| dbo:abstract |
An annular solar eclipse occurred on March 18, 1969. 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. Annularity was visible from part of Indonesia, and two atolls (Faraulep and Gaferut) in the Trust Territory of the Pacific Islands which belongs to the Federated States of Micronesia now. (en) 1969년 3월 18일 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) L'eclissi solare del 18 marzo 1969 è un evento astronomico che ha avuto luogo il suddetto giorno attorno alle ore 4.54 UTC. L'eclissi, di tipo anulare, è stata visibile in alcune parti dell'Asia (India), dell'Oceania (Australia) e dell'Oceano Pacifico. L'eclissi è durata 26 secondi e l'ombra lunare sulla superficie terrestre ha raggiunto una larghezza di 16 km; l'evento del 18 marzo 1969 è stata la prima eclissi solare del 1969 e la 158ª nel XX secolo. La precedente eclissi solare si è verificata il 22 settembre 1968, la seguente è avvenuta l'11 settembre 1969. (it) 1969年3月18日日食是一次日環食，發生於1969年3月18日（西半球的部分日偏食區域爲3月17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。此次日環食經過了印度尼西亞和太平洋群島託管地的部分島嶼，日偏食則覆蓋了东南亚、澳大利亚的大部分及周邊部分地區。 (zh) |
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An annular solar eclipse occurred on March 18, 1969. 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. Annularity was visible from part of Indonesia, and two atolls (Faraulep and Gaferut) in the Trust Territory of the Pacific Islands which belongs to the Federated States of Micronesia now. (en) 1969년 3월 18일 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) L'eclissi solare del 18 marzo 1969 è un evento astronomico che ha avuto luogo il suddetto giorno attorno alle ore 4.54 UTC. L'eclissi, di tipo anulare, è stata visibile in alcune parti dell'Asia (India), dell'Oceania (Australia) e dell'Oceano Pacifico. L'eclissi è durata 26 secondi e l'ombra lunare sulla superficie terrestre ha raggiunto una larghezza di 16 km; l'evento del 18 marzo 1969 è stata la prima eclissi solare del 1969 e la 158ª nel XX secolo. La precedente eclissi solare si è verificata il 22 settembre 1968, la seguente è avvenuta l'11 settembre 1969. (it) 1969年3月18日日食是一次日環食，發生於1969年3月18日（西半球的部分日偏食區域爲3月17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。此次日環食經過了印度尼西亞和太平洋群島託管地的部分島嶼，日偏食則覆蓋了东南亚、澳大利亚的大部分及周邊部分地區。 (zh) |
| rdfs:label |
Eclissi solare del 18 marzo 1969 (it) 1969년 3월 18일 일식 (ko) Solar eclipse of March 18, 1969 (en) 1969年3月18日日食 (zh) |
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