Solar Eclipse Prime Page

Total Solar Eclipse of 2290 Jun 08

Fred Espenak

Introduction


The Total Solar Eclipse of 2290 Jun 08 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 2290 Jun 08 at 05:35:48 TD (05:28:00 UT1). This is 2.4 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 4545.

The eclipse belongs to Saros 132 and is number 61 of 71 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 total solar eclipse of 2290 Jun 08 is followed two weeks later by a partial lunar eclipse on 2290 Jun 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 467.8 seconds for this eclipse. The uncertainty in ΔT is 122.3 seconds corresponding to a standard error in longitude of the eclipse path of ± 0.51°.

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 2290 Jun 08 .


Eclipse Data: Total Solar Eclipse of 2290 Jun 08

Eclipse Characteristics
Parameter Value
Eclipse Magnitude 1.03820
Eclipse Obscuration 1.07787
Gamma 0.87129
Conjunction Times
Event Calendar Date & Time Julian Date
Greatest Eclipse 2290 Jun 08 at 05:35:48.3 TD (05:28:00.4 UT1) 2557623.727783
Ecliptic Conjunction 2290 Jun 08 at 05:26:50.9 TD (05:19:03.1 UT1) 2557623.721563
Equatorial Conjunction 2290 Jun 08 at 05:35:23.5 TD (05:27:35.7 UT1) 2557623.727497
Geocentric Coordinates of Sun and Moon
2290 Jun 08 at 05:35:48.3 TD (05:28:00.4 UT1)
Coordinate Sun Moon
Right Ascension05h06m22.0s05h06m23.0s
Declination+22°49'46.7"+23°41'35.7"
Semi-Diameter 15'46.1" 16'14.7"
Eq. Hor. Parallax 08.7" 0°59'37.1"
Geocentric Libration of Moon
Angle Value
l 4.0°
b -1.1°
c -6.8°
Prediction Paramaters
Paramater Value
Ephemerides JPL DE406
ΔT 467.8 s
k (penumbra) 0.2725076
k (umbra) 0.2722810
Saros Series 132 (61/71)

Explanation of Solar Eclipse Data Tables

Penumbral Shadow Contacts and Extremes: Total Solar Eclipse of 2290 Jun 08

Contacts of Penumbral Shadow with Earth
Contact Event Contact Time
TD
Time
UT1
Latitude Longitude
First External ContactP103:21:36.003:13:48.131°49.3'N026°19.1'E
Last External ContactP407:50:05.007:42:17.231°21.0'N169°11.9'E
Extreme Northern and Southern Path Limits of Penumbra
Contact Event Contact Time
TD
Time
UT1
Latitude Longitude
North Extreme Path Limit 1N103:47:06.803:39:19.018°34.1'N026°56.9'E
South Extreme Path Limit 1S107:24:33.007:16:45.218°04.8'N168°37.1'E

Explanation of Penumbral Shadow Contacts and Extremes Tables

Umbral Shadow Contacts and Extremes: Total Solar Eclipse of 2290 Jun 08

Contacts of Umbral Shadow with Earth
Contact Event Contact Time
TD
Time
UT1
Latitude Longitude
First External ContactU104:42:33.404:34:45.553°16.2'N013°07.2'W
First Internal ContactU204:46:01.004:38:13.254°30.0'N015°48.7'W
Last Internal ContactU306:25:38.106:17:50.254°06.1'N148°59.4'W
Last External ContactU406:29:01.306:21:13.552°53.4'N151°35.5'W
Extreme Northern and Southern Path Limits of Umbra
Contact Event Contact Time
TD
Time
UT1
Latitude Longitude
North Extreme Path Limit 1N104:45:51.904:38:04.154°35.1'N015°54.2'W
South Extreme Path Limit 1S104:42:43.204:34:55.453°10.8'N013°01.9'W
North Extreme Path Limit 2N206:25:47.006:17:59.254°11.0'N148°54.2'W
South Extreme Path Limit 2S206:28:51.706:21:03.952°48.0'N151°40.5'W

Explanation of Umbral Shadow Contacts and Extremes Tables

Central Line Extremes and Duration: Total Solar Eclipse of 2290 Jun 08

Extreme Limits of the Central Line
Contact Event Contact Time
TD
Time
UT1
Latitude Longitude
Extreme Central Line Limit 1C104:44:15.904:36:28.153°52.6'N014°25.7'W
Extreme Central Line Limit 2C206:27:21.006:19:33.253°29.2'N150°19.6'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 Eclipse05:35:48.305:28:00.483°48.8'N098°00.6'E 29.0° 182.2° 264.8 km02m14.43s
Greatest Duration05:34:49.805:27:01.983°48.9'N095°19.7'E 29.0° 177.0° 264.9 km02m14.44s

Explanation of Greatest Eclipse and Greatest Duration

Polynomial Besselian Elements: Total Solar Eclipse of 2290 Jun 08

Polynomial Besselian Elements
2290 Jun 08 at 06:00:00.0 TD (=t0)
n x y d l1 l2 μ
0 0.23232 0.87023 22.8290 0.53833 -0.00779 270.1003
1 0.56644 -0.00270 0.0037 0.00009 0.00009 14.9994
2 -0.00003 -0.00021 -0.0000 -0.00001 -0.00001 -0.0000
3 -0.00001 0.00000 - - - -
Tan ƒ1 0.0046095
Tan ƒ2 0.0045866

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 2290 Jun 08

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 2290 Jun 08 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 467.8 seconds for this eclipse. The uncertainty in ΔT is 122.3 seconds corresponding to a standard error in longitude of the eclipse path of ± 0.51°.

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.