
The Kepler focal plane array - picture from NASA
In a previous piece “Megapixel mania” I berate the continued quest for increasing megapixels in cameras. Here is an example where a huge number of pixels is justified when combined with some interesting optics. And it doesn’t even take pictures!
The newly launched Kepler Space telescope is an interesting imaging platform and it has a number of claims to fame in the imaging field. It is the widest aperture space telescope containing a 0.95-meter aperture, wide field-of-view Schmidt telescope, with a 1.4-meter primary mirror. For more on the Schmidt design I wrote an article on telescope designs for the 2006 International Congress of Imaging Science, reprinted as http://www.imaging.org/pubs/reporter/issues/Reporter21_4.pdf .
Although it leads to a compact unit a key issue with the Schmidt design is a curved image plane. This did not stop the Kepler team. The image plane contains a Focal Plane Array (FPA) consisting of a 14” x 14” substrate onto which 25 CCD modules (21 science and 4 fine guidance) are mounted. The curvature of the substrate is designed to match the optimal focal surface of the Schmidt telescope, which is closely described by a 1.4 meter spherical surface. You can see the curvature in the attached picture, found on http://science.nasa.gov/headlines/y2009/20feb_kepler.htm.
With more than 95 megapixels, the FPA of 42 backside illuminated CCDs forms the largest array of CCDs ever launched into space by NASA. Each e2v CCD imaging sensor used has 2,200 by 1,044 active pixels; 27-micron size; and 28-by-55-millimeter image area. The devices are back thinned to yield high quantum efficiency over the 400 to 900 nm wavelength range of interest and to minimize intra-pixel variability
The interesting point with this array is that it is not a camera but a photometer array covering an area of sky around 100 square degrees (about the size of your hand at arms length). The aim is to measure changes as small as 10 ppm in the brightness of stars, indicative of a planet in transit. This is a planet detector, not a camera! As such the image science is different. The CCDs are not used to take sharp pictures; the images are intentionally defocused to about 10 arc seconds to improve the photometric precision. The total system PSF (i.e. optics plus CCD) ranges from 4 to 7 pixels in diameter. This broad PSF is highly desired in photometric applications such as Kepler because it significantly reduces the sensitivity to intra-pixel variations and minimizes the number of stars that will saturate on the CCDs. For more on the optical design check out http://kepler.nasa.gov/pdf_files/95_Million_Pixel_FPA.pdf .
Best of luck to the Kepler team – image science in action!
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