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Fine Guidance Sensor and Near Infrared Imager and Slitless Spectrograph information


FGS/NIRISS ETU, 2016
FGS Test unit undergoes cryogenic testing, 2012
Infographic of JWST instruments and their observation ranges of light by wavelength

Fine Guidance Sensor and Near Infrared Imager and Slitless Spectrograph (FGS-NIRISS) is an instrument on the James Webb Space Telescope (JWST) that combines a Fine Guidance Sensor and a science instrument, a near-infrared imager and a spectrograph.[1] The FGS/NIRISS was designed by the Canadian Space Agency (CSA) and built by Honeywell[2] as part of an international project to build a large infrared space telescope with the National Aeronautics and Space Administration (NASA) and the European Space Agency (ESA).[1] FGS-NIRISS observes light from the wavelengths of 0.8 to 5.0 microns.[1] The instrument has four different observing modes.[3]

Physically the FGS and NIRISS are combined, but optically they are separate with the FGS being used by the telescope to point it, whereas NIRISS is an independent science instrument.[3][4] The spectroscopic mode is capable of doing exoplanet spectroscopy.[5] The detector for NIRISS is a 2048 × 2048 pixel mercury cadmium telluride (HgCdTe) array, where each pixel is 18 microns on a side according to the STSCi.[6] The field of view is 2.2' × 2.2' which gives a plate scale of about 0.065 arcsec/pixel.[6]

The FGS will help the telescope aim and stay pointed at whatever it is commanded to look at.[7] FGS helps provide data to the JWST Attitude Control System (ACS) and to do this it has a big sky coverage and sensitivity, to give a high probability it can find a guide star.[8]

NIRISS is designed for performing:[9][10]

  • Near-infrared imaging
  • Wide-field slitless spectroscopy
  • Single object slitless spectroscopy
  • Aperture masking interferometry

The aperture masking interferometry mode uses a seven-hole aperture masking disc, and should allow the detection of exoplanets within certain ranges of light and types of stars.[9]

The Engineering Test Unit of the FGS was delivered to NASA in 2010.[11] The flight units were planned to be delivered later after the ETU, which enabled testing with other JWST hardware.[11] The flight units of FGS/NIRISS were delivered to NASA in August 2012.[12]

Commissioning is complete as of the following dates:

  • Single object slitless spectroscopy, 06/22/2022
  • Wide field slitless spectroscopy, 06/14/2022
  • Aperture masking interferometry, 06/14/2022
  • Imaging (parallel only), 06/08/2022
  1. ^ a b c "The James Webb Space Telescope". National Aeronautics and Space Administration. Archived from the original on December 14, 2021. Retrieved November 27, 2016.
  2. ^ "Canada's role in Webb". Canadian Space Agency. 18 February 2011. Archived from the original on 16 January 2024. Retrieved 7 March 2022.
  3. ^ a b Doyon, René; Hutchings, John B.; Beaulieu, Mathilde; Albert, Loic; Lafrenière, David; Willott, Chris; Touahri, Driss; Rowlands, Neil; Maszkiewicz, Micheal; Fullerton, Alex W.; Volk, Kevin; Martel, André R.; Chayer, Pierre; Sivaramakrishnan, Anand; Abraham, Roberto; Ferrarese, Laura; Jayawardhana, Ray; Johnstone, Doug; Meyer, Michael; Pipher, Judith L.; Sawicki, Marcin (22 August 2012). Clampin, Mark C; Fazio, Giovanni G; MacEwen, Howard A; Oschmann, Jacobus M (eds.). The JWST Fine Guidance Sensor (FGS) and Near-Infrared Imager and Slitless Spectrograph (NIRISS). Space Telescopes and Instrumentation 2012: Optical, Infrared, and Millimeter Wave. Vol. 8442. SPIE. pp. 84422R. Bibcode:2012SPIE.8442E..2RD. doi:10.1117/12.926578. S2CID 120702854.
  4. ^ "Webb's Instruments".
  5. ^ "ESA Science & Technology: The JWST instrument suite". sci.esa.int. ESA. Archived from the original on 27 December 2023. Retrieved 27 November 2016.
  6. ^ a b "NIRISS: Near-InfraRed Imager and Slitless Spectrograph". stsci.edu. Archived from the original on February 3, 2014. Retrieved 2016-11-27.
  7. ^ "Canada's Contribution to the James Webb Space Telescope – Canadian Space Agency". asc-csa.gc.ca. Archived from the original on 2016-11-27. Retrieved 2016-11-27.
  8. ^ "FGS – Fine Guidance Sensor". stsci.edu. Space Telescope Science Institute. Archived from the original on 11 December 2016. Retrieved 27 November 2016.
  9. ^ a b "JWST Near Infrared Imager and Slitless Spectrograph - JWST User Documentation". jwst-docs.stsci.edu. Retrieved 14 March 2022.
  10. ^ "JWST Pocket Guide January 2022" (PDF). stsci.edu. Space Telescope Science Institute. Archived (PDF) from the original on 10 June 2023. Retrieved 14 March 2022.
  11. ^ a b Chandler, Lynn; Chicone, Ruth Ann (8 September 2010). "NASA Goddard Receives the Webb Telescope's Guiding Light from Canada" (Press release). NASA & CSA. Goddard 10-077. Archived from the original on 22 December 2010.
  12. ^ Gutro, Rob (13 August 2012). "Second Flight Instrument Delivered for James Webb Space Telescope". www.nasa.gov. NASA. Archived from the original on 15 August 2012.

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