to re-create on Mars. The Mars Project also provides a case-study for further planetary colonization.

Mars overall surface area is similar to the dry land surface Earth, it has large water reserves, and has carbon (locked as carbon dioxide in the atmosphere). It may have gone through similar geological and hydrological processes as Earth and contain valuable mineral ores, but this is debated.

Mars's atmosphere is very thin (averaging 800 Pa or about 0.8% of Earth sea-level atmospheric pressure) and the climate is colder. Its gravity is only around a third that of Earth. Mars is often the topic of discussion regarding terraforming to make the entire planet or at least large portions of it habitable.

As of 2011, according to the Journal of Cosmology, an interplanetary trip to Mars from Earth, could take as little as 10 months, and it would be possible for a privately-funded one-way mission to Mars to depart as soon as 20 years from now. But returning would be virtually impossible (due to payload and energy restrictions).

In regards to volunteers, in 2011 a special edition of the Journal of Cosmology, detailing and promoting a privately-funded one-way mission to Mars prompted more than 400 readers to volunteer as colonists. This leads to the conclusion that there are people willing to take on the risk, but it also creates the need to select those that should and are more capable of being successful.

Solar energy would be a problem in mars, there is not only night time to consider but a large amount of dust.

Valles Marineris on Mars
Remote surface exploration in regions around the habitat complex is accomplished by using pressurized rovers. These vehicles would allow the crew to explore beyond the range permitted by their space suits while allowing them to operate in a shirtsleeve environment. Artist concept.

There is an ongoing debate on this topic on the Mars Civil-Cultural mailing list. One way that this topic can be explored is to look at the lessons learned from science fiction.


To do:
Transwiki of Wikipedia:Colonization of Mars


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Mine Wikipedia:Exploration of Mars

Life and fossils edit

There is increasing evidences that point to the, at least ancient, presence of life on Mars, this has created a strong scientific interest in colonizing Mars. A study from 2011 from NASA indicates that if life existed on at some point in Mars history, the best chances for it to have survived (or at least to have persisted longer) would have been below the surface. This hypothesis is based in geological studies performed by probes from NASA and the European Space Agency in more than 350 sites, along with what is known of mars today.

Water edit

Water is one of the most important substances for life as we know it. In the last three decades upon reviewing images of the surface of Mars taken by the Viking orbiters in the 70s, scientists became puzzled by the apparent sloping of rocky material around mountains and cliffs, these deposits, referred to as lobate debris apron, seems to extend sometimes for tens of miles. The debate around those formations generated the theory that they may have been formed by the lubrication of the rocky debris by a thin layer of ice, since similar features can be observed on Earth, for instance in Antarctica.

A new indication that water seems to exist on the planet came from data collected by the Shallow Subsurface Radar (SHARAD) instrument aboard the Mars Reconnaissance Orbiter probe, lunched in August 12, 2005 and operating at destination from 2006 onward. The radar results are consistent with massive deposits of water in middle latitudes, providing further support for the debris covered glacier hypothesis.

Equipment is available to extract in situ resources (water, air, etc.) from the Martian ground and atmosphere.

Agriculture edit

Martian soil contains several nutrients required to support to plant life. With fertilizer and environmental control, it could be used to grow plants.

Artifacts and equipment already available edit

There are several artifacts left on the surface of Mars from previous exploration and still working equipment, like monitoring satellites.


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Create list of items.

Colonies on the Moon edit


The Moon is Earth's only natural satellite, it is also known as Luna in Latin and other languages. Due to its proximity and relative familiarity, Earth's Moon is also frequently discussed as a target for colonization.

A colony on Luna has several important advantages over a colony on any other celestial body outside Earth. One big advantage is that it is close proximity to Earth. It would be comparatively easy to supply any colonization process, place and evacuate colonists, and use radio signals for reprogramming and remote control of robots and other devices on the Moon's surface. Another advantage is the low gravity, allowing for easier exchange of goods and services. But the topmost advantage is that we already have been there.

Astronaut Buzz Aldrin, lunar module pilot, walks on the surface of the Moon near the leg of the Lunar Module (LM) "Eagle" during the Apollo 11 extravehicular activity (EVA). Astronaut Neil A. Armstrong, commander, took this photograph with a 70mm lunar surface camera. While astronauts Armstrong and Aldrin descended in the Lunar Module (LM) "Eagle" to explore the Sea of Tranquility region of the Moon, astronaut Michael Collins, command module pilot, remained with the Command and Service Modules (CSM) "Columbia" in lunar orbit.

Solar energy on the moon is a possibility by the moon has two week nights and similar to Mars dust will constitute a problem, not atmospheric dust but the surface regolith is an extreme problem, making nuclear power more attractive.

A major drawback of the Moon is its low abundance of volatiles necessary for life such as hydrogen and carbon. Water ice deposits was found in relative abundance, especially in some polar craters, that could serve as significant sources for these elements.

India's first unmanned lunar probe, launched in 22 October 2008, Chandrayaan-1 intended to last for 2 years in a compressive mapping of moon resources has generated data that leads NASA's scientists to estimate the existence of 600 million metric tons of water ice in craters around the Moon's north pole.

