The Hubble Space Telescope


The Hubble Space Telescope orbits 600 kilometers above the Earth, completing one orbit about every 97 minutes. It provides amazing views of the universe that cannot be made using telescopes on the ground, whose views are obscured by the haze of the atmosphere.

Hubble was originally designed in the 1970s, and eventually launched in 1990. It was the first scientific device in orbit that was specifically designed for routine servicing by astronauts. Its modular design allows the astronauts to take it apart, replace worn out equipment, and upgrade its instruments.

Hubble's accomplishments are extraordinary. Previously, distances to far-off galaxies were not well known, and questions about the origins of the universe remained unanswered. Hubble data has changed all of that. Every day, the Hubble telescope collects 3 to 5 gigabytes of new data, and delivers 10 to 15 gigabytes of stored data to astronomers all over the world.



As of March 2000, Hubble had:

- Made over 330,000 observations of more than 25,000 astronomical objects.
- Generated 7.3 terabytes of data (enough to fill your computer every day for 10 years).
- Provided data for more than 2,663 scientific papers.
- Travelled about 2.4 billion kilometres - nearly the distance from Earth to Uranus.
- Received about 93 hours of upgrades in 3 successful Shuttle servicing missions.


Hubble is completely controlled by scientists on the ground. Four antennae send and receive information between the telescope and the Flight Operations Team at the Space Telescope Science Institute, via the Tracking and Data Relay Satellite system; there are currently five TDRS satellites located at various locations in the sky.



Every few years, a team of astronauts carried a selection of new equipment on the Space Shuttle designed to upgrade the Hubble telescope. This included improved instrumentation or electronics, new optical devices, or special instrument packages. At the right, you can see astronauts servicing the telescope, which has been docked inside the shuttle bay.
The telescope is manoeuvered into place using the 'Canadarm' robotic arm, by an astronaut inside the shuttle. As you can see, the shuttle was flying 'upside down', with Earth appearing to hang above them in the sky as they work.

Shown below are two images showing the release of the Hubble telescope back into its own orbit, also accomplished using the Canadarm.




Hubble needs electricity to operate. This is obtained using two wing-like solar arrays, each covered by solar cells that convert the sun's energy into 3,000 watts of electricity, to run the telescope's scientific instruments, computers, and radio transmitters. The solar arrays are designed for replacement by astronauts, when necessary. They can be rolled up or folded for shuttle trips to and from Hubble. Some of the electricity generated is stored in batteries so that the telescope can operate while it's in Earth's shadow (about 36 minutes out of each 97 minute orbit). Fully charged, each battery contains enough energy to operate the telescope for 7.5 hours.

As the Hubble telescope passes in and out of direct sunlight, it has to endure dramatic temperature extremes ... fluctuations of more than 100° Fahrenheit. To help protect the telescope, a blanket of multilayered insulation covers the aluminum shell housing the instruments. The telescope itself is held together by a truss made of graphite epoxy that is stiff, strong, and light, and that resists expanding and contracting.

The telescope uses a Cassegrain-type arrangement of mirrors, which have been polished very smooth ... if Hubble's primary mirror were scaled up to the diameter of the Earth, the biggest bump would be only 15 cm tall. Shortly after Hubble's original debut in 1990, scientists found that the primary mirror's shape was incorrect, causing 'spherical aberration'. Fortunately, corrective lenses were able to solve this problem. The mirrors are kept at a nearly constant room temperature (about 21° C) to avoid warping.

In March 2002, shuttle astronauts installed in the telescope a new 'Advanced Camera for Surveys', which increased Hubble’s ability to spot distant objects by a factor of ten. The ACS unit produces pictures in high resolution; at 16 million pixels per image, the pictures produced by this new instrument package are stunning.

NASA has released images taken by the new instruments, which we have included below. We should point out that the colours visible in the photos are not necessarily those you would see with your eyes alone; sometimes colours are added to make different parts of the object stand out more clearly.



Above is the Hubble Deep Field photograph, taken in 1995, which was at that time the deepest view of the universe, showing some 1500 galaxies at a distance of close to 10 billion light years. (The way the universe looked 10 billion years ago).

The image at the right, nicknamed Tadpole, was taken in April 2002 using the ACS instrument, and shows twice as many galaxies, at a greater distance. Moreover, this image was taken using a much shorter exposure time than the original one.






The Eagle Nebula (M16) is a region of our own galaxy, 6,500 light-years from Earth in the constellation Serpens, where stars are currently forming out of hydrogen gas. Ultraviolet light from newly-formed stars in or near the nebula is energizing the gas clouds, causing them to glow in visible light.

The image has been artificially coloured to show hydrogen atoms as green, sulfur ions as red, and doubly-ionized oxygen atoms as blue. These colour reassignments increase the detail visible in the image, because otherwise the actual red light produced by hydrogen and sulfur would be hard to tell apart.

In this image, the blue-green haze indicates light from hydrogen and oxygen surrounding the dark columns. The columns display reddish highlights identifying light from sulfur.

Dense, compact pockets of interstellar gas within the nebula are dense enough to collapse under their own weight, forming young stars. These will continue to grow as they accumulate more and more mass from their surroundings, eventually 'turning on' as nuclear fusion reactions begin.





The above picture shows two galaxies in mid-collision 300 million light-years away. The two galaxies will eventually merge into a single giant galaxy. Tidal streams of stars, gas and dust pass between them, and were spotted by the Hubble Space Telescope's Advanced Camera for Surveys in April 2002. This picture supplies a hint about what is likely to happen to our own Milky Way in several billion years when it collides with the neighboring Andromeda Galaxy. Such colliding galaxies have been observed elsewhere; strangely, most of the billions of stars within each galaxy are hardly affected.

NGC 2264, the 'Cone Nebula', is another dark pillar of gas and dust that is forming stars, in the constellation Monoceros, 2,500 light-years from Earth. Radiation from hot, young stars, near the top of this image, has eroded the nebula over billions of years. Escaping hydrogen gas has been heated to a glow, creating the reddish halo.


The Hubble telescope is no longer being maintained. It has been replaced by the James Webb space telescope, which is a lot more powerful.


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