Solar eclipse of November 2, 1910 | |
---|---|
Type of eclipse | |
Nature | Partial |
Gamma | 1.0603 |
Magnitude | 0.8515 |
Maximum eclipse | |
Coordinates | 61°54′N155°06′W / 61.9°N 155.1°W |
Times (UTC) | |
Greatest eclipse | 2:08:32 |
References | |
Saros | 122 (52 of 70) |
Catalog # (SE5000) | 9305 |
A partial solar eclipse occurred at the Moon's descending node of orbit on Wednesday, November 2, 1910, [1] [2] with a magnitude of 0.8515. 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 partial solar eclipse occurs in the polar regions of the Earth when the center of the Moon's shadow misses the Earth.
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. [3]
The partial solar eclipse on August 31, 1913 occurs in the next lunar year eclipse set.
Solar eclipse series sets from 1910 to 1913 | ||||||
---|---|---|---|---|---|---|
Ascending node | Descending node | |||||
Saros | Map | Gamma | Saros | Map | Gamma | |
117 | May 9, 1910 ![]() Total | −0.9437 | 122 | November 2, 1910 ![]() Partial | 1.0603 | |
127 | April 28, 1911 ![]() Total | −0.2294 | 132 | October 22, 1911 ![]() Annular | 0.3224 | |
137 | April 17, 1912 ![]() Hybrid | 0.528 | 142 | October 10, 1912 ![]() Total | −0.4149 | |
147 | April 6, 1913 ![]() Partial | 1.3147 | 152 | September 30, 1913 ![]() Partial | −1.1005 |
This eclipse is a part of Saros series 122, repeating every 18 years, 11 days, and containing 70 events. The series started with a partial solar eclipse on April 17, 991 AD. It contains total eclipses from July 12, 1135 through August 3, 1171; hybrid eclipses on August 13, 1189 and August 25, 1207; and annular eclipses from September 4, 1225 through October 10, 1874. The series ends at member 70 as a partial eclipse on May 17, 2235. 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 totality was produced by member 9 at 1 minutes, 25 seconds on July 12, 1135, and the longest duration of annularity was produced by member 50 at 6 minutes, 28 seconds on October 10, 1874. All eclipses in this series occur at the Moon’s descending node of orbit. [4]
Series members 46–68 occur between 1801 and 2200: | ||
---|---|---|
46 | 47 | 48 |
![]() August 28, 1802 | ![]() September 7, 1820 | ![]() September 18, 1838 |
49 | 50 | 51 |
![]() September 29, 1856 | ![]() October 10, 1874 | ![]() October 20, 1892 |
52 | 53 | 54 |
![]() November 2, 1910 | ![]() November 12, 1928 | ![]() November 23, 1946 |
55 | 56 | 57 |
![]() December 4, 1964 | ![]() December 15, 1982 | ![]() December 25, 2000 |
58 | 59 | 60 |
![]() January 6, 2019 | ![]() January 16, 2037 | ![]() January 27, 2055 |
61 | 62 | 63 |
![]() February 7, 2073 | ![]() February 18, 2091 | ![]() March 1, 2109 |
64 | 65 | 66 |
![]() March 13, 2127 | ![]() March 23, 2145 | ![]() April 3, 2163 |
67 | 68 | |
![]() April 14, 2181 | ![]() April 25, 2199 |
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 | ||||
---|---|---|---|---|
![]() September 8, 1801 (Saros 112) | ![]() August 7, 1812 (Saros 113) | ![]() July 8, 1823 (Saros 114) | ![]() June 7, 1834 (Saros 115) | ![]() May 6, 1845 (Saros 116) |
![]() April 5, 1856 (Saros 117) | ![]() March 6, 1867 (Saros 118) | ![]() February 2, 1878 (Saros 119) | ![]() January 1, 1889 (Saros 120) | ![]() December 3, 1899 (Saros 121) |
![]() November 2, 1910 (Saros 122) | ![]() October 1, 1921 (Saros 123) | ![]() August 31, 1932 (Saros 124) | ![]() August 1, 1943 (Saros 125) | ![]() June 30, 1954 (Saros 126) |
![]() May 30, 1965 (Saros 127) | ![]() April 29, 1976 (Saros 128) | ![]() March 29, 1987 (Saros 129) | ![]() February 26, 1998 (Saros 130) | ![]() January 26, 2009 (Saros 131) |
![]() December 26, 2019 (Saros 132) | ![]() November 25, 2030 (Saros 133) | ![]() October 25, 2041 (Saros 134) | ![]() September 22, 2052 (Saros 135) | ![]() August 24, 2063 (Saros 136) |
![]() July 24, 2074 (Saros 137) | ![]() June 22, 2085 (Saros 138) | ![]() May 22, 2096 (Saros 139) | ![]() April 23, 2107 (Saros 140) | ![]() March 22, 2118 (Saros 141) |
![]() February 18, 2129 (Saros 142) | ![]() January 20, 2140 (Saros 143) | ![]() December 19, 2150 (Saros 144) | ![]() November 17, 2161 (Saros 145) | ![]() October 17, 2172 (Saros 146) |
![]() September 16, 2183 (Saros 147) | ![]() August 16, 2194 (Saros 148) |
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 March 27, 1884 and August 20, 1971 | ||||
---|---|---|---|---|
March 27–29 | January 14 | November 1–2 | August 20–21 | June 8 |
108 | 110 | 112 | 114 | 116 |
![]() March 27, 1884 | ![]() August 20, 1895 | ![]() June 8, 1899 | ||
118 | 120 | 122 | 124 | 126 |
![]() March 29, 1903 | ![]() January 14, 1907 | ![]() November 2, 1910 | ![]() August 21, 1914 | ![]() June 8, 1918 |
128 | 130 | 132 | 134 | 136 |
![]() March 28, 1922 | ![]() January 14, 1926 | ![]() November 1, 1929 | ![]() August 21, 1933 | ![]() June 8, 1937 |
138 | 140 | 142 | 144 | 146 |
