There are two astronomical measures that are essential for computing prayer times. The next section provides information on how to calculate the above times mathematically for any location if the coordinates of the location are known. The mean time from sunset to sunrise (or from sunset to Fajr, in some schools of thought). The time at which darkness falls and there is no scattered light in the sky. The time at which the Sun disappears below the horizon. The time when the length of any object's shadow reaches a factor (usually 1 or 2) of the length of the object itself plus the length of that object's shadow at noon. When the Sun begins to decline after reaching its highest point in the sky. The time at which the first part of the Sun appears above the horizon. These times are defined in the following table: To determine the exact time period for each prayer (and also for fasting), we need to determine nine points of time per a day.
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