A penumbral lunar eclipse took place on Monday, October 27, 1958. [1]
A penumbral lunar eclipse took place on Monday, October 27, 1958. [1]
| Ascending node | Descending node | |||||
|---|---|---|---|---|---|---|
| Saros | Date Viewing | Type Chart | Saros | Date Viewing | Type Chart | |
| 110 | 1955 Jun 5  | Penumbral | 115 | 1955 Nov 29  | Partial | |
| 120 | 1956 May 24  | Partial | 125 | 1956 Nov 18  | Total | |
| 130 | 1957 May 13  | Total | 135 | 1957 Nov 7  | Total | |
| 140 | 1958 May 3  | Partial | 145 | 1958 Oct 27  | Penumbral | |
| Last set | 1954 Jul 16 | Last set | 1955 Jan 8 | |||
| Next set | 1958 Apr 4 | Next set | 1959 Sep 17 | |||
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 solar eclipses of Solar Saros 152.
| October 21, 1949 | November 2, 1967 |
|---|---|
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A partial lunar eclipse took place on Thursday, May 13, 1976, the first of two lunar eclipses in 1976, the second being a penumbral lunar eclipse on November 6, 1976. At maximum eclipse, a small bite out of the Moon should have been visible. The eclipse lasted for 1 hour, 15 minutes and 23.8 seconds, with just 12.17% of the Moon in shadow at maximum. Occurring only 1.1 days after perigee, the Moon's apparent diameter 5.4% larger than average.
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A partial lunar eclipse took place on Monday, June 14, 1965. At maximum eclipse, a small bite out of the Moon should have been visible. The eclipse lasted for 1 hour and 40 minutes, with just 18% of the Moon in shadow at maximum.
A total lunar eclipse took place on Thursday, November 7, 1957. The Moon barely edged into total eclipse for 27 minutes and 54 seconds. With the Moon just 3.5% of its diameter into the Earth's umbral shadow, the Moon may have been quite bright, but even so, this should have been worth seeing. The partial eclipse lasted for 3 hours and 27 minutes in total.
A partial lunar eclipse took place on Saturday, May 3, 1958. This was the first partial lunar eclipse of Saros cycle 140. While technically a partial eclipse, the Moon barely clipped the Earth's umbral shadow, which may have been very difficult to observe in practice; though a shading across the moon from the Earth's penumbral shadow should have been visible at maximum eclipse. The partial eclipse lasted for 21 minutes exactly. 0.919% of the Moon was in umbral shadow on Saturday, 3 May 1958.
