Solar Eclipse Prime Page

Annular Solar Eclipse of -1895 Oct 28 (1896 Oct 28 BCE)

Fred Espenak

Introduction

eclipse map

The Annular Solar Eclipse of -1895 Oct 28 (1896 Oct 28 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 -1895 Oct 28 at 00:11:54 TD (12:00:24 UT1). This is 0.4 days after the Moon reaches apogee. During the eclipse, the Sun is in the constellation Ophiuchus. The synodic month in which the eclipse takes place has a Brown Lunation Number of -47212.

The eclipse belongs to Saros 3 and is number 52 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 -1895 Oct 28 is a relatively long annular eclipse with a duration at greatest eclipse of 08m57s. It has an eclipse magnitude of 0.9130.

The annular solar eclipse of -1895 Oct 28 is followed two weeks later by a partial lunar eclipse on -1895 Nov 11.

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 43889.5 seconds for this eclipse. The uncertainty in ΔT is 3299.4 seconds corresponding to a standard error in longitude of the eclipse path of ± 13.79°.

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 -1895 Oct 28 .

Eclipse Data: Annular Solar Eclipse of -1895 Oct 28

Eclipse Characteristics
Parameter Value
Eclipse Magnitude 0.91297
Eclipse Obscuration 0.83352
Gamma-0.67813
Conjunction Times
Event Calendar Date and Time Julian Date
Greatest Eclipse -1895 Oct 28 at 00:11:53.5 TD (12:00:24.0 UT1) 1029209.000278
Ecliptic Conjunction -1895 Oct 28 at 00:03:43.5 TD (11:52:13.9 UT1) 1029208.994606
Equatorial Conjunction -1895 Oct 28 at 00:36:35.1 TD (12:25:05.6 UT1) 1029209.017426
Geocentric Coordinates of Sun and Moon
-1895 Oct 28 at 00:11:53.5 TD (12:00:24.0 UT1)
Coordinate Sun Moon
Right Ascension13h10m07.5s13h09m24.5s
Declination-07°36'32.1"-08°11'25.3"
Semi-Diameter 16'16.5" 14'41.9"
Eq. Hor. Parallax 08.9" 0°53'56.7"
Geocentric Libration of Moon
Angle Value
l 0.4°
b 0.8°
c 24.2°
Prediction Paramaters
Paramater Value
Ephemerides JPL DE406
ΔT 43889.5 s
k (penumbra) 0.2725076
k (umbra) 0.2722810
Saros Series 3 (52/72)

Explanation of Solar Eclipse Data Tables

Penumbral Shadow Contacts and Extremes: Annular Solar Eclipse of -1895 Oct 28

Contacts of Penumbral Shadow with Earth
Contact Event Contact Time
TD		 Time
UT1		 Latitude Longitude
First External ContactP121:22:10.309:10:40.808°28.5'S050°35.0'W
Last External ContactP403:01:24.914:49:55.442°11.3'S052°43.1'E
Extreme Northern and Southern Path Limits of Penumbra
Contact Event Contact Time
TD		 Time
UT1		 Latitude Longitude
North Extreme Path Limit 1N122:08:24.209:56:54.611°00.4'N059°31.6'W
South Extreme Path Limit 1S102:15:21.614:03:52.022°50.4'S060°28.8'E

Explanation of Penumbral Shadow Contacts and Extremes Tables

Umbral Shadow Contacts and Extremes: Annular Solar Eclipse of -1895 Oct 28

Contacts of Umbral Shadow with Earth
Contact Event Contact Time
TD		 Time
UT1		 Latitude Longitude
First External ContactU122:39:33.310:28:03.824°09.4'S072°13.3'W
First Internal ContactU222:49:10.110:37:40.527°16.5'S075°08.4'W
Last Internal ContactU301:34:18.713:22:49.160°40.2'S081°17.8'E
Last External ContactU401:43:56.113:32:26.557°38.0'S077°18.1'E
Extreme Northern and Southern Path Limits of Umbra
Contact Event Contact Time
TD		 Time
UT1		 Latitude Longitude
North Extreme Path Limit 1N122:40:58.810:29:29.223°24.0'S072°27.5'W
South Extreme Path Limit 1S122:47:51.510:36:22.027°59.1'S074°56.0'W
North Extreme Path Limit 2N201:42:30.813:31:01.256°53.9'S077°18.8'E
South Extreme Path Limit 2S201:35:36.713:24:07.261°21.3'S081°22.4'E

Explanation of Umbral Shadow Contacts and Extremes Tables

Central Line Extremes and Duration: Annular Solar Eclipse of -1895 Oct 28

Extreme Limits of the Central Line
Contact Event Contact Time
TD		 Time
UT1		 Latitude Longitude
Extreme Central Line Limit 1C122:44:18.010:32:48.425°39.0'S073°39.1'W
Extreme Central Line Limit 2C201:39:11.113:27:41.659°05.4'S079°12.9'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 Eclipse00:11:53.512:00:24.048°01.6'S157°33.1'E 47.0° 25.4° 448.6 km08m56.96s
Greatest Duration00:14:22.712:02:53.148°32.5'S018°04.8'W 47.0° 23.0° 447.0 km08m57.04s

Explanation of Greatest Eclipse and Greatest Duration

Polynomial Besselian Elements: Annular Solar Eclipse of -1895 Oct 28

Polynomial Besselian Elements
-1895 Oct 28 at 00:00:00.0 TD (=t0)
n x y d l1 l2 μ
0 -0.29332 -0.61948 -7.6041 0.57581 0.02951 182.2882
1 0.48104 -0.14686 -0.0161 -0.00000 -0.00000 15.0027
2 0.00003 0.00007 0.0000 -0.00001 -0.00001 -0.0000
3 -0.00001 0.00000 - - - -
Tan ƒ1 0.0047593
Tan ƒ2 0.0047356

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 = 0.000

Explanation of Polynomial Besselian Elements

Links for the Annular Solar Eclipse of -1895 Oct 28 (1896 Oct 28 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 Annular Solar Eclipse of -1895 Oct 28 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 43889.5 seconds for this eclipse. The uncertainty in ΔT is 3299.4 seconds corresponding to a standard error in longitude of the eclipse path of ± 13.79°.

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.