Solar eclipse of November 15, 2096 | |
---|---|
Type of eclipse | |
Nature | Annular |
Gamma | −0.20 |
Magnitude | 0.9237 |
Maximum eclipse | |
Duration | 533 s (8 min 53 s) |
Coordinates | 29°42′S163°18′E / 29.7°S 163.3°E |
Max. width of band | 294 km (183 mi) |
Times (UTC) | |
Greatest eclipse | 0:36:15 |
References | |
Saros | 144 (21 of 70) |
Catalog # (SE5000) | 9725 |
An annular solar eclipse will occur at the Moon's descending node of orbit between Wednesday, November 14 and Thursday, November 15, 2096, with a magnitude of 0.9237. A solar eclipse occurs when the Moon passes between Earth and the Sun, thereby totally or partly obscuring the image of the Sun for a viewer on Earth. An annular solar eclipse occurs when the Moon's apparent diameter is smaller than the Sun's, blocking most of the Sun's light and causing the Sun to look like an annulus (ring). An annular eclipse appears as a partial eclipse over a region of the Earth thousands of kilometres wide.
This eclipse is a member of a semester series. An eclipse in a semester series of solar eclipses repeats approximately every 177 days and 4 hours (a semester) at alternating nodes of the Moon's orbit. [1]
The solar eclipses on January 16, 2094 (total) and July 12, 2094 (partial) occur in the previous lunar year eclipse set, and the partial solar eclipses on April 1, 2098 and September 25, 2098 occur in the next lunar year eclipse set.
Solar eclipse series sets from 2094 to 2098 | ||||||
---|---|---|---|---|---|---|
Ascending node | Descending node | |||||
Saros | Map | Gamma | Saros | Map | Gamma | |
119 | June 13, 2094 ![]() Partial | −1.4613 | 124 | December 7, 2094 ![]() Partial | 1.1547 | |
129 | June 2, 2095 ![]() Total | −0.6396 | 134 | November 27, 2095 ![]() Annular | 0.4903 | |
139 | May 22, 2096 ![]() Total | 0.1196 | 144 | November 15, 2096 ![]() Annular | −0.20 | |
149 | May 11, 2097 ![]() Total | 0.8516 | 154 | November 4, 2097 ![]() Annular | −0.8926 | |
159 | May 1, 2098 | 164 | October 24, 2098 ![]() Partial | −1.5407 |
This eclipse is a part of Saros series 144, repeating every 18 years, 11 days, and containing 70 events. The series started with a partial solar eclipse on April 11, 1736. It contains annular eclipses from July 7, 1880 through August 27, 2565. There are no hybrid or total eclipses in this set. The series ends at member 70 as a partial eclipse on May 5, 2980. Its eclipses are tabulated in three columns; every third eclipse in the same column is one exeligmos apart, so they all cast shadows over approximately the same parts of the Earth.
The longest duration of annularity will be produced by member 51 at 9 minutes, 52 seconds on December 29, 2168. All eclipses in this series occur at the Moon’s descending node of orbit. [2]
Series members 5–26 occur between 1801 and 2200: | ||
---|---|---|
5 | 6 | 7 |
![]() May 25, 1808 | ![]() June 5, 1826 | ![]() June 16, 1844 |
8 | 9 | 10 |
![]() June 27, 1862 | ![]() July 7, 1880 | ![]() July 18, 1898 |
11 | 12 | 13 |
![]() July 30, 1916 | ![]() August 10, 1934 | ![]() August 20, 1952 |
14 | 15 | 16 |
![]() August 31, 1970 | ![]() September 11, 1988 | ![]() September 22, 2006 |
17 | 18 | 19 |
![]() October 2, 2024 | ![]() October 14, 2042 | ![]() October 24, 2060 |
20 | 21 | 22 |
![]() November 4, 2078 | ![]() November 15, 2096 | ![]() November 27, 2114 |
23 | 24 | 25 |
![]() December 7, 2132 | ![]() December 19, 2150 | ![]() December 29, 2168 |
26 | ||
![]() January 9, 2187 |
The metonic 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 descending node.
