A total eclipse of the Moon occurred on Saturday 13 April, 1968 UT, with maximum eclipse at 04:47 UT. A shallow total eclipse saw the Moon in relative darkness for 48 minutes and 30 seconds. The Moon was 11% of its diameter into the Earth's umbral shadow, and should have been significantly darkened. The partial eclipse lasted for 3 hours and 14 minutes in total.

The penumbral eclipse lasted for 5 hours and 10 minutes. The partial eclipse lasted for 3 hours and 14 minutes. The total eclipse lasted for 48 minutes and 30 seconds. Maximum eclipse was at 04:47:22 UT.

During this eclipse the Moon was just a day before perigee, making it very large. At maximum eclipse it was 0.563° in apparent diameter, which is 6.0% larger than average. The statistics page has information on the ranges of the sizes of the Sun and Moon, and the Moon data page displays detailed information on the Moon's key dates.

Interactive Map

This map shows the visibility of the eclipse at maximum eclipse, when it was visible within the bright area on the map. Note that the map is approximate, and if you were near the edge of the area of visibility, the moon was very close to the horizon and may not have been practically visible.

You can use the zoom controls to zoom in and out, and pan to see areas of interest. The green marker in the centre shows where the Moon will be directly overhead at maximum eclipse.

The interactive map is currently not available.

Overview Map

This map sourced from NASA Goddard Space flight Center: GSFC Eclipse Web SiteGSFC Eclipse Web Site
The primary source of all the information on eclipses presented here at Hermit Eclipse. (NASA Goddard Space flight Center)
https://eclipse.gsfc.nasa.gov/eclipse.html
shows the visibility of the eclipse. (Click on it for the full-sized version.)

Eclipse Season and Saros Series

This eclipse season contains 2 eclipses:

This was the 31st eclipse in lunar Saros series 131.The surrounding eclipses in this Saros series are:

This Saros series, lunar Saros series 131, is linked to solar Saros series 138. The nearest partner eclipses in that series are:

Eclipse Parameters

UT Date/time (max) 04:47:22 on 13 Apr UT TDT Date/time (max) 04:48:01 on 13 Apr TDT
Saros Series 131 Number in Series 31
Penumbral Magnitiude 2.0725 Central Magnitiude 1.1116
Gamma -0.4173 Path Width (km)
Delta T 0m39s Error ± 0m00s (95%)
Penumbral Duration 5h10m Partial Duration 3h14m
Total Duration 48m30s
Partial Rating Total Rating
Sun Distance 150030239 km (60.7%) Moon Distance 359993 km (7.1%)
Sun Diameter 0.532° Moon Diameter 0.553° - 0.563°
Apogee 23:29 on 1 Apr UT Perigee 06:49 on 14 Apr UT

Note that while all dates and times on this site (except where noted) are in UT, which is within a second of civil time, the dates and times shown in NASA's eclipse listingsGSFC Eclipse Web Site
The primary source of all the information on eclipses presented here at Hermit Eclipse. (NASA Goddard Space flight Center)
https://eclipse.gsfc.nasa.gov/eclipse.html
are in the TDT timescale.

The Sun and Moon distances are shown in km, and as a percentage of their minimum - maximum distances; hence 0% is the closest possible (Earth's perihelion, or the Moon's closest possible perigee) and 100% is the farthest (aphelion, the farthest apogee). The statistics page has information on the ranges of sizes of the Sun and Moon, and the Moon data page displays detailed information on the Moon's key dates.

Data last updated: 2015-06-21 22:11:46 UTC.