The letters L Lunar and S Solar are included with the Saros numbers to help distinguish the series that the eclipse belongs with. The Nodal Family is directly linked with the Saros Series. The North and South represent the node that the eclipse series originates from. The crescent is actually the Sun being eclipsed by the Moon during a solar eclipse, while the pinkish round circle is the Full Moon during a total lunar eclipse.
To adjust the times for your timezone, add or subtract the number of hours your timezone is from 0 UT. July 2, : Total solar eclipse July 16, : Partial lunar eclipse. December 26, : Annular solar eclipse January 10, : Penumbral lunar eclipse. On a worldwide scale, a solar eclipse always comes within one fortnight approximately two weeks of lunar eclipse.
The first solar eclipse of happens during the daylight hours on January 5 or 6 — depending on your location — when the new moon takes a bite out of the solar disk.
This total lunar eclipse will be visible from North and South America, plus much of Europe and Africa. One semester six lunar months or six new moons after the January , , partial solar eclipse, a total eclipse of the sun will take place on July 2, Then the partial lunar eclipse on July 16, , will happen one semester six lunar months or six full moons after the January total lunar eclipse.
Yesterday's Solar Eclipse Was First of Six Eclipses In 12222 With 'Super Wolf Blood Moon' Up Next
Fortnight approximate two-week separation between solar and lunar eclipses. A solar eclipse always takes place within one fortnight of any lunar eclipse. This year, we have a pair of eclipses one solar and one lunar in January and then in July We also have an annular solar eclipse on December 26, , followed by the penumbral lunar eclipse of January 10, 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. 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.
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.
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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.
NASA - Lunar Eclipse Page
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.
terbzabrialeli.cf 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.
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