Solar eclipse of June 30, 1992 | |
---|---|
Type of eclipse | |
Nature | Total |
Gamma | −0.7512 |
Magnitude | 1.0592 |
Maximum eclipse | |
Duration | 321 s (5 min 21 s) |
Coordinates | 25°12′S9°30′W / 25.2°S 9.5°W |
Max. width of band | 294 km (183 mi) |
Times (UTC) | |
Greatest eclipse | 12:11:22 |
References | |
Saros | 146 (26 of 76) |
Catalog # (SE5000) | 9491 |
A total solar eclipse occurred at the Moon's descending node of orbit on Tuesday, June 30, 1992, with a magnitude of 1.0592. 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 southeastern Uruguay and southern tip of Rio Grande do Sul, Brazil.
The path of totality was mostly on the sea and covered very little land. From the only land covered by it in southeasern Uruguay and southern tip of Brazil, totality occurred shortly after sunrise, with the solar zenith angle less than 3°. Observation from an airplane over the middle of South Atlantic Ocean, near the location of maximum eclipse, could offer a duration of totality of up to 10 minutes with the guarantee of clear weather. However, due to the limitations in the cruising capabilities and the economic cost, a feasible flight plan was to see 5 to 6 minutes of totality on the airplane. 48 people from the United States, Canada, Brazil, Germany, Japan and Great Britain boarded a VASP airline DC-10 plane, departing from Rio de Janeiro, Brazil, flying over the South Atlantic Ocean and returning to Rio de Janeiro. The passengers got off and the captain flew the airplane back to Sao Paulo. Although adjustment in the flying speed had to be made according to the take-off time and wind speed, the pilot flew the airplane into Moon's umbra within 1 second of the predicted time, and the passengers on board successfully saw the total eclipse. Accidentally, one of the ground support personnel did not exit the airplane before takeoff, and she also saw the eclipse. The pilots were also attracted by the eclipse, still watching the moon shadow moving into the distance and forgetting to fly the airplane back return even minutes after the third contact (the end of the total phase). The captain described this as the most unusual flight he ever commanded. VASP airline also provided a Boeing 737 plane to the Rio de Janeiro Planetarium . Planetarium staff, of their astronomy club, local dignitaries, politicians and celebrities were also invited. [1]
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. [2]
Solar eclipse series sets from 1990 to 1992 | ||||||
---|---|---|---|---|---|---|
Ascending node | Descending node | |||||
Saros | Map | Gamma | Saros | Map | Gamma | |
121 | January 26, 1990 ![]() Annular | −0.9457 | 126![]() Partial in Finland | July 22, 1990 ![]() Total | 0.7597 | |
131 | January 15, 1991 ![]() Annular | −0.2727 | 136![]() Totality in Playas del Coco, Costa Rica | July 11, 1991 ![]() Total | −0.0041 | |
141 | January 4, 1992 ![]() Annular | 0.4091 | 146 | June 30, 1992 ![]() Total | −0.7512 | |
151 | December 24, 1992 ![]() Partial | 1.0711 |
This eclipse is a part of Saros series 146, repeating every 18 years, 11 days, and containing 76 events. The series started with a partial solar eclipse on September 19, 1541. It contains total eclipses from May 29, 1938 through October 7, 2154; hybrid eclipses from October 17, 2172 through November 20, 2226; and annular eclipses from November 30, 2244 through August 10, 2659. The series ends at member 76 as a partial eclipse on December 29, 2893. 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 26 at 5 minutes, 21 seconds on June 30, 1992, and the longest duration of annularity will be produced by member 63 at 3 minutes, 30 seconds on August 10, 2659. All eclipses in this series occur at the Moon’s descending node of orbit. [3]
Series members 16–37 occur between 1801 and 2200: | ||
---|---|---|
16 | 17 | 18 |
![]() March 13, 1812 | ![]() March 24, 1830 | ![]() April 3, 1848 |
19 | 20 | 21 |
![]() April 15, 1866 | ![]() April 25, 1884 | ![]() May 7, 1902 |
22 | 23 | 24 |
![]() May 18, 1920 | ![]() May 29, 1938 | ![]() June 8, 1956 |
25 | 26 | 27 |
![]() June 20, 1974 | ![]() June 30, 1992 | ![]() July 11, 2010 |
28 | 29 | 30 |
![]() July 22, 2028 | ![]() August 2, 2046 | ![]() August 12, 2064 |
31 | 32 | 33 |
![]() August 24, 2082 | ![]() September 4, 2100 | ![]() September 15, 2118 |
34 | 35 | 36 |
![]() September 26, 2136 | ![]() October 7, 2154 | ![]() October 17, 2172 |
37 | ||
![]() October 29, 2190 |
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 September 12, 1931 and July 1, 2011 | ||||
---|---|---|---|---|
September 11–12 | June 30–July 1 | April 17–19 | February 4–5 | November 22–23 |
114 | 116 | 118 | 120 | 122 |
![]() September 12, 1931 | ![]() June 30, 1935 | ![]() April 19, 1939 | ![]() February 4, 1943 | ![]() November 23, 1946 |
124 | 126 | 128 | 130 | 132 |
![]() September 12, 1950 | ![]() June 30, 1954 | ![]() April 19, 1958 | ![]() February 5, 1962 | ![]() November 23, 1965 |
134 | 136 | 138 | 140 | 142 |
![]() September 11, 1969 | ![]() June 30, 1973 | ![]() April 18, 1977 | ![]() February 4, 1981 | ![]() November 22, 1984 |
144 | 146 | 148 | 150 | 152 |
![]() September 11, 1988 | ![]() June 30, 1992 | ![]() April 17, 1996 | ![]() February 5, 2000 | ![]() November 23, 2003 |
154 | 156 | |||
![]() September 11, 2007 | ![]() July 1, 2011 |
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.
