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About Hubble History
Frequently Asked Questions
Glossary
Further Information

HUBBLE INSTRUMENTS

Right from the very beginning the NASA/ESA Hubble Space Telescope has been designed to be a new type of mission - a permanent space-based observatory that could be regularly visited by the Space Shuttle and serviced.

At the same time astronauts would be able to replace or upgrade outdated science instruments

Hubble's position above the Earth's atmosphere means that these science instruments can produce high resolution images of astronomical objects.

Ground-based telescopes can seldom provide resolution better than 0.5-1.0 arc-seconds, except for very short times under the very best observing conditions. Hubble's resolution is about 5-10 times better, or 0.05-0.1 arc-seconds.

THE LAYOUT OF THE HUBBLE INSTRUMENTS

On board Hubble all the instruments are placed in the so-called radial instrument bay (the cylinder above) and axial bay (the boxes below).

On board Hubble all the instruments are placed in the so-called radial instrument bay (in red) and in the axial bay (in yellow).

Hubble's current complement of science instruments currently includes one camera (WFPC2), one imaging spectrograph (NICMOS), and fine guidance sensors (used for guiding the telescope).

Future Instruments (SM4 2008)

  • WFC3 - Wide Field Camera 3
  • COS - Cosmic Origins Spectrograph
  • A repaired ACS and STIS!

Present Instruments

  • ACS - Advanced Camera for Surveys
  • WFPC2- Wide Field and Planetary Camera 2
  • STIS - Space Telescope Imaging Spectrograph
  • NICMOS - Near Infrared Camera and Multi-object Spectrometer.
  • FGS - Fine Guidiance Sensors
  • (COSTAR) - Corrective Optics Space Telescope Axial Replacement

Former Instruments

  • FOC - Faint Object Camera
  • WFPC1 - Wide Field and Planetary Camera 1
  • FOS - Faint Object Spectrograph
  • GHRS - Goddard High Resolution Spectrograph
  • HSP - High Speed Photometer