About: Solar eclipse of June 8, 1937

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A total solar eclipse occurred on June 8, 1937. 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 crossed the Pacific Ocean starting in Gilbert and Ellice Islands (now belonging to Tuvalu and Kiribati) on June 9th (Wednesday ), and ending at sunset in Peru on June 8th (Tuesday). At sunrise totality lasted 3 minutes, 6.8 seconds and at sunset totality lasted 3 minutes, 5.1 second

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  • A total solar eclipse occurred on June 8, 1937. 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 crossed the Pacific Ocean starting in Gilbert and Ellice Islands (now belonging to Tuvalu and Kiribati) on June 9th (Wednesday ), and ending at sunset in Peru on June 8th (Tuesday). At sunrise totality lasted 3 minutes, 6.8 seconds and at sunset totality lasted 3 minutes, 5.1 seconds. American astronomy professor Ethelwynn Rice Beckwith traveled to Peru to see this eclipse, and described the event in detail for the Oberlin Alumnae Magazine in 1937, in an article titled "Three Minutes in Peru." With a maximum eclipse of 7 minutes and 4.06 seconds, this was the longest total solar eclipse since July 1, 1098 which lasted 7 minutes and 5.34 seconds. A longer total solar eclipse occurred on June 20, 1955. (en)
  • 1937年6月8日の日食は、1937年6月8日に観測された日食である。イギリス領ギルバートおよびエリス諸島、ペルーで皆既日食が観測され、太平洋の大部分、アメリカ南部、中央アメリカのほとんど、南アメリカの西半分で部分日食が観測された。これは1098年7月1日から1955年6月20日までの間に持続時間の最も長い皆既日食である。紀元前4000年から西暦6000年の1万年間に日食が23740回あり、そのうち6326回は皆既日食である。ただし、1937年6月8日の皆既日食より持続時間のもっと長いのは59回だけである。 (ja)
  • L'eclissi solare dell'8 giugno 1937 è un evento astronomico che ha avuto luogo il suddetto giorno attorno alle ore 20:41:08 UTC. Con la durata di 7 minuti e 5 secondi, è stata l'eclissi solare più lunga dall'. Un'eclissi solare totale più lunga si è verificata il 20 giugno 1955. (it)
  • 1937년 6월 8일 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)
  • De totale zonsverduistering van 8 juni 1937 trok veel over zee, maar was achtereenvolgens te zien op of in deze zeven (ei)landen: Vaitupu, Tuvalu, Nikumaroro, Hull-eiland, Kantoneiland, Enderbury en Peru. (nl)
  • 1937年6月8日日食是一次日全食，發生於1937年6月8日（東半球爲6月9日）。新月當天（即朔日），地球上觀測到月球和太阳的角距離極小，此時月球如果恰好在月球交點附近，穿過太阳和地球之間，與地球、太阳接近一直線，則會出現日食。月球本影接觸地表而使該區域完全得不到陽光，就會形成日全食，同時在本影兩側數千公里的半影範圍內遮擋部分陽光，形成日偏食。此次日全食經過了吉爾伯特及埃利斯群島和秘鲁，日偏食則覆蓋了太平洋大部、美国南部、中美洲絕大部分、南美洲西半部。此次日全食是自1098年7月1日以來最長的一次，但1955年6月20日就會有更長的日全食發生。 (zh)
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  • 1937年6月8日の日食は、1937年6月8日に観測された日食である。イギリス領ギルバートおよびエリス諸島、ペルーで皆既日食が観測され、太平洋の大部分、アメリカ南部、中央アメリカのほとんど、南アメリカの西半分で部分日食が観測された。これは1098年7月1日から1955年6月20日までの間に持続時間の最も長い皆既日食である。紀元前4000年から西暦6000年の1万年間に日食が23740回あり、そのうち6326回は皆既日食である。ただし、1937年6月8日の皆既日食より持続時間のもっと長いのは59回だけである。 (ja)
  • L'eclissi solare dell'8 giugno 1937 è un evento astronomico che ha avuto luogo il suddetto giorno attorno alle ore 20:41:08 UTC. Con la durata di 7 minuti e 5 secondi, è stata l'eclissi solare più lunga dall'. Un'eclissi solare totale più lunga si è verificata il 20 giugno 1955. (it)
  • 1937년 6월 8일 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)
  • De totale zonsverduistering van 8 juni 1937 trok veel over zee, maar was achtereenvolgens te zien op of in deze zeven (ei)landen: Vaitupu, Tuvalu, Nikumaroro, Hull-eiland, Kantoneiland, Enderbury en Peru. (nl)
  • 1937年6月8日日食是一次日全食，發生於1937年6月8日（東半球爲6月9日）。新月當天（即朔日），地球上觀測到月球和太阳的角距離極小，此時月球如果恰好在月球交點附近，穿過太阳和地球之間，與地球、太阳接近一直線，則會出現日食。月球本影接觸地表而使該區域完全得不到陽光，就會形成日全食，同時在本影兩側數千公里的半影範圍內遮擋部分陽光，形成日偏食。此次日全食經過了吉爾伯特及埃利斯群島和秘鲁，日偏食則覆蓋了太平洋大部、美国南部、中美洲絕大部分、南美洲西半部。此次日全食是自1098年7月1日以來最長的一次，但1955年6月20日就會有更長的日全食發生。 (zh)
  • A total solar eclipse occurred on June 8, 1937. 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 crossed the Pacific Ocean starting in Gilbert and Ellice Islands (now belonging to Tuvalu and Kiribati) on June 9th (Wednesday ), and ending at sunset in Peru on June 8th (Tuesday). At sunrise totality lasted 3 minutes, 6.8 seconds and at sunset totality lasted 3 minutes, 5.1 second (en)
rdfs:label
  • Eclissi solare dell'8 giugno 1937 (it)
  • 1937년 6월 8일 일식 (ko)
  • 1937年6月8日の日食 (ja)
  • Zonsverduistering van 8 juni 1937 (nl)
  • Solar eclipse of June 8, 1937 (en)
  • 1937年6月8日日食 (zh)
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