| dbo:abstract |
A penumbral lunar eclipse took place at the Moon's ascending of the orbit on Sunday, June 5, 1955 with a penumbral eclipse magnitude of 0.62181 (62.181%). A penumbral lunar eclipse takes place when the Moon moves through the faint, outer part of Earth's shadow, the penumbra. This type of eclipse is not as dramatic as other types of lunar eclipses and is often mistaken for a regular Full Moon. The Moon shines because its surface reflects the Sun's rays. A lunar eclipse happens when the Earth comes between the Sun and the Moon and blocks some or all of the Sun's light from reaching the Moon. A penumbral lunar eclipse occurs when the Sun, Earth, and the Moon are imperfectly aligned. When this happens, the Earth blocks some of the Sun's light from directly reaching the Moon's surface and covers all or part of the Moon with the outer part of its shadow, also known as the penumbra. Since the penumbra is much fainter than the dark core of the Earth's shadow, the umbra, a penumbral eclipse of the Moon is often difficult to tell apart from a normal Full Moon. Occurring only 0.5 days after apogee (Apogee on June 5, 1955), the moon's apparent diameter was 6.5% smaller than average (1888 arcseconds). (en) 1955年6月5日月食为一次在协调世界时1955年6月5日出現的半影月食。該次月食半影食分為0.648、全影食分為-0.445。 (zh) |
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wiki-commons:Special:FilePath/Lunar_eclipse_chart_close-1955Jun05.png?width=300 |
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dbc:20th-century_lunar_eclipses dbr:List_of_lunar_eclipses dbr:Solar_eclipse_of_May_30,_1946 dbr:List_of_20th-century_lunar_eclipses dbc:1955_in_science dbr:Saros_(astronomy) dbr:Lunar_eclipse dbr:Solar_eclipse_of_June_10,_1964 dbr:Solar_Saros_117 dbr:File:Lunar_eclipse_chart_close-1955Jun05.png dbr:File:Lunar_eclipse_from_moon-1955Jun05.png dbr:File:SE1946May30P.png dbr:File:SE1964Jun10P.png |
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dbt:Lunar_eclipse_set_1955–1958 dbt:Reflist dbt:Short_description dbt:LEplot1951_link dbt:Lunar-eclipse-stub dbt:Lunar_eclipses |
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dbc:20th-century_lunar_eclipses dbc:1955_in_science |
| rdfs:comment |
1955年6月5日月食为一次在协调世界时1955年6月5日出現的半影月食。該次月食半影食分為0.648、全影食分為-0.445。 (zh) A penumbral lunar eclipse took place at the Moon's ascending of the orbit on Sunday, June 5, 1955 with a penumbral eclipse magnitude of 0.62181 (62.181%). A penumbral lunar eclipse takes place when the Moon moves through the faint, outer part of Earth's shadow, the penumbra. This type of eclipse is not as dramatic as other types of lunar eclipses and is often mistaken for a regular Full Moon. The Moon shines because its surface reflects the Sun's rays. A lunar eclipse happens when the Earth comes between the Sun and the Moon and blocks some or all of the Sun's light from reaching the Moon. A penumbral lunar eclipse occurs when the Sun, Earth, and the Moon are imperfectly aligned. When this happens, the Earth blocks some of the Sun's light from directly reaching the Moon's surface and cover (en) |
| rdfs:label |
June 1955 lunar eclipse (en) 1955年6月5日月食 (zh) |
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freebase:June 1955 lunar eclipse wikidata:June 1955 lunar eclipse dbpedia-zh:June 1955 lunar eclipse https://global.dbpedia.org/id/4owoK |
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wikipedia-en:June_1955_lunar_eclipse?oldid=1121626510&ns=0 |
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wiki-commons:Special:FilePath/Lunar_eclipse_chart_close-1955Jun05.png wiki-commons:Special:FilePath/Lunar_eclipse_from_moon-1955Jun05.png wiki-commons:Special:FilePath/SE1946May30P.png wiki-commons:Special:FilePath/SE1964Jun10P.png |
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wikipedia-en:June_1955_lunar_eclipse |
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wikipedia-en:June_1955_lunar_eclipse |
