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South Pole Scope
Paleontologists dig for fossils in order to study the past. Astronomers do the same thing -- except the fossils they work with are made of light. With powerful telescopes that can see deep into space, astronomers can actually catch glimpses of radiation left over from cosmic events -- like, say, the explosion that created the universe. In this Science Update, you’ll hear about one research team’s effort to measure remnants of light from the Big Bang. Podcast
A telescope that's high and dry. I'm Bob Hirshon and this is Science Update.
While we're in the throes of winter, it's summer at the South Pole -- meaning
temperatures hit the balmy high of 22 degrees below zero. Nevertheless, it's
warm enough for scientists from the Center for Astrophysical Research in Antarctica
to tend to one of their newest telescopes. It's called DASI. And researchers
like Erik Leitch of the University of Chicago are using it to measure the Cosmic
Microwave Background. Leitch: DASI actually consists of 13 individual telescopes that work together to
construct an image of the sky. Leitch says the South Pole's an ideal place for
DASI because there's not much water vapor to interfere with measurements. Leitch: So, DASI is perfectly situated to give researchers a snapshot of a baby
universe -- when it was just 300,000 years old. For the American Association
for the Advancement of Science, I'm Bob Hirshon.
You've probably heard that the light from stars takes years to reach the Earth,
because the stars are so far away. So when you look up at the sky, you're really
seeing the stars that were there several years ago - stars that might actually
be burned out today. If you can see that far back in time with your naked eye, imagine what you
can do with a powerful and sensitive telescope like DASI. The light that DASI
measures, known as the Cosmic Microwave Background (CMB), is an invisible, low-frequency
light that's been traveling through the universe for almost as long as the universe
has existed: about 14 billion years. And it hasn't changed much in the journey.
So looking at the CMB is like looking at the universe just 300,000 years after
it was born. (To put that in perspective, that's like finding a photo of your
70-year-old grandmother that was taken when she was just twelve hours old.)
That's why the CMB is sometimes called "fossil light." Because this kind of light is very faint, astronomers need to minimize anything
that might interfere with it. As it turns out, water vapor in the Earth's atmosphere
is one of the biggest problems. That's because water vapor actually emits traces
of low-frequency light that's very similar to the CMB. As a result, if your
telescope is in a humid place, you can't tell if the light you're seeing is
from the ancient universe or from right here on Earth. At the South Pole, the humidity is as low as it gets, since cold air can't
hold very much moisture. And as Leitch explains, it's also high above sea level,
which means you're looking through as little of the atmosphere as possible.
That's why the South Pole is home to several powerful telescopes, including
the 13 that make up DASI. By studying patterns in the Cosmic Microwave Background,
the scientists who use it hope to learn more about how old the universe is,
how fast it's expanding, how much energy and matter is in it, and even how it's
shaped. Now try and answer these questions: Visit the Center for
Astrophysical Research in Antarctica's (CARA) website. Be sure to check
out the South
Pole Adventure Web Page where you will find an Antarctic webcam and other
interesting resources. You can even submit your own idea for an experiment to
be performed at the South Pole. If your experiment is chosen a member of CARA
will mentor you as you prepare your experimental design. You can also learn more
about DASI
and view pictures of it as it was being built.
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