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Astronomy and the radio spectrum
Astronomy and the radio spectrum. This part of the electromagnetic spectrum can largely pass through the atmosphere. Yellow lines are the main emission wavelengths of carbon monoxide (CO), hydrogen cyanide (HCN), ammonia (NH3), water (H2O), formaldehyde (H2CO) and hydrogen (H). Blue lines are wavelengths that are kept free of human radio traffic to prevent such "noise" drowning out astronomical sources. Short radio waves are absorbed in the lower atmosphere, so instruments to detect them must be on mountains or in space. Longer wavelengths can be detected at ground level. Radio wave sources include the Milky Way (upper center) and a variety of other bodies.
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Astronomy and the radio spectrum
Description:
Astronomy and the radio spectrum. This part of the electromagnetic spectrum can largely pass through the atmosphere. Yellow lines are the main emission wavelengths of carbon monoxide (CO), hydrogen cyanide (HCN), ammonia (NH3), water (H2O), formaldehyde (H2CO) and hydrogen (H). Blue lines are wavelengths that are kept free of human radio traffic to prevent such "noise" drowning out astronomical sources. Short radio waves are absorbed in the lower atmosphere, so instruments to detect them must be on mountains or in space. Longer wavelengths can be detected at ground level. Radio wave sources include the Milky Way (upper center) and a variety of other bodies.
Source name:
SCIENCE PHOTO LIBRARY
Unique identifier:
SS2117620
Legacy Identifier:
SA4850
Type:
Image
Size:
2738px × 1905px 632KB
Purpose / Rating
Tags
astronomy
astronomy detectors
electromagnetic spec.
em spectrum
R160/0215
R160/215
R1600215
radio astronomy
radio telescope
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