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[Ulushl'ooln$ and l('ray aslroltolny<br />

"Two things affect us most deeply' the stars above<br />

and the conscience within."-Folk wisdom<br />

by Alexander Mitrofanov<br />

HIS ARTICLE IS DEVOTED TO<br />

a modest but still glorious<br />

event. Thirty years ago-or/ to<br />

be exact, on |une 18,1962-the<br />

iirst nonsolar source of X rays was<br />

discovered. This source is in the<br />

constellation of Scorpio, and according<br />

to the accepted terminology is<br />

now called Sco X-1.<br />

The discovery was made cluite<br />

unexpectedly during a rocket experiment<br />

by the American scientists<br />

Bruno Rossi and George Clark<br />

of the Massachusetts Institute of<br />

Technology and Ricardo Giacconi,<br />

F. Paolini, and Herb Gursky of<br />

American Science and Engineering,<br />

Inc. The experimenters had planned<br />

to do research in the X-ray band of<br />

the spectrum (in the region 0.2 nm<br />

< 1" < 0.8 nm) on the fluorescence of<br />

the lunar sur{ace induced by the<br />

flow of fast particles coming from<br />

the hot solar corona (the solar<br />

wind). So-called "so[t" X rays can't<br />

be detected at the Earth's surface because<br />

they are absorbed in the atmosphere.<br />

So devices were installed<br />

onboard the Aerobee-150 rocket,<br />

which was capable of lifting scienti{ic<br />

ecluipment to an altitude of 200 km<br />

or more.<br />

At that time the existence of detectable<br />

celestial X-ray sources other<br />

than the Sun and Moon was consid-<br />

1X-ray solar radiation was discovered<br />

in the Iate 1940s by American<br />

scientists. In near-Earth orbit the flow<br />

of X-ray radiation {rom the "calm" Sun<br />

is about 106 photons/cm2 ' s. During<br />

ered improbable.l Indeed, the distances<br />

to the stars, even the nearest<br />

ones, are so large that the 1/R2 decrease<br />

in the flux of X rays from a star<br />

at a distance R would negate all attempts<br />

at detecting X-ray radiation<br />

from stars like the Sun and those that<br />

are even hotter and bigger.2<br />

It was estimated that the X-ray<br />

flux from hot stars should not be<br />

more than about 10r photon/cm2 ' s<br />

too faint to be detected by devices<br />

-far<br />

available at that time. Nevertheless,<br />

tn 1962 two of the three<br />

photon detectors in the X-ray experiment<br />

showed a sharp increase in the<br />

photon counting rate.<br />

During that historic flight the<br />

rocket rotated about its longitudinal<br />

axis, and the readings of the detectors<br />

were correlated with this rotation.<br />

Thus, despite the large angular<br />

view of the detectors, it was clear<br />

that the source o{ the X rays was<br />

located somewhere near the center<br />

of our galaxy. The exact direction to<br />

the source could not be established<br />

in that experiment, although evidently<br />

neither the Sun nor the Moon<br />

was connected in arry way with the<br />

increase in X-rayphotons. That very<br />

first experiment also showed the<br />

existence of a cosmic background of<br />

solar bursts it increases many times<br />

over.<br />

2Modern technology is capable of<br />

recording the X-ray radiation o{ the<br />

stellar coronas in ordinary stars-for<br />

example, Alpha Centauri, which is a<br />

star similar to our Sun.<br />

comparatively bright, continuous X-<br />

ray radiation.<br />

One year later the scientists again<br />

launched Aerobee, but this time<br />

with new equipment. The angular<br />

view of the X-ray detectors was decreasedby<br />

means of a Roentgen collimator<br />

whose walls were impervious<br />

to X rays. The same source<br />

discovered in 1952 was detected<br />

again! But this time its coordinates<br />

on the celestial sphere were determined.<br />

In another part of the sky a<br />

second bright X-ray source was<br />

found, in the Crab Nebula (TauX-1).<br />

There could no longer be any doubt:<br />

unusually bright X-ray sources exist<br />

outside our solar system (see figures<br />

I and2 on page 12). This discovery<br />

revolutionized our view of the structure<br />

of the universe and stimulated<br />

the development of a new experimental<br />

science: X-ray astronomy.<br />

You can read more about this in<br />

many fine books on popular astronomy.<br />

As for our story, we leave the sky<br />

along with the discovery that transformed<br />

astrophysics in our century<br />

andretumto Earth, to the experimental<br />

equipment that makes such discoveries<br />

possible. Let's take a closer<br />

look at one of the tools of X-ray optics-the<br />

collimator, which is a component<br />

of modern X-ray or gammaray<br />

telescopes (figures 3 and 4). Its<br />

design is rather simple: it consists of<br />

a system of parallel metal plates/<br />

masks, slits, and little identical tubes<br />

working together to limit the angular<br />

o<br />

Y C<br />

C)<br />

-C O<br />

-C a(s<br />

f<br />

_o<br />

E<br />

10 JUI.Y/AUOUSI 1SS4

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