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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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SUVO (Space Ultraviolet Optical Telescope)<br />

A proposed follow-on mission <strong>to</strong> the NGST (Next Generation<br />

Space Telescope) that would enable the ultraviolet<br />

light from faint remote cosmic sources <strong>to</strong> be captured<br />

and analyzed in unprecedented detail. <strong>The</strong> information it<br />

provided would allow astronomers <strong>to</strong> trace galaxy evolution<br />

back <strong>to</strong> the initial era <strong>of</strong> star formation, <strong>to</strong> gain new<br />

insight in<strong>to</strong> supermassive black holes, and <strong>to</strong> study metal<br />

element production in the present epoch. SUVO has<br />

been identified in NASA’s Office <strong>of</strong> Space Science Strategic<br />

Plan as a potential mission beyond 2007 but remains<br />

in the early concept definition phase.<br />

Svobodny Cosmodrome<br />

A former Russian strategic missile base, 120 km north <strong>of</strong><br />

Blagoveshensk, that has been converted <strong>to</strong> a launch site<br />

SWAS (Submillimeter Wave Astronomy Satellite) 425<br />

Surveyor Charles Conrad, <strong>Apollo</strong> 12 commander, examines the Surveyor 3 spacecraft. <strong>The</strong> Lunar Module Intrepid is in the right<br />

background. NASA<br />

for the Strela and Start-1 space launch vehicles. Further<br />

developments may eventually enable the launch <strong>of</strong> larger<br />

vehicles, including the Angara and Pro<strong>to</strong>n. Because <strong>of</strong> its<br />

location at a lower latitude than Plesetsk Cosmodrome,<br />

the only other spaceport on Russian soil, Svobodny is<br />

capable <strong>of</strong> launching vehicles in<strong>to</strong> orbit with a payload<br />

20% <strong>to</strong> 25% higher than this other base.<br />

SWAS (Submillimeter Wave Astronomy Satellite)<br />

A NASA satellite equipped with a 0.6-m telescope, for<br />

making observations in the 490 <strong>to</strong> 550 GHz submillimeter<br />

range, and an acous<strong>to</strong>-optical spectrometer. SWAS<br />

was used <strong>to</strong> study the cooling <strong>of</strong> molecular cloud cores—<br />

the sites <strong>of</strong> star formation in the Galaxy—by measuring<br />

spectral lines <strong>of</strong> molecular oxygen and water. It was the<br />

fourth SMEX (Small Explorer) spacecraft.

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