| Total eclipse | |
Totality withdiamond ring effect inLitoral Province, Bolivia | |
| Gamma | −0.3522 |
|---|---|
| Magnitude | 1.0535 |
| Maximum eclipse | |
| Duration | 263 s (4 min 23 s) |
| Coordinates | 35°24′S34°12′W / 35.4°S 34.2°W /-35.4; -34.2 |
| Max. width of band | 189 km (117 mi) |
| Times (UTC) | |
| Greatest eclipse | 13:40:06 |
| References | |
| Saros | 133 (44 of 72) |
| Catalog # (SE5000) | 9496 |
A totalsolar eclipse occurred at the Moon'sascending node of orbit on Thursday, November 3, 1994,[1][2][3][4][5][6][7][8][9][10][11] with amagnitude of 1.0535. Asolar eclipse occurs when theMoon passes betweenEarth and theSun, thereby totally or partly obscuring the image of the Sun for a viewer on Earth. A total solar eclipse occurs when the Moon'sapparent diameter is larger than the Sun's, blocking all direct sunlight, turning day into darkness. Totality occurs in a narrow path across Earth's surface, with the partial solar eclipse visible over a surrounding region thousands of kilometres wide. Occurring about 10 hours afterperigee (on November 3, 1994, at 23:40 UTC), the Moon's apparent diameter was larger.[12]
Totality was visible inPeru, northernChile,Bolivia, northernArgentina,Paraguay,Brazil andGough Island ofBritish overseas territory ofSaint Helena, Ascension and Tristan da Cunha. TheIguazu Falls, one of the largest waterfalls systems in the world, lay in the path of totality. A partial eclipse was visible for parts ofCentral America,South America,Antarctica, andSouthern Africa.
Jay Pasachoff led an observation team fromWilliams College inMassachusetts, observing the total eclipse at a military base nearPutre, Chile, in theAtacama Desert. The team took images of the corona and measured its brightness. Teams fromJapan andSouth Korea also conducted observations nearby.[13] TheRussian Academy of Sciences sent a team toCriciúma, Brazil, taking images of the corona inpolarized light and proposing reconstruction of its ray structure.[14]
| Country or territory | City or place | Start of partial eclipse | Start of total eclipse | Maximum eclipse | End of total eclipse | End of partial eclipse | Duration of totality (min:s) | Duration of eclipse (hr:min) | Maximum magnitude |
|---|---|---|---|---|---|---|---|---|---|
| Arequipa | 06:14:46 | 07:15:56 | 07:16:15 | 07:16:35 | 08:25:44 | 0:39 | 2:11 | 1.0009 | |
| Arica | 08:17:25 | 09:18:49 | 09:19:48 | 09:20:46 | 10:30:17 | 1:57 | 2:13 | 1.0061 | |
| Potosí | 07:20:12 | 08:23:47 | 08:25:08 | 08:26:30 | 09:38:45 | 2:43 | 2:19 | 1.0115 | |
| Asunción | 08:32:40 | 09:42:22 | 09:42:51 | 09:43:21 | 11:01:57 | 0:59 | 2:29 | 1.0013 | |
| Caraguatay | 08:33:12 | 09:42:16 | 09:43:53 | 09:45:31 | 11:03:32 | 3:15 | 2:30 | 1.0136 | |
| Ciudad del Este | 08:35:24 | 09:45:47 | 09:47:28 | 09:49:10 | 11:08:31 | 3:23 | 2:33 | 1.0142 | |
| Foz do Iguaçu | 09:35:28 | 10:45:51 | 10:47:33 | 10:49:16 | 12:08:38 | 3:25 | 2:33 | 1.0146 | |
| Criciúma | 09:45:28 | 10:58:46 | 11:00:47 | 11:02:49 | 12:24:16 | 4:03 | 2:39 | 1.0255 | |
| References:[1] | |||||||||
| Country or territory | City or place | Start of partial eclipse | Maximum eclipse | End of partial eclipse | Duration of eclipse (hr:min) | Maximum coverage | |||
|---|---|---|---|---|---|---|---|---|---|
| Bogotá | 06:08:03 | 06:55:47 | 07:48:15 | 1:40 | 32.05% | ||||
| Galápagos Islands | 05:37:33 (sunrise) | 05:57:05 | 06:52:44 | 1:15 | 69.86% | ||||
