Temperature spread
The air-temperature minus dew-point spread shows how much cooling is available before saturated conditions are reached.
Estimate when lenses, corrector plates, eyepieces and camera equipment may cool below the dew point, then plan sensible dew control before condensation forms.
Use current conditions, or values from the Clear Sky Indicator for the hour you plan to observe.
Exposed glass can radiate heat to the clear sky and become cooler than the surrounding air.
The selected cooling allowance is a practical planning estimate. Wind, cloud, dew shields, telescope orientation and local ground conditions can change the actual optic temperature.
Dew forms when an optical surface reaches the dew point—not simply when relative humidity is high.
The air-temperature minus dew-point spread shows how much cooling is available before saturated conditions are reached.
An optic facing a clear sky can cool below ambient air temperature, so it may dew before nearby metalwork or the weather station.
A dew heater should normally keep the optic only a few degrees above the dew point. Excess heat can create local air currents and degrade images.
Humidity, fog, wind and cloud can change quickly. Recheck conditions during the session and inspect exposed optics regularly.
The calculator uses the Magnus approximation for dew point. Projected humidity assumes broadly unchanged water-vapour content as the air cools.
Dew point = --