Solar Eclipse Prime Page

Total Solar Eclipse of 2654 Jun 07

Fred Espenak

Introduction


The Total Solar Eclipse of 2654 Jun 07 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 2654 Jun 07 at 06:09:48 TD (05:37:49 UT1). This is 0.2 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 9047.

The eclipse belongs to Saros 167 and is number 26 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 2654 Jun 07 is a relatively long total eclipse with a duration at greatest eclipse of 04m12s. It has an eclipse magnitude of 1.0703.

The total solar eclipse of 2654 Jun 07 is preceded two weeks earlier by a partial lunar eclipse on 2654 May 23.

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 1918.4 seconds for this eclipse. The uncertainty in ΔT is 460.1 seconds corresponding to a standard error in longitude of the eclipse path of ± 1.92°.

The following links provide maps and data for the eclipse.

The tables below contain detailed predictions and additional information on the Total Solar Eclipse of 2654 Jun 07 .


Eclipse Data: Total Solar Eclipse of 2654 Jun 07

Eclipse Characteristics
Parameter Value
Eclipse Magnitude 1.07028
Eclipse Obscuration 1.14550
Gamma 0.76643
Conjunction Times
Event Calendar Date & Time Julian Date
Greatest Eclipse 2654 Jun 07 at 06:09:47.7 TD (05:37:49.3 UT1) 2690570.734598
Ecliptic Conjunction 2654 Jun 07 at 06:17:29.8 TD (05:45:31.4 UT1) 2690570.739947
Equatorial Conjunction 2654 Jun 07 at 06:25:26.8 TD (05:53:28.3 UT1) 2690570.745467
Geocentric Coordinates of Sun and Moon
2654 Jun 07 at 06:09:47.7 TD (05:37:49.3 UT1)
Coordinate Sun Moon
Right Ascension05h02m21.8s05h01m41.9s
Declination+22°41'45.8"+23°27'46.3"
Semi-Diameter 15'47.3" 16'43.1"
Eq. Hor. Parallax 08.7" 1°01'21.5"
Geocentric Libration of Moon
Angle Value
l 0.3°
b -1.0°
c -4.2°
Prediction Paramaters
Paramater Value
Ephemerides JPL DE406
ΔT 1918.4 s
k (penumbra) 0.2725076
k (umbra) 0.2722810
Saros Series 167 (26/72)

Explanation of Solar Eclipse Data Tables

Penumbral Shadow Contacts and Extremes: Total Solar Eclipse of 2654 Jun 07

Contacts of Penumbral Shadow with Earth
Contact Event Contact Time
TD
Time
UT1
Latitude Longitude
First External ContactP103:53:39.303:21:40.917°20.8'N032°06.5'E
Last External ContactP408:25:49.807:53:51.437°37.2'N170°22.8'E
Extreme Northern and Southern Path Limits of Penumbra
Contact Event Contact Time
TD
Time
UT1
Latitude Longitude
North Extreme Path Limit 1N104:21:19.203:49:20.802°32.6'N031°37.8'E
South Extreme Path Limit 1S107:58:12.707:26:14.323°16.8'N168°50.6'E

Explanation of Penumbral Shadow Contacts and Extremes Tables

Umbral Shadow Contacts and Extremes: Total Solar Eclipse of 2654 Jun 07

Contacts of Umbral Shadow with Earth
Contact Event Contact Time
TD
Time
UT1
Latitude Longitude
First External ContactU105:01:35.504:29:37.134°36.2'N005°51.6'E
First Internal ContactU205:06:25.504:34:27.036°25.9'N003°26.6'E
Last Internal ContactU307:12:59.706:41:01.254°59.8'N153°32.8'W
Last External ContactU407:17:49.606:45:51.153°26.5'N157°05.5'W
Extreme Northern and Southern Path Limits of Umbra
Contact Event Contact Time
TD
Time
UT1
Latitude Longitude
North Extreme Path Limit 1N105:06:01.504:34:03.036°41.6'N003°21.9'E
South Extreme Path Limit 1S105:02:01.404:30:03.034°19.5'N005°55.9'E
North Extreme Path Limit 2N207:13:23.706:41:25.255°13.0'N153°17.7'W
South Extreme Path Limit 2S207:17:23.806:45:25.453°12.2'N157°19.4'W

Explanation of Umbral Shadow Contacts and Extremes Tables

Central Line Extremes and Duration: Total Solar Eclipse of 2654 Jun 07

Extreme Limits of the Central Line
Contact Event Contact Time
TD
Time
UT1
Latitude Longitude
Extreme Central Line Limit 1C105:03:58.904:32:00.535°29.7'N004°40.9'E
Extreme Central Line Limit 2C207:15:26.206:43:27.854°12.3'N155°22.6'W

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 Eclipse06:09:47.705:37:49.370°34.2'N060°56.7'E 39.7° 147.5° 357.8 km04m12.37s
Greatest Duration06:10:38.705:38:40.370°49.4'N069°57.4'E 39.7° 149.1° 357.5 km04m12.38s

Explanation of Greatest Eclipse and Greatest Duration

Polynomial Besselian Elements: Total Solar Eclipse of 2654 Jun 07

Polynomial Besselian Elements
2654 Jun 07 at 06:00:00.0 TD (=t0)
n x y d l1 l2 μ
0 -0.24304 0.73310 22.6936 0.53108 -0.01500 269.9894
1 0.57304 0.11402 0.0037 0.00001 0.00001 14.9994
2 0.00004 -0.00020 -0.0000 -0.00001 -0.00001 -0.0000
3 -0.00001 -0.00000 - - - -
Tan ƒ1 0.0046153
Tan ƒ2 0.0045923

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 Total Solar Eclipse of 2654 Jun 07

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 Total Solar Eclipse of 2654 Jun 07 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 1918.4 seconds for this eclipse. The uncertainty in ΔT is 460.1 seconds corresponding to a standard error in longitude of the eclipse path of ± 1.92°.

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.