| Quito | 06:05:12 | 06:57:28 | 07:55:23 | 1:50 | 54.12% | ||||
| Leticia | 06:07:23 | 07:04:02 | 08:07:39 | 2:00 | 56.19% | ||||
| Lima | 06:10:01 | 07:08:15 | 08:13:37 | 2:04 | 94.49% | ||||
| La Paz | 07:15:44 | 08:18:54 | 09:30:30 | 2:15 | 96.11% | ||||
| Iquique | 08:19:40 | 09:22:16 | 10:32:54 | 2:13 | 96.40% | ||||
| Sucre | 07:19:42 | 08:24:49 | 09:38:42 | 2:19 | 99.39% | ||||
| Antofagasta | 08:24:33 | 09:26:55 | 10:36:57 | 2:12 | 85.24% | ||||
| Pedro Juan Caballero | 08:30:12 | 09:41:15 | 11:01:39 | 2:31 | 95.08% | ||||
| Santiago | 08:42:11 | 09:41:37 | 10:47:04 | 2:05 | 56.35% | ||||
| Encarnación | 08:37:14 | 09:48:30 | 11:08:24 | 2:31 | 97.60% | ||||
| Buenos Aires | 08:48:54 | 09:56:35 | 11:11:07 | 2:22 | 71.07% | ||||
| São Paulo | 09:41:33 | 10:57:48 | 12:22:49 | 2:41 | 82.18% | ||||
| Montevideo | 08:50:52 | 09:59:59 | 11:15:54 | 2:25 | 73.58% | ||||
| Rio de Janeiro | 09:46:03 | 11:03:43 | 12:29:35 | 2:44 | 73.89% | ||||
| King Edward Point | 10:48:38 | 11:50:39 | 12:53:27 | 2:05 | 39.73% | ||||
| Edinburgh of the Seven Seas | 13:03:19 | 14:25:50 | 15:42:52 | 2:40 | 92.88% | ||||
| Bouvet Island | 14:33:42 | 15:36:37 | 16:36:12 | 2:03 | 51.94% | ||||
| Antananarivo | 17:32:37 | 17:55:07 | 17:58:22 (sunset) | 0:26 | 25.47% | ||||
| Île de la Possession | 19:11:52 | 20:01:38 | 20:27:46 (sunset) | 1:16 | 51.99% | ||||
| Cape Town | 16:00:38 | 17:08:14 | 18:08:57 | 2:08 | 86.75% | ||||
| Windhoek | 16:14:02 | 17:15:01 | 18:09:34 | 1:56 | 42.15% | ||||
| Maseru | 16:14:37 | 17:16:32 | 18:12:23 | 1:58 | 75.77% | ||||
| Toliara | 17:27:57 | 18:17:03 | 18:19:29 (sunset) | 0:52 | 66.89% | ||||
| Johannesburg | 16:18:49 | 17:18:53 | 18:13:05 | 1:54 | 64.35% | ||||
| Gaborone | 16:19:19 | 17:19:06 | 18:12:55 | 1:54 | 56.67% | ||||
| Mbabane | 16:20:38 | 17:19:38 | 18:13:03 | 1:53 | 67.57% | ||||
| Maputo | 16:21:50 | 17:20:08 | 18:07:26 (sunset) | 1:46 | 67.51% | ||||
| Harare | 16:32:40 | 17:24:08 | 18:02:58 (sunset) | 1:30 | 36.40% | ||||
| References:[1] | |||||||||
Shown below are two tables displaying details about this particular solar eclipse. The first table outlines times at which the Moon's penumbra or umbra attains the specific parameter, and the second table describes various other parameters pertaining to this eclipse.[15]
| Event | Time (UTC) |
|---|---|
| First Penumbral External Contact | 1994 November 03 at 11:06:00.2 UTC |
| First Umbral External Contact | 1994 November 03 at 12:02:38.7 UTC |
| First Central Line | 1994 November 03 at 12:03:41.3 UTC |
| First Umbral Internal Contact | 1994 November 03 at 12:04:44.0 UTC |
| First Penumbral Internal Contact | 1994 November 03 at 13:09:15.5 UTC |
| Ecliptic Conjunction | 1994 November 03 at 13:36:30.1 UTC |
| Greatest Eclipse | 1994 November 03 at 13:40:06.0 UTC |
| Greatest Duration | 1994 November 03 at 13:42:38.8 UTC |
| Equatorial Conjunction | 1994 November 03 at 13:48:07.6 UTC |
| Last Penumbral Internal Contact | 1994 November 03 at 14:10:44.2 UTC |
| Last Umbral Internal Contact | 1994 November 03 at 15:15:21.7 UTC |
| Last Central Line | 1994 November 03 at 15:16:24.9 UTC |
| Last Umbral External Contact | 1994 November 03 at 15:17:28.1 UTC |
| Last Penumbral External Contact | 1994 November 03 at 16:14:07.1 UTC |
| Parameter | Value |
|---|---|
| Eclipse Magnitude | 1.05351 |
| Eclipse Obscuration | 1.10989 |
| Gamma | −0.35216 |
| Sun Right Ascension | 14h33m55.8s |
| Sun Declination | -15°05'51.1" |
