Template:Lunar Saros series 110
This eclipse is a part of Saros series 110, repeating every 18 years, 11 days, and containing 72 events. The series started with a penumbral lunar eclipse on May 28, 747 AD. It contains partial eclipses from August 23, 891 AD through April 18, 1288; total eclipses from April 29, 1306 through September 5, 1522; and a second set of partial eclipses from September 16, 1540 through April 22, 1883. The series ends at member 72 as a penumbral eclipse on July 18, 2027.
The longest duration of totality was produced by member 38 at 103 minutes, 8 seconds on July 3, 1414. All eclipses in this series occur at the Moon’s ascending node of orbit.[1]
| Greatest | First | |||
|---|---|---|---|---|
| The greatest eclipse of the series occurred on 1414 Jul 03, lasting 103 minutes, 8 seconds.[2] | Penumbral | Partial | Total | Central |
| 747 May 28 |
891 Aug 23 |
1306 Apr 29 |
1360 May 31 | |
| Last | ||||
| Central | Total | Partial | Penumbral | |
| 1468 Aug 04 |
1522 Sep 05 |
1883 Apr 22 |
2027 Jul 18
| |
Eclipses are tabulated in three columns; every third eclipse in the same column is one exeligmos apart, so they all cast shadows over approximately the same parts of the Earth.
| Series members 60–72 occur between 1801 and 2027: | |||||
|---|---|---|---|---|---|
| 60 | 61 | 62 | |||
| 1811 Mar 10 | 1829 Mar 20 | 1847 Mar 31 | |||
| 63 | 64 | 65 | |||
| 1865 Apr 11 | 1883 Apr 22 | 1901 May 03 | |||
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| ||||
| 66 | 67 | 68 | |||
| 1919 May 15 | 1937 May 25 | 1955 Jun 05 | |||
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| 69 | 70 | 71 | |||
| 1973 Jun 15 | 1991 Jun 27 | 2009 Jul 07 | |||
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| 72 | |||||
| 2027 Jul 18 | |||||
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References
- ^ "NASA - Catalog of Lunar Eclipses of Saros 110". eclipse.gsfc.nasa.gov.
- ^ Listing of Eclipses of series 110