Fine Guidance Sensor for the Hubble Space Telescope is a system of three instruments used for pointing the telescope in space, and also for astrometry and its related sciences. Each FGS uses a combination of optics and electronics to provide for pointing the telescope at a certain location in the sky. There are three Hubble FGS, and they have been upgraded over the lifetime of the telescope by mannedSpace Shuttle missions. The instruments can support pointing of 2 milli-arc seconds. The three FGS are part of the Hubble Space Telescope's Pointing Control System, aka PCS. The FGS function in combination with the Hubble main computer and gyroscopes, with the FGS providing data to the computer as sensors which enables the HST to track astronomical targets. The FGS can be used to locate something in space, and then lock-on to it. It can provide the movements the telescope must make to keep the object in view, for the main instruments to record data on. The FGS were originally made by the optics company Perkin-Elmer, and as removable and repairable instruments it has been possible to refurbish them over the lifetime of the telescope. The first replacement FGS was installed in 1997, swapping out FGS1. In May 2009, on STS-125 a FGS was replaced during the mission to the Hubble telescope by the SpaceShuttle. The astronaut crew performed an EVA to service the FGS and other components on the telescope in Earth orbit. This was the SM4 mission. An example of astrometry science with the Hubble FGS system is observations of the Low-Mass Binary star systemL722-22. Observations were taken of the system in 1990s, and the data helped determine the mass of each of the components of L722-22, which is also known as LHS 1047 and GJ 1005. The FGS are white-light shearing interferometers. The FGS weigh 220 kg and have dimensions of roughly 0.5 m × 1.0 m × 1.6 meters.
Observations
The smallest KBO yet detected at that time was discovered in 2009 by poring over data from the Hubble Space Telescope's fine guidance sensors. They detected a transit of an object against a distant star, which, based on the duration and amount of dimming, was calculated to be a KBO about in diameter. It has been suggested that the Kepler observatory may be able to detect objects in the Oort cloud by their occultation of background stars, and the Whipple proposal would also try to use this concept A Hubble FGS has also been used for astrometry, tracking the movement of different starts. This ability was used for exoplanet research, where the motion of the star caused by the movement of planets around it was detected. Hubble was used via the FGS sensors to detect the motion of star caused by an exoplanet orbiting it. Asteroids studied include Ausonia, Eunomia, Ariadne, Nysa, and Hektor.
