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

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Statsionar<br />

See Raduga.<br />

stay time<br />

<strong>The</strong> average time spent by a gas molecule in a liquid-fuel<br />

rocket engine’s combustion chamber before exiting<br />

from the nozzle and producing thrust.<br />

STEDI (Student Explorer Demonstration Initiative)<br />

A program, managed by USRA (Universities Space<br />

Research Association) for NASA, that is designed <strong>to</strong><br />

demonstrate that a small scientific or technology-based<br />

satellite could be designed, fabricated, launched, and<br />

operated for around $10 million. It is part <strong>of</strong> NASA’s<br />

“smaller, cheaper, faster” initiative for research spacecraft.<br />

Stella<br />

A French geodetic satellite, carrying 60 laser reflec<strong>to</strong>rs<br />

mounted on a dense sphere <strong>of</strong> uranium alloy, that is<br />

tracked <strong>to</strong> measure small perturbations in Earth’s gravitational<br />

field. Reflected laser beams enable measurements,<br />

accurate <strong>to</strong> about 1 cm, <strong>of</strong> the geoid, oceanic and terrestrial<br />

tides, and tec<strong>to</strong>nic movements. Stella’s twin, Starlette,<br />

launched in 1975, is also still in use.<br />

Launch<br />

Date: September 26, 1993<br />

Vehicle: Ariane 4<br />

Site: Kourou<br />

Orbit: 793 × 803 km × 98.7°<br />

Mass: 48 kg<br />

Stennis Space Center (SSC)<br />

One <strong>of</strong> 10 NASA field centers in the United States. Previously<br />

known as the Mississippi Test Facility, it was<br />

renamed in 1988 after U.S. Sena<strong>to</strong>r John C. Stennis.<br />

Located in Hancock County, Mississippi, about 80 km<br />

northeast <strong>of</strong> New Orleans, it is the primary center for<br />

testing and flight certifying rocket propulsion systems for<br />

the Space Shuttle and future generations <strong>of</strong> space vehicles.<br />

In the past it was the static test site for Saturn- and<br />

Nova-class launch vehicles. All Space Shuttle Main<br />

Engines must pass a series <strong>of</strong> test firings at Stennis Space<br />

Center prior <strong>to</strong> being installed in the back <strong>of</strong> the Orbiter.<br />

Stennis is also NASA’s lead center for commercial remote<br />

sensing within the Mission <strong>to</strong> Planet Earth Enterprise.<br />

STENTOR (Satellite de Télécommunications<br />

pour Expériences de Nouvelles Technologies<br />

en Orbite)<br />

An experimental communications satellite developed by<br />

CNES (the French space agency) in association with<br />

Stewart, Homer J. 419<br />

French Telecom. STENTOR will carry out propagation<br />

and transmission experiments, especially at wavelengths<br />

that are shorter than those currently used for satellites<br />

communications. Launch was scheduled for the second<br />

half <strong>of</strong> 2002.<br />

STEP (Satellite Test <strong>of</strong> the Equivalence Principle)<br />

A satellite designed <strong>to</strong> test, in microgravity, a wellestablished<br />

physical law—the Equivalence Principle—that<br />

all falling objects accelerate at the same rate. Until now,<br />

this principle escaped deep scrutiny because experiments<br />

have always been limited by gravitational conditions at<br />

the Earth’s surface. STEP, which involves a collaboration<br />

between NASA and ESA (European Space Agency), will<br />

test the principle <strong>to</strong> an accuracy 100,000 times greater<br />

than that achieved in terrestrial labora<strong>to</strong>ries. It will also<br />

conduct experiments in quantum mechanics and gravity<br />

variations. STEP was selected by NASA for study as a<br />

SMEX (Small Explorer).<br />

step principle<br />

A design feature <strong>of</strong> rockets in which one stage is mounted<br />

directly on<strong>to</strong> another. When a lower stage is used up, it is<br />

ejected, and the next upper stage takes over. With each<br />

stage’s ejection, the weight <strong>of</strong> the spacecraft decreases, so<br />

the next stage has less work <strong>to</strong> do.<br />

step rocket<br />

A multistage rocket.<br />

STEREO (Solar-Terrestrial Relations Observa<strong>to</strong>ry)<br />

A mission <strong>to</strong> understand the origin <strong>of</strong> coronal mass ejections—powerful<br />

eruptions on the Sun in which as much<br />

as 10 billion <strong>to</strong>ns <strong>of</strong> the solar atmosphere can be blown<br />

in<strong>to</strong> interplanetary space—and their consequences for<br />

Earth. It will consist <strong>of</strong> two spacecraft, one leading and<br />

the other lagging Earth in its orbit. <strong>The</strong>se spacecraft will<br />

each carry instrumentation for solar imaging and for insitu<br />

sampling <strong>of</strong> the solar wind. STEREO, the third <strong>of</strong><br />

NASA’s Solar Terrestrial Probe missions, is being<br />

designed and built at the Johns Hopkins University<br />

Applied Physics Labora<strong>to</strong>ry and is scheduled for launch<br />

in 2005.<br />

Stewart, Homer J. (1915–)<br />

A prominent aerospace engineer involved with the U.S.<br />

space program. Stewart earned a B.S. in aeronautic engineering<br />

from the University <strong>of</strong> Minnesota in 1936,<br />

joined the faculty <strong>of</strong> the California Institute <strong>of</strong> Technology<br />

(Caltech) in 1938, and earned his doc<strong>to</strong>rate from<br />

Caltech two years later. In 1939, he <strong>to</strong>ok part in pioneering<br />

rocket research with other Caltech engineers and<br />

scientists, including Frank Malina, in the foothills <strong>of</strong><br />

Pasadena. Out <strong>of</strong> their efforts, JPL ( Jet Propulsion

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