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A D V A N C E D M A T E R I A L S & P R O C E S S E S | M A Y 2 0 1 6

2 8

DESIGNING SPACE MATERIALS

TO WITHSTAND COSMIC DUST

Materials used to construct spacecraft and protective gear

including the

International Space Station and space suits for astronauts

must be lightweight

yet strong enough to guard against cosmic dust that travels at hypervelocity.

Graham Rideal, Whitehouse Scientific Ltd., Waverton, UK

H

ypervelocity is defined as speeds

in excess of 2-3 km/sec (7000

mph). While such speeds do not

occur naturally on Earth, they are com-

mon in space. Hypervelocity impact

between objects can generate pres-

sures of up to 1 TPa (150million psi) and

temperatures high enough to vaporize

the colliding bodies.

While collisions of large objects are

comparatively rare, notable exceptions

include craters on the surface of the

moon and the giant asteroid believed to

have killed off the dinosaurs. The 150-km

crater on the Yucatan Peninsula in Mex-

ico (Fig. 1) is widely assumed to have

been caused by a 100-km-wide asteroid

travelling at 30 km/sec (70,000 mph).

Smaller meteors have also been known

to knock out satellites (Fig. 2).

The most frequent collisions in

space, however, occur from cosmic

dust whose size varies from roughly

1 mm to below 1

μ

m. Evidence of these

collisions was first seen on spacecraft

returning to Earth whose surfaces were

peppered with microindentations.

CAPTURE AND ANALYSIS

Several methods of collecting cos-

mic dust for analysis exist, but one tech-

nique, which also allows their speed

to be calculated, uses aerogel foam

(Fig. 3). This ultra-lightweight ceramic

foam is approximately 1000 times lighter

than glass. When the specialized foam

is mounted outside spacecraft, cosmic

dust penetrates its structure. It can then

be subsequently recoveredandanalyzed

Fig. 1 —

Simulation of an asteroid impact in Mexico. Courtesy of National Geographic.

Fig. 2 —

Meteor damage to a satellite. Courtesy of University of Kent.

and its penetration depth recorded

(Fig. 4). Individual particles are collected

andmicroscopically measured, enabling

accurate density calculations.