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The series started with partial solar eclipse on April 17, It contains one hybrid eclipse on July 14, , and total eclipses from July 25, through October 29, The series ends at member 72 as a partial eclipse on June 5, The longest duration of totality will be 6 minutes, 34 seconds on May 28, The metonic series repeats eclipses every 19 years Eclipses occur in nearly the same calendar date.
All eclipses in this table occur at the Moon's descending node.
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From Wikipedia, the free encyclopedia. Solar eclipse of December 14, Map. A Catalogue of Eclipse Cycles. Utrecht University. Retrieved 6 October Solar eclipses. Eclipse chasing Solar viewer Planetary transit Solar eclipses in fiction. Categories : Total solar eclipses in science in South America 21st-century solar eclipses December events.
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On this website, the Gregorian calendar is used for all calendar dates from Oct 15 onwards. Before that date, the Julian calendar is used. For more information on this topic, see Calendar Dates. The Julian calendar does not include the year 0. This is the 14th eclipse of Saros [ 4 ] Espenak and Meeus, The family begins with a series of 18 partial eclipses from to Complete details for the entire series of 72 eclipses in the order: 18 partial, 6 annular, 1 hybrid, 39 total and 8 partial spanning years can be found at:. Partial Solar Eclipse of June The next partial solar eclipse occurs at the Moon's descending node in Taurus.
The event is visible from high latitudes in the Northern Hemisphere Figure 2. The eclipse begins at sunrise in Siberia and northern China where the penumbral shadow first touches Earth at UT. Two hours later, greatest eclipse occurs at UT. At that time, an eclipse of magnitude 0. Although most of Alaska and northern Canada will witness the partial eclipse, the southern limit of the penumbra falls along a curve from south of Fairbanks to central New Brunswick and Nova Scotia.
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Reykjavik, Iceland receives a 0. Northern most Norway, Sweden and Finland also get a midnight Sun eclipse with the event hanging above the northern horizon. The partial eclipse ends at UT when the penumbra leaves Earth just north of Newfoundland in the Atlantic Ocean. Eclipse times and local circumstances for major cities in North America, Europe and Asia are given in Table 2. The Sun's altitude, azimuth, the eclipse magnitude and obscuration are given at the instant of maximum eclipse.
This is the 68th eclipse of Saros The family began with a group of 8 partial eclipses from the years to The Saros ends with a small partial eclipse in Complete details for the entire series of 72 eclipses in the order: 8 partial, 40 total, 2 hybrid, 15 annular and 7 partial spanning years can be found at:. Total Lunar Eclipse of June The Moon passes deeply through Earth's umbral shadow during this rather long event. The total phase itself lasts minutes. The last eclipse to exceed this duration was in July The Moon's contact times with Earth's umbral and penumbral shadows are listed below.
At the instant of greatest eclipse [ 5 ] the umbral eclipse magnitude [ 6 ] will reach 1. The Moon's southern limb will lay Thus, the northern regions of the Moon will probably appear brighter than the southern regions that lie deeper in the shadow. Since the Moon samples a large range of umbral depths during totality, its appearance will change dramatically with time. It is difficult to predict the exact brightness distribution in the umbra so observers are encouraged to estimate the Danjon value at different times during totality see Danjon Scale of Lunar Eclipse Brightness.
December 2011 Lunar Eclipse Aspects
Note that it may also be necessary to assign different Danjon values to different portions of the Moon i. Nearly 30 years ago Jul 06 , the author watched another total lunar eclipse with the Moon in the same part of the sky. I was amazed at how brilliantly the summer Milky Way glowed since it was all but invisible during the partial phases. Observers will have a similar opportunity during June's eclipse.
Solar eclipse of December 16, 2085
The summer constellations are well placed for viewing so a number of bright stars can be used for magnitude comparisons with the totally eclipsed Moon. Figure 3 shows the path of the Moon through the penumbra and umbra as well as a map of Earth showing the regions of eclipse visibility. The entire event will be seen from the eastern half of Africa, the Middle East, central Asia and western Australia. Observers throughout Europe will miss the early stages of the eclipse because they occur before moonrise.
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Fortunately, totality will be seen throughout the continent except for northern Scotland and northern Scandinavia. Eastern Asia, eastern Australia, and New Zealand will miss the last stages of eclipse because they occur after moonset. Again, the total phase will be seen from most of these regions.
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Even observers in eastern Brazil, Uruguay and Argentina will witness totality. However, none of the eclipse will be visible from North America. At mid-eclipse, the Moon is near the zenith for observers from Reunion and Mauritius.
Table 3 lists predicted umbral immersion and emersion times for 20 well-defined lunar craters. The timing of craters is useful in determining the atmospheric enlargement of Earth's shadow see Crater Timings During Lunar Eclipses. The June 15 total lunar eclipse is the 34th member of Saros , a series of 71 eclipses occurring in the following order: 8 penumbral, 20 partial, 14 total, 22 partial, and 7 penumbral lunar eclipses Espenak and Meeus, a spanning years. Complete details for Saros can be found at:.