Solar eclipse of August 17, 1803 (original) (raw)
An annular solar eclipse occurred on August 17, 1803. 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.The eclipse was visible in Africa, Asia, Europe, Indonesia and Indian Ocean, while the annularity was visible in northern Africa, Middle East, and Indian Ocean.
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| dbo:abstract | An annular solar eclipse occurred on August 17, 1803. 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.The eclipse was visible in Africa, Asia, Europe, Indonesia and Indian Ocean, while the annularity was visible in northern Africa, Middle East, and Indian Ocean. (en) 1803년 8월 17일 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) 1803年8月17日日食为一次在协调世界时1803年8月17日出現的日環食。該次日食食分為0.9657，食甚維持3分47秒。 (zh) |
| dbo:wikiPageExternalLink | http://eclipse.gsfc.nasa.gov/SEsearch/SEdata.php%3FEcl=18030817 http://eclipse.gsfc.nasa.gov/SEsearch/SEsearchmap.php%3FEcl=18030817 |
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| rdfs:comment | An annular solar eclipse occurred on August 17, 1803. 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.The eclipse was visible in Africa, Asia, Europe, Indonesia and Indian Ocean, while the annularity was visible in northern Africa, Middle East, and Indian Ocean. (en) 1803년 8월 17일 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) 1803年8月17日日食为一次在协调世界时1803年8月17日出現的日環食。該次日食食分為0.9657，食甚維持3分47秒。 (zh) |
| rdfs:label | 1803년 8월 17일 일식 (ko) Solar eclipse of August 17, 1803 (en) 1803年8月17日日食 (zh) |
| owl:sameAs | freebase:Solar eclipse of August 17, 1803 yago-res:Solar eclipse of August 17, 1803 wikidata:Solar eclipse of August 17, 1803 dbpedia-be:Solar eclipse of August 17, 1803 dbpedia-fa:Solar eclipse of August 17, 1803 dbpedia-ko:Solar eclipse of August 17, 1803 dbpedia-zh:Solar eclipse of August 17, 1803 https://global.dbpedia.org/id/4vfBd |
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