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History of X-Ray Astronomy

How do X-ray telescopes differ from optical telescopes?

X-rays do not reflect off mirrors the same way that visible light does. Because of their high-energy, X-ray photons penetrate into the mirror in much the same way that bullets slam into a wall. Likewise, just as bullets ricochet when they hit a wall at a grazing angle, so too will X-rays ricochet off mirrors (see diagram below). These properties mean that X-ray telescopes must be very different from optical telescopes.

Xrays ricochet off mirrors.
small arrow bullet View the schematic image
small arrow bullet Watch the animation (java)

The mirrors look more like barrels. The mirrors have to be precisely shaped and aligned nearly parallel to incoming X-rays. Thus they look more like barrels than the familiar dish shape of optical telescopes.

The first experimental X-ray telescopes. The first imaging X-ray telescope was made by a team of scientists under the direction of Riccardo Giacconi at American Science and Engineering in Cambridge, MA. It was flown on a small sounding rocket in 1963 and made crude images of hot spots in the upper atmosphere of the Sun.

This telescope was about the same diameter and length as the optical telescope Galileo used in 1610. Over a period of 380 years, optical telescopes improved in sensitivity by 100 million times from Galileo's telescope to the Hubble Space Telescope. Remarkably, Chandra represents a leap of 100 million in sensitivity, yet it took only 36 years to achieve!

Why are X-ray observatories in space?

The building and operation of an X-ray observatory is a marvel of modern technology and ingenuity. Engineers, technicians and scientists design and build large, curving mirrors that can be nested inside one another to increase the total reflecting area of the telescope. The mirrors focus X-ray photons onto state-of-the-art detectors which record the direction and in some cases, the energy of the photons.

Because the Earth's atmosphere absorbs X-rays, X-ray observatories must be placed high above the Earth's surface. This means that the ultra-precise mirrors and detectors, together with the sophisticated electronics that conveys the information back to Earth must be able to withstand the rigors of a rocket launch, and operate in the hostile environment of space.
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