An annular solar eclipse occurred at the Moon's ascending node of the orbit on Wednesday, August 22, 1979. 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. A small annular eclipse covered only 93% of the Sun in a very broad path, 953 km wide at maximum, and lasted 6 minutes and 3 seconds. This was the second solar eclipse in 1979, the first one a total solar eclipse on February 26.
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| - Eclissi solare del 22 agosto 1979 (it)
- 1979년 8월 22일 일식 (ko)
- Solar eclipse of August 22, 1979 (en)
- 1979年8月22日日食 (zh)
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| - L'eclissi solare del 22 agosto 1979 è un evento astronomico che ha avuto luogo il suddetto giorno attorno alle ore 17.22 UTC. L'eclissi, di tipo anulare, è stata visibile in alcune parti del Sud America, dell'Antartide e dell'Oceano Pacifico. L'eclissi è durata 6 minuti e 3 secondi e l'ombra lunare sulla superficie terrestre ha raggiunto una larghezza di 953 km. L'eclissi del 22 agosto 1979 è stata la seconda eclissi solare nel 1979 e la 181ª nel XX secolo. La precedente eclissi solare si è verificata il 26 febbraio 1979, la seguente è avvenuta il 16 febbraio 1980. (it)
- 1979년 8월 22일 일식은 달이 지구와 태양 사이를 지나면서 태양을 다 가리지 못하고 태양의 가장자리가 고리 모양으로 보이는 금환일식이다. 금환일식은 달의 시직경이 태양의 시직경보다 작아 태양을 다 가리지 못할 때 일어난다. 금환일식은 매우 좁은 지역에서만 관측 가능하며, 대부분의 다른 지역에서는 부분일식으로 관측된다 (ko)
- 1979年8月22日日食是一次日環食,發生於1979年8月22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。月球穿過太阳和地球之間,但距地球較遠,本影未能接觸地表,而使偽本影覆蓋的區域內看到月球的角直徑小於太陽,就形成日環食,同時在偽本影兩側數千公里的半影範圍內形成日偏食。此次日環食經過了南极洲埃爾斯沃思地,日偏食則覆蓋了南美洲南部、南极洲靠近南美洲的一部分及周邊部分地區。 (zh)
- An annular solar eclipse occurred at the Moon's ascending node of the orbit on Wednesday, August 22, 1979. 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. A small annular eclipse covered only 93% of the Sun in a very broad path, 953 km wide at maximum, and lasted 6 minutes and 3 seconds. This was the second solar eclipse in 1979, the first one a total solar eclipse on February 26. (en)
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