Eclipse solar diamond ring
1344×768 · AVIF · CC BY 4.0

The diamond ring effect occurs seconds before totality in a total solar eclipse, when the last sunlight shines through lunar valleys.
About this subject
The diamond ring effect is one of the most striking moments of a total solar eclipse. It occurs immediately before or after the phase of totality, when a single point of sunlight passes through a valley on the Moon's edge, creating an intense glow resembling a jewel. This phenomenon is directly related to Baily's beads, which are the last rays of sunlight filtering between lunar mountains and craters.
Scientifically, the diamond ring effect is important for precise measurements of lunar topography. During an eclipse, astronomers can use the exact moment of the light's disappearance and reappearance to map the Moon's profile with high accuracy. Moreover, the phenomenon helps determine the duration of totality and predict future eclipses with precision.
Historically, the observation of the diamond ring effect has fascinated cultures worldwide. Ancient Chinese and Babylonian records already described the sudden brightness before total darkness. Today, photographers and enthusiasts travel to remote locations to capture this fleeting instant, which lasts only a few seconds. The rarity and beauty of the event make each observation a unique experience, and the quest for the best angle and composition has become a tradition among eclipse chasers.
Frequently Asked Questions
What causes the diamond ring effect in an eclipse?
The effect is caused by the last sunlight passing through a valley on the Moon's irregular edge, creating a bright point that looks like a diamond, seconds before or after totality.
Is it safe to look directly at the diamond ring effect?
No. Even during the effect, the sunlight is still intense and can cause permanent eye damage. Eclipse glasses or solar filters are required before and after totality.
How long does the diamond ring effect last?
It typically lasts only a few seconds, at most 10 to 15 seconds, depending on the Moon's speed relative to the Sun and lunar topography.
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