A partial eclipse of the Sun occurred on Thursday 14 October, 2004 UT, lasting from 00:54–05:04 UT. This was a deep partial eclipse, with 93% of the Sun covered for viewers closest to the center. This provided a significant spectacle for those who saw it in eastern Russia, Japan and north-east China.
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: | 00:54:38 UT |
Maximum eclipse: | 02:59:20 UT |
Partial eclipse ended: | 05:04:20 UT |
During this eclipse the Sun was 0.535° in apparent diameter, 0.3% larger than average. The Moon was just 4 days before perigee, making it relatively large. At maximum eclipse it was 0.531° in apparent diameter, which is around 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, and the Moon data page displays detailed information on the Moon's key dates.
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)
https://eclipse.gsfc.nasa.gov/eclipse.html shows the visibility of the partial solar eclipse. (Click on it for the
full-sized version.)
This eclipse season contains 2 eclipses:
This was the 54th eclipse in solar Saros series 124.The surrounding eclipses in this Saros series are:
This Saros series, solar Saros series 124, is linked to lunar Saros series 117. The nearest partner eclipses in that series are:
UT Date/time (max) | 02:59:18 on 14 Oct UT | TDT Date/time (max) | 03:00:23 on 14 Oct TDT |
---|---|---|---|
Saros Series | 124 | Number in Series | 54 |
Penumbral Magnitiude | Central Magnitiude | 0.9282 | |
Gamma | 1.0348 | Path Width (km) | 0 |
Delta T | 1m05s | Error | ± 0m00s (95%) |
Penumbral Duration | Partial Duration | ||
Total Duration | |||
Partial Rating | Total Rating | ||
Sun Distance | 149205321 km (43.6%) | Moon Distance | 375221 km (37.4%) |
Sun Diameter | 0.535° | Moon Diameter | 0.531° - 0.531° |
Apogee | 22:11 on 5 Oct UT | Perigee | 00:04 on 18 Oct UT |
Contact p1 | 00:54:38 on 14 Oct UT | Contact p2 | |
Contact u1 | Contact u2 | ||
Max eclipse | 02:59:20 on 14 Oct UT | ||
Contact u3 | Contact u4 | ||
Contact p3 | Contact p4 | 05:04:20 on 14 Oct 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)
https://eclipse.gsfc.nasa.gov/eclipse.html 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.