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

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376 SIM (Space Interferometry Mission)<br />

stein earned a B.S. in mechanical engineering (1929) and<br />

an M.E. (1934) from Rose Polytechnic Institute, and<br />

later received an honorary doc<strong>to</strong>rate from Case Institute<br />

<strong>of</strong> Technology. He began his career with NASA’s predecessor,<br />

NACA (the National Advisory Committee for<br />

Aeronautics), at its Langley Research Center in 1929. In<br />

1943, he transferred <strong>to</strong> Lewis, where he carried out pioneering<br />

research on large-scale ramjet engines. After<br />

World War II, Silverstein conceived, designed, and built<br />

the first supersonic propulsion wind tunnel in the<br />

United States. <strong>The</strong> 10-ft by 10-ft Supersonic Wind Tunnel<br />

is still operational at Glenn. In 1958, Silverstein<br />

moved <strong>to</strong> NACA Headquarters in Washing<strong>to</strong>n, D.C.,<br />

where he helped create and then direct efforts leading <strong>to</strong><br />

the Mercury spaceflights. He later named and laid the<br />

groundwork for the <strong>Apollo</strong> missions. When he returned<br />

<strong>to</strong> Cleveland <strong>to</strong> become direc<strong>to</strong>r <strong>of</strong> NASA Lewis, Silverstein<br />

was a driving force behind the creation <strong>of</strong> the Centaur<br />

launch vehicle, particularly the hydrogen-oxygen<br />

upper stage propulsion system. He retired from NASA<br />

in 1970 <strong>to</strong> take a position with Republic Steel. In 1997,<br />

he was awarded the Guggenheim Medal for his “technical<br />

contributions and visionary leadership in advancing<br />

technology <strong>of</strong> aircraft and propulsion performance, and<br />

foresight in establishing the Mercury and Gemini manned<br />

spaceflight activities.” 73<br />

SIM (Space Interferometry Mission)<br />

A major space-based observa<strong>to</strong>ry in NASA’s Origins Program<br />

and the first spacecraft <strong>to</strong> carry an optical interferometer<br />

as its main instrument. SIM is designed<br />

specifically for the precise measurement <strong>of</strong> star positions.<br />

One <strong>of</strong> its prime goals will be <strong>to</strong> search for extrasolar<br />

planets as small as Earth in orbit around nearby stars.<br />

SIM will combine the light from two sets <strong>of</strong> four 30-cmdiameter<br />

telescopes arrayed across a 10-m boom <strong>to</strong><br />

achieve a resolution approaching that <strong>of</strong> a 10-m-diameter<br />

mirror. This will allow it <strong>to</strong> perform extremely sensitive<br />

astrometry so that it will be able <strong>to</strong> detect very small<br />

wobbles in the movement <strong>of</strong> a star due <strong>to</strong> unseen com-<br />

Chronology <strong>of</strong> American SIGINT Satellites<br />

1st Generation 2nd Generation 3rd Generation 4th Generation 5th Generation<br />

1960s 1970s 1980s 1990s 2000+<br />

GEO-USAF COMINT Canyon Chalet/Vortex Mercury-ELINT<br />

GEO-CIA ELINT Rhyolite/Aquacade Magnum/Orion Men<strong>to</strong>r Intruder<br />

HEO-USAF ELINT Jumpseat Trumpet Prowler<br />

LEO-USAF ELINT Ferret Subsats Subsats SB-WASS<br />

LEO-Navy ELINT GRAB NOSS NOSS SB-WASS<br />

panions. Objects <strong>of</strong> Earth mass could be inferred around<br />

a star up <strong>to</strong> 30 light-years away. Through a process known<br />

as synthesis imaging, SIM will also generate images <strong>of</strong><br />

objects such as dust disks around stars and look for gaps<br />

or clearings in the debris that might indicate the presence<br />

<strong>of</strong> unseen worlds. Scheduled for launch in 2005, SIM will<br />

conduct its seven-year mission from a heliocentric,<br />

Earth-trailing orbit.<br />

Simons, David G. (1922–)<br />

A U.S. Air Force major who established a new human<br />

altitude record <strong>of</strong> 30,942 m (101,516 ft) when he flew<br />

aboard the second Project Manhigh mission on August<br />

19–20, 1957. During his 32-hour flight, most <strong>of</strong> it at the<br />

edge <strong>of</strong> space, Simons recorded that the silence <strong>of</strong> the<br />

upper stra<strong>to</strong>sphere is “like no earthly quiet” and that the<br />

color <strong>of</strong> the sky at this height is “deep indigo, intense,<br />

almost black.” He was among the first <strong>to</strong> report the psychologically<br />

dangerous euphoria known as the break-<strong>of</strong>f<br />

phenomenon.<br />

Singer, Samuel Frederick (1924–)<br />

A physicist at the University <strong>of</strong> Maryland who proposed<br />

a Minimum Orbital Unmanned Satellite <strong>of</strong> the Earth<br />

(MOUSE) at the fourth Congress <strong>of</strong> the International<br />

Astronautics Federation in Zurich, Switzerland, in the<br />

summer <strong>of</strong> 1953. It had been based upon two years <strong>of</strong><br />

previous study conducted under the auspices <strong>of</strong> the<br />

British Interplanetary Society, which had built on the<br />

postwar research <strong>of</strong> the V-2 rocket. <strong>The</strong> Upper Atmosphere<br />

Rocket Research Panel at White Sands discussed<br />

Singer’s plan in April 1954. In May, Singer presented his<br />

MOUSE proposal at the Hayden Planetarium’s fourth<br />

Space Travel Symposium. MOUSE was the first satellite<br />

proposal widely discussed in nongovernmental engineering<br />

and scientific circles, although it was never adopted.<br />

single-stage-<strong>to</strong>-orbit (SSTO)<br />

A reusable single-stage rocket that can take <strong>of</strong>f and land<br />

repeatedly and is able <strong>to</strong> boost payloads in<strong>to</strong> orbit.

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