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

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deceleration<br />

Slowing down, or negative acceleration.<br />

decompression sickness<br />

A disorder caused by reduced barometric pressure and<br />

evolved or trapped gas bubbles in the body. It is marked<br />

by pain in the extremities, occasionally leading <strong>to</strong> severe<br />

central nervous system and neurocircula<strong>to</strong>ry collapse.<br />

Deep Impact<br />

NASA Discovery Program mission <strong>to</strong> collide with a<br />

comet and study material thrown out by the impact from<br />

beneath the comet’s surface. If launched as planned on<br />

January 6, 2004, Deep Impact will encounter comet Tempel<br />

1 on July 4, 2005. <strong>The</strong> mission hardware consists <strong>of</strong> a<br />

flyby spacecraft and a smart impac<strong>to</strong>r that will separate<br />

from the flyby probe 24 hours before collision. <strong>The</strong> 500kg<br />

cylindrical copper impac<strong>to</strong>r has an active guidance<br />

system <strong>to</strong> steer it <strong>to</strong> its impact on the sunlit side <strong>of</strong> the<br />

comet’s surface at a relative velocity <strong>of</strong> 10 km/s. Prior <strong>to</strong><br />

collision, the impac<strong>to</strong>r will send back close-up images <strong>of</strong><br />

the comet. <strong>The</strong> impact itself will create a fresh crater,<br />

larger than a football field and deeper than a seven-s<strong>to</strong>ry<br />

building. Two visible imaging systems on the flyby craft<br />

will record the impact events and the subsurface<br />

cometary structure, while two near-infrared imaging spectrometers<br />

will determine the composition <strong>of</strong> the<br />

cometary material. This is the first attempt <strong>to</strong> peer<br />

beneath the surface <strong>of</strong> a comet <strong>to</strong> its freshly exposed interior<br />

for clues <strong>to</strong> the early formation <strong>of</strong> the Solar System.<br />

Images from the cameras on both the impac<strong>to</strong>r and the<br />

flyby craft will be sent <strong>to</strong> Earth in near real-time and be<br />

made available on the Internet. <strong>The</strong> mission is under the<br />

direction <strong>of</strong> principal investiga<strong>to</strong>r Michael A’Hearn <strong>of</strong><br />

the University <strong>of</strong> Maryland and is managed by JPL.<br />

Deep Impact An artist’s rendering <strong>of</strong> the Deep Impact flyby<br />

craft releasing the impac<strong>to</strong>r, 24 hours before the impact event.<br />

Pictured from left <strong>to</strong> right are comet Tempel 1, the impac<strong>to</strong>r,<br />

and the flyby craft. NASA<br />

Deep Space Communications Complex (DSCC) 99<br />

deep space<br />

An imprecise term that may be used <strong>to</strong> refer <strong>to</strong> all space<br />

beyond the Earth-Moon system or, alternatively, all<br />

space beyond the orbit <strong>of</strong> Mars.<br />

Deep Space 1 (DS1)<br />

An experimental probe designed <strong>to</strong> test 12 advanced<br />

spacecraft and science-instrument technologies that may<br />

be used on future interplanetary missions. DS1 was powered<br />

by a type <strong>of</strong> ion engine known as XIPS (xenon-ion<br />

propulsion system). Such systems have been used for station<br />

keeping by some satellites for a number <strong>of</strong> years, but<br />

the DS1 ion drive was larger, more efficient, and worked<br />

longer than any previously flown. In fact, DS1’s engine<br />

accumulated more operating time in space than any other<br />

propulsion system in the his<strong>to</strong>ry <strong>of</strong> spaceflight. Among<br />

the other devices and techniques successfully tested during<br />

the probe’s primary mission were an au<strong>to</strong>nomous navigation<br />

system, a miniature camera and spectrometer, an<br />

ion and electron spectrometer, a solar-energy concentra<strong>to</strong>r<br />

array, and experiments in low-power electronics.<br />

DS1’s primary mission lasted two years and included a<br />

flyby <strong>of</strong> the 3-km-wide asteroid Braille on July 29, 1999.<br />

An extended mission culminating in an encounter with<br />

comet Borrelly began in September 1999 but was soon<br />

threatened by the failure <strong>of</strong> the craft’s most important<br />

navigational instrument, its star tracker, which enabled<br />

DS1 <strong>to</strong> orient itself relative <strong>to</strong> stellar patterns. Rather than<br />

abandon the project, NASA engineers uploaded new s<strong>of</strong>tware<br />

<strong>to</strong> turn an onboard camera in<strong>to</strong> a replacement star<br />

tracker, despite major differences between the two devices.<br />

It proved a valuable fix: on September 22, 2001, DS1 flew<br />

past Borrelly’s nucleus at a distance <strong>of</strong> only 2,171 km,<br />

snapping 30 or so superb black-and-white pho<strong>to</strong>s and collecting<br />

data on gases and dust around the comet. <strong>The</strong><br />

spacecraft’s ion engine was turned <strong>of</strong>f on December 18,<br />

2001, but its radio receiver remains active in case future<br />

generations want <strong>to</strong> contact the probe.<br />

Launch<br />

Date: Oc<strong>to</strong>ber 24, 1998<br />

Vehicle: Delta 7325<br />

Site: Cape Canaveral<br />

Mass, including propellant: 486 kg<br />

Deep Space 2 (DS2)<br />

See Mars Microprobe Mission.<br />

Deep Space Communications Complex (DSCC)<br />

Any one <strong>of</strong> the three Deep Space Network tracking sites<br />

at Golds<strong>to</strong>ne, California; near Madrid, Spain; and near<br />

Canberra, Australia. <strong>The</strong>se sites are spaced about equally

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