NASA's Webb telescope in full focus, ready for instrument commissioning
Engineering images of sharply focused stars in the field of view of each instrument demonstrate that the telescope is fully aligned and in focus. For this test, Webb pointed at part of the Large Magellanic Cloud, a small satellite galaxy of the Milky Way, providing a dense field of hundreds of thousands of stars across all the observatory's sensors. The sizes and positions of the images shown here depict the relative arrangement of each of Webb's instruments in the telescope's focal plane, each pointing at a slightly offset part of the sky relative to one another. Webb's three imaging instruments are NIRCam (images shown here at a wavelength of 2 microns), NIRISS (image shown here at 1.5 microns), and MIRI (shown at 7.7 microns, a longer wavelength revealing emission from interstellar clouds as well as starlight). NIRSpec is a spectrograph rather than imager but can take images, such as the 1.1 micron image shown here, for calibrations and target acquisition. The dark regions visible in parts of the NIRSpec data are due to structures of its microshutter array, which has several hundred thousand controllable shutters that can be opened or shut to select which light is sent into the spectrograph. Lastly, Webb's Fine Guidance Sensor tracks guide stars to point the observatory accurately and precisely; its two sensors are not generally used for scientific imaging but can take calibration images such as those shown here. This image data is used not just to assess image sharpness but also to precisely measure and calibrate subtle image distortions and alignments between sensors as part of Webb's overall instrument calibration process. Credit: NASA/STScI

The alignment of NASA's James Webb Space Telescope is complete. The observatory has been found to be capable of capturing crisp, well-focused images with each of its four powerful onboard science instruments. After completing the seventh and final stage of telescope alignment, the team held a set of key decision meetings and unanimously agreed that the next and final series of preparations, known as science instrument commissioning, is ready to begin. The scientific operations will begin in the summer.

A series of images show the alignment of the telescope across all of the instruments at the observatory.

The test images from a successfully aligned telescope demonstrate what people can achieve when there is a bold scientific vision to explore the universe.

The optical performance of the telescope continues to be better than the predictions of the engineering team. Each instrument is successfully capturing images with the light being delivered to them, thanks to the mirrors that are directing fully focused light from space down into each instrument. The image quality delivered to all instruments is limited by the size of the telescope, meaning that the detail that can be seen is as good as possible. From this point forward, there will be no major changes to the mirrors.

With the completion of telescope alignment and half a lifetime of effort, my role on the James Webb Space Telescope mission has come to an end. We are surrounded by a symphony of creation. It is my hope that everyone can see them.

The team will now focus on science instrument commissioning. Each instrument has a highly sophisticated set of detectors that help it perform the science it was designed to achieve. During the instrument commissioning phase, the specialized characteristics of these instruments will be configured and operated in various combinations to confirm their readiness for science. The Mission Operations Center at the Space Telescope Science Institute in Baltimore is where key personnel involved with the commissioning of each instrument have arrived after the formal conclusion of telescope alignment.

Webb Telescope Completes Alignment Phase. Credit: NASA’s Goddard Space Flight Center

As part of scientific instrument commissioning, the telescope will be commanded to point to different areas in the sky where the total amount of solar radiation hitting the observatory will vary to confirm thermal stability when changing targets. Maintenance observations every two days will monitor the mirror alignment, and when needed, apply corrections to keep the mirrors in their aligned locations.

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