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Telescopes focus electromagnetic radiation for closer observation.
Telescopes are used to observe and magnify images in outer space. The electromagnetic spectrum consists of many wavelengths, which constitute visible light, infrared, microwave, and X-ray radiation. Telescopes can be manufactured to view these certain types of radiation.
Various wavelengths of electromagnetic radiation.
Earth's atmosphere partially blocks or absorbs certain wavelengths of radiation, e.g. UV, gamma rays, X-rays, before they can reach Earth's surface. All these wavelengths contain useful information and a telescope outside (beyond) the atmosphere can make use of them too.
Absorption and re-emission.
The atmosphere absorbs the electromagnetic solar radiation.
Telescopes focus electromagnetic radiation for closer observation.
Telescopes are used to observe and magnify images in outer space. The electromagnetic spectrum consists of many wavelengths, which constitute visible light, infrared, microwave, and X-ray radiation. Telescopes can be manufactured to view these certain types of radiation.
The frequency is the arrangement of the forms of electromagnetic radiation according to their wavelengths.
The atmosphere tends to block many of those frequencies. (It's not so much dry, it's as high as possible.)
Current telescopes detect different wavelengths of "light," which, in general, is called electromagnetic radiation. Earth's atmosphere is transparent to infrared radiation - it can easily transmit though our atmosphere. Therefore we can easily detect it from within Earth's atmosphere. However, X-Rays do not easily transmit through the Earth's atmosphere, so we must place our X-Ray detectors OUTSIDE of our atmosphere, ie. in orbit around the earth.
Various wavelengths of electromagnetic radiation.
the electromagnetic spectrum. ============================
Because radiation at those wavelengths is absorbed in the atmosphere, and very little of it ever reaches the ground. Operated on the ground, those telescopes would see almost nothing.
Earth's atmosphere partially blocks or absorbs certain wavelengths of radiation, e.g. UV, gamma rays, X-rays, before they can reach Earth's surface. All these wavelengths contain useful information and a telescope outside (beyond) the atmosphere can make use of them too.
All wavelengths of electromagnetic radiation do.
Absorption and re-emission.