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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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42 asteroid missions<br />

asteroid missions<br />

See comet and asteroid missions.<br />

Astra<br />

Acommunications satellite system supported by a fleet<br />

<strong>of</strong> (at mid-2002 count) 12 communications satellites for<br />

direct-<strong>to</strong>-home reception <strong>of</strong> TV, radio, and computer<br />

data. <strong>The</strong> system is owned and operated by SES Astra<br />

(headquartered in Betzdorf, Luxembourg), a subsidiary<br />

<strong>of</strong> SES Global. Seven <strong>of</strong> the Astra satellites are co-located<br />

at 19.2° E, three at 28.2° E, and one each at 5.2° E and<br />

24.2° E. <strong>The</strong>ir footprints provide coverage across the<br />

whole <strong>of</strong> Europe.<br />

Astro (shuttle science payload)<br />

A 12-<strong>to</strong>n Space Shuttle–borne ultraviolet observa<strong>to</strong>ry<br />

that consists <strong>of</strong> three ultraviolet instruments: the Ultraviolet<br />

Imaging Telescope for imaging in the spectral range<br />

<strong>of</strong> 120 <strong>to</strong> 310 nm, the Hopkins Ultraviolet Telescope for<br />

spectropho<strong>to</strong>metry in the range <strong>of</strong> 43 <strong>to</strong> 185 nm, and the<br />

Wisconsin Ultraviolet Pho<strong>to</strong>polarimetry Experiment for<br />

spectropolarimetry in the range <strong>of</strong> 125 <strong>to</strong> 320 nm. Astro<br />

is attached <strong>to</strong> and controlled from the Shuttle throughout<br />

its mission. Astro-1 also gathered X-ray data in the<br />

0.3- <strong>to</strong> 12-keV range using the BBXRT(Broad Band X-ray<br />

Telescope). Astro-2 featured a Guest Observer Program<br />

but did not carry the BBXRT. (See table, “Astro Flights.”)<br />

Astro Flights<br />

Spacecraft Date<br />

Shuttle<br />

Deployment<br />

Mission Orbit<br />

Astro-1 Dec. 2, 1990 STS-35 190 km × 28°<br />

Astro-2 Mar. 2, 1995 STS-67 187 km × 28°<br />

astro-<br />

A prefix (from the Greek astron) meaning “star” or “stars”<br />

and, by extension, sometimes used as the equivalent <strong>of</strong><br />

“celestial,” as in astronautics.<br />

Astro-<br />

<strong>The</strong> prelaunch designation <strong>of</strong> a series <strong>of</strong> Japanese astronomical<br />

satellites built by ISAS (Institute <strong>of</strong> Space and<br />

Astronautical Science) <strong>to</strong> carry out observations <strong>of</strong> cosmic<br />

sources at X-ray and other wavelengths. This series<br />

has included Astro-A (Hino<strong>to</strong>ri), Astro-B (Tenma),<br />

Astro-C (Ginga), and Astro-D (ASCA). Astro-E suffered<br />

a launch failure, while Astro-F, in a break with tradition,<br />

has already been named IRIS (Infrared Imaging Surveyor).<br />

Astrobiology Explorer (ABE)<br />

A proposed orbiting infrared telescope, with a mirror<br />

about 40 cm in diameter, that would search for the spectral<br />

signatures <strong>of</strong> complex interstellar organic compounds<br />

in the range <strong>of</strong> 2.5 <strong>to</strong> 20 microns (millionths <strong>of</strong> a meter).<br />

This data would enable astrobiologists <strong>to</strong> learn more<br />

about the galactic abundance, distribution, and identities<br />

<strong>of</strong> molecules that may play a role in the origin <strong>of</strong> life.<br />

ABE, led by Scott Sandford <strong>of</strong> the Ames Research Center,<br />

is one <strong>of</strong> four MIDEX (Medium-class Explorer)<br />

missions selected by NASA in April 2002 for further<br />

development, two <strong>of</strong> which will be launched in 2007 and<br />

2008.<br />

astrodynamics<br />

<strong>The</strong> science concerned with all aspects <strong>of</strong> the motion <strong>of</strong><br />

satellites, rockets, and spacecraft. It involves the practical<br />

application <strong>of</strong> celestial mechanics, astroballistics, propulsion<br />

theory, and allied fields.<br />

Astro-E<br />

<strong>The</strong> fifth in a series <strong>of</strong> Japanese astronomy satellites designed<br />

<strong>to</strong> observe celestial X-ray sources. Launched on<br />

February 10, 2000, it failed <strong>to</strong> reach orbit after the first<br />

stage <strong>of</strong> its M-5 launch vehicle malfunctioned. Astro-E<br />

carried three main science instruments developed in partnership<br />

with the Goddard Space Flight Center and the<br />

Massachusetts Institute <strong>of</strong> Technology: an X-ray spectrometer<br />

<strong>to</strong> provide high-resolution spectroscopy in the<br />

0.4- <strong>to</strong> 10-keV range, four X-ray imaging spectrometers <strong>to</strong><br />

take X-ray images <strong>of</strong> objects in the 0.4- <strong>to</strong> 12-keV range,<br />

and hard X-ray imaging detec<strong>to</strong>rs <strong>to</strong> measure high-energy<br />

X-rays above 10 keV. It was intended <strong>to</strong> complement the<br />

Chandra X-ray Observa<strong>to</strong>ry and XMM-New<strong>to</strong>n (X-ray<br />

Multi-Mirror).<br />

Astro-F<br />

See IRIS (Infrared Imaging Surveyor).<br />

Astron<br />

A Soviet astrophysics satellite that carried science instruments<br />

from the Soviet Union and France and made observations<br />

<strong>of</strong> cosmic ultraviolet and X-ray sources from a<br />

highly elliptical orbit.<br />

Launch<br />

Date: March 23, 1983<br />

Vehicle: Pro<strong>to</strong>n-K<br />

Site: Baikonur<br />

Orbit: 28,386 × 175,948 km × 34.7°<br />

Mass: 3,250 kg

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