align=center bgcolor=#e7dcc3 colspan=2 | Total Lunar Eclipse of 13 August 1859[1] | ||
---|---|---|---|
Gamma | 0.0038 | ||
Magnitude | 1.8148 | ||
Series (and member) | 126 (36 of 70) | ||
align=center bgcolor=#c0b0e0 colspan=2 | Duration (hr:mn:sc) | ||
align=center bgcolor=#b0a0e0 | Totality | 1:46:28 | |
align=center bgcolor=#c0a0e0 | Partial | 3:56:00 | |
align=center bgcolor=#d0d0e0 | Penumbral | 6:15:01 | |
align=center bgcolor=#a0d0e0 colspan=2 | Contacts (UTC) | ||
align=center bgcolor=#d0d0e0 | P1 | 13:26:47 | |
align=center bgcolor=#c0a0e0 | U1 | 14:36:18 | |
align=center bgcolor=#b0a0e0 | U2 | 15:41:04 | |
align=center bgcolor=#a0a0e0 | Greatest | 16:34:18 | |
align=center bgcolor=#b0a0e0 | U3 | 17:27:32 | |
align=center bgcolor=#c0a0e0 | U4 | 18:32:19 | |
align=center bgcolor=#d0d0e0 | P4 | 19:41:48 |
The eclipse was visible in Asia, Europe, Australia/Oceania, Africa, and most of Alaska.
Lunar Saros 126, which repeats every 18 years and 11 days, contains 70 member events. In Lunar Saros 126, there are 14 total eclipses. The first total eclipse in this series was on June 19, 1769, and the last one was on November 9, 2003. The longest totality in this series was on August 13, 1859 when totality was 106 minutes and 28 seconds.[3] [4]
First eclipse | |||
---|---|---|---|
Penumbral | Partial | Total | |
18 July 1228 | 24 March 1625 | 19 June 1769 | |
Last eclipse | |||
Penumbral | Partial | Total | |
19 August 2472 | 5 June 2346 | 9 November 2003 |