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Stanford torus - Wikipedia, the free encyclopedia

Stanford torus

From Wikipedia, the free encyclopedia

Exterior view of a Stanford torus. Bottom center is the non-rotating primary solar mirror, which reflects sunlight onto the angled ring of secondary mirrors around the hub. Painting by Donald E. Davis.
Exterior view of a Stanford torus. Bottom center is the non-rotating primary solar mirror, which reflects sunlight onto the angled ring of secondary mirrors around the hub. Painting by Donald E. Davis.
External view of a Stanford torus with some of the radiation-shielding "chevron" mirrors removed to show interior space.
External view of a Stanford torus with some of the radiation-shielding "chevron" mirrors removed to show interior space.
Interior of a Stanford torus, painted by Donald E. Davis
Interior of a Stanford torus, painted by Donald E. Davis

The Stanford torus is a proposed design for a space habitat capable of housing approximately 10,000 to 140,000 permanent residents. It consists of a torus or donut-shaped ring that is one statute mile (1.6 km) in diameter and rotates once per minute to provide between 0.9g and 1.0g of artificial gravity on the inside of the outer ring via centripetal acceleration.

Sunlight is provided to the interior of the torus by a system of mirrors. The ring is connected to a hub via a number of "spokes", which serve as conduits for people and materials travelling to and from the hub. Since the hub is at the rotational axis of the station, it experiences the least artificial gravity and is the easiest location for spacecraft to dock. Zero-gravity industry is performed in a non-rotating module attached to the hub's axis.

The interior space of the torus itself is used as living space, and is large enough that a "natural" environment can be simulated; the torus appears similar to a long, narrow, straight glacial valley whose ends curve upward and eventually meet overhead to form a complete circle. The population density is similar to a dense suburb, with part of the ring dedicated to agriculture and part to housing.

The Stanford Torus was proposed during the 1975 NASA Summer Study, conducted at Stanford University, with the purpose of speculating on designs for future space colonies.[1] (Gerard O'Neill later proposed his Island One or Bernal sphere as an alternative to the torus.) "Stanford torus" refers only to this particular version of the design, as the concept of a ring-shaped rotating space station was previously proposed by Wernher von Braun in 1952.

[edit] Stanford tori in fiction

There have been many wheel-shaped space stations in science fiction, perhaps the most famous being the Earth-orbiting Space Station V depicted in Arthur C. Clarke's and Stanley Kubrick's 1968 book/movie 2001: A Space Odyssey. But, as mentioned above, these are fundamentally different, being space stations, not space habitats. They are buildings in space, rather than towns in space, and their origins go back further.

Some works, however, have structures that more closely resemble the Stanford Torus idea:

  • The novels of the Gaea Trilogy by John Varley are set on an unusual organic satellite of Saturn that is shaped as a Stanford Torus.
  • In the anime series Mobile Suit Gundam Wing, most of the many space colonies in Earth orbit are based on the Stanford torus.
  • Hideo Kojima's Playstation 2 video game Zone of the Enders is set aboard a Stanford torus-type space station orbiting Jupiter called Antillia Colony.
  • The video game Startopia is set aboard a series of Stanford tori.
  • The Citadel in the video game Mass Effect contains a massive Stanford torus known as the Presidium in which the galaxy's major decisions are made.
  • Saturnalia and A Lion on Tharthee by Grant Callin features SpaceHome, a group of torii space stations connected in a pinwheel fashion.
  • James P. Hogan wrote several novels that included a Stanford torus, including The Two Faces of Tomorrow, Endgame Enigma, and Voyage From Yesteryear.

[edit] See also

[edit] References

  1. ^ Johnson, Holbrow. "Space Settlements: A Design Study", National Aeronautics and Space Administration, 1977. 


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