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Obscuration of the Sun by the Moon during total solar eclipse generates the\udchanging of the sky brightness. Sky Quality Meter (SQM) was employed to measure the sky\udbrightness during the 2016 total solar eclipse. The sky was still bright at the first contact time.\udIt is shown by the SQM value of zero. Approaching the second contact time, the SQM value is\udrising up started at the value of 5.92 mpsas. The curvature profile of the SQM measurement value\udis similar to the curvature profile of the SQM measurement at the dawn and dusk. However, the\ud\udflatness part of the curvature is much shorter than night time value of SQM. The maximum of\udSQM measurement value is lower than the SQM measurement value during the night in Ternate.\udIt is 12.47 mpsas and happened at the maximum phase of the eclipse. It was confirmed by the\udfact that at the time of totality, the sky close to the horizon was still bright. There is a\uddiscrepancy between the predicted and actual second and third contact and maximum eclipse\udtime. By assigning the maximum of SQM measurement value as the reference value of maximum\udeclipse time, the actual second and third time can be calculated. The shape of curvature between\udthe actual second and third contact time is symmetry

The sky brightness measurement during the 2016 solar eclipse in Ternate