Key to Solar Eclipse Figure (below)
ThePartial Solar Eclipse of 2025 Sep 21 is visible from the following geographic regions:
The map to the right depicts the geographic regions of eclipse visibility. Click on the map to enlarge it. For an explanation of the features appearing in the map, seeKey to Solar Eclipse Maps.
The instant ofgreatest eclipse takes place on 2025 Sep 21 at 19:43:04 TD (19:41:52 UT1). This is 4.6 days before the Moon reaches apogee. During the eclipse, the Sun is in the constellationVirgo. Thesynodic month in which the eclipse takes place has aBrown Lunation Number of 1271.
The eclipse belongs toSaros 154 and is number 7 of 71 eclipses in the series.All eclipses in this series occur at the Moonsdescending node.The Moon moves northward with respect to the node with each succeeding eclipse in the series andgamma increases.
This is a very deep partial eclipse. It has aneclipse magnitude of 0.8550, whileGamma has a value of -1.0651.
The partial solar eclipse of 2025 Sep 21 is preceded two weeks earlier by a total lunar eclipse on 2025 Sep 07.
These eclipses all take place during a singleeclipse season.
The eclipse predictions are given in bothTerrestrial Dynamical Time (TD) andUniversal Time (UT1).The parameterΔT is used to convert between these two times (i.e.,UT1 = TD - ΔT).ΔT has a value of 72.1 seconds for this eclipse.
The following links provide maps and data for the eclipse.
Michael ZeilerGreatAmericanEclipse.com and
Fred EspenakEclipseWise.com have created a series of eclipse animations - one for every solar eclipse during the 21st Century.
The animation of thePartial Solar Eclipse of 2025 Sep 21 shows the path of the Moon's penumbral shadow as it sweeps across a global map of Earth (an orthographic projection).The vantage point of the animation is as seen from the Moon. The daylight hemisphere of Earth then faces the Moon and the lunar shadows appear perfectly circular with no distorted projection effects as they race across Earth.
The Moon's large penumbral shadow is lightly shaded and is outlined with a solid black edge. A partial eclipse is visible from within the penumbra.
The map to the right shows a single frame from the medium size animation for thePartial Solar Eclipse of 2025 Sep 21.In the upper left corner is the type of eclipse and the eclipse date. To the upper right is the Universal Time. The lower left corner is not used for partial solar eclipses.To the lower right is the credit for the animation.
Animations for thePartial Solar Eclipse of 2025 Sep 21 are available in three sizes/resolutions: small, medium, and large. They can be viewed through the following links:

These animations may be freely used and shared through Creative Commons.
You may use and distribute these eclipse animations as long as they are not modified and you include an attribution.
Solar Eclipse Global Animation byFred Espenak and Michael Zeiler is licensed under aCreative Commons Attribution-NoDerivatives 4.0 International License. Based on work atEclipseWise.com andGreatAmericanEclipse.com
Attribution:"Global Map Animation of Eclipse courtesy of Michael Zeiler (GreatAmericanEclipse.com) and Fred Espenak (EclipseWise.com)".
