The timings of the phases of the eclipse are as follows. You would have been able to see each phase of the eclipse if the Moon was up at the corresponding time as seen from your location; however the penumbral phase would have been very difficult to see in practice:
|Penumbral eclipse began:||16:44:07 UT|
|Partial eclipse began:||18:05:47 UT|
|Maximum eclipse:||18:51:19 UT|
|Partial eclipse ended:||19:36:53 UT|
|Penumbral eclipse ended:||20:58:30 UT|
During this eclipse the Moon was at perigee, making it extremely large. At maximum eclipse it was 0.567° in apparent diameter, which is 6.8% larger 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. The bright area in the middle saw the whole eclipse; the yellow band to the right saw the start of the eclipse, and the blue band to the left saw the end. 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. Hover your mouse over the tags to see what was visible from each area on the map. The green marker in the centre shows where the Moon was 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 51st eclipse in lunar Saros series 118.The surrounding eclipses in this Saros series are:
|UT Date/time (max)||18:51:20 on 7 Sep UT||TDT Date/time (max)||18:52:25 on 7 Sep TDT|
|Saros Series||118||Number in Series||50|
|Penumbral Magnitiude||1.1329||Central Magnitiude||0.1837|
|Gamma||-0.9262||Path Width (km)|
|Delta T||1m05s||Error||± 0m00s (95%)|
|Penumbral Duration||4h14m||Partial Duration||1h31m|
|Sun Distance||150737073 km (75.3%)||Moon Distance||357293 km (1.8%)|
|Sun Diameter||0.529°||Moon Diameter||0.557° - 0.567°|
|Apogee||01:23 on 26 Aug UT||Perigee||03:08 on 8 Sep UT|
|Contact p1||16:44:07 on 7 Sep UT||Contact p2|
|Contact u1||18:05:47 on 7 Sep UT||Contact u2|
|Max eclipse||18:51:19 on 7 Sep UT|
|Contact u3||Contact u4||19:36:53 on 7 Sep UT|
|Contact p3||Contact p4||20:58:30 on 7 Sep 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: 2015-04-05 21:25:26 UTC.