Solar eclipse of September 9, 1904 | |
---|---|
Type of eclipse | |
Nature | Total |
Gamma | −0.1625 |
Magnitude | 1.0709 |
Maximum eclipse | |
Duration | 380 s (6 min 20 s) |
Coordinates | 3°42′S 134°30′W / 3.7°S 134.5°W |
Max. width of band | 234 km (145 mi) |
Times (UTC) | |
Greatest eclipse | 20:44:21 |
References | |
Saros | 133 (39 of 72) |
Catalog # (SE5000) | 9291 |
A total solar eclipse occurred on September 9, 1904.[1][2][3] 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 from German New Guinea (the part now belonging to Marshall Islands) on September 10 and Chile on September 9.
The event is mentioned in James Joyce's novel Ulysses.
The National Astronomical Observatory of Chile established an observation station in Taltal, Antofagasta, but the eclipse was clouded out and could not be seen. In the capital city Santiago, a partial eclipse was seen just before sunset.[4]
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.[5]
Solar eclipse series sets from 1902 to 1907 | ||||
---|---|---|---|---|
Descending node | Ascending node | |||
108 | April 8, 1902 Partial |
113 | October 1, 1902 | |
118 | March 29, 1903 Annular |
123 | September 21, 1903 Total | |
128 | March 17, 1904 Annular |
133 | September 9, 1904 Total | |
138 | March 6, 1905 Annular |
143 | August 30, 1905 Total | |
148 | February 23, 1906 Partial |
153 | August 20, 1906 Partial |
Solar Saros 133, repeating every 18 years, 11 days, contains 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, with a hybrid eclipse on January 24, 1544. It has total eclipses from February 3, 1562, through June 21, 2373. The series ends at member 72 as a partial eclipse on September 5, 2499. The longest duration of totality was 6 minutes, 49.97 seconds on August 7, 1850.[6] The total eclipses of this saros series are getting shorter and farther south with each iteration. All eclipses in this series occurs at the Moon’s ascending node.
Series members 30–56 occur between 1742 and 2211 | ||
---|---|---|
30 | 31 | 32 |
June 3, 1742 | June 13, 1760 | June 24, 1778 |
33 | 34 | 35 |
July 4, 1796 | July 17, 1814 | July 27, 1832 |
36 | 37 | 38 |
August 7, 1850 | August 18, 1868 |
August 29, 1886 |
39 | 40 | 41 |
September 9, 1904 |
September 21, 1922 |
October 1, 1940 |
42 | 43 | 44 |
October 12, 1958 |
October 23, 1976 |
November 3, 1994 |
45 | 46 | 47 |
November 13, 2012 |
November 25, 2030 |
December 5, 2048 |
48 | 49 | 50 |
December 17, 2066 |
December 27, 2084 |
January 8, 2103 |
51 | 52 | 53 |
January 19, 2121 |
January 30, 2139 |
February 9, 2157 |
54 | 55 | 56 |
February 21, 2175 |
March 3, 2193 |
March 15, 2211 |
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. In the 18th century:
Inex series members between 1801 and 2200: | ||
---|---|---|
Near lunar perigee | After lunar apogee Before lunar perigee |
Before lunar apogee After lunar perigee |
November 9, 1817 (Saros 130) |
October 20, 1846 (Saros 131) |
September 29, 1875 (Saros 132) |
September 9, 1904 (Saros 133) |
August 21, 1933 (Saros 134) |
July 31, 1962 (Saros 135) |
July 11, 1991 (Saros 136) |
June 21, 2020 (Saros 137) |
May 31, 2049 (Saros 138) |
May 11, 2078 (Saros 139) |
April 23, 2107 (Saros 140) |
April 1, 2136 (Saros 141) |
March 12, 2165 (Saros 142) |
February 21, 2194 (Saros 143) |
In the 23rd century:
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 1901 and 2100 | |||
---|---|---|---|
September 9, 1904 (Saros 133) |
August 10, 1915 (Saros 134) |
July 9, 1926 (Saros 135) | |
June 8, 1937 (Saros 136) |
May 9, 1948 (Saros 137) |
April 8, 1959 (Saros 138) | |
March 7, 1970 (Saros 139) |
February 4, 1981 (Saros 140) |
January 4, 1992 (Saros 141) | |
December 4, 2002 (Saros 142) |
November 3, 2013 (Saros 143) |
October 2, 2024 (Saros 144) | |
September 2, 2035 (Saros 145) |
August 2, 2046 (Saros 146) |
July 1, 2057 (Saros 147) | |
May 31, 2068 (Saros 148) |
May 1, 2079 (Saros 149) |
March 31, 2090 (Saros 150) |