Visibility
It was completely visible over eastern Asia, New Zealand, northwestern North America, seen rising over Asia and Australia and setting over North America and western South America.
| Total eclipse | |||||||||||||||||
| Date | 30 January 1972 | ||||||||||||||||
|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
| Gamma | −0.42729 | ||||||||||||||||
| Magnitude | 1.04971 | ||||||||||||||||
| Saros cycle | 133 (24 of 71) | ||||||||||||||||
| Totality | 34 minutes, 47.7 seconds | ||||||||||||||||
| Partiality | 203 minutes, 24.7 seconds | ||||||||||||||||
| Penumbral | 340 minutes, 25.4 seconds | ||||||||||||||||
| |||||||||||||||||
A total lunar eclipse took place on Sunday, January 30, 1972, the first of two lunar eclipses in 1972. The moon entered the Earth's penumbral shadow at 30 January 1972 08:03:12.5 UTC and exited at 30 January 1972 13:43:37.9 UTC. The moon entered the Earth's umbral shadow at 30 January 1972 09:11:38.4 UTC and exited at 30 January 1972 12:35:03.1 UTC. Totality lasted 34 minutes, 47.7 seconds (34.795 min), between 10:35:57.4 UTC and 11:10:45.1 UTC. The moon was 6.6 days before apogee (Apogee on Sunday, February 6, 1972), making it 1.6% smaller than average, only 0.2% larger than the July 1972's lunar eclipse. [1]
It was completely visible over eastern Asia, New Zealand, northwestern North America, seen rising over Asia and Australia and setting over North America and western South America.
| Lunar eclipse series sets from 1969–1973 | ||||||||
|---|---|---|---|---|---|---|---|---|
| Ascending node | Descending node | |||||||
| Saros | Date Viewing | Type Chart | Gamma | Saros | Date Viewing | Type Chart | Gamma | |
| 108 | 1969 Aug 27  | Penumbral | −1.54066 | 113 | 1970 Feb 21  | Partial | 0.96198 | |
| 118 | 1970 Aug 17  | Partial | −0.80534 | 123 | 1971 Feb 10  | Total | 0.27413 | |
| 128 | 1971 Aug 06  | Total | −0.07944 | 133 | 1972 Jan 30  | Total | −0.42729 | |
| 138 | 1972 Jul 26  | Partial | 0.71167 | 143 | 1973 Jan 18  | Penumbral | −1.08446 | |
| 148 | 1973 Jul 15  | Penumbral | 1.51782 | |||||
| Last set | 1969 Sep 25 | Last set | 1969 Apr 02 | |||||
| Next set | 1973 Jun 15 | Next set | 1973 Dec 10 | |||||
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 140.
| January 25, 1963 | February 4, 1981 |
|---|---|
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A penumbral lunar eclipse will occur at the Moon’s descending node of orbit on Friday, August 29, 2053, with an umbral magnitude of −0.0319. It will be a relatively rare total penumbral lunar eclipse, with the Moon passing entirely within the penumbral shadow without entering the darker umbral shadow. A lunar eclipse occurs when the Moon moves into the Earth's shadow, causing the Moon to be darkened. A penumbral lunar eclipse occurs when part or all of the Moon's near side passes into the Earth's penumbra. Unlike a solar eclipse, which can only be viewed from a relatively small area of the world, a lunar eclipse may be viewed from anywhere on the night side of Earth. Occurring about 4.7 days after apogee, the Moon's apparent diameter will be smaller.
