A Guide to the Best Astronomical Events in 12222: When, Where And How To Shoot Them

Live Eclipse Animation will start at:. You are using an outdated browser, to view the animation please update or switch to a modern browser. Alternatively you can view the old animation by clicking here. Detailed eclipse path map. Portion of Sun covered by the Moon Eclipse obscuration.

How to See Two Total Solar Eclipses in Chile on the Path of Totality

An Eclipse Never Comes Alone! A solar eclipse always occurs about two weeks before or after a lunar eclipse. All eclipses — This is the first eclipse this season. Countdown until eclipse begins 78 Days 6 Hrs 41 Mins 4 Secs. The lunar eclipse diagrams also include the path of the Moon through Earth's shadow. Contact times for each principal phase are tabulated along with the magnitudes and geocentric coordinates of the Sun and Moon at greatest eclipse.

Unless otherwise stated, all times and dates used in this publication are in Universal Time or UT1. Partial Solar Eclipse of January At greatest eclipse [5] UT1 [2] , the eclipse magnitude [6] is 0. This is 3. Local circumstances and eclipse times for a number of cities in Asia appear in Table 1.

What the Eclipse Will Look Like Near the Maximum Point

All times are given in Local Time. This event is the 58th eclipse of Saros The entire series of 70 eclipses spans the years through Only 3 members of this series were total in the years , , and Saros also has 2 hybrid, 37 annular, and 28 partial eclipses. Complete details for the series can be found at: Saros Click for detailed diagram Total Lunar Eclipse of January The apparent diameter of the Moon is larger than average since the eclipse occurs 0.

This is the last of three consecutive total lunar eclipses in and , each one separated by six months previous total lunar eclipses occurred on Jan 31 and Jul In this particular case, the Moon passes deeply into the umbral shadow leading to a relatively long total eclipse lasting 1 hour 2 minutes.

Cancer New Moon Solar Eclipse - Honor Your Sensitivity - Guru Rattana Blog

The times of the major eclipse phases are listed as follows. At the instant of greatest eclipse [1] UT1 the Moon lies at the zenith for a point near eastern Cuba.

'Ring of fire' annular eclipse coming Dec. 26

The umbral eclipse magnitude [3] peaks at 1. As a result, the southern half of the Moon will appear much darker than the northern half because the Moon samples a large range of umbral depths during the total phase. The exact brightness distribution in the umbra is difficult to predict, so observers are encouraged to estimate the Danjon value at mid-totality see Danjon Scale of Lunar Eclipse Brightness. It may also be necessary to assign different Danjon values to different portions of the Moon e.

Much of the eclipse will be seen in central and eastern Europe, but observers there will miss the later stages of the eclipse because they occur after moonset. Likewise parts of the central Pacific experience moonrise after the eclipse begins. Table 2 lists predicted umbral immersion and emersion times for 25 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 January 21 eclipse is the 27th eclipse of Saros This series began on Apr 01 and is composed of 72 lunar eclipses in the following sequence: 8 penumbral, 10 partial, 26 total, 10 partial, and 18 penumbral eclipses Espenak and Meeus, a.

In this context, the January 21 eclipse is the 9th total eclipse in the series. The last total eclipse is on Jul 26 and the final eclipse of the series is on May Complete details for this Saros series can be found at: Saros Click for detailed diagram Total Solar Eclipse of July The eagerly awaited total solar eclipse of July 02 is the first one since the Great American Total Eclipse of Such a close Moon during a total eclipse typically produces a long duration of totality - especially if the path passes near the Equator.

In the case of the July 02 event, the maximum duration is just over 4. The total eclipse is visible from within a narrow corridor that traverses the Pacific Ocean and southern South America. A partial eclipse is seen within the much broader path of the Moon's penumbral shadow, which includes the Pacific Ocean and most of South America Figure 3. Oeno Island is a remote coral atoll and is part of the Pitcairn Islands. Unfortunately, there is no other landfall along the entirety of the Pacific track of kilometers.

