Solar Eclipse Prime Page

Total Solar Eclipse of 2097 May 11

Fred Espenak

Introduction


The Total Solar Eclipse of 2097 May 11 is visible from the following geographic regions:

  • Partial Eclipse: Asia, North America, north Europe
  • Total Eclipse: Alaska, Russia

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, see Key to Solar Eclipse Maps.

The instant of greatest eclipse takes place on 2097 May 11 at 18:34:31 TD (18:32:27 UT1). This is 1.3 days before the Moon reaches perigee. During the eclipse, the Sun is in the constellation Aries. The synodic month in which the eclipse takes place has a Brown Lunation Number of 2157.

The eclipse belongs to Saros 149 and is number 25 of 71 eclipses in the series. All eclipses in this series occur at the Moon’s ascending node. The Moon moves southward with respect to the node with each succeeding eclipse in the series and gamma decreases.

The total solar eclipse of 2097 May 11 is preceded two weeks earlier by a partial lunar eclipse on 2097 Apr 26.

These eclipses all take place during a single eclipse season.

The eclipse predictions are given in both Terrestrial Dynamical Time (TD) and Universal Time (UT1). The parameter ΔT is used to convert between these two times (i.e., UT1 = TD - ΔT). ΔT has a value of 124.3 seconds for this eclipse.

The following links provide maps and data for the eclipse.

The tables below contain detailed predictions and additional information on the Total Solar Eclipse of 2097 May 11 .


Eclipse Data: Total Solar Eclipse of 2097 May 11

Eclipse Characteristics
Parameter Value
Eclipse Magnitude 1.05381
Eclipse Obscuration 1.11052
Gamma 0.85156
Conjunction Times
Event Calendar Date & Time Julian Date
Greatest Eclipse 2097 May 11 at 18:34:31.4 TD (18:32:27.2 UT1) 2487105.272536
Ecliptic Conjunction 2097 May 11 at 18:43:07.2 TD (18:41:03.0 UT1) 2487105.278506
Equatorial Conjunction 2097 May 11 at 19:07:38.5 TD (19:05:34.2 UT1) 2487105.295535
Geocentric Coordinates of Sun and Moon
2097 May 11 at 18:34:31.4 TD (18:32:27.2 UT1)
Coordinate Sun Moon
Right Ascension03h17m49.7s03h16m33.2s
Declination+18°13'35.1"+19°01'53.0"
Semi-Diameter 15'50.2" 16'32.8"
Eq. Hor. Parallax 08.7" 1°00'43.7"
Geocentric Libration of Moon
Angle Value
l -2.8°
b -1.1°
c -13.6°
Prediction Paramaters
Paramater Value
Ephemerides JPL DE406
ΔT 124.3 s
k (penumbra) 0.2725076
k (umbra) 0.2722810
Saros Series 149 (25/71)

Explanation of Solar Eclipse Data Tables

Penumbral Shadow Contacts and Extremes: Total Solar Eclipse of 2097 May 11

Contacts of Penumbral Shadow with Earth
Contact Event Contact Time
TD
Time
UT1
Latitude Longitude
First External ContactP116:21:50.616:19:46.312°32.9'N160°01.5'W
Last External ContactP420:46:55.720:44:51.450°33.9'N018°28.5'W
Extreme Northern and Southern Path Limits of Penumbra
Contact Event Contact Time
TD
Time
UT1
Latitude Longitude
North Extreme Path Limit 1N116:48:53.916:46:49.601°43.6'S162°01.5'W
South Extreme Path Limit 1S120:19:57.920:17:53.737°07.2'N020°55.2'W

Explanation of Penumbral Shadow Contacts and Extremes Tables

Umbral Shadow Contacts and Extremes: Total Solar Eclipse of 2097 May 11

Contacts of Umbral Shadow with Earth
Contact Event Contact Time
TD
Time
UT1
Latitude Longitude
First External ContactU117:38:00.117:35:55.834°55.3'N171°50.9'E
First Internal ContactU217:42:36.017:40:31.736°55.4'N169°39.8'E
Last Internal ContactU319:26:03.919:23:59.669°26.9'N039°35.8'E
Last External ContactU419:30:43.319:28:39.068°22.3'N033°08.1'E
Extreme Northern and Southern Path Limits of Umbra
Contact Event Contact Time
TD
Time
UT1
Latitude Longitude
North Extreme Path Limit 1N117:42:21.117:40:16.837°05.2'N169°38.3'E
South Extreme Path Limit 1S117:38:16.417:36:12.134°44.7'N171°52.1'E
North Extreme Path Limit 2N219:26:19.019:24:14.769°31.7'N039°59.2'E
South Extreme Path Limit 2S219:30:26.819:28:22.668°16.3'N032°46.1'E

Explanation of Umbral Shadow Contacts and Extremes Tables

Central Line Extremes and Duration: Total Solar Eclipse of 2097 May 11

Extreme Limits of the Central Line
Contact Event Contact Time
TD
Time
UT1
Latitude Longitude
Extreme Central Line Limit 1C117:40:15.917:38:11.635°53.8'N170°47.1'E
Extreme Central Line Limit 2C219:28:25.719:26:21.568°55.0'N036°13.3'E

Explanation of Central Line Extremes Table

Greatest Eclipse and Greatest Duration
Event Time
TD
Time
UT1
Latitude Longitude Sun
Altitude
Sun
Azimuth
Path Width Central
Duration
Greatest Eclipse18:34:31.418:32:27.267°24.7'N150°20.3'W 31.3° 120.5° 339.5 km03m09.98s
Greatest Duration18:35:50.518:33:46.268°02.4'N149°11.4'W 31.3° 121.8° 338.6 km03m10.00s

Explanation of Greatest Eclipse and Greatest Duration

Polynomial Besselian Elements: Total Solar Eclipse of 2097 May 11

Polynomial Besselian Elements
2097 May 11 at 19:00:00.0 TD (=t0)
n x y d l1 l2 μ
0 -0.06890 0.88345 18.2287 0.53452 -0.01158 105.8909
1 0.54096 0.20238 0.0099 -0.00008 -0.00008 15.0015
2 0.00006 -0.00016 -0.0000 -0.00001 -0.00001 -0.0000
3 -0.00001 -0.00000 - - - -
Tan ƒ1 0.0046292
Tan ƒ2 0.0046062

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 = 19.000

Explanation of Polynomial Besselian Elements

Links for the Total Solar Eclipse of 2097 May 11

Links to Additional Solar Eclipse Information

Eclipse Predictions

Predictions for the Total Solar Eclipse of 2097 May 11 were generated using the JPL DE406 solar and lunar ephemerides. The lunar coordinates were calculated with respect to the Moon's Center of Mass. The predictions are given in both Terrestrial Dynamical Time (TD) and Universal Time (UT1). The parameter ΔT is used to convert between these two times (i.e., UT1 = TD - ΔT). ΔT has a value of 124.3 seconds for this eclipse.

Acknowledgments

Some of the content on this website is based on the book Thousand 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 are NOT altered (except for re-sizing) and the embedded credit line is NOT removed or covered.