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News Release from: Optical Surfaces | Subject: High precision mirrors
Edited by the Engineeringtalk Editorial
Team on 25 February 2005
Mirrors shed light on Pinwheel Galaxy
Using high precision mirrors supplied by Optical Surfaces, the UV/optical telescope aboard the NASA Swift Explorer satellite has revealed new information about Pinwheel Galaxy.
Using high precision mirrors supplied by Optical Surfaces, the UV/optical telescope aboard the NASA Swift Explorer satellite has revealed new information about Pinwheel Galaxy (M101) - a bright, face-on, spiral galaxy located in the constellation Ursa Major, about 15 million light years from Earth The satellite was designed to observe gamma rays bursts, the most energetic phenomena in the universe
This article was originally published on Engineeringtalk on 8 Jun 2007 at 8.00am (UK)
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Optical Surfaces has established an international reputation for supplying high precision spectrograph optics for land and space based telescopes.
As a result of their high-energy output, they can be seen at greater distances and therefore yield data from close to the origins of the universe.
The UV/optical telescope (UVOT) on the NASA Mission was successfully launched in November 2004 to provide ultraviolet and optical data on these gamma-ray bursts.
Based on a Ritchey-Chretien cassegrain design the UVOT offers a wide field of view and high spatial resolution, which placed high demands on the precision and mounting requirements of the telescope optics.
Chosen for its international reputation in large and demanding high precision optics, Optical Surfaces produced the primary and secondary hyperbolic focusing mirrors and filter mounts for the UVOT.
Based on a lightweight conical back design the F#2 primary of 310mm diameter was matched to a hyperbolic secondary to give a uniform lambda/25 RMS.
surface finish to nurse every photon into the correct place.
The challenging process of mounting and testing the optics to ensure they met specification was achieved using the company's own in-house test and calibration facilities.
The UVOT consists of a Ritchey-Chretien telescope feeding a compact image intensified photon-counting detector operating over the wavelength range 170 to 550nm.
UVOT images are taken through a number of filters each sensitive to light of a different colour, ranging from ultraviolet light through the blue to yellow portion of the visible spectrum.
The resultant "false-colour" images show the shortest wavelength ultraviolet rays as blue, and the longest wavelengths as red.
The first images from the UVOT have shown that hot young stars are being formed in abundance in M101, especially in the spiral arms of the galaxy, where they show up in ultraviolet light.
The central regions of the galaxy have cooler, old stars, which appear 'red' in the picture.
A number of foreground stars, located in our own Galaxy, also reveal themselves by their red colour.
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