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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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312 Osumi<br />

OSO (Orbiting Solar Observa<strong>to</strong>ry)<br />

(continued from page 308)<br />

extrasolar sources at ultraviolet, X-ray, and gamma-ray<br />

wavelengths. OSO-1 was the first satellite <strong>to</strong> carry<br />

onboard tape recorders for data s<strong>to</strong>rage and instruments<br />

that could be accurately pointed. <strong>The</strong> two-section observa<strong>to</strong>ry<br />

was stabilized because the lower section, the<br />

“wheel,” spun as a gyroscope at a near constant 30 rpm.<br />

<strong>The</strong> upper fan-shaped section, the “sail,” was joined <strong>to</strong><br />

the wheel by a connecting shaft and remained pointed at<br />

the Sun during the OSO daytime. Experiments in the<br />

wheel scanned the Sun every two seconds and those in<br />

the sail pointed continuously at the Sun. (See table,<br />

“OSO Missions,” on page 308.)<br />

Osumi<br />

<strong>The</strong> first Japanese satellite. It comprised the fourth stage<br />

<strong>of</strong> a Lambda 4S launcher and transmitted in orbit for<br />

about 17 hours.<br />

Launch<br />

Date: February 11, 1970<br />

Vehicle: Lambda 4S<br />

Site: Kagoshima<br />

Mass: 24 kg<br />

Orbit: 340 × 5,140 km × 31° orbit<br />

overshoot boundary<br />

<strong>The</strong> upper side <strong>of</strong> a reentry corridor, marking the region<br />

above which the atmospheric density is so low that the<br />

spacecraft cannot decelerate sufficiently and instead skips<br />

back in<strong>to</strong> space.<br />

OWL (Orbiting Wide-angle Light-collec<strong>to</strong>rs)<br />

A proposed space mission <strong>to</strong> study cosmic rays <strong>of</strong> the<br />

highest energy. <strong>The</strong>se particles are so rare that only a few<br />

have ever been seen; they may have as much energy as a<br />

fast-thrown baseball, and it is not even known whether<br />

they are pro<strong>to</strong>ns, heavy nuclei, or pho<strong>to</strong>ns. OWL will<br />

employ Earth as a particle detec<strong>to</strong>r by using two highaltitude<br />

spacecraft <strong>to</strong> obtain a binocular view <strong>of</strong> the light<br />

flashes produced by super-energetic cosmic rays interacting<br />

with the atmosphere. It has been identified in<br />

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

mission beyond 2007, but it remains in the very early<br />

concept definition phase.<br />

oxidizer<br />

A substance that supports the combustion reaction <strong>of</strong> a<br />

fuel or propellant.<br />

OSO An engineer checks two spectrometers on OSO 8.<br />

Hughes Aircraft<br />

oxidizer-<strong>to</strong>-fuel ratio<br />

<strong>The</strong> ratio between the mass <strong>of</strong> oxidizer burned per mass<br />

<strong>of</strong> fuel burned (liquid engines only).<br />

oxygen, regenerative<br />

A spacecraft’s oxygen supply that is recycled for repeated<br />

use after being cleaned <strong>of</strong> carbon dioxide. This is accomplished<br />

by human-made chemical devices or (in theory)<br />

by plant life onboard. <strong>The</strong> latter is suggested for interplanetary<br />

missions, which will be <strong>of</strong> long duration.<br />

oxygen-hydrocarbon engine<br />

A rocket engine that operates on a propellant <strong>of</strong> liquid<br />

oxygen as oxidizer and a hydrocarbon fuel, such as the<br />

propellant derivatives.

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