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

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294 NEAR-Shoemaker (Near-Earth Asteroid Rendezvous)<br />

NEAR-Shoemaker (Near-Earth Asteroid<br />

Rendezvous)<br />

<strong>The</strong> first spacecraft <strong>to</strong> orbit and (though this was not originally<br />

planned) <strong>to</strong> land on an asteroid—Eros. Built and<br />

operated by the Applied Physics Labora<strong>to</strong>ry at Johns<br />

Hopkins University, the probe was originally known simply<br />

as NEAR (Near-Earth Asteroid Rendezvous) but was<br />

renamed NEAR-Shoemaker in memory <strong>of</strong> the American<br />

geologist Eugene Shoemaker (1928–1997). It was the<br />

inaugural mission in NASA’s Discovery Program and<br />

the first probe powered by solar cells <strong>to</strong> operate beyond<br />

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

On June 27, 1997, NEAR-Shoemaker flew by the asteroid<br />

253 Mathilde at a distance <strong>of</strong> 1,200 km and found it<br />

<strong>to</strong> be composed <strong>of</strong> extremely dark material with many<br />

large impact craters, including one about 9 km deep. A<br />

deep-space maneuver in July 1997 brought the probe<br />

back around Earth on January 23, 1998, for a gravity<br />

assistthat put the spacecraft on course for its rendezvous<br />

with the Manhattan-sized asteroid 433 Eros.<br />

NEAR’s instruments included a multispectral imager,<br />

a telescope with a CCD (charge-coupled device) array <strong>to</strong><br />

determine the size, shape, and spin characteristics <strong>of</strong> the<br />

asteroid and <strong>to</strong> map its surface; an X-ray/gamma-ray<br />

spectrometer <strong>to</strong> determine the surface/near-surface elemental<br />

composition; a near-infrared spectrometer <strong>to</strong> map<br />

the mineralogical composition; a magne<strong>to</strong>meter <strong>to</strong> measure<br />

the magnetic field <strong>of</strong> Eros; and a laser altimeter <strong>to</strong><br />

measure the distance between the spacecraft and the<br />

asteroid’s surface.<br />

Launch<br />

Date: February 17, 1996<br />

Vehicle: Delta 7925<br />

Site: Cape Canaveral<br />

Size: 2.8 × 1.7 m<br />

Mass: 818 kg (<strong>to</strong>tal), 55 kg (science payload)<br />

NEAR entered an orbit <strong>of</strong> 323 × 370 km around Eros<br />

on February 14, 2000, then moved <strong>to</strong> gradually smaller<br />

orbits over the next year or so, returning a <strong>to</strong>tal <strong>of</strong> 160,000<br />

images. During the final days <strong>of</strong> its mission, NEAR<br />

maneuvered <strong>to</strong> within 24 km and then, despite the fact<br />

that it had not been built as a lander, became the first<br />

spacecraft actually <strong>to</strong> <strong>to</strong>uch down on an asteroid. NEAR-<br />

Shoemaker was designed only <strong>to</strong> orbit Eros. But with all<br />

<strong>of</strong> its objectives fulfilled, it was decided <strong>to</strong> try <strong>to</strong> bring the<br />

craft in for what mission controllers called a “controlled<br />

crash.” In the final moments before it landed on February<br />

12, 2001, NEAR-Shoemaker returned pictures showing<br />

surface details as small as a few tens <strong>of</strong> centimeters across.<br />

Finally, in one <strong>of</strong> the great moments <strong>of</strong> space exploration,<br />

NEAR-Shoemaker <strong>The</strong> location <strong>of</strong> the landing site <strong>of</strong> NEAR-<br />

Shoemaker on the asteroid Eros. NASA<br />

the probe landed so smoothly that its radio beacon continued<br />

<strong>to</strong> send out a signal from its new home.<br />

Nedelin Catastrophe<br />

See Marsnik.<br />

negative g<br />

Acceleration that a subject experiences as acting from<br />

below (feet-<strong>to</strong>-head direction). Also known as “eyeballs<br />

up.” See also positive g (“eyeballs down”), prone g (“eyeballs<br />

out”), and supine g (“eyeballs in”).<br />

Neptune Orbiter<br />

An important component <strong>of</strong> NASA’s future investigation<br />

<strong>of</strong> the outer Solar System, including Neptune’s moon<br />

Tri<strong>to</strong>n, which may be an icy, organic-rich, captured<br />

Kuiper Belt object. <strong>The</strong> Neptune Orbiter is identified in<br />

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

mission beyond 2007 but remains in the early concept<br />

definition phase.<br />

NERVA (Nuclear Engine for Rocket Vehicle<br />

Application)<br />

A program conducted by NASA and the U.S. A<strong>to</strong>mic<br />

Energy Commission <strong>to</strong> develop a nuclear propulsion<br />

system for use on long-range manned missions. Canceled<br />

in 1969 because <strong>of</strong> high projected development costs, it<br />

was intended <strong>to</strong> result in large, heavy-lift launch vehicles<br />

capable <strong>of</strong> supplying a then-planned lunar base. NERVA<br />

was also <strong>to</strong> have played an integral part in a proposed<br />

manned mission <strong>to</strong> Mars, which was at one time scheduled<br />

for launch in November 1981 with a manned landing<br />

in August 1982.

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