The Pointing Control System (PCS) aligns Hubble so that the telescope
points to and remains locked on a target. The PCS is
designed for stable pointing to within .01 arcsec and is capable of
holding a target for up to 24 hours while Hubble continues to orbit
the Earth at 17,500 mph. If the telescope were in Los Angeles, it could
hold a beam of light on a dime in San Francisco without
the beam straying from the coin's diameter.
Hubble employs a variety of sensors to detect
its own orientation and position. All work in tandem to send the correct
information to the actuators to adjust Hubble's position on command.
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Fine Guidance Sensors (FGS) (3) |
These sensors are locked onto two guide stars to keep Hubble
in the same relative position of these stars. |
Coarse Sun Sensors (CSS) (4) |
Measure Hubble's orientation to the sun. Also assist in deciding
when to open and close the aperture door. |
Magnetic Sensing System (MSS) (2) |
Measures Hubble's orientation relative to Earth's magnetic field. |
Rate Sensor Units (RSU) (3) |
Each RSU contains two gyroscopes, used for maintaining stable
pointing. |
Fixed Head Star Trackers (FHST) (3) |
An electro-optical detector that maps areas of the sky to determine
Hubble's orientation in space.
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