Saros cycle series 112 for lunar eclipses occurs at the moon's ascending node, 18 years 11 and 1/3 days. It contains 72 events, with 15 total eclipses, starting in 1364 and ending in 1616. Solar Saros 119 interleaves with this lunar Saros with an event occurring every 9 years 5 days alternating between each saros series. [1]
This lunar saros is linked to Solar Saros 119.
The series contains 15 total lunar eclipses between 1364 and 1616. It contains twenty-one partial eclipses from 985 AD to 1346 and twenty-two more between 1634 and 2013.
The last occurrence of this series was a partial lunar eclipse on April 25, 2013, which was the last partial lunar eclipse of this series. The next occurrence on May 7, 2031, will be the first of the final set of penumbral lunar eclipses.
The series started on May 20, 859 AD.
The series will end on July 12, 2139.
Summary
Lunar Saros series 112, repeating every 18 years and 11 days, has a total of 72 lunar eclipse events including 15 total lunar eclipses.
First Penumbral Lunar Eclipse: 859 May 20
First Partial Lunar Eclipse: 985 Aug 03
First Total Lunar Eclipse: 1364 Mar 18
First Central Lunar Eclipse: 1436 Apr 30
Greatest Eclipse of the Lunar Saros 112: 1490 Jun 02
Last Central Lunar Eclipse: 1562 Jul 16
Last Total Lunar Eclipse: 1616 Aug 27
Last Partial Lunar Eclipse: 2013 Apr 25
Last Penumbral Lunar Eclipse: 2139 Jul 12
The greatest eclipse of the series occurred on 1490 Jun 02, lasting 100 minutes.
A partial lunar eclipse took place on 5 July 2001, the second of three lunar eclipses in 2001.
A partial lunar eclipse took place on April 25, 2013, the first of three lunar eclipses in 2013. Only a tiny sliver of the Moon was covered by the Earth's umbral shadow at maximum eclipse, but the entire northern half of the Moon was darkened from being inside the penumbral shadow. This was one of the shortest partial eclipses of the Moon for the 21st century, lasting 27 minutes. This was the last of 58 umbral lunar eclipses of Lunar Saros 112.
A penumbral lunar eclipse took place on January 31, 1999, the first of two lunar eclipses in 1999.
A penumbral lunar eclipse took place at the Moon’s ascending node on February 11, 2017, the first of two lunar eclipses in 2017. It was not quite a total penumbral lunar eclipse. It occurred the same day as comet 45P/Honda–Mrkos–Pajdušáková made a close approach to Earth. It also occurred on the Lantern Festival, the first since February 9, 2009.
A partial lunar eclipse took place on Saturday, April 15, 1995, the first of two lunar eclipses in 1995, the second being with a penumbral lunar eclipse on Sunday, October 8.
A total lunar eclipse took place on October 28, 1985, the second of two total lunar eclipses in 1985, the first being on May 4, 1985.
A penumbral lunar eclipse took place on January 20, 1981. In a rare total penumbral eclipse, the entire Moon was partially shaded by the Earth, and the shading across the Moon should have been quite visible at maximum eclipse. The penumbral phase lasted for 4 hours and 24 minutes in all, though for most of it, the eclipse was extremely difficult or impossible to see.
A partial lunar eclipse occurred on the 16 and 17 July 2019. The Moon was covered about 65% by the Earth's umbral shadow at maximum eclipse.
A partial lunar eclipse will take place on Friday, 19 November 2021.
A partial lunar eclipse took place on April 4, 1977.
A penumbral lunar eclipse will take place on May 7, 2031.
A partial lunar eclipse will take place on November 30, 2039.
A partial lunar eclipse took place on March 24, 1959.
A penumbral lunar eclipse will take place on May 17, 2049.
An annular solar eclipse took place on May 9–10 (UTC), 2013, with a magnitude of 0.9544. A solar eclipse occurs when the Moon passes between Earth and the Sun, thereby totally or partly obscuring the image of the Sun for a viewer on Earth. An annular solar eclipse occurs when the Moon's apparent diameter is smaller than the Sun's, blocking most of the Sun's light and causing the Sun to look like an annulus (ring). An annular eclipse appears as a partial eclipse over a region of the Earth thousands of kilometres wide.
An annular solar eclipse occurred on June 10, 2002. A solar eclipse occurs when the Moon passes between Earth and the Sun, thereby totally or partly obscuring the image of the Sun for a viewer on Earth. An annular solar eclipse occurs when the Moon's apparent diameter is smaller than the Sun's, blocking most of the Sun's light and causing the Sun to look like an annulus (ring). An annular eclipse appears as a partial eclipse over a region of the Earth thousands of kilometres wide. Annularity was visible in Indonesia, Palau, Northern Mariana on June 11th (Tuesday), and the western tip of Jalisco, Mexico on June 10th (Monday).
An annular solar eclipse will occur on Friday, November 4, 2078. A solar eclipse occurs when the Moon passes between Earth and the Sun, thereby totally or partly obscuring the image of the Sun for a viewer on Earth. An annular solar eclipse occurs when the Moon's apparent diameter is smaller than the Sun's, blocking most of the Sun's light and causing the Sun to look like an annulus (ring). An annular eclipse appears as a partial eclipse over a region of the Earth thousands of kilometres wide. The path of annularity will cross Pacific Ocean, South America, and Atlantic Ocean. The tables below contain detailed predictions and additional information on the Annular Solar Eclipse of 4 November 2078.
Saros cycle series 114 for lunar eclipses occurs at the moon's ascending node, 18 years 11 and 1/3 days. It contains 71 member events, with 13 total eclipses, starting in 1458 and ending in 1674. Solar saros 121 interleaves with this lunar saros with an event occurring every 9 years 5 days alternating between each saros series.
Saros cycle series 126 for lunar eclipses occurs at the moon's ascending node, 18 years 11 and 1/3 days. It contains 70 member events, with 14 total eclipses, starting in 1769 and ending in 2003.
A partial lunar eclipse took place on March 13, 1941.