![]() March 27, 1941 | ![]() January 14, 1945 | ![]() November 1, 1948 | ![]() August 20, 1952 | ![]() June 8, 1956 |
148 | 150 | 152 | 154 | |
![]() March 27, 1960 | ![]() January 14, 1964 | ![]() November 2, 1967 | ![]() August 20, 1971 |
A partial solar eclipse occurred at the Moon’s descending node of orbit on Saturday, February 5, 2000, with a magnitude of 0.5795. 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 partial solar eclipse occurs in the polar regions of the Earth when the center of the Moon's shadow misses the Earth. It was only visible over Antarctica.
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.
A partial solar eclipse will occur at the Moon's descending node of orbit on Thursday, September 25, 2098, with a magnitude of 0.7871. 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 partial solar eclipse occurs in the polar regions of the Earth when the center of the Moon's shadow misses the Earth.
A partial solar eclipse occurred at the Moon's descending node of orbit on Thursday, July 22, 1971, with a magnitude of 0.0689. 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 partial solar eclipse occurs in the polar regions of the Earth when the center of the Moon's shadow misses the Earth. This was the 70th and final solar eclipse from Solar Saros 116.
An annular solar eclipse occurred at the Moon's descending node of orbit on Wednesday, August 20, 1952, with a magnitude of 0.942. 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 Peru including the capital city Lima, northeastern Chile, Bolivia including the constitutional capital Sucre and seat of government La Paz, Argentina, Paraguay, southern Brazil and Uruguay.
An annular solar eclipse will occur at the Moon's descending node of orbit on Thursday, October 13, 2061, with a magnitude of 0.9469. 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 partial solar eclipse will occur at the Moon's descending node of orbit on Monday, May 20, 2069, with a magnitude of 0.0879. 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 partial solar eclipse occurs in the polar regions of the Earth when the center of the Moon's shadow misses the Earth.
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.
An annular solar eclipse will occur at the Moon's descending node of orbit on Tuesday, October 24, 2079, with a magnitude of 0.9484. 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 partial solar eclipse will occur at the Moon's descending node of orbit on Friday, August 13, 2083, with a magnitude of 0.6146. 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 partial solar eclipse occurs in the polar regions of the Earth when the center of the Moon's shadow misses the Earth.
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.
An annular solar eclipse occurred at the Moon's descending node of orbit on Sunday, March 29, 1903, with a magnitude of 0.9767. 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 China, Russia on March 29 (Sunday), and Northern Canada on March 28 (Saturday).
An annular solar eclipse occurred at the Moon's descending node of orbit on Wednesday, November 12, 1947, with a magnitude of 0.965. 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 the Pacific Ocean, Peru, Ecuador, Colombia and Brazil.
An annular solar eclipse occurred at the Moon's descending node of orbit on Wednesday, April 19, 1939, with a magnitude of 0.9731. 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 partial solar eclipse occurred at the Moon's descending node of orbit on Monday, March 16, 1942, with a magnitude of 0.6393. 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 partial solar eclipse occurs in the polar regions of the Earth when the center of the Moon's shadow misses the Earth.
An annular solar eclipse occurred at the Moon's descending node of orbit on Friday, April 8, 1921, with a magnitude of 0.9753. 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 northern Scotland, northwestern tip of Norway, and islands in the Arctic Ocean in Russian SFSR.
A partial solar eclipse occurred at the Moon's descending node of orbit on Saturday, December 24, 1927, with a magnitude of 0.549. 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 partial solar eclipse occurs in the polar regions of the Earth when the center of the Moon's shadow misses the Earth.
A partial solar eclipse occurred at the Moon's descending node of orbit on Tuesday, May 18, 1920, with a magnitude of 0.9734. 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 partial solar eclipse occurs in the polar regions of the Earth when the center of the Moon's shadow misses the Earth.
A partial solar eclipse occurred at the Moon's descending node of orbit on Tuesday, June 19, 1917, with a magnitude of 0.4729. 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 partial solar eclipse occurs in the polar regions of the Earth when the center of the Moon's shadow misses the Earth.