Solar Eclipse Prime Page

Hybrid Solar Eclipse of -0100 May 17 (0101 May 17 BCE)

Fred Espenak

Introduction

eclipse map

The Hybrid Solar Eclipse of -0100 May 17 (0101 May 17 BCE) is visible from the geographic regions shown on the map to the right. 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 -0100 May 17 at 10:37:08 TD (07:24:21 UT1). This is 5.2 days after the Moon reaches perigee. During the eclipse, the Sun is in the constellation Taurus. The synodic month in which the eclipse takes place has a Brown Lunation Number of -25016.

The eclipse belongs to Saros 65 and is number 37 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 -0100 May 17 is one of the rare hybrid solar eclipses. In this particular case the eclipse path starts out as total but later changes to annular. It is a relatively long hybrid eclipse with a duration at greatest eclipse of 01m44s. The eclipse magnitude is 1.0170, while Gamma has a value of -0.1911.

The hybrid solar eclipse of -0100 May 17 is preceded two weeks earlier by a penumbral lunar eclipse on -0100 May 03, and it is followed two weeks later by a penumbral lunar eclipse on -0100 Jun 01.

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 11566.5 seconds for this eclipse. The uncertainty in ΔT is 294.8 seconds corresponding to a standard error in longitude of the eclipse path of ± 1.23°.

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 -0100 May 17 .

Eclipse Data: Hybrid Solar Eclipse of -0100 May 17

Eclipse Characteristics
Parameter Value
Eclipse Magnitude 1.01701
Eclipse Obscuration 1.03431
Gamma-0.19106
Conjunction Times
Event Calendar Date and Time Julian Date
Greatest Eclipse -0100 May 17 at 10:37:08.0 TD (07:24:21.5 UT1) 1684669.808582
Ecliptic Conjunction -0100 May 17 at 10:35:03.3 TD (07:22:16.8 UT1) 1684669.807139
Equatorial Conjunction -0100 May 17 at 10:29:16.4 TD (07:16:29.9 UT1) 1684669.803123
Geocentric Coordinates of Sun and Moon
-0100 May 17 at 10:37:08.0 TD (07:24:21.5 UT1)
Coordinate Sun Moon
Right Ascension03h21m01.7s03h21m18.1s
Declination+18°39'30.6"+18°29'11.9"
Semi-Diameter 15'43.6" 15'44.6"
Eq. Hor. Parallax 08.6" 0°57'46.6"
Geocentric Libration of Moon
Angle Value
l 5.2°
b 0.2°
c -13.3°
Prediction Paramaters
Paramater Value
Ephemerides JPL DE406
ΔT 11566.5 s
k (penumbra) 0.2725076
k (umbra) 0.2722810
Saros Series 65 (37/71)

Explanation of Solar Eclipse Data Tables

Penumbral Shadow Contacts and Extremes: Hybrid Solar Eclipse of -0100 May 17

Contacts of Penumbral Shadow with Earth
Contact Event Contact Time
TD		 Time
UT1		 Latitude Longitude
First External ContactP107:48:58.804:36:12.326°15.7'S028°40.3'E
First Internal ContactP209:52:08.906:39:22.442°42.7'S006°27.3'E
Last Internal ContactP311:22:16.908:09:30.404°08.6'S144°21.7'E
Last External ContactP413:25:26.510:12:40.012°46.9'N119°22.2'E
Extreme Northern and Southern Path Limits of Penumbra
Contact Event Contact Time
TD		 Time
UT1		 Latitude Longitude
North Extreme Path Limit 1N109:02:22.805:49:36.300°05.4'S000°47.3'E
South Extreme Path Limit 1S109:15:59.506:03:13.061°28.4'S035°42.8'E
North Extreme Path Limit 2N212:11:43.008:58:56.538°39.0'N149°05.1'E
South Extreme Path Limit 2S211:58:43.508:45:57.025°17.5'S127°27.8'E

Explanation of Penumbral Shadow Contacts and Extremes Tables

Umbral Shadow Contacts and Extremes: Hybrid Solar Eclipse of -0100 May 17

Contacts of Umbral Shadow with Earth
Contact Event Contact Time
TD		 Time
UT1		 Latitude Longitude
First External ContactU108:49:32.105:36:45.629°54.7'S015°08.7'E
First Internal ContactU208:49:36.505:36:50.029°55.1'S015°07.8'E
Last Internal ContactU312:24:46.709:12:00.209°04.2'N133°13.8'E
Last External ContactU412:24:48.009:12:01.509°04.3'N133°13.6'E
Extreme Northern and Southern Path Limits of Umbra
Contact Event Contact Time
TD		 Time
UT1		 Latitude Longitude
North Extreme Path Limit 1N108:49:34.205:36:47.729°53.9'S015°07.8'E
South Extreme Path Limit 1S108:49:34.405:36:47.929°56.0'S015°08.7'E
North Extreme Path Limit 2N212:24:47.309:12:00.809°03.9'N133°13.6'E
South Extreme Path Limit 2S212:24:47.409:12:00.909°04.6'N133°13.8'E

Explanation of Umbral Shadow Contacts and Extremes Tables

Central Line Extremes and Duration: Hybrid Solar Eclipse of -0100 May 17

Extreme Limits of the Central Line
Contact Event Contact Time
TD		 Time
UT1		 Latitude Longitude
Extreme Central Line Limit 1C108:49:34.305:36:47.829°54.9'S015°08.3'E
Extreme Central Line Limit 2C212:24:47.409:12:00.809°04.2'N133°13.7'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 Eclipse10:37:08.007:24:21.508°21.9'N022°36.9'E 79.0° 340.3° 59.3 km01m44.45s
Greatest Duration10:38:43.907:25:57.408°38.8'N071°20.2'E 79.0° 336.1° 59.3 km01m44.47s

Explanation of Greatest Eclipse and Greatest Duration

Polynomial Besselian Elements: Hybrid Solar Eclipse of -0100 May 17

Polynomial Besselian Elements
-0100 May 17 at 11:00:00.0 TD (=t0)
n x y d l1 l2 μ
0 0.26231 -0.10569 18.6626 0.54612 -0.00003 346.9909
1 0.51221 0.19202 0.0097 0.00011 0.00011 15.0019
2 0.00001 -0.00011 -0.0000 -0.00001 -0.00001 -0.0000
3 -0.00001 -0.00000 - - - -
Tan ƒ1 0.0045976
Tan ƒ2 0.0045747

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 = 11.000

Explanation of Polynomial Besselian Elements

Links for the Hybrid Solar Eclipse of -0100 May 17 (0101 May 17 BCE)

Links to Additional Solar Eclipse Information

Calendar

The Gregorian calendar (also called the Western calendar) is internationally the most widely used civil calendar. It is named for Pope Gregory XIII, who introduced it in 1582. On this website, the Gregorian calendar is used for all calendar dates from 1582 Oct 15 onwards. Before that date, the Julian calendar is used. For more information on this topic, see Calendar Dates.

The Julian calendar does not include the year 0. Thus the year 1 BCE is followed by the year 1 CE (See: BCE/CE Dating Conventions). This is awkward for arithmetic calculations. Years in this catalog are numbered astronomically and include the year 0. Historians should note there is a difference of one year between astronomical dates and BCE dates. Thus, the astronomical year 0 corresponds to 1 BCE, and astronomical year -1 corresponds to 2 BCE, etc..

Eclipse Predictions

Predictions for the Hybrid Solar Eclipse of -0100 May 17 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 11566.5 seconds for this eclipse. The uncertainty in ΔT is 294.8 seconds corresponding to a standard error in longitude of the eclipse path of ± 1.23°.

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.