22 eclipse events between June 23, 2047 and November 16, 2134 | ||||
---|---|---|---|---|
June 22–23 | April 10–11 | January 27–29 | November 15–16 | September 3–5 |
118 | 120 | 122 | 124 | 126 |
![]() June 23, 2047 | ![]() April 11, 2051 | ![]() January 27, 2055 | ![]() November 16, 2058 | ![]() September 3, 2062 |
128 | 130 | 132 | 134 | 136 |
![]() June 22, 2066 | ![]() April 11, 2070 | ![]() January 27, 2074 | ![]() November 15, 2077 | ![]() September 3, 2081 |
138 | 140 | 142 | 144 | 146 |
![]() June 22, 2085 | ![]() April 10, 2089 | ![]() January 27, 2093 | ![]() November 15, 2096 | ![]() September 4, 2100 |
148 | 150 | 152 | 154 | 156 |
![]() June 22, 2104 | ![]() April 11, 2108 | ![]() January 29, 2112 | ![]() November 16, 2115 | ![]() September 5, 2119 |
158 | 160 | 162 | 164 | |
![]() June 23, 2123 | ![]() November 16, 2134 |
This eclipse is a part of a tritos cycle, repeating at alternating nodes every 135 synodic months (≈ 3986.63 days, or 11 years minus 1 month). Their appearance and longitude are irregular due to a lack of synchronization with the anomalistic 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 | ||||
---|---|---|---|---|
![]() March 4, 1802 (Saros 117) | ![]() February 1, 1813 (Saros 118) | ![]() January 1, 1824 (Saros 119) | ![]() November 30, 1834 (Saros 120) | ![]() October 30, 1845 (Saros 121) |
![]() September 29, 1856 (Saros 122) | ![]() August 29, 1867 (Saros 123) | ![]() July 29, 1878 (Saros 124) | ![]() June 28, 1889 (Saros 125) | ![]() May 28, 1900 (Saros 126) |
![]() April 28, 1911 (Saros 127) | ![]() March 28, 1922 (Saros 128) | ![]() February 24, 1933 (Saros 129) | ![]() January 25, 1944 (Saros 130) | ![]() December 25, 1954 (Saros 131) |
![]() November 23, 1965 (Saros 132) | ![]() October 23, 1976 (Saros 133) | ![]() September 23, 1987 (Saros 134) | ![]() August 22, 1998 (Saros 135) | ![]() July 22, 2009 (Saros 136) |
![]() June 21, 2020 (Saros 137) | ![]() May 21, 2031 (Saros 138) | ![]() April 20, 2042 (Saros 139) | ![]() March 20, 2053 (Saros 140) | ![]() February 17, 2064 (Saros 141) |
![]() January 16, 2075 (Saros 142) | ![]() December 16, 2085 (Saros 143) | ![]() November 15, 2096 (Saros 144) | ![]() October 16, 2107 (Saros 145) | ![]() September 15, 2118 (Saros 146) |
![]() August 15, 2129 (Saros 147) | ![]() July 14, 2140 (Saros 148) | ![]() June 14, 2151 (Saros 149) | ![]() May 14, 2162 (Saros 150) | ![]() April 12, 2173 (Saros 151) |
![]() March 12, 2184 (Saros 152) | ![]() February 10, 2195 (Saros 153) |
This eclipse is a part of the long period inex cycle, repeating at alternating nodes, every 358 synodic months (≈ 10,571.95 days, or 29 years minus 20 days). Their appearance and longitude are irregular due to a lack of synchronization with the anomalistic 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 | ||
---|---|---|
![]() June 6, 1807 (Saros 134) | ![]() May 15, 1836 (Saros 135) | ![]() April 25, 1865 (Saros 136) |
![]() April 6, 1894 (Saros 137) | ![]() March 17, 1923 (Saros 138) | ![]() February 25, 1952 (Saros 139) |
![]() February 4, 1981 (Saros 140) | ![]() January 15, 2010 (Saros 141) | ![]() December 26, 2038 (Saros 142) |
![]() December 6, 2067 (Saros 143) | ![]() November 15, 2096 (Saros 144) | ![]() October 26, 2125 (Saros 145) |
![]() October 7, 2154 (Saros 146) | ![]() September 16, 2183 (Saros 147) |
An annular solar eclipse occurred at the Moon's descending node of orbit on Friday, September 22, 2006, with a magnitude of 0.9352. A solar eclipse occurs when the Moon passes between Earth and the Sun, thereby totally or partly obscuring the image of the Sun for a viewer on Earth. An annular solar eclipse occurs when the Moon's apparent diameter is smaller than the Sun's, blocking most of the Sun's light and causing the Sun to look like an annulus (ring). An annular eclipse appears as a partial eclipse over a region of the Earth thousands of kilometres wide. The path of annularity of this eclipse passed through Guyana, Suriname, French Guiana, the northern tip of Roraima and Amapá of Brazil, and the southern Atlantic.
