This rear fan holder has been specifically designed for Sky-Watcher Newton telescopes with a 200 mm primary mirror, with a clear objective: to effectively prevent dew formation on the primary mirror, a common issue during humid nights, both in visual observing and astrophotography.
At this mirror size, internal thermal turbulence is generally a secondary concern. Here, the fan is primarily used to direct airflow onto the surface of the primary mirror, preventing condensation and allowing observing or imaging sessions to last significantly longer.
The airflow is directed precisely toward the primary mirror, which allows:
The system remains highly effective as long as the telescope is not pointed straight up toward the zenith for an extended period. In cases of very high humidity combined with prolonged zenith pointing, as with any passive ventilation solution, effectiveness may naturally be reduced.
The fan used is a PC-grade fan, selected for its quiet operation and reliability. All potential vibration sources have been carefully addressed:
Thanks to these design choices, vibrations are strongly damped, allowing the fan to be safely used:
The fan can remain in operation:
For even greater peace of mind, a version with an integrated speed controller is available. It allows fine adjustment of the fan speed, resulting in even quieter operation, especially appreciated for long-exposure imaging.
The fan can also be controlled via an ASIair or any compatible 12 V power management system.
The fan operates on 12 V. The product is supplied with a 12 V cigarette-lighter power cable.
The 12 V power source itself is not included (external battery or power supply required).
Each holder is designed and assembled in our workshop, then visually inspected before shipping.
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