Solar eclipse of March 29, 1903 | |
---|---|
Type of eclipse | |
Nature | Annular |
Gamma | 0.8413 |
Magnitude | 0.9767 |
Maximum eclipse | |
Duration | 113 s (1 min 53 s) |
Coordinates | 56°12′N130°18′E / 56.2°N 130.3°E |
Max. width of band | 153 km (95 mi) |
Times (UTC) | |
Greatest eclipse | 1:35:23 |
References | |
Saros | 118 (62 of 72) |
Catalog # (SE5000) | 9288 |
An annular solar eclipse occurred at the Moon's descending node of orbit on Sunday, March 29, 1903, [1] [2] 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 (now northwestern China, Mongolia and northeastern China), Russia on March 29 (Sunday), and Northern Canada on March 28 (Saturday).
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 eclipses on May 7, 1902 and October 31, 1902 occur in the previous lunar year eclipse set, and the partial solar eclipse on July 21, 1906 occurs in the next lunar year eclipse set.
Solar eclipse series sets from 1902 to 1906 | ||||||
---|---|---|---|---|---|---|
Descending node | Ascending node | |||||
Saros | Map | Gamma | Saros | Map | Gamma | |
108 | April 8, 1902 ![]() Partial | 1.5024 | 113 | October 1, 1902 | ||
118 | March 29, 1903 ![]() Annular | 0.8413 | 123 | September 21, 1903 ![]() Total | −0.8967 | |
128 | March 17, 1904 ![]() Annular | 0.1299 | 133 | September 9, 1904 ![]() Total | −0.1625 | |
138 | March 6, 1905 ![]() Annular | −0.5768 | 143![]() | August 30, 1905 ![]() Total | 0.5708 | |
148 | February 23, 1906 ![]() Partial | −1.2479 | 153 | August 20, 1906 ![]() Partial | 1.3731 |
This eclipse is a part of Saros series 118, repeating every 18 years, 11 days, and containing 72 events. The series started with a partial solar eclipse on May 24, 803 AD. It contains total eclipses from August 19, 947 AD through October 25, 1650; hybrid eclipses on November 4, 1668 and November 15, 1686; and annular eclipses from November 27, 1704 through April 30, 1957. The series ends at member 72 as a partial eclipse on July 15, 2083. 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 34 at 6 minutes, 59 seconds on May 16, 1398, and the longest duration of annularity was produced by member 59 at 1 minutes, 58 seconds on February 23, 1849. All eclipses in this series occur at the Moon’s descending node of orbit. [4]
Series members 57–72 occur between 1801 and 2083: | ||
---|---|---|
57 | 58 | 59 |
![]() February 1, 1813 | ![]() February 12, 1831 | ![]() February 23, 1849 |
60 | 61 | 62 |
![]() March 6, 1867 | ![]() March 16, 1885 | ![]() March 29, 1903 |
63 | 64 | 65 |
![]() April 8, 1921 | ![]() April 19, 1939 | ![]() April 30, 1957 |
66 | 67 | 68 |
![]() May 11, 1975 | ![]() May 21, 1993 | ![]() June 1, 2011 |
69 | 70 | 71 |
![]() June 12, 2029 | ![]() June 23, 2047 | ![]() July 3, 2065 |
72 | ||
![]() July 15, 2083 |
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 | ||||
---|---|---|---|---|
![]() January 1, 1805 (Saros 109) | ![]() October 31, 1826 (Saros 111) | ![]() August 28, 1848 (Saros 113) | ||
![]() July 29, 1859 (Saros 114) | ![]() June 28, 1870 (Saros 115) | ![]() May 27, 1881 (Saros 116) | ![]() April 26, 1892 (Saros 117) | ![]() March 29, 1903 (Saros 118) |
![]() February 25, 1914 (Saros 119) | ![]() January 24, 1925 (Saros 120) | ![]() December 25, 1935 (Saros 121) | ![]() November 23, 1946 (Saros 122) | ![]() October 23, 1957 (Saros 123) |
![]() September 22, 1968 (Saros 124) | ![]() August 22, 1979 (Saros 125) | ![]() July 22, 1990 (Saros 126) | ![]() June 21, 2001 (Saros 127) | ![]() May 20, 2012 (Saros 128) |
![]() April 20, 2023 (Saros 129) | ![]() March 20, 2034 (Saros 130) | ![]() February 16, 2045 (Saros 131) | ![]() January 16, 2056 (Saros 132) | ![]() December 17, 2066 (Saros 133) |
![]() November 15, 2077 (Saros 134) | ![]() October 14, 2088 (Saros 135) | ![]() September 14, 2099 (Saros 136) | ![]() August 15, 2110 (Saros 137) | ![]() July 14, 2121 (Saros 138) |
![]() June 13, 2132 (Saros 139) | ![]() May 14, 2143 (Saros 140) | ![]() April 12, 2154 (Saros 141) | ![]() March 12, 2165 (Saros 142) | ![]() February 10, 2176 (Saros 143) |