A total solar eclipse will occur at the Moon's ascending node of orbit between Monday, May 21 and Tuesday, May 22, 2096, with a magnitude of 1.0737. A solar eclipse occurs when the Moon passes between Earth and the Sun, thereby totally or partly obscuring the image of the Sun for a viewer on Earth. A total solar eclipse occurs when the Moon's apparent 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. This will be the first eclipse of saros series 139 to exceed series 136 in length of totality. The length of totality for saros 139 is increasing, while that of Saros 136 is decreasing.
A total solar eclipse occurred at the Moon's ascending node of orbit on Sunday, October 12, 1958, with a magnitude of 1.0608. A solar eclipse occurs when the Moon passes between Earth and the Sun, thereby totally or partly obscuring the image of the Sun for a viewer on Earth. A total solar eclipse occurs when the Moon's apparent 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. Totality was visible in Tokelau, Cook Islands, French Polynesia, Chile and Argentina. This solar eclipse occurred over 3 months after the final game of 1958 FIFA World Cup.
An annular solar eclipse occurred at the Moon's descending node of orbit on Monday, August 21, 1933, with a magnitude of 0.9801. A solar eclipse occurs when the Moon passes between Earth and the Sun, thereby totally or partly obscuring the image of the Sun for a viewer on Earth. An annular solar eclipse occurs when the Moon's apparent diameter is smaller than the Sun's, blocking most of the Sun's light and causing the Sun to look like an annulus (ring). An annular eclipse appears as a partial eclipse over a region of the Earth thousands of kilometres wide. Annularity was visible from Italian Libya, Egypt, Mandatory Palestine including Jerusalem and Amman, French Mandate for Syria and the Lebanon, Iraq including Baghdad, Persia, Afghanistan, British Raj, Siam, Dutch East Indies, North Borneo, and Australia.
An annular solar eclipse will occur at the Moon's descending node of orbit on Monday, May 31, 2049, with a magnitude of 0.9631. A solar eclipse occurs when the Moon passes between Earth and the Sun, thereby totally or partly obscuring the image of the Sun for a viewer on Earth. An annular solar eclipse occurs when the Moon's apparent diameter is smaller than the Sun's, blocking most of the Sun's light and causing the Sun to look like an annulus (ring). An annular eclipse appears as a partial eclipse over a region of the Earth thousands of kilometres wide.
An annular solar eclipse will occur at the Moon's ascending node of orbit on Friday, July 2, 2038, with a magnitude of 0.9911. A solar eclipse occurs when the Moon passes between Earth and the Sun, thereby totally or partly obscuring the image of the Sun for a viewer on Earth. An annular solar eclipse occurs when the Moon's apparent diameter is smaller than the Sun's, blocking most of the Sun's light and causing the Sun to look like an annulus (ring). An annular eclipse appears as a partial eclipse over a region of the Earth thousands of kilometres wide.