| Sun Semi-Diameter | 16'07.4" |
| Sun Equatorial Horizontal Parallax | 08.9" |
| Moon Right Ascension | 14h33m36.5s |
| Moon Declination | -15°26'53.7" |
| Moon Semi-Diameter | 16'43.0" |
| Moon Equatorial Horizontal Parallax | 1°01'21.1" |
| ΔT | 60.6 s |
This eclipse is part of aneclipse season, a period, roughly every six months, when eclipses occur. Only two (or occasionally three) eclipse seasons occur each year, and each season lasts about 35 days and repeats just short of six months (173 days) later; thus two full eclipse seasons always occur each year. Either two or three eclipses happen each eclipse season. In the sequence below, each eclipse is separated by afortnight.
| November 3 Ascending node (new moon) | November 18 Descending node (full moon) |
|---|---|
| Total solar eclipse Solar Saros 133 | Penumbral lunar eclipse Lunar Saros 145 |
This eclipse is a member of asemester series. An eclipse in a semester series of solar eclipses repeats approximately every 177 days and 4 hours (a semester) at alternatingnodes of the Moon's orbit.[16]
| Solar eclipse series sets from 1993 to 1996 | ||||||
|---|---|---|---|---|---|---|
| Descending node | Ascending node | |||||
| Saros | Map | Gamma | Saros | Map | Gamma | |
| 118 | May 21, 1993 Partial | 1.1372 | 123 | November 13, 1993 Partial | −1.0411 | |
| 128 Partial inBismarck, ND, USA | May 10, 1994 Annular | 0.4077 | 133 Totality inBolivia | November 3, 1994 Total | −0.3522 | |
| 138 | April 29, 1995 Annular | −0.3382 | 143 Totality inDundlod,India | October 24, 1995 Total | 0.3518 | |
| 148 | April 17, 1996 Partial | −1.058 | 153 | October 12, 1996 Partial | 1.1227 | |
This eclipse is a part ofSaros series 133, repeating every 18 years, 11 days, and containing 72 events. The series started with a partial solar eclipse on July 13, 1219. It contains annular eclipses from November 20, 1435 through January 13, 1526; a hybrid eclipse on January 24, 1544; and total eclipses from February 3, 1562 through June 21, 2373. The series ends at member 72 as a partial eclipse on September 5, 2499. Its eclipses are tabulated in three columns; every third eclipse in the same column is oneexeligmos apart, so they all cast shadows over approximately the same parts of the Earth.
The longest duration of annularity was produced by member 25 at 1 minutes, 14 seconds on November 30, 1453, and the longest duration of totality was produced by member 61 at 6 minutes, 50 seconds on August 7, 1850. All eclipses in this series occur at the Moon’sascending node of orbit.[17]
| Series members 34–55 occur between 1801 and 2200: | ||
|---|---|---|
| 34 | 35 | 36 |
July 17, 1814 | July 27, 1832 | August 7, 1850 |
| 37 | 38 | 39 |
August 18, 1868 | August 29, 1886 | September 9, 1904 |
| 40 | 41 | 42 |
September 21, 1922 | October 1, 1940 | October 12, 1958 |
| 43 | 44 | 45 |
October 23, 1976 | November 3, 1994 | November 13, 2012 |
| 46 | 47 | 48 |
November 25, 2030 | December 5, 2048 | December 17, 2066 |
| 49 | 50 | 51 |
December 27, 2084 | January 8, 2103 | January 19, 2121 |
| 52 | 53 | 54 |
January 30, 2139 | February 9, 2157 | February 21, 2175 |
| 55 | ||
March 3, 2193 | ||
Themetonic series repeats eclipses every 19 years (6939.69 days), lasting about 5 cycles. Eclipses occur in nearly the same calendar date. In addition, the octon subseries repeats 1/5 of that or every 3.8 years (1387.94 days). All eclipses in this table occur at the Moon's ascending node.
