Atmospheric Transmission--Good News and Bad News
This page has been translated into
Swedish, thanks to Daniela Milton (June 2014).
It is not coincidence that our eyes are sensitive to optical light waves. Optical
light can travel nearly unimpeded through our atmosphere, and so our eyes have adapted
themselves to be sensitive at these wavelengths. For thousands of years, optical
light was our only "window" on the Universe, and even then the primary
the naked eye. When Galileo first turned his telescope skyward, he opened this window
a little farther and saw many marvelous things for the first time. Yet, as is discussed elsewhere in these pages, optical light is a small portion of the entire range
of electromagnetic radiation. How much more could we learn about the Universe if
we could use the entire EM spectrum?
This graphic shows schematically how the atmosphere lets some light through while
blocking most kinds of light like X-ray, ultraviolet, and parts of the infrared.
(Click on the graphic to see a larger, more readable version.)
Most of the rest of the EM spectrum gets absorbed or blocked by the atmosphere, and
it's a good thing, too! Just a tiny portion of ultraviolet light leaking through
the atmosphere is enough to give us a painful sunburn if we aren't careful. Can
you imagine what earth would be like if ultraviolet or X-ray light could get
through the atmosphere? Suffice it to say that we wouldn't be around to
"see" it--we would have long since been fried by our own sun! The atmosphere is
"good news" from the perspective of life on earth. But
the atmosphere is "bad news" if we want to see the Universe at these
Radio light was the first window after the optical one to be used for astronomy. This is
because certain portions of the radio spectral region can pass through the atmosphere
and be detected from cosmic sources. As a matter of fact, radio astronomy grew
out of the development of radar techniques during World War II. As the first sensitive
radio receivers were built, users noticed a persistent faint radio noise that they
could not identify. It turns out this "noise" was due to cosmic sources of radio
radiation being picked up by accident. Radio astronomy was born!
Certain portions of the infrared spectral region can get through the atmosphere, at
least partially. Observatories at high altitude (above most of the water vapor in
the atmosphere) can do quite well in certain small wavelength ranges. And special
infrared telescopes have been flown on high-flying aircraft to open this window
even further. However, many portions of the infrared spectrum get completely
absorbed in the atmosphere.
While much can be learned from optical observations, there is also much unique
to be gained from observations in other wavelength ranges that are hidden by the
curtain of our atmosphere. For astronomers to observe in most of the EM spectrum,
we need to get telescopes in space. It has only been over the last 35 years that this
has been possible, with rockets that can lift special telescopes above the atmospheric
curtain. Telescopes have now been flown to observe across the entire spectrum!
For astronomers, that's good news!
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Bill Blair (firstname.lastname@example.org)