Visibility
| Total eclipse | |||||||||||||||||
| Date | 6 September 1979 | ||||||||||||||||
|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
| Gamma | −0.43050 | ||||||||||||||||
| Magnitude | 1.09358 | ||||||||||||||||
| Saros cycle | 137 (25 of 80) | ||||||||||||||||
| Totality | 44 minutes, 24.7 seconds | ||||||||||||||||
| Partiality | 191 minutes, 54.2 seconds | ||||||||||||||||
| Penumbral | 305 minutes, 15.4 seconds | ||||||||||||||||
| |||||||||||||||||
A total lunar eclipse took place on Thursday, September 6, 1979, the second of two lunar eclipses in 1979. A shallow total eclipse saw the Moon in relative darkness for 44 minutes and 24.7 seconds. The Moon was 9.358% of its diameter into the Earth's umbral shadow, and should have been significantly darkened. The partial eclipse lasted for 3 hours, 11 minutes and 54.1 seconds in total. [1]
This event followed the annular solar eclipse of August 22, 1979.
| Lunar eclipse series sets from 1977–1980 | ||||||||
|---|---|---|---|---|---|---|---|---|
| Ascending node | Descending node | |||||||
| Saros | Date Viewing | Type Chart | Gamma | Saros | Date Viewing | Type Chart | Gamma | |
| 112 | 1977 Apr 04  | Partial | −0.91483 | 117 | 1977 Sep 27  | Penumbral | 1.07682 | |
| 122 | 1978 Mar 24  | Total | −0.21402 | 127 | 1978 Sep 16  | Total | 0.29510 | |
| 132 | 1979 Mar 13  | Partial | 0.52537 | 137 | 1979 Sep 06  | Total | −0.43050 | |
| 142 | 1980 Mar 01  | Penumbral | 1.22701 | 147 | 1980 Aug 26  | Penumbral | −1.16082 | |
| Last set | 1976 May 13 | Last set | 1976 Nov 06 | |||||
| Next set | 1981 Jan 20 | Next set | 1980 Jul 27 | |||||
It is part of Saros series 137.
A lunar eclipse will be preceded and followed by solar eclipses by 9 years and 5.5 days (a half saros). [2] This lunar eclipse is related to two annular solar eclipses of Solar Saros 144.
| August 31, 1970 | September 11, 1988 |
|---|---|
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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.
