The timings of the eclipse are as follows. You would have been able to see the eclipse if the Moon was up as seen from your location; but note that this penumbral eclipse would have been very difficult to see in practice:
|Penumbral eclipse began:||12:14:59 UT|
|Maximum eclipse:||14:32:59 UT|
|Penumbral eclipse ended:||16:50:59 UT|
During this eclipse the Moon was at apogee, making it very small. At maximum eclipse it was 0.498° in apparent diameter, which is 6.3% smaller than average. The statistics page has information on the ranges of the sizes of the Sun and Moon.
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.
This map sourced from NASA's Eclipse Web Site shows the visibility of the eclipse. (Click on it for the full-sized version.)
This eclipse season contains 2 eclipses:
This was the 11th eclipse in lunar Saros series 145.The surrounding eclipses in this Saros series are:
|UT Date/time (max)||14:32:59 on 28 Nov UT||TDT Date/time (max)||14:34:07 on 28 Nov TDT|
|Saros Series||145||Number in Series||10|
|Penumbral Magnitiude||0.9155||Central Magnitiude||-0.1873|
|Gamma||-1.0869||Path Width (km)|
|Delta T||1m08s||Error||± 0m01s (95%)|
|Penumbral Duration||4h36m||Partial Duration|
|Partial Rating||Total Rating|
|Sun Distance||147565394 km (9.7%)||Moon Distance||406347 km (99.3%)|
|Sun Diameter||0.540°||Moon Diameter||0.490° - 0.498°|
|Perigee||10:22 on 14 Nov UT||Apogee||19:35 on 28 Nov UT|
|Contact p1||12:14:59 on 28 Nov UT||Contact p2|
|Contact u1||Contact u2|
|Max eclipse||14:32:59 on 28 Nov UT|
|Contact u3||Contact u4|
|Contact p3||Contact p4||16:50:59 on 28 Nov UT|
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.
Data last updated: 2015-06-21 22:11:46 UTC.