Total Lunar Eclipse December 19, 1964 | |
---|---|
(No photo) | |
The moon passes west to east (right to left) across the Earth's umbral shadow, shown in hourly intervals. | |
Series | 134 (24 of 73) |
Duration (hr:mn:sc) | |
Totality | |
Partial | |
Penumbral | |
Contacts | |
P1 | UTC |
U1 | |
U2 | |
Greatest | |
U3 | |
U4 | |
P4 |
A total lunar eclipse took place on Saturday, December 19, 1964. A shallow total eclipse saw the Moon in relative darkness for 58 minutes and 54 seconds. The Moon was 17% of its diameter into the Earth's umbral shadow, and should have been significantly darkened. The partial eclipse lasted for 3 hours and 16 minutes in total.[1] The eclipse afforded astrophysicist J. M. Saari the opportunity to make infrared pyrometric scans of the lunar surface with improved equipment, following up on Richard W. Shorthill's discovery of "hot spots" in the Tycho crater during the March 13, 1960 eclipse. [2]
Visibility
editRelated lunar eclipses
editLunar year series
editDescending node | Ascending node | |||||||
---|---|---|---|---|---|---|---|---|
Saros | Date Viewing |
Type Chart |
Gamma | Saros | Date Viewing |
Type Chart |
Gamma | |
109 | 1962 Jul 17 |
Penumbral |
1.33712 | 114 | 1963 Jan 09 |
Penumbral |
-1.01282 | |
119 | 1963 Jul 06 |
Partial |
0.61972 | 124 | 1963 Dec 30 |
Total |
-0.28889 | |
129 | 1964 Jun 25 |
Total |
-0.14611 | 134 | 1964 Dec 19 |
Total |
0.38008 | |
139 | 1965 Jun 14 |
Partial |
-0.90055 | 144 | 1965 Dec 08 |
Penumbral |
1.07748 | |
Last set | 1962 Aug 15 | Last set | 1962 Feb 19 | |||||
Next set | 1966 May 04 | Next set | 1966 Oct 29 |
See also
editNotes
edit- ^ Hermit Eclipse: Saros cycle 134
- ^ F. Link, Eclipse Phenomena in Astronomy (Springer, 2012) p119
External links
edit- 1964 Dec 19 chart Eclipse Predictions by Fred Espenak, NASA/GSFC