| 词条 | May 2013 lunar eclipse |
| 释义 |
| type = penumbral | image = Lunar eclipse chart close-2013May25.png | alt = Chart demonstrating the May 2013 lunar eclipse. The moon barely grazed the inside of the northern penumbral shadow of the Earth. | caption = Chart demonstrating the eclipse | date = 25 May 2013 | gamma = 0.0157 | magnitude = 1.5350 | saros_ser = 150 | saros_no = 1 of 71 | penumbral = 33 minutes, 34 seconds | p1 = 3:53:15 | greatest = 4:09:58 | p4 = 4:26:49 | previous = April 2013 | next = April 2014 }} A penumbral lunar eclipse took place on May 24–25, 2013, the second of three lunar eclipses in 2013. It was visually imperceptible due to the small entry into the penumbral shadow. This event marked the beginning of Saros series 150. Visibility
MapGalleryRelated eclipsesLunar year (354 days)This eclipse is the one of five lunar eclipses in a short-lived series. The lunar year series repeats after 12 lunations or 354 days (Shifting back about 10 days in sequential years). Because of the date shift, the Earth's shadow will be about 11 degrees west in sequential events. {{Lunar eclipse set 2009-2013}}Saros seriesThis is the first lunar eclipse of Saros series 150.[1] The next occurrence will also be a penumbral eclipse on June 5, 2031. Solar Saros 157 interleaves with this lunar saros with an event occurring every 9 years 5 days alternating between each saros series. Partial eclipses in series 150 will occur between August 20, 2157 and past the year 3000. Total eclipses will occur between April 29, 2572 and August 28, 2770. See also
Notes and references1. ^http://www.hermit.org/Eclipse/gen_stats.cgi?mode=query&page=full&qtype=type&body=L&saros=150 External links
1 : 21st-century lunar eclipses |
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