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The Complete Book of Spaceflight: From Apollo 1 to Zero Gravity

The Complete Book of Spaceflight: From Apollo 1 to Zero Gravity

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descent module <strong>to</strong> hold three spacesuited cosmonauts.<br />

It also carried solar panels—a feature <strong>of</strong> early<br />

Soyuz spacecraft that had been dispensed with after<br />

Soyuz 11 <strong>to</strong> save weight—enabling the vehicle <strong>to</strong> function<br />

independently <strong>of</strong> Salyut for up <strong>to</strong> four days.<br />

Soyuz TM<br />

A modernized version <strong>of</strong> the T with improved power<br />

supplies, new parachutes, and extra space for equip-<br />

space cannon<br />

(continued from page 386)<br />

than rocket fuel. Cannon projectiles are accurate, thanks<br />

<strong>to</strong> the fixed geometry <strong>of</strong> the gun barrel, and are much<br />

simpler and cheaper than rockets. However, there are also<br />

serious drawbacks. <strong>The</strong> payload must be slender enough<br />

<strong>to</strong> fit in<strong>to</strong> a gun barrel and sturdy enough <strong>to</strong> withstand<br />

the huge accelerations <strong>of</strong> launch, which can easily exceed<br />

10,000g.<br />

Long before the first test flights <strong>of</strong> the V-2 (see “V”<br />

weapons), the Paris Gun <strong>of</strong> World War I set impressive<br />

altitude and speed records for artificial objects. In the<br />

1950s, as the rocket became established as the primary<br />

means <strong>of</strong> reaching space, the Canadian engineer Gerald<br />

Bull began a lifelong struggle <strong>to</strong> use guns for cheap access<br />

<strong>to</strong> the high atmosphere and Earth orbit. His HARP<br />

(High Altitude Research Project) in the 1960s showed<br />

that a suborbital cannon can be cost-effective for studying<br />

the upper atmosphere, between 50 km and 130 km,<br />

and has the potential <strong>to</strong> launch vast numbers <strong>of</strong> satellites<br />

each year in all kinds <strong>of</strong> weather. A further development<br />

<strong>of</strong> this concept was Lawrence Livermore Lab’s SHARP<br />

(Super High Altitude Research Project).<br />

Even if shot out <strong>of</strong> an extremely powerful cannon, a<br />

projectile would need <strong>to</strong> include a rocket in order <strong>to</strong><br />

enter a stable orbit. This is for two reasons. First, reaching<br />

orbital velocity (with an extra margin for air resistance) is<br />

difficult using a cannon alone. Second, by Kepler’s first<br />

law, any orbit is an ellipse with one focus at the Earth’s<br />

center. If the payload is launched from a point A on the<br />

Earth’s surface, its orbit necessarily would intersect the<br />

surface again at a symmetrically placed point B. An<br />

orbital adjustment is therefore essential.<br />

Plans also exist for accelerating a payload by magnetic<br />

forces on a “rail gun” consisting <strong>of</strong> parallel conduc<strong>to</strong>rs,<br />

in<strong>to</strong> which a very large electric current is directed. <strong>The</strong><br />

same problems apply here, plus the added one <strong>of</strong> s<strong>to</strong>ring<br />

and then suddenly releasing a great amount <strong>of</strong> electrical<br />

space colony 389<br />

ment. It can carry an extra 200 kg in<strong>to</strong> orbit and return<br />

up <strong>to</strong> 150 kg <strong>to</strong> Earth—100 kg more than Soyuz T. First<br />

used with Mir, it remains in service ferrying cosmonauts,<br />

astronauts, and freight <strong>to</strong> and from the ISS.<br />

Soyuz TMA<br />

A version <strong>of</strong> the Soyuz spacecraft specially adapted <strong>to</strong><br />

serve as a lifeboat for crew return <strong>to</strong> Earth in the event<br />

<strong>of</strong> an emergency aboard the ISS. See ACRV.<br />

energy. This kind <strong>of</strong> technology might be appropriate for<br />

future use on the Moon but is at an even earlier stage<br />

than the space cannon. See Valier-Oberth Moon gun.<br />

space colony<br />

A large, self-contained, artificial environment in space,<br />

also known as a space habitat, which is the permanent<br />

home <strong>of</strong> an entire community. <strong>The</strong> first fictional account<br />

<strong>of</strong> a space colony appears in 1869, in Edward Everett<br />

Hale’s novel <strong>The</strong> Brick Moon. 140 Other early portrayals <strong>of</strong><br />

the idea are <strong>to</strong> be found in novels by Jules Verne in 1878<br />

and Kurd Lasswitz in 1897. In the 1920s, J. D. Bernal<br />

described spherical colonies that have come <strong>to</strong> be known<br />

as Bernal spheres. 25 <strong>The</strong> companion idea <strong>of</strong> mobile<br />

colonies, or generation starships, that could carry large<br />

numbers <strong>of</strong> people relatively slowly <strong>to</strong> other stars was<br />

envisioned in 1918 by Robert Goddard. 114 A vastly more<br />

ambitious scheme for completely encircling a star with<br />

artificial habitats was described by Freeman Dyson 83 in<br />

the 1960s. Indeed, the development <strong>of</strong> concepts about<br />

space colonies is deeply entwined with evolving notions<br />

about the colonization <strong>of</strong> other worlds, terraforming,<br />

and space stations. When does a space station become a<br />

space colony? In his 1952 novel, Islands in the Sky, 53<br />

Arthur C. Clarke depicts structures that are somewhere<br />

between the two, while by 1961, in A Fall <strong>of</strong> Moondust, 54<br />

he has moved on <strong>to</strong> even larger structures placed at the<br />

stable Lagrangian points in Earth’s orbit where they<br />

would remain fixed relative <strong>to</strong> both Earth and the Moon.<br />

In 1956, Darrell Romick advanced a yet more ambitious<br />

proposal for a rotating cylinder 1 km long and 300 m in<br />

diameter that would be home <strong>to</strong> 20,000 people. In 1963,<br />

Dandridge Cole suggested hollowing out an ellipsoidal<br />

asteroid about 30 km long, rotating it about the major<br />

axis <strong>to</strong> simulate gravity, reflecting sunlight inside with<br />

mirrors, and creating on the inner shell a pas<strong>to</strong>ral setting<br />

as a permanent habitat for a colony. Related ideas, about<br />

the use <strong>of</strong> extraterrestrial resources <strong>to</strong> manufacture

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