The region enjoys especially dry and clear weather - so much so that a string of major international astronomical observatories have been built there, including Cerro Tololo, La Silla and Gemini South. After crossing the Andes, the lunar shadow descends into Argentina for the last segment of its track. The shadow covers the kilometer-stretch across Argentina in only 3 minutes. In Argentina, San Juan lies just inside the southern limit while Cordoba is 75 kilometers north of the track.

Just before the path ends, it barely misses Buenos Aires, the northern edge only 30 kilometers south of the center of the capital. Nevertheless, all roads leading from Buenos Aires to the central line will probably be clogged with traffic on eclipse day. As the duration of each succeeding eclipse decreased, the paths reversed their southern migration and drifted northward during the 18th and 19th centuries. This effect occurred as a result of the Northern Hemisphere season shifting from winter to summer when the Northern Hemisphere tipped towards the Sun. The southbound trend of the Saros series resumed with the eclipse of May At this point, the duration of totality at greatest eclipse had again increased to over 5 minutes.

The most recent member occurred on Jun 21 and its path crossed southern Africa on the summer solstice. After , the next member occurs on Jul 13 and passes through Australia and New Zealand. On Jul 24, the series returns to the African continent producing a path through South Africa. The duration of totality drops as Saros continues to produce total eclipses during the 21st century. The last total eclipse of the series occurs on Aug 15 and lasts a maximum of 1 minute 38 seconds.

The final 20 eclipses of the series are all partial events in the polar regions of the Southern Hemisphere. The family terminates with the partial eclipse of Feb Click for detailed diagram Partial Lunar Eclipse of July It takes place 4. At the instant of greatest eclipse UT1 the Moon lies near the zenith from a location in South Africa. The event is well placed for observers in Europe, Africa, and South Asia.

None of the eclipse will be visible from North America. South America will see later stages of the eclipse, which begins before the Moon rises. Table 5 lists predicted umbral immersion and emersion times for 25 well-defined lunar craters. The July 16 eclipse is the 21st eclipse of Saros This series began on Dec 09 and is composed of 79 lunar eclipses in the following sequence: 16 penumbral, 7 partial, 27 total, 8 partial, and 21 penumbral eclipses Espenak and Meeus, a.

The first total eclipse is on Aug 17 and the final eclipse of the series is on Apr Click for detailed diagram Annular Solar Eclipse of December The last eclipse of the year is the third solar eclipse. A partial eclipse is visible from a much larger region covering much of Asia, northeast Africa, Oceana and western Australia Figure 6.


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The path width is kilometers and the duration of annularity is 2 minutes 59 seconds. Although Bahrain lies just outside the path, the southern half of Qatar is within the path of annularity. Continuing to the southeast, the path crosses the southern United Arab Emirates and northern Oman before entering the Arabian Sea.

The antumbral shadow reaches the southwest coast of the Indian subcontinent at UT1. Traveling with a ground speed of about 1. It sweeps over northern Sri Lanka before heading into the Bay of Bengal. Greatest eclipse occurs in eastern Sumatra at UT1, with an annular duration of 3 minutes 39 seconds.

Racing across the South China Sea, the central track crosses Borneo and the Celebes Sea as it curves to the northeast and passes south of the Philippines archipelago. As it heads across the western Pacific, the antumbral shadow encounters Guam at UT1.


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During the course of its 3. Path coordinates and central line circumstances are presented in Table 6. Local circumstances and eclipse times for a number of cities in Asia are listed in Table 7. The Sun's altitude and azimuth, eclipse magnitude and eclipse obscuration are all given at the instant of maximum eclipse.

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Eclipses During 12222

The December 26 Solar Eclipse Circumstances Calculator is an interactive web page that can quickly calculate the local circumstances for the eclipse from any geographic location not included in Table 7. This is the 46th eclipse of Saros Espenak and Meeus, The series began on Aug 13 with a string of 20 partial eclipses.

The series continued with 33 consecutive annular eclipses from Mar 17 to Mar Saros then changes character with 2 hybrid eclipses from Mar 23 to Apr The first of 7 total eclipses occurs on Apr The series reverts back to partial with the eclipse of Jun It will continue producing partial eclipses until the series ends on Sep In all, Saros produces 71 solar eclipses in the sequence of 20 partial, 33 annular, 2 hybrid, 7 total and 9 partial eclipses.