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Celebrate Saturn’s Opposition on March 21, 2010 with the Saturn Opposition/Spring Cleaning Sale! |
The BRC-250 employs non-spherical surfaces for both the primary and secondary mirrors, and when they are combined with two supplementary lenses, elimates spherical aberration, coma, and even astigmatism with a flat field. It produces a focal ratio of f/5 with a 100mm 5º diameter image circle. It also produces an amazing 2 micron stellar image at the center of the field. The BRC-250 employs the Baker method to flatten the field over a wide field. However, because its primary and secondary mirrors are hyperbolic, production was difficult. Today, Takahashi's unique technique in polishing non-spherical surfaces has enabled the first mass production of Baker Ritchey-Chretiens. The large 100mm diameter image makes the BRC-250 a versatile astrograph. The following formats cam be used: 35mm, 6x7, 6x9, and 4x5. The BRC-250 is temperature-compensated by using a space-age state-of-the-art carbon fiber tube which assures precise focus that will not change with temperature fluctuations. The extremely small stellar images makes the BRC-250 the perfect instrument for CCD imaging. The 100mm diameter image circle will accomodate the largest commercially available CCD cameras Takahashi 250mm f/5 Baker Ritchey-Chretien OTA Specifications:
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