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

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262 Mars Express<br />

Mars Express<br />

(continued from page 259)<br />

with some heritage from European instruments lost on<br />

the ill-fated Mars 96, as well as a communications package<br />

<strong>to</strong> support Mars lander missions from 2003 <strong>to</strong> 2007.<br />

Beagle 2<br />

<strong>The</strong> miniature lander <strong>to</strong> be carried aboard Mars Express.<br />

It is dedicated <strong>to</strong> looking for traces <strong>of</strong> life and conducting<br />

geochemical analyses, and is named after the ship in<br />

which Charles Darwin sailed <strong>to</strong> the Galapagos. Changes<br />

in the mission specification meant that the mass <strong>of</strong> Beagle<br />

2 had <strong>to</strong> be trimmed from 90 kg <strong>to</strong> 60 kg, echoing<br />

economies that proved necessary on the original Beagle.<br />

(So cramped was that ship that a padre had <strong>to</strong> give up his<br />

berth so that Darwin could go.)<br />

Once it has safely reached the surface by a combination<br />

<strong>of</strong> aeroshell, parachutes, and air bags, Beagle 2 will<br />

deploy a battery <strong>of</strong> ingenious, tiny instruments. <strong>The</strong>se<br />

include a “mole” that can burrow along or through soil<br />

and collect samples for analysis by a mass spectrometer.<br />

<strong>The</strong> mole is placed on the surface by a robotic arm and<br />

can be pulled back in<strong>to</strong> its s<strong>to</strong>rage tube aboard the lander<br />

by means <strong>of</strong> an attached cable. To expose fresh material<br />

from inside rocks, Beagle 2 also carries a modified dentist’s<br />

drill. Samples will be subjected <strong>to</strong> “stepped combustion”—heated<br />

<strong>to</strong> successively higher temperatures—and<br />

then analyzed. An elevated ratio <strong>of</strong> carbon-12 <strong>to</strong> carbon-<br />

13 would be interesting, because living things preferentially<br />

use the lighter form <strong>of</strong> carbon. Beagle 2 will also<br />

Mars Express <strong>The</strong> Beagle lander with its solar panels outspread<br />

and its instrument arm deployed. All rights reserved Beagle 2<br />

sniff the atmosphere for tiny amounts <strong>of</strong> methane, which<br />

would suggest that there might be microbes alive <strong>to</strong>day<br />

on Mars.<br />

Mars Global Surveyor (MGS)<br />

A NASA orbiter launched in November 1996 and<br />

designed <strong>to</strong> investigate, over the course <strong>of</strong> a full Martian<br />

year, the surface, atmosphere, and magnetic properties <strong>of</strong><br />

Mars in unprecedented detail. It is the inaugural mission<br />

in a decade <strong>of</strong> planned intensive in situ research <strong>of</strong> the<br />

Red Planet and also a replacement mission <strong>to</strong> achieve<br />

most <strong>of</strong> the goals <strong>of</strong> the failed Mars Observer. It has<br />

been so successful that its operation has been extended<br />

until late 2004. During this bonus phase, MGS will help<br />

scout landing sites for the Mars Exploration Rovers.<br />

MGS carries four main science instruments. <strong>The</strong> Mars<br />

Orbiter Camera provides daily wide-angle images <strong>of</strong> Mars<br />

similar <strong>to</strong> weather pho<strong>to</strong>s <strong>of</strong> Earth and narrow-angle<br />

images <strong>of</strong> objects as small as 1.5 m across. <strong>The</strong> Mars<br />

Orbiter Laser Altimeter bounces a laser beam <strong>of</strong>f the surface<br />

<strong>to</strong> measure accurately the height <strong>of</strong> mountains and<br />

the depth <strong>of</strong> valleys. <strong>The</strong> <strong>The</strong>rmal Emission Spectrometer<br />

scans emitted heat <strong>to</strong> study both the atmosphere and the<br />

mineral composition <strong>of</strong> the surface. Finally, the Magne<strong>to</strong>meter<br />

and Electron Reflection experiment provides data<br />

on the magnetic state <strong>of</strong> the crustal rocks, which in turn<br />

sheds light on the early magnetic his<strong>to</strong>ry <strong>of</strong> the planet.<br />

Launch<br />

Date: November 7, 1996<br />

Vehicle: Delta 7925<br />

Site: Cape Canaveral<br />

Mars, manned missions<br />

For most <strong>of</strong> the twentieth century, humans dreamed <strong>of</strong><br />

traveling <strong>to</strong> Mars and there has been no shortage <strong>of</strong><br />

plans, proposals, and statements <strong>of</strong> intent <strong>to</strong> make the<br />

dream a reality. <strong>The</strong> first detailed study <strong>of</strong> a manned Mars<br />

mission appeared in Wernher von Braun’s book <strong>The</strong><br />

Mars Project, published in 1952. Von Braun proposed flying<br />

10 spacecraft, each with a crew <strong>of</strong> 70, in convoy <strong>to</strong><br />

Mars. Fifty <strong>of</strong> the astronauts would land on the Red<br />

Planet and stay there for a year before returning <strong>to</strong> Earth.<br />

By 1956, in <strong>The</strong> Exploration <strong>of</strong> Mars, written in collaboration<br />

with Willy Ley, von Braun had scaled back the mission<br />

<strong>to</strong> a dozen crew members and two spacecraft: a<br />

winged glider (carrying a small ascent rocket) that would<br />

land on Mars, and a mother ship in orbit that would be<br />

used for the return home.<br />

During the early years <strong>of</strong> the <strong>Apollo</strong> program, Mars<br />

was seen as the next obvious, and not <strong>to</strong>o distant, step. A<br />

variety <strong>of</strong> studies appeared, including a proposal by Ernst

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