An annular solar eclipse occurred at the Moon's descending node of orbit on Friday, January 25, 1963, with a magnitude of 0.9951. A solar eclipse occurs when the Moon passes between Earth and the Sun, thereby totally or partly obscuring the image of the Sun for a viewer on Earth. An annular solar eclipse occurs when the Moon's apparent diameter is smaller than the Sun's, blocking most of the Sun's light and causing the Sun to look like an annulus (ring). An annular eclipse appears as a partial eclipse over a region of the Earth thousands of kilometres wide. The path of annularity crossed Chile, Argentina, South Africa, southern Basutoland and Malagasy Republic. Occurring 3.7 days before perigee, the Moon's apparent diameter was larger. The moon was 374,860 km from the Earth.
A total solar eclipse will occur at the Moon's descending node of orbit on Tuesday, January 27, 2093, with a magnitude of 1.034. A solar eclipse occurs when the Moon passes between Earth and the Sun, thereby totally or partly obscuring the image of the Sun for a viewer on Earth. A total solar eclipse occurs when the Moon's apparent 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.
A total solar eclipse will occur at the Moon's descending node of orbit on Saturday, September 4, 2100, with a magnitude of 1.0402. It will be the last solar eclipse of the 21st century. A solar eclipse occurs when the Moon passes between Earth and the Sun, thereby totally or partly obscuring the image of the Sun for a viewer on Earth. A total solar eclipse occurs when the Moon's apparent 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.
An annular solar eclipse will occur at the Moon's descending node of orbit on Sunday, January 16, 2056, with a magnitude of 0.9759. A solar eclipse occurs when the Moon passes between Earth and the Sun, thereby totally or partly obscuring the image of the Sun for a viewer on Earth. An annular solar eclipse occurs when the Moon's apparent diameter is smaller than the Sun's, blocking most of the Sun's light and causing the Sun to look like an annulus (ring). An annular eclipse appears as a partial eclipse over a region of the Earth thousands of kilometres wide.
An annular solar eclipse will occur at the Moon's descending node of orbit on Saturday, June 11, 2067, with a magnitude of 0.967. A solar eclipse occurs when the Moon passes between Earth and the Sun, thereby totally or partly obscuring the image of the Sun for a viewer on Earth. An annular solar eclipse occurs when the Moon's apparent diameter is smaller than the Sun's, blocking most of the Sun's light and causing the Sun to look like an annulus (ring). An annular eclipse appears as a partial eclipse over a region of the Earth thousands of kilometres wide.
An annular solar eclipse will occur at the Moon's ascending node of orbit on Sunday, December 16, 2085, with a magnitude of 0.9971. A solar eclipse occurs when the Moon passes between Earth and the Sun, thereby totally or partly obscuring the image of the Sun for a viewer on Earth. An annular solar eclipse occurs when the Moon's apparent diameter is smaller than the Sun's, blocking most of the Sun's light and causing the Sun to look like an annulus (ring). An annular eclipse appears as a partial eclipse over a region of the Earth thousands of kilometres wide. If a moon with same apparent diameter in this eclipse near the Aphelion, it will be Total Solar Eclipse, but in this time of the year, just 2 weeks and 4 days before perihelion, it is an Annular Solar Eclipse.
An annular solar eclipse will occur at the Moon's descending node of orbit on Saturday, January 27, 2074, with a magnitude of 0.9798. A solar eclipse occurs when the Moon passes between Earth and the Sun, thereby totally or partly obscuring the image of the Sun for a viewer on Earth. An annular solar eclipse occurs when the Moon's apparent diameter is smaller than the Sun's, blocking most of the Sun's light and causing the Sun to look like an annulus (ring). An annular eclipse appears as a partial eclipse over a region of the Earth thousands of kilometres wide.
A total solar eclipse will occur at the Moon's descending node of orbit on Monday, August 24, 2082, with a magnitude of 1.0452. A solar eclipse occurs when the Moon passes between Earth and the Sun, thereby totally or partly obscuring the image of the Sun for a viewer on Earth. A total solar eclipse occurs when the Moon's apparent 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.
