Solar Eclipse Prime Page

Total Solar Eclipse of 1910 May 09

Fred Espenak

Introduction


The Total Solar Eclipse of 1910 May 09 is visible from the following geographic regions:

  • Partial Eclipse: Antarctica, Australia, south Indies
  • Total Eclipse: Antarctica, Tasmania

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 1910 May 09 at 05:42:13 TD (05:42:02 UT1). This is 0.4 days after 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 -156.

The eclipse belongs to Saros 117 and is number 63 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 solar eclipse of 1910 May 09 is a relatively long total eclipse with a duration at greatest eclipse of 04m15s. It has an eclipse magnitude of 1.0600.

The total solar eclipse of 1910 May 09 is followed two weeks later by a total lunar eclipse on 1910 May 24.

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 10.8 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 1910 May 09 .


Eclipse Data: Total Solar Eclipse of 1910 May 09

Eclipse Characteristics
Parameter Value
Eclipse Magnitude 1.06000
Eclipse Obscuration 1.12360
Gamma-0.94372
Conjunction Times
Event Calendar Date & Time Julian Date
Greatest Eclipse 1910 May 09 at 05:42:12.6 TD (05:42:01.7 UT1) 2418800.737520
Ecliptic Conjunction 1910 May 09 at 05:32:47.7 TD (05:32:36.8 UT1) 2418800.730982
Equatorial Conjunction 1910 May 09 at 05:03:20.8 TD (05:03:10.0 UT1) 2418800.710532
Geocentric Coordinates of Sun and Moon
1910 May 09 at 05:42:12.6 TD (05:42:01.7 UT1)
Coordinate Sun Moon
Right Ascension03h01m00.1s03h02m29.5s
Declination+17°07'25.6"+16°13'49.4"
Semi-Diameter 15'50.4" 16'42.2"
Eq. Hor. Parallax 08.7" 1°01'18.1"
Geocentric Libration of Moon
Angle Value
l 0.9°
b 1.3°
c -14.7°
Prediction Paramaters
Paramater Value
Ephemerides JPL DE406
ΔT 10.8 s
k (penumbra) 0.2725076
k (umbra) 0.2722810
Saros Series 117 (63/71)

Explanation of Solar Eclipse Data Tables

Penumbral Shadow Contacts and Extremes: Total Solar Eclipse of 1910 May 09

Contacts of Penumbral Shadow with Earth
Contact Event Contact Time
TD
Time
UT1
Latitude Longitude
First External ContactP103:38:20.003:38:09.255°55.3'S061°36.6'E
Last External ContactP407:46:22.107:46:11.315°34.9'S147°36.1'E
Extreme Northern and Southern Path Limits of Penumbra
Contact Event Contact Time
TD
Time
UT1
Latitude Longitude
North Extreme Path Limit 1N104:15:38.904:15:28.043°59.2'S042°30.7'E
South Extreme Path Limit 1S107:08:58.207:08:47.302°39.5'S161°03.9'E

Explanation of Penumbral Shadow Contacts and Extremes Tables

Umbral Shadow Contacts and Extremes: Total Solar Eclipse of 1910 May 09

Contacts of Umbral Shadow with Earth
Contact Event Contact Time
TD
Time
UT1
Latitude Longitude
First External ContactU105:04:55.405:04:44.572°51.8'S105°37.3'E
First Internal ContactU205:13:54.405:13:43.672°02.1'S118°51.4'E
Last Internal ContactU306:10:56.206:10:45.448°45.0'S155°49.3'E
Last External ContactU406:19:53.606:19:42.844°28.9'S156°32.2'E
Extreme Northern and Southern Path Limits of Umbra
Contact Event Contact Time
TD
Time
UT1
Latitude Longitude
North Extreme Path Limit 1N105:05:16.405:05:05.672°52.1'S105°02.7'E
South Extreme Path Limit 1S105:13:38.205:13:27.472°00.1'S119°16.1'E
North Extreme Path Limit 2N206:19:32.406:19:21.544°20.9'S156°42.6'E
South Extreme Path Limit 2S206:11:12.306:11:01.548°51.2'S155°40.6'E

Explanation of Umbral Shadow Contacts and Extremes Tables

Central Line Extremes and Duration: Total Solar Eclipse of 1910 May 09

Extreme Limits of the Central Line
Contact Event Contact Time
TD
Time
UT1
Latitude Longitude
Extreme Central Line Limit 1C105:09:08.505:08:57.772°37.7'S111°54.2'E
Extreme Central Line Limit 2C206:15:41.306:15:30.446°28.0'S156°16.7'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 Eclipse05:42:12.605:42:01.748°10.6'S125°11.5'E 18.8° 328.0° 594.5 km04m15.32s
Greatest Duration05:42:47.505:42:36.748°00.2'S125°30.1'E 18.8° 327.6° 596.8 km04m15.33s

Explanation of Greatest Eclipse and Greatest Duration

Polynomial Besselian Elements: Total Solar Eclipse of 1910 May 09

Polynomial Besselian Elements
1910 May 09 at 06:00:00.0 TD (=t0)
n x y d l1 l2 μ
0 0.51113 -0.81195 17.1291 0.53214 -0.01395 270.9117
1 0.54135 0.21659 0.0108 0.00002 0.00002 15.0020
2 0.00001 -0.00006 -0.0000 -0.00001 -0.00001 -0.0000
3 -0.00001 -0.00000 - - - -
Tan ƒ1 0.0046300
Tan ƒ2 0.0046069

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 = 6.000

Explanation of Polynomial Besselian Elements

Links for the Total Solar Eclipse of 1910 May 09

Links to Additional Solar Eclipse Information

Eclipse Predictions

Predictions for the Total Solar Eclipse of 1910 May 09 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 10.8 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.