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

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146 GAIA (Global Astrometric Interferometer for Astrophysics)<br />

GAIA (Global Astrometric Interferometer for<br />

Astrophysics)<br />

A proposal for an advanced space astrometry (stardistance<br />

measurement) mission <strong>to</strong> build on the work<br />

started by Hipparcos. It has been recommended within<br />

the context <strong>of</strong> ESA’s (European Space Agency’s) Horizon<br />

2000 Plus plan for long-term space science. GAIA<br />

would measure the distance and velocity <strong>of</strong> more than a<br />

billion stars in the galaxy <strong>to</strong> an accuracy 100 <strong>to</strong> 1,000<br />

times higher than that possible with Hipparcos. It would<br />

also carry out a special study <strong>of</strong> some 200,000 stars within<br />

650 light-years <strong>of</strong> the Sun in a search for Jupiter-mass<br />

planets. GAIA is expected <strong>to</strong> be launched around<br />

2010–2012 and <strong>to</strong> operate for five years.<br />

Galaxy<br />

A constellation <strong>of</strong> about 10 geostationary communications<br />

satellites owned and operated by PanAmSat. <strong>The</strong><br />

latest members <strong>of</strong> the constellation are Galaxy 3C,<br />

launched on June 2, 2002, by a Zenit 35L from the Sea<br />

Launch platform; and Galaxy 13, which was scheduled<br />

for launch in the last quarter <strong>of</strong> 2002.<br />

GALEX (Galaxy Evolution Explorer)<br />

A SMEX (Small Explorer) mission designed <strong>to</strong> make<br />

ultraviolet observations that will shed light on the origin<br />

and evolution <strong>of</strong> galaxies. GALEX is equipped with a 50cm<br />

telescope sensitive in the region <strong>of</strong> 130 <strong>to</strong> 300 nm and<br />

an efficient spectroscope that can obtain the spectra <strong>of</strong><br />

about 100,000 galaxies per year. Partners in the project<br />

include NASA, JPL (Jet Propulsion Labora<strong>to</strong>ry), the<br />

Orbital Science Corporation, and various universities in<br />

California, France, and Japan. GALEX will probably be<br />

launched in 2003.<br />

Galileo<br />

See article, pages 147–148.<br />

Galileo satellite navigation system<br />

A planned European satellite navigation system, similar<br />

<strong>to</strong> GPS (the U.S. military’s Global Positioning System)<br />

but run on a purely civilian basis. It is being developed<br />

by ESA (European Space Agency) in collaboration with<br />

the European Union (the first such joint project) and is<br />

expected <strong>to</strong> be operational by 2008. Its goal is <strong>to</strong> provide<br />

the world in general and Europeans in particular with an<br />

accurate, secure, and certified satellite positioning system<br />

with applications in road, rail, air, and maritime traffic<br />

control, synchronization <strong>of</strong> data transmission between<br />

banks, and so forth. Although Galileo will be in commercial<br />

competition with GPS (and so, not surprisingly,<br />

has been opposed by the U.S. government), it will also<br />

complement GPS and provide redundancy. <strong>The</strong> Galileo<br />

GALEX An artist’s conception <strong>of</strong> GALEX in orbit. NASA/JPL<br />

system will consist <strong>of</strong> 30 satellites (27 in operation and 3<br />

in reserve), deployed in three circular medium Earth<br />

orbits at an altitude <strong>of</strong> 23,616 km and an inclination <strong>of</strong><br />

56° <strong>to</strong> the equa<strong>to</strong>r. Two control centers will be set up in<br />

Europe <strong>to</strong> moni<strong>to</strong>r the operation <strong>of</strong> the satellites and<br />

manage the navigation system. A precursor <strong>of</strong> the system<br />

is EGNOS (European Global Navigation Overlay Service),<br />

which refines current GPS data and foreshadows<br />

the services Galileo will provide.<br />

Gamma<br />

An orbiting Soviet gamma-ray and X-ray telescope<br />

derived from Soyuz-manned spacecraft hardware. It was<br />

originally conceived in 1965 as part <strong>of</strong> a “Cloud Space<br />

Station”—a primary space station from which a number<br />

<strong>of</strong> man-tended, free-flying spacecraft would operate. This<br />

had evolved by the early 1970s in<strong>to</strong> the MKBS/MOK<br />

space station complex. Various spacecraft with specialized<br />

labora<strong>to</strong>ries or instrument sets, including Gamma,<br />

would fly au<strong>to</strong>nomously away from the N-1–launched<br />

main station. <strong>The</strong> Soyuz propulsion system would be<br />

used, but the descent and orbital modules were replaced<br />

by a large pressurized cylinder containing the scientific<br />

instruments. Work on the instrument payload for<br />

Gamma began in 1972, and French participation began<br />

(continued on page 148)

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