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Solar eclipse of April 8, 1652

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Nature
  
Total

Magnitude
  
1.0412

Max. width of band
  
213 km (132 mi)

Start date
  
April 8, 1652

Gamma
  
0.7713

Duration
  
169 sec (2 m 49 s)

Greatest eclipse
  
10:22:28

Solar eclipse of April 8, 1652

A total solar eclipse occurred on April 8, 1652. 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. A total solar eclipse occurs when the Moon's apparent diameter is larger than the Sun's, blocking all direct sunlight, turning day into darkness. Totality occurs in a narrow path across Earth's surface, with the partial solar eclipse visible over a surrounding region thousands of kilometres wide. The path of totality intersected the United Kingdom, as well as passing just off the west coast of Norway.

Contents

Observations

Observed from Carrickfergus, Scotland, Dr. Wyberg wrote:

"[The Sun was reduced] to a very slender crescent of light, the Moon all at once threw herself within the margin of the solar disc with such agility that she seemed to revolve like an upper millstone, affording a pleasant spectacle of rotatory motion."

Because this eclipse occurred on a Monday that day became popularly known as Mirk Monday.

It is a part of solar Saros 133.

References

Solar eclipse of April 8, 1652 Wikipedia


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