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

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410 speed <strong>of</strong> sound<br />

speed <strong>of</strong> sound<br />

<strong>The</strong> speed at which small disturbances travel through a<br />

medium. In the case <strong>of</strong> a gas, such as air, the speed <strong>of</strong><br />

sound is independent <strong>of</strong> pressure but varies with the<br />

square root <strong>of</strong> temperature. Since temperature decreases<br />

with increasing altitude in the atmosphere, so <strong>to</strong>o does<br />

the speed <strong>of</strong> sound; in air at 0°C, it is about 1,220 km/hr<br />

(760 mph), though it also varies slightly with humidity.<br />

<strong>The</strong> various regimes <strong>of</strong> flight are subsonic (well below the<br />

speed <strong>of</strong> sound), transonic (near sonic speed), supersonic<br />

(up <strong>to</strong> 5 times sonic speed), and hypersonic (above 5 times<br />

sonic speed). Compressibility effects start <strong>to</strong> become<br />

important in the transonic regime and very significant at<br />

supersonic speeds, when shock waves are present. In the<br />

hypersonic regime, the high energies involved have significant<br />

effects on the air itself. <strong>The</strong> important parameter<br />

in each <strong>of</strong> these situations is the Mach number—the<br />

ratio <strong>of</strong> the speed <strong>of</strong> the object <strong>to</strong> the local speed <strong>of</strong><br />

sound.<br />

Spektr<br />

See Mir.<br />

SPIDR (Spectroscopy and Pho<strong>to</strong>metry <strong>of</strong> the<br />

Intergalactic Medium’s Diffuse Radiation)<br />

A mission <strong>to</strong> map the web <strong>of</strong> hot gas that spans the universe.<br />

Half <strong>of</strong> the normal matter in the nearby universe is<br />

in filaments <strong>of</strong> hot gas, and SPIDR would observe it for<br />

the first time. SPIDR’s data would answer fundamental<br />

questions concerning the formation and evolution <strong>of</strong><br />

galaxies, clusters <strong>of</strong> galaxies, and other large structures in<br />

Some Space Spin-<strong>of</strong>fs<br />

the universe. SPIDR has been selected by NASA for<br />

study as a Small Explorer mission.<br />

spin-<strong>of</strong>f<br />

A commercial or other non-space benefit derived from<br />

space research. Some <strong>of</strong> the numerous devices and technologies<br />

developed originally for use in spaceflight or<br />

space science are listed in the table (“Some Space Spin<strong>of</strong>fs”).<br />

spin stabilization<br />

A simple and effective method <strong>of</strong> keeping a spacecraft<br />

pointed in a certain direction. A spinning spacecraft<br />

resists perturbing forces in the same way that a spinning<br />

gyroscope or a <strong>to</strong>p does. Also, because, in space, forces<br />

that slow the rate <strong>of</strong> spin are negligible, once a spacecraft<br />

is set spinning, the rate <strong>of</strong> rotation stays the same. With<br />

a spinner, there are inherent inefficiencies because only<br />

some <strong>of</strong> the solar cells are illuminated at any one instant<br />

and because most <strong>of</strong> the radio wave energy, radiating<br />

from the nondirectional antennas in all directions, is not<br />

directed at Earth. Thrusters are fired <strong>to</strong> make desired<br />

changes in the spin-stabilized attitude. <strong>The</strong>y may require<br />

complicated systems <strong>to</strong> de-spin antennas or optical<br />

instruments that must be pointed at targets.<br />

SPIRIT (Space Infrared Interferometric Telescope)<br />

A highly sensitive orbiting observa<strong>to</strong>ry that would allow<br />

the far infrared background <strong>to</strong> be resolved almost completely<br />

in<strong>to</strong> individual sources. SPIRIT is identified in<br />

NASA’s Office <strong>of</strong> Space Science Strategic Plan as a poten-<br />

Device/Technique Origin<br />

Medical imaging Signal-processing techniques <strong>to</strong> clarify images from spacecraft<br />

Bar coding NASA tracking system for spacecraft parts<br />

Firefighter suits Fire-resistant fabric for use in spacesuits<br />

Smoke detec<strong>to</strong>r Toxic vapor detec<strong>to</strong>rs aboard the Skylab space station<br />

Sun tiger glasses Protective lenses for welders working on spacecraft<br />

Car design s<strong>of</strong>tware NASA s<strong>of</strong>tware for use in spacecraft and airplane design<br />

Cordless <strong>to</strong>ols Portable, self-contained drills <strong>to</strong> enable <strong>Apollo</strong> astronauts <strong>to</strong> obtain moon samples<br />

Fisher space pen Developed for use in space. Pressurized gas pushes the ink <strong>to</strong>ward the ballpoint even in zero<br />

gravity, while special ink works at temperature extremes<br />

Invisible braces Translucent ceramic developed for use in spacecraft and aircraft<br />

Joystick controller Control stick for the <strong>Apollo</strong> Lunar Rover<br />

Scratch-resistant lenses Dual ion-beam bonding, in which a diamondlike coat is applied <strong>to</strong> plastic<br />

Freeze-dried food Meals for early astronauts

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