Building Telescopes on the Moon Could Transform Astronomy—And It’s Becoming an Achievable Goal

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Building Telescopes on the Moon Could Transform Astronomy—And It’s Becoming an Achievable Goal
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The Moon still has much to tell us about the early solar system. Encouragingly, it also has scientific value as a platform for observational astronomy.

Several types of astronomy would benefit. The most obvious is radio astronomy, which can be conducted from the side of the Moon that always faces away from Earth—the far side.The lunar far side is permanently shielded from the radio signals generated by humans on Earth. During the lunar night, it is also protected from the Sun. These characteristics make it probablyas no other planet or moon has a side that permanently faces away from the Earth.

Radio waves are a form of electromagnetic energy—as are, for example, infrared, ultraviolet and visible-light waves. They are defined by having different wavelengths in the electromagnetic spectrum.. But radio waves at these wavelengths reach the Moon’s surface unimpeded. For astronomy, this is the last unexplored region of the electromagnetic spectrum, and it is best studied from the lunar far side.

Observations of the cosmos at these wavelengths come under the umbrella of “low frequency radio astronomy.” These wavelengths are uniquely able to probe the structure of the early universe, especially the cosmic “, was in the form of neutral hydrogen atoms. These emit and absorb radiation with a characteristic wavelength of 21cm. Radio astronomers have been using this property to study hydrogen clouds in our own galaxy—the Milky Way—since the 1950s.

Because the universe is constantly expanding, the 21cm signal generated by hydrogen in the early universe has been shifted to much longer wavelengths. As a result, hydrogen from the cosmic “dark ages” will appear to us with wavelengths greater than 10m. The lunar far side may be the only place where we can study this.

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