Solar Eclipse Prime Page

Annular Solar Eclipse of 0878 May 06

Fred Espenak

Introduction

eclipse map

The Annular Solar Eclipse of 0878 May 06 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 0878 May 06 at 05:48:06 TD (05:09:11 UT1). This is 5.7 days after the Moon reaches apogee. 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 -12920.

The eclipse belongs to Saros 110 and is number 24 of 72 eclipses in the series. All eclipses in this series occur at the Moon’s descending node. The Moon moves northward with respect to the node with each succeeding eclipse in the series and gamma increases.

The annular solar eclipse of 0878 May 06 is preceded two weeks earlier by a total lunar eclipse on 0878 Apr 20.

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 2335.3 seconds for this eclipse. The uncertainty in ΔT is 70.9 seconds corresponding to a standard error in longitude of the eclipse path of ± 0.30°.

The following links provide maps and data for the eclipse.

The tables below contain detailed predictions and additional information on the Annular Solar Eclipse of 0878 May 06 .

Eclipse Data: Annular Solar Eclipse of 0878 May 06

Eclipse Characteristics
Parameter Value
Eclipse Magnitude 0.97109
Eclipse Obscuration 0.94301
Gamma-0.97155
Conjunction Times
Event Calendar Date and Time Julian Date
Greatest Eclipse 0878 May 06 at 05:48:06.1 TD (05:09:10.9 UT1) 2041872.714709
Ecliptic Conjunction 0878 May 06 at 05:58:53.2 TD (05:19:57.9 UT1) 2041872.722198
Equatorial Conjunction 0878 May 06 at 05:27:59.1 TD (04:49:03.9 UT1) 2041872.700739
Geocentric Coordinates of Sun and Moon
0878 May 06 at 05:48:06.1 TD (05:09:10.9 UT1)
Coordinate Sun Moon
Right Ascension03h07m02.2s03h07m42.8s
Declination+17°38'25.9"+16°45'00.3"
Semi-Diameter 15'46.3" 15'16.1"
Eq. Hor. Parallax 08.7" 0°56'02.2"
Geocentric Libration of Moon
Angle Value
l -4.9°
b 1.2°
c -17.4°
Prediction Paramaters
Paramater Value
Ephemerides JPL DE406
ΔT 2335.3 s
k (penumbra) 0.2725076
k (umbra) 0.2722810
Saros Series 110 (24/72)

Explanation of Solar Eclipse Data Tables

Penumbral Shadow Contacts and Extremes: Annular Solar Eclipse of 0878 May 06

Contacts of Penumbral Shadow with Earth
Contact Event Contact Time
TD		 Time
UT1		 Latitude Longitude
First External ContactP103:30:19.402:51:24.146°11.6'S065°08.7'E
Last External ContactP408:05:56.507:27:01.227°03.7'S147°31.9'E
Extreme Northern and Southern Path Limits of Penumbra
Contact Event Contact Time
TD		 Time
UT1		 Latitude Longitude
North Extreme Path Limit 1N104:14:09.903:35:14.633°34.5'S047°01.4'E
South Extreme Path Limit 1S107:22:05.406:43:10.114°01.7'S163°17.9'E

Explanation of Penumbral Shadow Contacts and Extremes Tables

Umbral Shadow Contacts and Extremes: Annular Solar Eclipse of 0878 May 06

Contacts of Umbral Shadow with Earth
Contact Event Contact Time
TD		 Time
UT1		 Latitude Longitude
First External ContactU105:18:21.904:39:26.671°45.7'S093°33.3'E
First Internal ContactU205:27:51.904:48:56.672°21.6'S106°13.3'E
Last Internal ContactU306:08:37.605:29:42.363°01.3'S147°33.2'E
Last External ContactU406:18:01.605:39:06.359°26.6'S151°16.3'E
Extreme Northern and Southern Path Limits of Umbra
Contact Event Contact Time
TD		 Time
UT1		 Latitude Longitude
North Extreme Path Limit 1N105:18:33.304:39:38.071°44.7'S093°17.9'E
South Extreme Path Limit 1S105:27:44.104:48:48.872°21.6'S106°24.5'E
North Extreme Path Limit 2N206:17:50.405:38:55.159°23.3'S151°23.9'E
South Extreme Path Limit 2S206:08:45.505:29:50.263°03.4'S147°27.1'E

Explanation of Umbral Shadow Contacts and Extremes Tables

Central Line Extremes and Duration: Annular Solar Eclipse of 0878 May 06

Extreme Limits of the Central Line
Contact Event Contact Time
TD		 Time
UT1		 Latitude Longitude
Extreme Central Line Limit 1C105:22:41.704:43:46.472°10.5'S099°08.1'E
Extreme Central Line Limit 2C206:13:44.805:34:49.561°05.3'S149°46.6'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 Eclipse05:48:06.105:09:10.957°45.8'S110°36.8'E 13.0° 341.4° 455.2 km02m28.03s
Greatest Duration05:40:07.705:01:12.559°28.1'S115°16.1'E 12.3° 348.4° 435.4 km02m28.13s

Explanation of Greatest Eclipse and Greatest Duration

Polynomial Besselian Elements: Annular Solar Eclipse of 0878 May 06

Polynomial Besselian Elements
0878 May 06 at 06:00:00.0 TD (=t0)
n x y d l1 l2 μ
0 0.27718 -0.93705 17.6450 0.55535 0.00915 271.3712
1 0.51949 0.09463 0.0107 -0.00012 -0.00011 15.0021
2 0.00002 -0.00006 -0.0000 -0.00001 -0.00001 -0.0000
3 -0.00001 -0.00000 - - - -
Tan ƒ1 0.0046111
Tan ƒ2 0.0045881

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 Annular Solar Eclipse of 0878 May 06

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 Annular Solar Eclipse of 0878 May 06 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 2335.3 seconds for this eclipse. The uncertainty in ΔT is 70.9 seconds corresponding to a standard error in longitude of the eclipse path of ± 0.30°.

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.