| Eclipse Characteristics | |
| Parameter | Value |
| Eclipse Magnitude | 0.85504 |
| Eclipse Obscuration | 0.79691 |
| Gamma | -1.06509 |
| Conjunction Times | ||
| Event | Calendar Date and Time | Julian Date |
| Greatest Eclipse | 2025 Sep 21 at 19:43:04.2 TD (19:41:52.2 UT1) | 2460940.320743 |
| Ecliptic Conjunction | 2025 Sep 21 at 19:55:17.4 TD (19:54:05.4 UT1) | 2460940.329229 |
| Equatorial Conjunction | 2025 Sep 21 at 20:51:38.8 TD (20:50:26.8 UT1) | 2460940.368365 |
| Geocentric Coordinates of Sun and Moon | ||
| 2025 Sep 21 at 19:43:04.2 TD (19:41:52.2 UT1) | ||
| Coordinate | Sun | Moon |
| Right Ascension | 11h56m36.9s | 11h54m42.8s |
| Declination | +00°22'00.7" | -00°29'14.7" |
| Semi-Diameter | 15'55.9" | 15'02.8" |
| Eq. Hor. Parallax | 08.8" | 0°55'13.2" |
| Geocentric Libration of Moon | |
| Angle | Value |
| l | 4.2° |
| b | 1.3° |
| c | 21.9° |
| Prediction Parameters | |
| Paramater | Value |
| Ephemerides | JPL DE405 |
| ΔT | 72.1 s |
| k (penumbra) | 0.2725076 |
| k (umbra) | 0.2722810 |
| Saros Series | 154 ( 7/71) |
| Contacts of Penumbral Shadow with Earth | |||||
| Contact Event | Contact | Time TD | Time UT1 | Latitude | Longitude |
| First External Contact | P1 | 17:30:51.3 | 17:29:39.3 | 13°58.3'S | 174°04.9'W |
| Last External Contact | P4 | 21:54:55.1 | 21:53:43.0 | 72°16.0'S | 061°16.0'W |
| Extreme Northern and Southern Path Limits of Penumbra | |||||
| Contact Event | Contact | Time TD | Time UT1 | Latitude | Longitude |
| North Extreme Path Limit 1 | N1 | 18:03:05.9 | 18:01:53.8 | 01°05.3'S | 177°49.5'E |
| South Extreme Path Limit 1 | S1 | 21:22:43.0 | 21:21:30.9 | 59°30.1'S | 052°44.9'W |
Explanation of Penumbral Shadow Contacts and Extremes Tables
| Polynomial Besselian Elements | ||||||
| 2025 Sep 21 at 20:00:00.0 TD (=t0) | ||||||
| n | x | y | d | l1 | l2 | μ |
| 0 | -0.39007 | -1.00183 | 0.3647 | 0.56251 | 0.01627 | 121.7819 |
| 1 | 0.45316 | -0.25216 | -0.0156 | 0.00009 | 0.00009 | 15.0048 |
| 2 | 0.00000 | 0.00005 | -0.0000 | -0.00001 | -0.00001 | -0.0000 |
| 3 | -0.00001 | 0.00000 | - | - | - | - |
| Tan ƒ1 | 0.0046583 |
| Tan ƒ2 | 0.0046351 |
At time t1 (decimal hours), each besselian element is evaluated by:
x = x0 + x1*t + x2*t2 + x3*t3 (or x = Σ [xn*tn]; n = 0 to 3)
where: t = t1 - t0 (decimal hours) and t0 = 20.000
•Decade Tables of Solar Eclipses:
|1901 - 1910 |1911 - 1919 |1921 - 1930 |1931 - 1940 |1941 - 1950 |
|1951 - 1960 |1961 - 1970 |1971 - 1980 |1981 - 1990 |1991 - 2000 |
|2001 - 2010 |2011 - 2020 |2021 - 2030 |2031 - 2040 |2041 - 2050 |
|2051 - 2060 |2061 - 2070 |2071 - 2080 |2081 - 2090 |2091 - 2100 |
Predictions for thePartial Solar Eclipse of 2025 Sep 21 were generated using theJPL DE405solar and lunar ephemerides. The lunar coordinates were calculated with respect to the Moon'sCenter of Mass. The predictions are given in bothTerrestrial Dynamical Time (TD) andUniversal Time (UT1).The parameterΔT is used to convert between these two times (i.e.,UT1 = TD - ΔT).ΔT has a value of 72.1 seconds for this eclipse.
Some of the content on this website is based on the books21st Century Canon of Solar Eclipses andThousand Year Canon of Solar Eclipses 1501 to 2500. All eclipse calculations are by Fred Espenak, and he assumes full responsibility for their accuracy.
Permission is granted to reproduce eclipse data when accompanied by a link to this page and an acknowledgment:
"Eclipse Predictions by Fred Espenak, www.EclipseWise.com"
The use of diagrams and maps is permitted provided that they areNOT altered (except for re-sizing) and the embedded credit line isNOT removed or concealed.
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Last Updated: 2022 Mar 03