Solar Eclipse Prime Page

Partial Solar Eclipse of 2452 Mar 21

Fred Espenak

Introduction

eclipse map

The Partial Solar Eclipse of 2452 Mar 21 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 2452 Mar 21 at 17:01:30 TD (16:45:07 UT1). This is 5.1 days after the Moon reaches apogee. During the eclipse, the Sun is in the constellation Pisces. The synodic month in which the eclipse takes place has a Brown Lunation Number of 6546.

The eclipse belongs to Saros 127 and is number 82 of 82 eclipses in the series. Thus, the 2452 Mar 21 event is the last eclipse of 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.

This is an extremely shallow partial eclipse. It has an eclipse magnitude of only 0.0261, while Gamma has a value of -1.5455. This is a very deep partial eclipse. It has an eclipse magnitude of 0.0261, while Gamma has a value of -1.5455.

The partial solar eclipse of 2452 Mar 21 is followed two weeks later by a total lunar eclipse on 2452 Apr 04.

Another solar eclipse occurs one synodic month after the 2452 Mar 21 eclipse. It is the partial solar eclipse of 2452 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 983.0 seconds for this eclipse. The uncertainty in ΔT is 251.6 seconds corresponding to a standard error in longitude of the eclipse path of ± 1.05°.

The following links provide maps and data for the eclipse.

The tables below contain detailed predictions and additional information on the Partial Solar Eclipse of 2452 Mar 21 .

Eclipse Data: Partial Solar Eclipse of 2452 Mar 21

Eclipse Characteristics
Parameter Value
Eclipse Magnitude 0.02615
Eclipse Obscuration 0.00498
Gamma-1.54551
Conjunction Times
Event Calendar Date and Time Julian Date
Greatest Eclipse 2452 Mar 21 at 17:01:29.6 TD (16:45:06.6 UT1) 2616715.197992
Ecliptic Conjunction 2452 Mar 21 at 16:44:12.1 TD (16:27:49.1 UT1) 2616715.185985
Equatorial Conjunction 2452 Mar 21 at 15:23:17.3 TD (15:06:54.3 UT1) 2616715.129795
Geocentric Coordinates of Sun and Moon
2452 Mar 21 at 17:01:29.6 TD (16:45:06.6 UT1)
Coordinate Sun Moon
Right Ascension00h06m41.9s00h09m27.7s
Declination+00°43'26.0"-00°31'33.9"
Semi-Diameter 16'05.0" 15'08.8"
Eq. Hor. Parallax 08.8" 0°55'35.2"
Geocentric Libration of Moon
Angle Value
l -4.5°
b 1.9°
c -21.9°
Prediction Paramaters
Paramater Value
Ephemerides JPL DE406
ΔT 983.0 s
k (penumbra) 0.2725076
k (umbra) 0.2722810
Saros Series 127 (82/82)

Explanation of Solar Eclipse Data Tables

Penumbral Shadow Contacts and Extremes: Partial Solar Eclipse of 2452 Mar 21

Contacts of Penumbral Shadow with Earth
Contact Event Contact Time
TD		 Time
UT1		 Latitude Longitude
First External ContactP116:36:46.916:20:23.969°06.3'S024°38.9'E
Last External ContactP417:26:46.617:10:23.653°09.1'S013°03.3'E
Extreme Northern and Southern Path Limits of Penumbra
Contact Event Contact Time
TD		 Time
UT1		 Latitude Longitude
North Extreme Path Limit 1N116:41:55.616:25:32.671°03.4'S023°08.7'E
South Extreme Path Limit 1S117:21:46.417:05:23.451°04.9'S014°22.7'E

Explanation of Penumbral Shadow Contacts and Extremes Tables

Polynomial Besselian Elements: Partial Solar Eclipse of 2452 Mar 21

Polynomial Besselian Elements
2452 Mar 21 at 17:00:00.0 TD (=t0)
n x y d l1 l2 μ
0 0.73621 -1.35896 0.7268 0.56326 0.01702 73.3761
1 0.45674 0.25242 0.0159 -0.00011 -0.00011 15.0041
2 -0.00002 0.00006 -0.0000 -0.00001 -0.00001 0.0000
3 -0.00001 -0.00000 - - - -
Tan ƒ1 0.0047026
Tan ƒ2 0.0046791

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 = 17.000

Explanation of Polynomial Besselian Elements

Links for the Partial Solar Eclipse of 2452 Mar 21

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 Partial Solar Eclipse of 2452 Mar 21 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 983.0 seconds for this eclipse. The uncertainty in ΔT is 251.6 seconds corresponding to a standard error in longitude of the eclipse path of ± 1.05°.

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.