1. Related eclipses
     Part 1 of 2    Part 2 of 2  

2. Saros 125

3. Notes

4. References

An annular solar eclipse occurred on June 28, 1889. A solar eclipse occurs when the Moon passes between Earth and the Sun, thereby totally or partly obscuring the image of the Sun for a viewer on Earth. An annular solar eclipse occurs when the Moon's apparent diameter is smaller than the Sun's, blocking most of the Sun's light and causing the Sun to look like an annulus (ring). An annular eclipse appears as a partial eclipse over a region of the Earth thousands of kilometres wide. The path of annularity crossed Atlantic Ocean, Africa and Indian Ocean. This was the 47th solar eclipse of Solar Saros 125. The green line means eclipse begins or ends at sunrise or sunset. The magenta line means mid eclipse at sunrise or sunset, or northern or southern penumbra limits. The green point means eclipse obscuration of 50%. The red line means antumbral northern and southern limits. This is an image below, with a height of 600 pixels, and a width of 520 pixels.

Related eclipses

It is a part of solar Saros 125.

The last seven annular solar eclipses of Solar Saros 125 without a penumbra southern limit (six after 1889)

Part 1 of 2

Part 2 of 2

Saros 125

Notes

References

• NASA chart graphics
• Googlemap

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