Terraforming the Dwarf Planet: ⚳ Ceres Megasatellite World
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Terraforming the Dwarf Planet: ⚳ Ceres Megasatellite World
288 | 4 год. назад | 11 - 0
In the near future, humanity stands a good chance of expanding its presence beyond Earth. This includes establishing infrastructure in Low Earth Orbit (LEO), on the surface of (and in orbit around) the Moon, and on Mars. This presents numerous challenges, as living in space and on other celestial bodies entails all kinds of potential risks and health hazards – not the least of which are radiation and long-term exposure to low gravity.
These issues demand innovative solutions; and over the years, several have been proposed! A good example is Dr. Pekka Janhunen‘s concept for a megasatellite settlement in orbit around the dwarf planet Ceres, the largest object in the Main Asteroid Belt. This settlement would provide artificial gravity for its residents while the local resources would allow for a closed-loop ecosystem to created inside – effectively bringing “terraforming” to a space settlement.
The paper that describes his concept recently appeared online, and is something that Dr. Janhunen described to Universe Today as, “Terraforming from the user perspective: creating an artificial environment, near Ceres and of Ceres materials, that can scale up to the same and larger population than Earth has today.”
“They provide Earth-like 1 g gravity, which is essential for human health, in particular essential for children to grow to healthy adults with fully developed muscles and bones. Ceres has nitrogen for making the habitat atmospheres, and it is large enough to provide almost unlimited resources. At the same time it is also small enough that its gravity is rather low so that lifting material from the surface is cheap.”
According to his study, the megasatellite settlement would consist of spinning habitats attached to a disk-shaped frame through passive magnetic bearings. This would allow for simulated gravity within the habitats, facilitate intra-settlement travel and ensure that population density remains low.
Dr. Janhunen estimates that it could be kept to 500 people per km2 (190 people per mi2), whereas cities like Manhattan and Mumbai have densities of roughly 27,500 and 32,303 people per km2 (or 71,340 and 83,660 people per mi2), respectively. The settlement would initially be furnished with soil 1.5 m (~5 ft) in depth, which could be upgraded to 4 m (~13 ft).
This would allow for greenspaces with gardens and trees that would produce the settlement’s oxygen and scrub the atmosphere of CO2 (as well as additional radiation shielding). Similarly, Ceres is known to have abundant supplies of ammonia salts on its surface (particularly around the bright spots in the Occator crater) that could be imported to the settlement and converted to nitrogen for use as a buffer gas.
Planar and parabolic mirrors located around the frame would direct concentrated sunlight to the habitats, providing illumination and allowing for photosynthesis to occur. While the creation of such a settlement presents many technical challenges and would require a massive commitment in resources, it would actually be easier in many respects that colonizing the Moon or Mars.
/Description by article "A Habitat at Ceres Could be the Gateway to the Outer Solar System" in Universe Today/
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