From Wikipedia, the free encyclopedia
From the center to outer edge of the FGS field of view is 14.1 arcminutes [1] This is a diagram of the field of view of each Hubble Space Telescope instrument, including the three FGS instruments (FGS field of view(s) highlighted in yellow)
A Fine Guidance Sensor being refurbished between servicing missions SM3A and SM4
A fine guidance sensors in space on STS Servicing Mission 2 in 1997

Fine Guidance Sensor (FGS) 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. [2] To enable aiming the telescope at a specific spot in the sky, each FGS combines optics and electronics. [2] There are three Hubble FGS, and they have been upgraded over the lifetime of the telescope by crewed Space Shuttle missions. [3] The instruments can support pointing of 2 milli-arc seconds (units of degree). [4] The three FGS are part of the Hubble Space Telescope's Pointing Control System, aka PCS. [5] 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. [6]

The FGS can be used to locate something in space, and then lock-on to it. [7] It can provide the movements the telescope must make to keep the object in view, for the main instruments to record data on. [8]

The FGS were originally made by the optics company Perkin-Elmer, and as removable and repairable instruments it has been possible to refurbish them over the lifetime of the telescope. [8] The first replacement FGS was installed in 1997, swapping out FGS1. [5]

In May 2009, on STS-125 a FGS was replaced during the mission to the Hubble telescope by the Space Shuttle. [9] The astronaut crew performed an EVA (spacewalk) to service the FGS and other components on the telescope in Earth orbit. [9] This was the SM4 mission. [6]

An example of astrometry science with the Hubble FGS system is observations of the Low-Mass Binary star system L722-22. [10] 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. [10]

The FGS are white-light shearing interferometers. [5] The FGS weigh 220 kg (485 lb) and have dimensions of roughly 0.5 m × 1.0 m × 1.6 meters. [11]

Observations

The smallest Kuiper Belt Object (KBO) yet detected at that time was discovered in 2009 by poring over data from the Hubble Space Telescope's fine guidance sensors. [12] 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 1,000 meters (3,200 ft) in diameter. [12] It has been suggested that the Kepler observatory may be able to detect objects in the Oort cloud by their occultation of background stars, [13] 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 stars. [14] This ability was used for exoplanet research, where the motion of the star caused by the movement of planets around it was detected. [14] Hubble was used via the FGS sensors to detect the motion of star caused by an exoplanet orbiting it. [15] The effect on the red dwarf Gliese 876's by companion Gliese 876b was measured. [15]

FGS was used to study Double-star systems (aka Binary star systems) and to measure distances to astronomical bodies. [15]

FGS has also been used to observe asteroids and calculate their size. [16] Asteroids studied include (63) Ausonia, (15) Eunomia, (43) Ariadne, (44) Nysa, and (624) Hektor. [16]

See also

References

  1. ^ "Hubble Space Telescope Systems" (PDF). Goddard Space Flight Center, Astrophysics Science Division. p. 20. Retrieved November 27, 2023.
  2. ^ a b "Hubble's Instruments: FGS - Fine Guidance Sensors". www.spacetelescope.org. Retrieved 2017-03-03.
  3. ^ "NASA - Refurbished Fine Guidance Sensor (FGS)". www.nasa.gov. Retrieved 2017-03-03.
  4. ^ Fine Guidance Sensors Aboard the Hubble Space Telescope, the Scientific Capabilities of these Interferometer
  5. ^ a b c "Fine Guidance Sensors". Space Telescope Science Institute. Retrieved November 27, 2023.
  6. ^ a b "NASA - Hubble Space Telescope Servicing Mission 4
    Fine Guidance Sensor"    . www.nasa.gov. Retrieved 2017-03-03.
  7. ^ "Fine guidance sensors: Hubble's unsung heros". NewsTimes. Retrieved 2017-04-12.
  8. ^ a b "Fine guidance sensors: Hubble's unsung heros". NewsTimes. Retrieved 2017-03-03.
  9. ^ a b "Photo Index 1". spaceflight.nasa.gov. Archived from the original on 2009-05-26. Retrieved 2017-03-03.
  10. ^ a b Hershey, John L.; Taff, L. G. (1998-01-01). "Hubble Space Telescope Fine Guidance Sensor Astrometry of the Low-Mass Binary L722-22". The Astronomical Journal. 116 (3): 1440. Bibcode: 1998AJ....116.1440H. doi: 10.1086/300516. ISSN  1538-3881.
  11. ^ "Hubble instruments". sci.esa.int. Retrieved 2017-03-03.
  12. ^ a b "HubbleSite - NewsCenter - Hubble Finds Smallest Kuiper Belt Object Ever Seen (12/16/2009) - the Full Story". Archived from the original on 2016-07-06. Retrieved 2017-03-21.
  13. ^ DETECTABILITY OF OORT CLOUD OBJECTS USING KEPLER - 2009
  14. ^ a b ""Out of Whack" Planetary System Offers Clues to a Disturbing Past". UT News | The University of Texas at Austin. 2010-05-24. Archived from the original on 2016-03-10. Retrieved 2018-01-28.
  15. ^ a b c "Hubble Space Telescope – Fine Guidance Sensors". 27 January 2017.
  16. ^ a b Tanga, P.; Hestroffer, D.; Cellino, A.; Lattanzi, M.; Martino, M. Di; Zappalà, V. (2003-04-01). "Asteroid observations with the Hubble Space Telescope FGS". Astronomy & Astrophysics. 401 (2): 733–741. Bibcode: 2003A&A...401..733T. doi: 10.1051/0004-6361:20030032. ISSN  0004-6361.

External links

Retrieved from " https://en.wikipedia.org/?title=Fine_Guidance_Sensor_(HST)&oldid=1187125067"