An annular solar eclipse will occur at the Moon's ascending node of orbit on Saturday, March 21, 2099, with a magnitude of 0.93. A solar eclipse occurs when the Moon passes between Earth and the Sun, thereby totally or partly obscuring the image of the Sun for a viewer on Earth. An annular solar eclipse occurs when the Moon's apparent diameter is smaller than the Sun's, blocking most of the Sun's light and causing the Sun to look like an annulus (ring). An annular eclipse appears as a partial eclipse over a region of the Earth thousands of kilometres wide.
An annular solar eclipse will occur at the Moon's ascending node of orbit between Wednesday, March 10 and Thursday, March 11, 2100, with a magnitude of 0.9338. A solar eclipse occurs when the Moon passes between Earth and the Sun, thereby totally or partly obscuring the image of the Sun for a viewer on Earth. An annular solar eclipse occurs when the Moon's apparent diameter is smaller than the Sun's, blocking most of the Sun's light and causing the Sun to look like an annulus (ring). An annular eclipse appears as a partial eclipse over a region of the Earth thousands of kilometers wide. The path of annularity will move from Indonesia at sunrise, over the islands of Hawaii and Maui around noon, and through the northwestern United States at sunset.
An annular solar eclipse will occur at the Moon's ascending node of orbit on Thursday, July 23, 2093, with a magnitude of 0.9463. A solar eclipse occurs when the Moon passes between Earth and the Sun, thereby totally or partly obscuring the image of the Sun for a viewer on Earth. An annular solar eclipse occurs when the Moon's apparent diameter is smaller than the Sun's, blocking most of the Sun's light and causing the Sun to look like an annulus (ring). An annular eclipse appears as a partial eclipse over a region of the Earth thousands of kilometres wide.
An annular solar eclipse will occur at the Moon's descending node of orbit on Friday, June 22, 2085, with a magnitude of 0.9704. A solar eclipse occurs when the Moon passes between Earth and the Sun, thereby totally or partly obscuring the image of the Sun for a viewer on Earth. An annular solar eclipse occurs when the Moon's apparent diameter is smaller than the Sun's, blocking most of the Sun's light and causing the Sun to look like an annulus (ring). An annular eclipse appears as a partial eclipse over a region of the Earth thousands of kilometres wide.
An annular solar eclipse occurred at the Moon's ascending node of orbit on Thursday, July 20, 1944, with a magnitude of 0.97. A solar eclipse occurs when the Moon passes between Earth and the Sun, thereby totally or partly obscuring the image of the Sun for a viewer on Earth. An annular solar eclipse occurs when the Moon's apparent diameter is smaller than the Sun's, blocking most of the Sun's light and causing the Sun to look like an annulus (ring). An annular eclipse appears as a partial eclipse over a region of the Earth thousands of kilometres wide. Annularity was visible from British Uganda, Anglo-Egyptian Sudan, British Kenya, Ethiopia, British Somaliland, British Raj, Burma, Thailand, French Indochina, Philippines, South Seas Mandate in Japan the Territory of New Guinea.
An annular solar eclipse occurred at the Moon's ascending node of orbit on Friday, February 24, 1933, with a magnitude of 0.9841. A solar eclipse occurs when the Moon passes between Earth and the Sun, thereby totally or partly obscuring the image of the Sun for a viewer on Earth. An annular solar eclipse occurs when the Moon's apparent diameter is smaller than the Sun's, blocking most of the Sun's light and causing the Sun to look like an annulus (ring). An annular eclipse appears as a partial eclipse over a region of the Earth thousands of kilometres wide. Annularity was visible from Chile, Argentina, Portuguese Angola, French Equatorial Africa, Belgian Congo, Anglo-Egyptian Sudan, Ethiopia, French Somaliland, southeastern Italian Eritrea, and Mutawakkilite Kingdom of Yemen, Aden Protectorate and Aden Province in British Raj.