Solar Eclipse Prime Page

Hybrid Solar Eclipse of 2013 Nov 03

Fred Espenak

Introduction


The Hybrid Solar Eclipse of 2013 Nov 03 is visible from the following geographic regions:

  • Partial Eclipse: east Americas, south Europe, Africa
  • Hybrid Eclipse: Atlantic, central Africa

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 2013 Nov 03 at 12:47:36 TD (12:46:29 UT1). This is 2.9 days before the Moon reaches perigee. During the eclipse, the Sun is in the constellation Libra. The synodic month in which the eclipse takes place has a Brown Lunation Number of 1124.

The eclipse belongs to Saros 143 and is number 23 of 72 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 2013 Nov 03 is one of the rare hybrid solar eclipses. In this particular case the eclipse path starts out as annular but later changes to total. It is a relatively long hybrid eclipse with a duration at greatest eclipse of 01m40s. The eclipse magnitude is 1.0159, while Gamma has a value of 0.3272.

The hybrid solar eclipse of 2013 Nov 03 is preceded two weeks earlier by a penumbral lunar eclipse on 2013 Oct 18.

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 67.2 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 Hybrid Solar Eclipse of 2013 Nov 03 .


Eclipse Data: Hybrid Solar Eclipse of 2013 Nov 03

Eclipse Characteristics
Parameter Value
Eclipse Magnitude 1.01587
Eclipse Obscuration 1.03200
Gamma 0.32715
Conjunction Times
Event Calendar Date & Time Julian Date
Greatest Eclipse 2013 Nov 03 at 12:47:36.1 TD (12:46:28.9 UT1) 2456600.032279
Ecliptic Conjunction 2013 Nov 03 at 12:51:04.5 TD (12:49:57.3 UT1) 2456600.034691
Equatorial Conjunction 2013 Nov 03 at 12:39:54.2 TD (12:38:47.0 UT1) 2456600.026933
Geocentric Coordinates of Sun and Moon
2013 Nov 03 at 12:47:36.1 TD (12:46:28.9 UT1)
Coordinate Sun Moon
Right Ascension14h35m19.9s14h35m37.0s
Declination-15°12'22.5"-14°53'30.7"
Semi-Diameter 16'07.4" 16'07.6"
Eq. Hor. Parallax 08.9" 0°59'11.0"
Geocentric Libration of Moon
Angle Value
l -4.2°
b -0.4°
c 19.6°
Prediction Paramaters
Paramater Value
Ephemerides JPL DE406
ΔT 67.2 s
k (penumbra) 0.2725076
k (umbra) 0.2722810
Saros Series 143 (23/72)

Explanation of Solar Eclipse Data Tables

Penumbral Shadow Contacts and Extremes: Hybrid Solar Eclipse of 2013 Nov 03

Contacts of Penumbral Shadow with Earth
Contact Event Contact Time
TD
Time
UT1
Latitude Longitude
First External ContactP110:05:41.210:04:34.023°50.6'N058°21.8'W
First Internal ContactP212:14:17.312:13:10.155°48.9'N073°49.3'W
Last Internal ContactP313:21:08.213:20:01.032°42.3'N055°49.7'E
Last External ContactP415:29:29.315:28:22.100°08.5'S033°49.7'E
Extreme Northern and Southern Path Limits of Penumbra
Contact Event Contact Time
TD
Time
UT1
Latitude Longitude
North Extreme Path Limit 1N111:51:55.111:50:47.967°43.5'N050°16.3'W
South Extreme Path Limit 1S111:09:38.511:08:31.300°03.5'S081°15.5'W
North Extreme Path Limit 2N213:43:37.613:42:30.446°26.8'N043°38.1'E
South Extreme Path Limit 2S214:25:27.614:24:20.424°01.2'S056°46.3'E

Explanation of Penumbral Shadow Contacts and Extremes Tables

Umbral Shadow Contacts and Extremes: Hybrid Solar Eclipse of 2013 Nov 03

Contacts of Umbral Shadow with Earth
Contact Event Contact Time
TD
Time
UT1
Latitude Longitude
First External ContactU111:06:24.611:05:17.430°26.4'N071°15.1'W
First Internal ContactU211:06:28.911:05:21.630°27.1'N071°15.9'W
Last Internal ContactU314:28:50.114:27:42.906°31.8'N047°10.4'E
Last External ContactU414:28:50.814:27:43.506°31.7'N047°10.3'E
Extreme Northern and Southern Path Limits of Umbra
Contact Event Contact Time
TD
Time
UT1
Latitude Longitude
North Extreme Path Limit 1N111:06:27.211:05:20.030°27.9'N071°15.2'W
South Extreme Path Limit 1S111:06:26.311:05:19.130°25.7'N071°15.8'W
North Extreme Path Limit 2N214:28:50.514:27:43.306°31.5'N047°10.4'E
South Extreme Path Limit 2S214:28:50.414:27:43.106°31.9'N047°10.3'E

Explanation of Umbral Shadow Contacts and Extremes Tables

Central Line Extremes and Duration: Hybrid Solar Eclipse of 2013 Nov 03

Extreme Limits of the Central Line
Contact Event Contact Time
TD
Time
UT1
Latitude Longitude
Extreme Central Line Limit 1C111:06:26.711:05:19.530°26.8'N071°15.5'W
Extreme Central Line Limit 2C214:28:50.414:27:43.206°31.7'N047°10.4'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 Eclipse12:47:36.112:46:28.903°29.4'N011°58.8'W 70.9° 192.0° 57.5 km01m39.55s
Greatest Duration12:51:58.212:50:51.003°00.9'N010°29.9'W 70.7° 198.8° 57.7 km01m39.72s

Explanation of Greatest Eclipse and Greatest Duration

Polynomial Besselian Elements: Hybrid Solar Eclipse of 2013 Nov 03

Polynomial Besselian Elements
2013 Nov 03 at 13:00:00.0 TD (=t0)
n x y d l1 l2 μ
0 0.18319 0.29472 -15.2097 0.54630 0.00014 19.1106
1 0.54695 -0.12008 -0.0126 -0.00011 -0.00011 15.0013
2 0.00003 0.00008 0.0000 -0.00001 -0.00001 -0.0000
3 -0.00001 0.00000 - - - -
Tan ƒ1 0.0047137
Tan ƒ2 0.0046902

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 = 13.000

Explanation of Polynomial Besselian Elements

Links for the Hybrid Solar Eclipse of 2013 Nov 03

Links to Additional Solar Eclipse Information

Eclipse Predictions

Predictions for the Hybrid Solar Eclipse of 2013 Nov 03 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 67.2 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.