Fi
rst visualized in 1946 and then launched in 1990, the Hubble telescope
monitors the heavens from its position orbiting the Earth. Images from the
Hubble telescope are much clearer than those taken by telescopes on the Earth as
there is no atmosphere, which means light is coming only from distant space
objects and not reflecting off the various atmospheric layers. Named after Edwin
Hubble, the man who made the astonishing discovery that the universe is expanding
with his observations of distant galaxies, the telescope now monitors distant
galactic events.
Creating the telescope was a massive challenge. Not only would it be a high
performance telescope capable of viewing distant galaxies clearly,
it would have
to cope with massive changes in temperature as it orbits the Earth traveling
closer and then further from the Sun. Scientists came up with a multi layered
insulating shroud which keeps the telescope at a more or less constant
temperature.
A big job, the mirrors for the telescope were ground and then polished from early
1979 to May 1981, a total of two years! They were kept as light as possible using
a low expansion glass to which was added a reflective coat of aluminum and a
protective layer of magnesium fluoride.
Once the telescope was launched, the problems weren’t over and in 1993 just
a few
years after launch, a service mission had to be launched to fix a malfunctioning
mirror that was causing a loss of picture quality. In 2007, after over a decade
and a half of service, its main camera and several gyroscopes that keep the
telescope stable stopped working. A service mission will fix these problems
allowing the telescope to continue to take wonderful images until 2013 when it
will be replaced by the new James Webb Space Telescope. The new telescope will
be able to take even more detailed and spectacular pictures, but only in
infrared.
The Hubble telescope has given us unprecedented images of comets, planets, stars
and galaxies as well as establishing the existence of black holes which can only
be seen through their effect on light and nearby
objects.