| 20 eclipse events between June 10, 1964 and August 21, 2036 | ||||
|---|---|---|---|---|
| June 10–11 | March 28–29 | January 14–16 | November 3 | August 21–22 |
| 117 | 119 | 121 | 123 | 125 |
June 10, 1964 | March 28, 1968 | January 16, 1972 | November 3, 1975 | August 22, 1979 |
| 127 | 129 | 131 | 133 | 135 |
June 11, 1983 | March 29, 1987 | January 15, 1991 | November 3, 1994 | August 22, 1998 |
| 137 | 139 | 141 | 143 | 145 |
June 10, 2002 | March 29, 2006 | January 15, 2010 | November 3, 2013 | August 21, 2017 |
| 147 | 149 | 151 | 153 | 155 |
June 10, 2021 | March 29, 2025 | January 14, 2029 | November 3, 2032 | August 21, 2036 |
This eclipse is a part of atritos cycle, repeating at alternating nodes every 135synodic months (≈ 3986.63 days, or 11 years minus 1 month). Their appearance and longitude are irregular due to a lack of synchronization with theanomalistic month (period of perigee), but groupings of 3 tritos cycles (≈ 33 years minus 3 months) come close (≈ 434.044 anomalistic months), so eclipses are similar in these groupings.
| Series members between 1801 and 2200 | ||||
|---|---|---|---|---|
April 14, 1809 (Saros 116) | March 14, 1820 (Saros 117) | February 12, 1831 (Saros 118) | January 11, 1842 (Saros 119) | December 11, 1852 (Saros 120) |
November 11, 1863 (Saros 121) | October 10, 1874 (Saros 122) | September 8, 1885 (Saros 123) | August 9, 1896 (Saros 124) | July 10, 1907 (Saros 125) |
June 8, 1918 (Saros 126) | May 9, 1929 (Saros 127) | April 7, 1940 (Saros 128) | March 7, 1951 (Saros 129) | February 5, 1962 (Saros 130) |
January 4, 1973 (Saros 131) | December 4, 1983 (Saros 132) | November 3, 1994 (Saros 133) | October 3, 2005 (Saros 134) | September 1, 2016 (Saros 135) |
August 2, 2027 (Saros 136) | July 2, 2038 (Saros 137) | May 31, 2049 (Saros 138) | April 30, 2060 (Saros 139) | March 31, 2071 (Saros 140) |
February 27, 2082 (Saros 141) | January 27, 2093 (Saros 142) | December 29, 2103 (Saros 143) | November 27, 2114 (Saros 144) | October 26, 2125 (Saros 145) |
September 26, 2136 (Saros 146) | August 26, 2147 (Saros 147) | July 25, 2158 (Saros 148) | June 25, 2169 (Saros 149) | May 24, 2180 (Saros 150) |
April 23, 2191 (Saros 151) | ||||
This eclipse is a part of the long periodinex cycle, repeating at alternating nodes, every 358synodic months (≈ 10,571.95 days, or 29 years minus 20 days). Their appearance and longitude are irregular due to a lack of synchronization with theanomalistic month (period of perigee). However, groupings of 3 inex cycles (≈ 87 years minus 2 months) comes close (≈ 1,151.02 anomalistic months), so eclipses are similar in these groupings.
| Series members between 1801 and 2200 | ||
|---|---|---|
March 4, 1821 (Saros 127) | February 12, 1850 (Saros 128) | January 22, 1879 (Saros 129) |
January 3, 1908 (Saros 130) | December 13, 1936 (Saros 131) | November 23, 1965 (Saros 132) |
November 3, 1994 (Saros 133) | October 14, 2023 (Saros 134) | September 22, 2052 (Saros 135) |
September 3, 2081 (Saros 136) | August 15, 2110 (Saros 137) | July 25, 2139 (Saros 138) |
July 5, 2168 (Saros 139) | June 15, 2197 (Saros 140) | |
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