An annular eclipse of the Sun occurred on Friday 10 May, 2013 UT, lasting from 21:25 on 9 May–03:25 UT. The Sun was 95% covered in a moderate annular eclipse, lasting 6 minutes and 3 seconds and covering a broad path up to 173 km wide. It was visible from northern Australia into the central Pacific. The partial eclipse was visible over Australia and the South Pacific.
The timings of the phases of the overall eclipse
worldwide are as follows. In any particular
place it would have been seen for a significantly shorter
duration as the shadow moved across the Earth:
| Partial eclipse began: |
21:25:10 on 9 May UT |
| Annular eclipse began: |
22:30:34 on 9 May UT |
| Maximum eclipse: |
00:25:13 UT |
| Annular eclipse ended: |
02:19:58 UT |
| Partial eclipse ended: |
03:25:23 UT |
During this eclipse the Sun was 0.528° in apparent
diameter, 0.9% smaller than average. The Moon was just 3 days before apogee, making it fairly small.
At maximum eclipse it was 0.504° in
apparent diameter, which is 5.1% smaller than average; this was not
large enough to cover the Sun, which is why this
was an annular eclipse.
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.
The annular eclipse began in Western Australia, then crossed the Northern Territory and the Cape York Peninsula, Papua New Guinea, and the Solomon Islands. It then passed over some of the islands of Kiribati before finishing in the ocean.
Interactive Map
This map shows the visibility of the eclipse.
The shaded area saw the annular solar eclipse; however, near the edges of
this area, the eclipse was very short. The bold line shows the centre
of the path, where the eclipse lasted longest.
Use the zoom controls to zoom in and out; hover your mouse over any
point on the centreline to see the time and
duration of the eclipse at that point. You can pan and zoom the map to
see detail for any part of the eclipse path.
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)
shows the visibility of the annular solar eclipse. It also shows the broader area in which a partial eclipse was seen. (Click on it for the
full-sized version.)
Eclipse Season and Saros Series
This eclipse season contains 3 eclipses:
This was the 31st eclipse in solar Saros series 138.The surrounding eclipses in this Saros series are:
This Saros series, solar Saros series 138,
is linked to lunar Saros series 131. The
nearest partner eclipses in that series are:
Eclipse Parameters
| UT Date/time (max) | 00:25:12 on 10 May UT |
TDT Date/time (max) | 00:26:20 on 10 May TDT |
| Saros Series | 138 |
Number in Series | 31 |
| Penumbral Magnitiude | |
Central Magnitiude | 0.9544 |
| Gamma | -0.2694 |
Path Width (km) | 173 |
| Delta T | 1m08s |
Error | ± 0m02s (95%) |
| Penumbral Duration | |
Partial Duration | |
| Total Duration | 6m03s |
| |
| Partial Rating | |
Total Rating | |
| Sun Distance | 151057990 km (82.0%) |
Moon Distance | 401063 km (88.8%) |
| Sun Diameter | 0.528° |
Moon Diameter | 0.496° - 0.504° |
| Perigee | 19:48 on 27 Apr UT |
Apogee | 13:32 on 13 May UT |
| Contact p1 | 21:25:10 on 9 May UT |
Contact p2 | |
| Contact u1 | 22:30:34 on 9 May UT |
Contact u2 | 22:34:47 on 9 May UT |
| Max eclipse | 00:25:13 on 10 May UT |
| Contact u3 | 02:15:42 on 10 May UT |
Contact u4 | 02:19:58 on 10 May UT |
| Contact p3 | |
Contact p4 | 03:25:23 on 10 May 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)
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.
