| Penumbral eclipse | |||||||||
 Hourly movements of the moon through the Earth's southern penumbral shadow | |||||||||
| Date | 8 November 2060 | ||||||||
|---|---|---|---|---|---|---|---|---|---|
| Gamma | 1.5332 [1] | ||||||||
| Magnitude | -0.9375 [2] | ||||||||
| Saros cycle | 156 (1 of 81 [1] ) | ||||||||
| Penumbral | 43 min [2] | ||||||||
| |||||||||
A penumbral lunar eclipse will occur on November 8, 2060. [2] It will be too small to be visually perceptible.
In the unlikely assumption that it is perceptible, it would be visible over North America and South America, and will be seen rising over Africa and Europe.[ citation needed ]
Lunar Saros series 156, has 81 lunar eclipses. Solar Saros 163 interleaves with this lunar saros with an event occurring every 9 years 5 days alternating between each saros series.
This eclipse series will begin in AD 2421 with a partial eclipse at the northern edge of the Earth's shadow. Each successive Saros cycle, the Moon's orbital path is shifted northward with respect to the Earth's shadow, with the first total eclipse occurring in 2565. For the following 469[ citation needed ] years, total eclipses occur, with the first central eclipse being predicted to occur in 2655. The first partial eclipse after this is predicted to occur in the year 3052, and the final partial eclipse of the series will occur in 3142. [3] The total lifetime of the lunar Saros series 131 is 1442.4 years. [4] Solar Saros 138 interleaves with this lunar saros with an event occurring every 9 years 5 days alternating between each saros series.
Because of the ⅓ fraction of days in a Saros cycle, the visibility of each eclipse will differ for an observer at a given fixed locale. Solar Saros 163 interleaves with this lunar saros with an event occurring every 9 years 5 days alternating between each saros series. Lunar Saros series 156, repeating every 18 years and 11 days, has a total of 80 lunar eclipse events including 41 umbral lunar eclipses (14 partial lunar eclipses and 27 total lunar eclipses). Solar Saros 163 interleaves with this lunar saros with an event occurring every 9 years 5 days alternating between each saros series.
| Descending node | Ascending node | |||||
|---|---|---|---|---|---|---|
| 111 | 2056 Jun 27  | penumbral | 116 | 2056 Dec 22  | penumbral | |
| 121 | 2057 Jun 17  | partial | 126 | 2057 Dec 11  | partial | |
| 131 | 2058 Jun 06  | total | 136 | 2058 Nov 30  | total | |
| 141 | 2059 May 27  | partial | 146 | 2059 Nov 19  | partial | |
| 156 | 2060 Nov 08  | penumbral | ||||
This eclipse is the fifth and final of five Metonic cycle lunar eclipses on the same date, November 8–9, each separated by 19 years: The Metonic cycle repeats nearly exactly every 19 years and represents a Saros cycle plus one lunar year. Because it occurs on the same calendar date, the Earth's shadow will be in nearly the same location relative to the background stars.
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A total lunar eclipse occurred on February 20 and February 21, 2008. It was visible in the eastern evening sky on February 20 for all of North and South America, and on February 21 in the predawn western sky from most of Africa and Europe. Greatest Eclipse occurring on Thursday, February 21, 2008, at 03:26:03 UTC, totality lasting 49 minutes and 45.6 seconds.
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A total lunar eclipse took place on Saturday, April 13, 1968, the first of two total eclipses in 1968, the second being on October 6, 1968.
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A total lunar eclipse will take place on September 19, 2043.
A total lunar eclipse will take place on March 13, 2044.
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A total solar eclipse will occur at the Moon's ascending node of orbit on Friday, November 14, 2031, with a magnitude of 1.0106. It is a hybrid event, with portions of its central path near sunrise and sunset as an annular eclipse. 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. A total solar eclipse occurs when the Moon's apparent diameter is larger than the Sun's, blocking all direct sunlight, turning day into darkness. Totality occurs in a narrow path across Earth's surface, with the partial solar eclipse visible over a surrounding region thousands of kilometres wide. Occurring about 3.1 days before perigee, the Moon's apparent diameter will be larger.
A total solar eclipse will occur at the Moon's ascending node of orbit on Thursday, November 25, 2049, with a magnitude of 1.0057. It is a hybrid event, with only a fraction of its path as total, and longer sections at the start and end as an annular eclipse. 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. Occurring about 3.2 days before perigee, the Moon's apparent diameter will be larger.
An annular solar eclipse will occur at the Moon's descending node of orbit on Sunday, October 24, 2060, with a magnitude of 0.9277. 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. Occurring about 18 hours before apogee, the Moon's apparent diameter will be smaller.
An annular solar eclipse will occur at the Moon's descending node of orbit on Saturday, June 11, 2067, with a magnitude of 0.967. 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. Occurring about 4.3 days before apogee, the Moon's apparent diameter will be smaller.
An annular solar eclipse will occur at the Moon's descending node of orbit on Friday, November 4, 2078, with a magnitude of 0.9255. 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. Occurring about 22 hours before apogee, the Moon's apparent diameter will be smaller.
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