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Fine Guidance Sensor/Near InfraRed Imager and Slitless Spectrograph (FGS/NIRISS)

Status:

The Fine Guidance Sensor (FGS) allows Webb to point precisely, so that it can obtain high-quality images. The FGS was delivered to NASA Goddard in July of 2012.

FGS flight instrument FGS flight instrument

Learn More About FGS/NIRISS:

The Near Infrared Imager and Slitless Spectrograph part of the FGS/NIRISS will be used to investigate the following science objectives: first light detection, exoplanet detection and characterization, and exoplanet transit spectroscopy. It has a wavelength range of 0.8 to 5.0 microns, and is a specialized instrument with three main modes, each of which addresses a separate wavelength range. FGS is a "guider," which helps point the telescope. 

Instrument wavelength ranges

FGS

FGS/NIRISS is being built by the Canadian Space Agency.

Links & Resources:

Image Gallery View our FGS/NIRISS image gallery and our instrument-related video page.

Watch the Video Snap Shot of the FGS engineering test unit arriving at NASA Goddard:

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