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James Webb Space Telescope

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    Monitoring Webb’s Mirrors for Optimal Optics

    This image is composed of three square panels in a row, taken by one of the James Webb Space Telescope’s onboard instruments known as the Near Infrared Camera. Each of the three panels contains their own different image that are set on a black background. The panel on the left has a small very blurry, and pixelated white and gray hexagon at the center. From each of the flat surfaces of the hexagon, a small gray and pixelated triangle with its tip facing away, totaling six gray pixelated triangles pointing away from the central hexagon. This picture is ‘selfie’ using a specialized ‘pupil imaging’ lens, designed to take images of the mirror segments and not of the sky. The central panel shows the 18 hexagons of Webb’s primary mirror, akin to the hexagons of a beehive in bright white and gray, but are intentionally defocused and very blurry and pixelated. From the edges of the outer hexagons, light white and gray streak extend nearly all the way to the edge of the picture. The panel on the right is very similar to the image in the center panel, but the hexagon at the very center has black dots at each of the sixe points of the hexagon. At the outer edges it also has streaking blurry gray and white lines that emanate away from the center towards the edge of the picture

    NASA’s James Webb Space Telescope is the largest and most powerful telescope ever launched to space. Its mirror is composed of 18 individual segments that have been aligned so accurately, that they effectively work as a single giant (21.6-foot, or 6.5-meter) reflector. The process of adjusting each of these separately functioning hexagonal mirror segments requires …

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