A partial eclipse of the Sun occurred on Monday 19 March, 2007 UT, lasting from 00:38–04:25 UT. This was a deep partial eclipse, with 88% of the Sun covered for viewers closest to the center. This provided a significant spectacle for those who saw it over most of Asia.

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: 00:38:26 UT
Maximum eclipse: 02:31:56 UT
Partial eclipse ended: 04:25:00 UT

During this eclipse the Sun was 0.536° in apparent diameter, 0.5% larger than average. The Moon was at perigee, making it fairly large. At maximum eclipse it was 0.556° in apparent diameter, which is 4.6% larger than average. This has no real effect on this eclipse, since the Moon's central shadow misses the Earth, making this a partial eclipse. The statistics page has information on the ranges of the sizes of the Sun and Moon.

Overview Map

This map sourced from NASA's Eclipse Web Site shows the visibility of the partial solar eclipse. (Click on it for the full-sized version.)

Eclipse Season and Saros Series

This eclipse season contains 2 eclipses:

This was the 20th eclipse in solar Saros series 149.The surrounding eclipses in this Saros series are:

Eclipse Parameters

UT Date/time (max) 02:31:52 on 19 Mar UT TDT Date/time (max) 02:32:57 on 19 Mar TDT
Saros Series 149 Number in Series 19
Penumbral Magnitiude Central Magnitiude 0.8756
Gamma 1.0728 Path Width (km) 0
Delta T 1m05s Error ± 0m00s (95%)
Penumbral Duration Partial Duration
Total Duration
Partial Rating Total Rating
Sun Distance 148918195 km (37.7%) Moon Distance 358253 km (3.7%)
Sun Diameter 0.536° Moon Diameter 0.556° - 0.556°
Apogee 03:38 on 7 Mar UT Perigee 18:39 on 19 Mar UT
Contact p1 00:38:26 on 19 Mar UT Contact p2
Contact u1 Contact u2
Max eclipse 02:31:56 on 19 Mar UT
Contact u3 Contact u4
Contact p3 Contact p4 04:25:00 on 19 Mar 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 listings 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.

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