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A total solar eclipse occurred on December 22, 1870. 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.Totality was visible from southern Portugal and Spain, across northern Algeria, then crossing Sicily, Greece, Bulgaria, and ending in the south-west of the Russian Empire.

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  • A total solar eclipse occurred on December 22, 1870. 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.Totality was visible from southern Portugal and Spain, across northern Algeria, then crossing Sicily, Greece, Bulgaria, and ending in the south-west of the Russian Empire. (en)
  • L'eclissi solare del 22 dicembre 1870 fu visibile dal sud del Portogallo e dalla Spagna, attraverso il nord dell'Algeria, quindi attraversava la Sicilia, la Grecia, la Bulgaria e fino al termine in Ucraina. Essa fu parte del ciclo di Saros 120. (it)
  • 1870년 12월 22일 일식은 달이 지구와 태양 사이를 지나면서 태양을 완전히 가리는 개기일식이다. 개기일식은 달의 시직경이 태양의 시직경보다 커서 태양을 다 가릴 수 있을 때 일어난다. 개기일식은 매우 좁은 지역에서만 관측 가능하며, 대부분의 다른 지역에서는 부분일식으로 관측된다. (ko)
  • 1870年12月22日日食为一次在协调世界时1870年12月22日出現的日全食。該次日食食分為1.0248,食甚維持2分11秒。 (zh)
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  • A total solar eclipse occurred on December 22, 1870. 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.Totality was visible from southern Portugal and Spain, across northern Algeria, then crossing Sicily, Greece, Bulgaria, and ending in the south-west of the Russian Empire. (en)
  • L'eclissi solare del 22 dicembre 1870 fu visibile dal sud del Portogallo e dalla Spagna, attraverso il nord dell'Algeria, quindi attraversava la Sicilia, la Grecia, la Bulgaria e fino al termine in Ucraina. Essa fu parte del ciclo di Saros 120. (it)
  • 1870년 12월 22일 일식은 달이 지구와 태양 사이를 지나면서 태양을 완전히 가리는 개기일식이다. 개기일식은 달의 시직경이 태양의 시직경보다 커서 태양을 다 가릴 수 있을 때 일어난다. 개기일식은 매우 좁은 지역에서만 관측 가능하며, 대부분의 다른 지역에서는 부분일식으로 관측된다. (ko)
  • 1870年12月22日日食为一次在协调世界时1870年12月22日出現的日全食。該次日食食分為1.0248,食甚維持2分11秒。 (zh)
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  • Eclissi solare del 22 dicembre 1870 (it)
  • 1870년 12월 22일 일식 (ko)
  • Solar eclipse of December 22, 1870 (en)
  • 1870年12月22日日食 (zh)
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