The existence of numerous craters near the poles of the Moon that have interiors that are in permanent sun shadow, makes them capable of maintaining very low temperatures. Without the effects from the Sun's radiation water can be indefinitely kept as ice. If this estimation is verified, mining this resource, could serve as a source of life support for future lunar bases as water and oxygen or as propellant for future spacecraft if converted to methane, dramatically reducing the cost of space exploration. NASA in April 2012 contracted Astrobotic Technology Inc. to determine whether its polar rover can deploy an ice-prospecting payload to the Moon, aiming for such verification.

There are also several magma caves that would facilitate the creation of protected habitats.

Scientist-Astronaut Harrison H. Schmitt is photographed standing next to a huge, split boulder at Station 6 (base of North Massif) during the third Apollo 17 extravehicular activity (EVA-3) at the Taurus-Littrow landing site on the Moon. 1972
Lunar base concept drawing from NASA in 1977
"Self-growing lunar factory." An artist's conception of a robotic lunar factory that's capable of self-expansion. NASA, 1982
Inflatable module for lunar base: With a number of studies ongoing for possible lunar expeditions, many concepts for living and working on Earth's natural satellite have been examined. This art concept reflects the evaluation and study at JSC by the Man Systems Division and Johnson Engineering personnel. A sixteen-meter diameter inflatable habitat such as the one depicted here could accommodate the needs of a dozen astronauts living and working on the surface of the Moon. Depicted are astronauts exercising, a base operations center, a pressurized lunar rover, a small clean room, a fully equipped life sciences lab, a lunar lander, selenological work, hydroponic gardens, a wardroom, private crew quarters, dust-removing devices for lunar surface work and an airlock. NASA, 1989
Heavy, pressurized lunar rover intended to enable up to four crew to rove for two weeks on the moon's surface. A crew airlock permits crew to exit and enter the rover and may double as a docking adapter to the moon base. A smaller sample lock permits retrieval of lunar samples using remote manipulators mounted on the rover front. A cupola, similar to the cupola on the International Space Station, is a secondary driving station and permits views of the lunar terrain o360 degrees around the horizon and to much greater distances than the lower driving station. NASA, 1990.
Early Lunar Outpost based on a module like those used for the International Space Station. Equipment is mounted in modular racks. Most equipment directly supports human life support, human health, and habitation. NASA, 1990
This artist's rendering represents a concept of possible activities during future space exploration missions. It depicts a human tended lunar base. NASA, April 2004
Artists impression of a terraformed Moon. Image is derived from LRO LOLA data. The water coverage is 50%. The weather is based on what we know of weather on Titan, the only small body with a thick atmosphere. Since it has a slow rotation the atmosphere may super rotate like Venus', but due to the small size there should be no polar collar, so no ice caps.

According to M.J. Fogg, "it is just possible to terraform the Earth's moon, so long as you are prepared to keep its imported volatiles topped up every few thousand years or so".</ref> </ref>

The lunar space elevator
Diagram showing equatorial and polar Lunar space elevator. Not to scale.
Three crew members work in the area of their lunar lander on the lunar surface in this NASA artist's rendering. NASA had selected Altair as the name of the lunar lander the Constellation Program would use to put humans on the moon. Project Altair Manager Lauri Hansen made the announcement at the industry event at NASA's Johnson Space Center in Houston. Altair would be capable of landing four astronauts on the moon, providing life support and a base for week long initial surface exploration missions, and returning the crew to the Orion spacecraft that would bring them home to Earth. Altair would have launched aboard an Ares V rocket into low-Earth orbit, where it would rendezvous with the Orion crew vehicle.


To do:
Transwiki Wikipedia:Colonization of the Moon

Planed Moon Colonies edit


Mercury edit

There is a suggestion that Mercury could be colonized using the same technology, approach and equipment that is used in colonization of the Moon.


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Transwiki Wikipedia:Colonization of Mercury

Venus edit

While the surface of Venus is far too hot and features atmospheric pressure at least 90 times that at sea level on Earth, its massive atmosphere offers an alternate location for colonization. At a height of approximately 50 km, the pressure is reduced to a few atmospheres, and the temperature would be between 40-100° C, depending on the height. This part of the atmosphere is probably within dense clouds which contain some sulphuric acid. Even these have a certain benefit to colonization, as they present a possible source for the extraction of water. Thus, the most likely colony on Venus would be a floating city in the clouds that stays above 50 km above the surface.


To do:
Transwiki Wikipedia:Colonization of Venus

Europa edit

The Artemis Project designed a plan to colonize Europa, one of Jupiter's moons. Scientists were to inhabit igloos and drill down into the Europan ice crust, exploring any sub-surface ocean. It also discusses use of "air pockets" for human inhabitation.

Gas Giants edit

It may also be possible to colonize the three furthest gas giants with floating cities in their atmospheres. By heating hydrogen balloons large masses can be suspended underneath at roughly Earth gravity. Jupiter would be unsuitable for habitation due to its high gravity, escape velocity and radiation. Such colonies could export Helium-3 which would be used to fuel fusion reactors for energy.

Stars edit


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Dyson sphere