![]() January 9, 2187 (Saros 144) | ![]() December 9, 2197 (Saros 145) |
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 will occur at the Moon's descending node of orbit on Tuesday, January 5, 2038, with a magnitude of 0.9728. 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 Tuesday, May 10, 1994, with a magnitude of 0.9431. 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 eclipse was visible over a wide swath of North America, from Baja California across the Midwest of the United States up through Ontario and Nova Scotia in Canada. Occurring only 1.6 days after apogee, the moon's apparent diameter was smaller than the sun. This solar eclipse belonged to Saros series 128.
An annular solar eclipse occurred at the Moon's descending node of orbit on Sunday, September 11, 1988, with a magnitude of 0.9377. 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 in southeastern Somalia, the Indian Ocean and Macquarie Island of Australia.
An annular solar eclipse occurred at the Moon's descending node of orbit on Thursday, September 11, 1969, with a magnitude of 0.969. 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, Bolivia and the southwestern tip of Brazilian state Mato Grosso. Places west of the International Date Line witnessed the eclipse on Friday, September 12, 1969.
An annular solar eclipse occurred at the Moon's ascending node of orbit on Friday, August 11, 1961, with a magnitude of 0.9375. 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 small annular eclipse covered only 94% of the Sun in a very broad path, 499 km wide at maximum, and lasted 6 minutes and 35 seconds.
A partial solar eclipse occurred at the Moon's descending node of orbit on Sunday, March 27, 1960, with a magnitude of 0.7058. 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 was observable from parts of the Antarctic Ocean and Indian Ocean.
An annular solar eclipse will occur at the Moon's descending node of orbit on Wednesday, November 5, 2059, with a magnitude of 0.9417. 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 Sun will be 94% covered in a moderate annular eclipse, lasting 7 minutes exactly and covering a broad path up to 238 km wide.
A partial solar eclipse will occur at the Moon's descending node of orbit on Sunday, August 2, 2065, with a magnitude of 0.4903. 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 total solar eclipse will occur at the Moon's descending node of orbit on Thursday, May 31, 2068, with a magnitude of 1.011. 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 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.
A total solar eclipse will occur at the Moon's descending node of orbit between Thursday, April 10 and Friday, April 11, 2070, with a magnitude of 1.0472. 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 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.
An annular solar eclipse will occur at the Moon's descending node of orbit on Monday, November 4, 2097, with a magnitude of 0.9494. 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 Wednesday, April 21, 2088, with a magnitude of 1.0474. 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 occurred at the Moon's descending node of orbit on Friday, August 10, 1934, with a magnitude of 0.9436. 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 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 Sunday, January 14, 1945, with a magnitude of 0.997. 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 Eastern Cape in South Africa, and northeastern Tasmania Island and Furneaux Group in Australia.
An annular solar eclipse occurred at the Moon's descending node of orbit on Saturday, March 17, 1923, with a magnitude of 0.931. 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, Falkland Islands including capital Stanley, Gough Island in Tristan da Cunha, South West Africa, Bechuanaland Protectorate (today's Botswana, Southern Rhodesia including capital Salisbury, Portuguese Mozambique, Nyasaland, French Madagascar.
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.