Quick Facts
Near InfraRed Spectrograph (NIRSpec)
![An image of Webb's iInstrument infrared sensitivity wavelength ranges.](https://science.nasa.gov/wp-content/uploads/2023/09/instrumentranges.jpg?w=4096&format=jpeg)
The Near InfraRed Spectrograph (NIRSpec) operates over a wavelength range of 0.6 to 5 microns. A spectrograph (also sometimes called a spectrometer) is used to disperse light from an object into a spectrum. Analyzing the spectrum of an object can tell us about its physical properties, including temperature, mass, and chemical composition. The atoms and molecules in the object actually imprint lines on its spectrum that uniquely fingerprint each chemical element present and can reveal a wealth of information about physical conditions in the object. Spectroscopy and spectrometry (the sciences of interpreting these lines) are among the sharpest tools in the shed for exploring the cosmos.
Many of the objects that the Webb is studying, such as the first galaxies to form after the Big Bang, are so faint, that the Webb's giant mirror must stare at them for hundreds of hours in order to collect enough light to form a spectrum. In order to study thousands of galaxies during its 5 year mission, the NIRSpec is designed to observe 100 objects simultaneously. The NIRSpec is the first spectrograph in space that has this remarkable multi-object capability. To make it possible, Goddard scientists and engineers had to invent a new technology microshutter system to control how light enters the NIRSpec.
NIRSpec Innovations
![Closeup of microshutter array](https://science.nasa.gov/wp-content/uploads/2023/09/microshutters1.jpg?w=4096&format=jpeg)
One unique technology in the NIRSpec that enables it to obtain those 100 simultaneous spectra is a micro-electromechanical system called a "microshutter array." NIRSpec's microshutter cells, each approximately as wide as a human hair, have lids that open and close when a magnetic field is applied. Each cell can be controlled individually, allowing it to be opened or closed to view or block a portion of the sky.
It is this adjustability that allows the instrument to do spectroscopy on so many objects simultaneously. Because the objects NIRSpec is looking at are so far away and so faint, the instrument needs a way to block out the light of nearer bright objects. Microshutters operate similarly to people squinting to focus on an object by blocking out interfering light. (Read more about NIRSpec's microshutter technology.)
Video: NIRSpec 3d Diagram Rotation
NIRSpec Image Gallery
Gallery of the development, testing and commissioning of the NIRSpec in reverse chronological order.
The image below is a SLIDESHOW. Hover over the image to see the image title and controls. Click the image to go to a detail page with more info and the ability to download the image at various resolutions (click downward arrow in lower right corner).
Microshutters Image Gallery
Gallery of the development, testing of the microshutters in reverse chronological order.
The image below is a SLIDESHOW. Hover over the image to see the image title and controls. Click the image to go to a detail page with more info and the ability to download the image at various resolutions (click downward arrow in lower right corner).
In Depth: Technical Details About NIRSpec
The NIRSpec enables scientists to obtain simultaneous spectra of more than 100 objects in a 9-square-arcminute field of view. It provides medium-resolution spectroscopy over a wavelength range of 1 to 5 micrometers and lower-resolution spectroscopy from 0.6 to 5 micrometers. The NIRSpec employs a micro-electromechanical system "microshutter array" for aperture control, and it has two HgCdTe detector arrays.
Resources:
![NIRSpec Engineering Diagram](https://science.nasa.gov/wp-content/uploads/2023/09/nirspec-cad-sm.jpg?w=4096&format=jpeg)
NIRSpec was developed by ...
NIRSpec was built for the European Space Agency by Airbus Industries with the microshutter array (MSA) and detector sub-systems fabricated by NASA.
![From left to right: Ralf Ehrenwinkler (Airbus DS), Frank Merkle (Airbus DS), Kai Hoffmann (Airbus DS), Robert Eder (Airbus DS), Max Speckmaier (Airbus DS) and Maurice te Plate (ESA)](https://science.nasa.gov/wp-content/uploads/2023/09/16500218037-1e75160524-k.jpg?w=4096&format=jpeg)
![JWST Team Photo with Completed Flight Instrument module"](https://science.nasa.gov/wp-content/uploads/2023/09/webb-jwstteam-photo2.jpg?w=4096&format=jpeg)