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

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88 Copernicus Observa<strong>to</strong>ry<br />

longest Mercury orbital mission and spent eight days in<br />

space aboard Gemini 5. He earned a B.S. in aeronautical<br />

engineering from the Air Force Institute <strong>of</strong> Technology in<br />

1956. Having received an Army commission, he transferred<br />

<strong>to</strong> the Air Force and flew F-84 and F-86 jets in Germany<br />

for four years. Back in the United States he<br />

received his degree and then attended the Air Force<br />

Experimental Flight Test School at Edwards Air Force<br />

Base before being assigned as an aeronautical engineer<br />

and test pilot in the Performance Engineering Branch <strong>of</strong><br />

the Flight Test Division at Edwards. In 1959, he was<br />

selected by NASA and on May 15–16, 1963, piloted his<br />

Faith 7 capsule on the sixth and final Mercury Project<br />

mission. Electrical problems near the end <strong>of</strong> the mission<br />

meant he had <strong>to</strong> manually fire his retrorockets and steer<br />

the capsule through reentry. Problems also beset Cooper<br />

on his next flight, a then-record eight-day trip aboard<br />

Gemini 5 in August 1965. Trouble with fuel supplies,<br />

power systems, and a computer-generated command led<br />

Gemini 5 <strong>to</strong> land 166 km short <strong>of</strong> its designated target.<br />

Cooper retired from NASA and the Air Force in 1970,<br />

and has since been involved in technical research with<br />

several companies. 60<br />

Copernicus Observa<strong>to</strong>ry<br />

See OAO-3 (Orbiting Astronomical Observa<strong>to</strong>ry 3).<br />

Coriolis<br />

A test mission for the U.S. Air Force that carries two scientific<br />

payloads: Wind, and the Solar Mass Ejection<br />

Imager (SMEI). Wind is a Navy experiment built by the<br />

Naval Research Labora<strong>to</strong>ry <strong>to</strong> passively measure ocean<br />

surface wind directions, while SMEI is an Air Force<br />

Research Labora<strong>to</strong>ry experiment <strong>to</strong> observe coronal mass<br />

ejections in visible light. <strong>The</strong> spacecraft’s two payloads<br />

will collect data continuously during a three-year mission.<br />

Launch was scheduled for January 2003 from Vandenberg<br />

Air Force Base by a Titan II rocket in<strong>to</strong> a circular<br />

830 km × 98.7° orbit.<br />

Coriolis effect<br />

<strong>The</strong> deflection <strong>of</strong> the flight path <strong>of</strong> a spacecraft caused by<br />

Earth’s rotation. Over the northern hemisphere, the deviation<br />

is <strong>to</strong> the right; over the southern hemisphere, it is<br />

<strong>to</strong> the left.<br />

corona<br />

<strong>The</strong> outermost layer <strong>of</strong> the Sun’s (or some other star’s)<br />

atmosphere, visible <strong>to</strong> the eye during a <strong>to</strong>tal solar eclipse;<br />

it can also be observed through special filters and, best <strong>of</strong><br />

all, by X-ray cameras aboard satellites. <strong>The</strong> corona is very<br />

hot—up <strong>to</strong> 1.5 million degrees Celsius—and is the source<br />

<strong>of</strong> the solar wind.<br />

Corona<br />

America’s first series <strong>of</strong> pho<strong>to</strong>-reconnaissance or IMINT<br />

(imagery intelligence) satellites, involving more than one<br />

hundred launches between 1959 and 1972. <strong>The</strong> program<br />

had the cover name Discoverer and was only declassified<br />

in 1995. A Discoverer satellite would be placed in a polar<br />

orbit by a Thor-Agena rocket in order <strong>to</strong> take pho<strong>to</strong>graphic<br />

swaths as it passed over the Soviet Union. It then<br />

collected its exposed film in a heat-resistant “bucket” at<br />

the nose, and the bucket would reenter over the Pacific<br />

Ocean, deploy two small parachutes, and be recovered in<br />

midair by an aircraft <strong>to</strong>wing a trapeze-like snare. Bizarre as<br />

this sounds, the program proved successful after a shaky<br />

start—the first 12 launches failed, and the thirteenth,<br />

though achieving orbit, did not carry a camera. Discoverer<br />

14 marked the program’s first triumph. Its returning<br />

bucket was caught by a C-119 cargo plane on August 18,<br />

1960, and provided the earliest pho<strong>to</strong>s <strong>of</strong> the Soviet<br />

Union’s Plesetsk rocket base. In that single day, Corona<br />

yielded more valuable images <strong>of</strong> the Soviet Union than<br />

did the entire U-2 spy plane program. It proved conclusively<br />

that the Soviets’ intercontinental ballistic missile<br />

(ICBM) arsenal did not number in the hundreds, as was<br />

widely feared, but rather amounted <strong>to</strong> somewhere<br />

between 25 and 50. This knowledge, however, was hidden<br />

from the American public for years. Corona showed that<br />

the supposed missile gap that Kennedy played upon in his<br />

presidential campaign was a myth—a fact he would have<br />

learned at the time had he taken up Eisenhower’s <strong>of</strong>fer <strong>of</strong><br />

intelligence briefings. Corona allowed the U.S. intelligence<br />

community <strong>to</strong> catalog Soviet air defense and<br />

antiballistic missile sites, nuclear weapons–related facilities,<br />

and submarine bases, along with military installations<br />

in China and Eastern Europe. It also provided pictures <strong>of</strong><br />

the 1967 Arab-Israeli war and Soviet arms control compliance.<br />

Its retrieval system helped NASA develop a safe<br />

means <strong>of</strong> recovering manned spacecraft, and its imaging<br />

systems provided the basis for the cameras carried by the<br />

Lunar Orbiters in 1966 and 1967. 74<br />

Coronas<br />

An international project <strong>to</strong> study the Sun and its interaction<br />

with Earth using spacecraft launched by Russia and<br />

carrying experiments developed by Russia and Ukraine<br />

with involvement from scientists in other European<br />

countries and the United States. Coronas satellites are<br />

equipped <strong>to</strong> study solar activity including flares, active<br />

regions, and mass ejections, in various regions <strong>of</strong> the<br />

spectrum from radio waves <strong>to</strong> gamma rays. Coronas-I<br />

reentered the atmosphere on March 4, 2001, two days<br />

before Mir was de-orbited, leaving Russia temporarily<br />

without a single working science payload in orbit.<br />

Coronas-F carries three main groups <strong>of</strong> instruments <strong>to</strong>

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