The timings of the phases of the eclipse are as follows. You will be able to see each phase of the eclipse if the Moon is up at the corresponding time as seen from your location; however the penumbral phase will be very difficult to see in practice, so you may want to start watching at the partial phase:
|Penumbral eclipse begins:||08:18:44 UT|
|Partial eclipse begins:||09:13:50 UT|
|Total eclipse begins:||10:15:38 UT|
|Maximum eclipse:||10:55:02 UT|
|Total eclipse ends:||11:34:27 UT|
|Partial eclipse ends:||12:36:15 UT|
|Penumbral eclipse ends:||13:31:21 UT|
During this eclipse the Moon will be at perigee, making it extremely large. At maximum eclipse it will be 0.568° in apparent diameter, which is 6.9% 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 at various stages. The bright area in the middle will see the whole eclipse; the coloured bands to the right will see the start of the eclipse, and those on the left will see the end. Note that the map is approximate, and if you are near the edge of the area of visibility, the moon will be very close to the horizon and may not be 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 will be visible from each area on the map. 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 is the 27th eclipse in lunar Saros series 137.The surrounding eclipses in this Saros series are:
|UT Date/time (max)||10:55:03 on 8 Oct UT||TDT Date/time (max)||10:56:23 on 8 Oct TDT|
|Saros Series||137||Number in Series||26|
|Penumbral Magnitiude||2.3057||Central Magnitiude||1.3497|
|Gamma||-0.2889||Path Width (km)|
|Delta T||1m20s||Error||± 0m14s (95%)|
|Penumbral Duration||5h13m||Partial Duration||3h22m|
|Partial Rating||Total Rating|
|Sun Distance||149468517 km (49.1%)||Moon Distance||356827 km (0.8%)|
|Sun Diameter||0.534°||Moon Diameter||0.558° - 0.568°|
|Apogee||01:34 on 25 Sep UT||Perigee||12:12 on 8 Oct UT|
|Contact p1||08:18:44 on 8 Oct UT||Contact p2|
|Contact u1||09:13:50 on 8 Oct UT||Contact u2||10:15:38 on 8 Oct UT|
|Max eclipse||10:55:02 on 8 Oct UT|
|Contact u3||11:34:27 on 8 Oct UT||Contact u4||12:36:15 on 8 Oct UT|
|Contact p3||Contact p4||13:31:21 on 8 Oct 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.