قالب:Saros 125 summary
This eclipse is a part of Saros series 125, repeating every 18 years, 11 days, and containing 72 events. The series started with a penumbral lunar eclipse on July 17, 1163. It contains partial eclipses from January 17, 1470 through June 6, 1686; total eclipses from June 17, 1704 through March 19, 2155; and a second set of partial eclipses from March 29, 2173 through June 25, 2317. The series ends at member 72 as a penumbral eclipse on September 9, 2443.
The longest duration of totality was produced by member 37 at 100 minutes, 23 seconds on August 22, 1812. All eclipses in this series occur at the Moon’s descending node of orbit.[1]
| Greatest | First | |||
|---|---|---|---|---|
| The greatest eclipse of the series occurred on 1812 Aug 22, lasting 100 minutes, 23 seconds.[2] | Penumbral | Partial | Total | Central |
| 1163 Jul 17 |
1470 Jan 17 |
1704 Jun 17 |
1758 Jul 20 | |
| Last | ||||
| Central | Total | Partial | Penumbral | |
| 1920 Oct 27 ملف:Lunar eclipse chart close-1920Oct27.png |
2155 Mar 19 |
2317 Jun 25 |
2443 Sep 09 | |
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.
المراجع
- ^ "NASA - Catalog of Lunar Eclipses of Saros 125". eclipse.gsfc.nasa.gov.
- ^ Listing of Eclipses of series 125