At UT1 the lunar shadow lifts off Earth and returns to space. Central line coordinates and circumstances are presented in Table 3. Partial phases of the eclipse are visible across the southern Pacific Ocean and South America.
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Local circumstances for a number of cities in South America are found in Table 4. The Sun's altitude and azimuth, the eclipse magnitude and obscuration are all given at the instant of maximum eclipse at each location. The Jul 02 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 4.
This is the 58th eclipse of Saros Espenak and Meeus, All eclipses in the series occur at the Moon's ascending node and gamma decreases with each member in the family. The series is a mature one that began with a modest partial eclipse on Oct After 20 partial eclipses in the series and more than 3 centuries, the first umbral eclipse occurred on May The event was a 2-minute total eclipse through New England, eastern Canada and Greenland. During the next 2 centuries, the umbral duration continued to increase as each path shifted progressively southward.
The greatest umbral duration of Saros occurred during the total eclipse of Aug Unfortunately, the 5 minute 40 second total eclipse was only visible from equatorial Africa, which was virtually inaccessible to astronomers of the 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. 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.
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. 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.
A full report on eclipses during will be published in Observer's Handbook: It offers a graphically intuitive interface and contains maps, diagrams, tables, and information about every solar and lunar eclipse from BCE to CE. This period includes solar eclipses and lunar eclipses.
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Each map in the atlas covers a year period. The supplemental Five Millennium Catalog of Solar Eclipses contains pages of tables giving details for each eclipse. The Fifty Year Canon of Solar Eclipses contains maps of every solar eclipse from to along with path coordinate tables for all central eclipses. NASA's Solar Eclipse Bulletins were special publications issued periodically that focused on major upcoming solar eclipses. Each bulletin contained detailed eclipse predictions, local circumstances, maps and climatological data along the eclipse path.
The NASA eclipse bulletins ended with the eclipse bulletin. All eclipse calculations are by Fred Espenak, and he assumes full responsibility for their accuracy.
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Some of the information presented on this web site is based on data originally published in:. Permission is freely granted to reproduce this data when accompanied by an acknowledgment:. Website: Robert M. Candey Email: Robert. Candey nasa.
Solar Eclipse Page eclipse. Solar Eclipses: Past and Future The following links give information on all eclipses of the Sun and Moon from through the current year. Decade Solar Eclipse Tables: - - - - - - - - - - Solar Eclipses on Google Maps: - - - - - - - - - - World Atlas of Solar Eclipse Maps: Index Page - - - - - - - - - - North America Solar Eclipse Maps: - Index Page NASA Solar Eclipse Bulletins - NASA Technical Publications for Eclipses from to Solar Eclipses: - The table below lists every solar eclipse from through Click on any of the following values to link to additional information or maps: Calendar Date - link to global map showing eclipse visibility TD of Greatest Eclipse - link to animation of the Moon's penumbral and umbral shadows across Earth Eclipse Type - link to Google Map of eclipse path Saros Series - link to table of all eclipses in this the Saros cycle Central Duration - link to table of geographic coordinates for the path of a total, annular or hybrid eclipse Geographic Region of Eclipse Visibility - link to detailed description of an eclipse from RASC Observer's Handbook The Key to Solar Eclipse Table contains a detailed description of each item in the table.
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America, Iceland Jul 01 Partial 0. America Mar 20 Total 1. America, n S.