Azure Spy
Azure Spy D203F750 High-Precision Optical Reflector Telescope Primary Mirror – Ø203 mm, Focal Length 750 mm
Azure Spy D203F750 High-Precision Optical Reflector Telescope Primary Mirror – Ø203 mm, Focal Length 750 mm
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The Azure Spy D203F750 Optical Reflector Telescope Primary Mirror is engineered for high-performance astronomy and scientific observation, offering exceptional image clarity, brightness, and resolution. With a large 203 mm aperture and a 750 mm focal length, this precision-crafted parabolic mirror provides outstanding light-gathering ability and sharp, high-contrast imaging, making it ideal for both deep-sky and planetary observations.
Manufactured from premium-grade optical glass, the mirror is polished and coated to achieve a highly reflective surface, ensuring maximum light transmission and minimal distortion. Its parabolic shape corrects spherical aberrations, delivering crisp, distortion-free images even at higher magnifications. This makes it a perfect choice for Dobsonian, Newtonian, and custom reflector telescope builds.
The 750 mm focal length offers a versatile focal ratio, balancing wide-field deep-sky viewing with detailed planetary imaging. This mirror is also suitable for astrophotography setups, providing a reliable optical foundation for capturing galaxies, nebulae, star clusters, and planetary details with exceptional precision.
Key Specifications:
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Brand: Azure Spy
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Type: High-Precision Reflector Telescope Primary Mirror
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Clear Aperture (Ø): 203 mm (8 inches)
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Focal Length: 750 mm
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Design: Parabolic Primary Mirror
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Optical Glass: Precision-polished, high-reflectivity coating
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Optical Performance: High light-gathering power, sharp resolution, minimal aberrations
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Applications: Newtonian/Dobsonian telescopes, custom telescope builds, planetary and deep-sky observation, astrophotography, scientific research
The Azure Spy D203F750 Primary Mirror is the ideal choice for astronomy enthusiasts, telescope makers, and astrophotographers seeking a large-aperture, precision-engineered mirror that delivers telescope-grade performance and long-term reliability.
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