The partial solar eclipses on December 18, 2188 (part of Saros 164) and November 18, 2199 (part of Saros 165) are also a part of this series but are not included in the table below.
Series members between 1801 and 2134 | ||||
---|---|---|---|---|
![]() December 10, 1806 (Saros 129) | ![]() November 9, 1817 (Saros 130) | ![]() October 9, 1828 (Saros 131) | ![]() September 7, 1839 (Saros 132) | ![]() August 7, 1850 (Saros 133) |
![]() July 8, 1861 (Saros 134) | ![]() June 6, 1872 (Saros 135) | ![]() May 6, 1883 (Saros 136) | ![]() April 6, 1894 (Saros 137) | ![]() March 6, 1905 (Saros 138) |
![]() February 3, 1916 (Saros 139) | ![]() January 3, 1927 (Saros 140) | ![]() December 2, 1937 (Saros 141) | ![]() November 1, 1948 (Saros 142) | ![]() October 2, 1959 (Saros 143) |
![]() August 31, 1970 (Saros 144) | ![]() July 31, 1981 (Saros 145) | ![]() June 30, 1992 (Saros 146) | ![]() May 31, 2003 (Saros 147) | ![]() April 29, 2014 (Saros 148) |
![]() March 29, 2025 (Saros 149) | ![]() February 27, 2036 (Saros 150) | ![]() January 26, 2047 (Saros 151) | ![]() December 26, 2057 (Saros 152) | ![]() November 24, 2068 (Saros 153) |
![]() October 24, 2079 (Saros 154) | ![]() September 23, 2090 (Saros 155) | ![]() August 24, 2101 (Saros 156) | ![]() July 23, 2112 (Saros 157) | ![]() June 23, 2123 (Saros 158) |
![]() May 23, 2134 (Saros 159) |
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 | ||
---|---|---|
![]() October 29, 1818 (Saros 140) | ![]() October 9, 1847 (Saros 141) | ![]() September 17, 1876 (Saros 142) |
![]() August 30, 1905 (Saros 143) | ![]() August 10, 1934 (Saros 144) | ![]() July 20, 1963 (Saros 145) |
![]() June 30, 1992 (Saros 146) | ![]() June 10, 2021 (Saros 147) | ![]() May 20, 2050 (Saros 148) |
![]() May 1, 2079 (Saros 149) | ![]() April 11, 2108 (Saros 150) | ![]() March 21, 2137 (Saros 151) |
![]() March 2, 2166 (Saros 152) | ![]() February 10, 2195 (Saros 153) |
{{cite web}}
: CS1 maint: multiple names: authors list (link)A total solar eclipse occurred at the Moon's ascending node of orbit on Sunday, November 3, 2013, with a magnitude of 1.0159. It was a hybrid eclipse of the Sun with a small portion over the western Atlantic Ocean at sunrise as an annular eclipse and the rest of the path as a narrow total solar eclipse. 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 hybrid solar eclipse occurs when the Moon's apparent diameter is smaller than the Sun's in sunrise and sunset, but at Greatest Eclipse the Moon's apparent diameter is larger than the Sun's.
An annular solar eclipse occurred at the Moon's descending node of orbit on Sunday, December 4, 1983, with a magnitude of 0.9666. 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 Cape Verde, Annobón Island of Equatorial Guinea, Gabon, the People's Republic of Congo, Zaire, northern Uganda, southern Sudan, northwestern Kenya, Ethiopia and Somalia. The Sun's altitude was 66°. Occurring 6.5 days before apogee, the Moon's apparent diameter was near the average diameter.
A partial solar eclipse will occur at the Moon's descending node of orbit on Tuesday, April 11, 2051, with a magnitude of 0.9849. 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 occurred at the Moon's ascending node of orbit on Wednesday, February 14, 1934, with a magnitude of 1.0321. 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 the Dutch East Indies, North Borneo, and the South Seas Mandate of Japan.
A partial solar eclipse occurred at the Moon's ascending node of orbit on Saturday, October 12, 1996, with a magnitude of 0.7575. 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 ascending node of orbit on Wednesday, May 30, 1984, with a magnitude of 0.998. 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 Mexico, the United States, Azores Islands, Morocco and Algeria. It was the first annular solar eclipse visible in the US in 33 years. The Moon's apparent diameter was near the average diameter because it occurred 6.7 days after apogee and 7.8 days before perigee.
A partial solar eclipse occurred at the Moon’s ascending node of orbit on Saturday, April 30, 2022, with a magnitude of 0.6396. 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. The eclipse was visible in parts of Argentina, Chile, Uruguay, Paraguay, Bolivia, Peru, Brazil, and Antarctica.
An annular solar eclipse occurred at the Moon's descending node of orbit on Monday, April 18, 1977, with a magnitude of 0.9449. 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 South West Africa, Angola, Zambia, southeastern Zaire, northern Malawi, Tanzania, Seychelles and the whole British Indian Ocean Territory.
An annular solar eclipse will occur at the Moon's descending node of orbit on Monday, November 15, 2077, with a magnitude of 0.9371. A solar eclipse occurs when the Moon passes between Earth and the Sun, thereby totally or partially 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 will cross North America and South America. This will be the 47th solar eclipse of Saros cycle 134. A small annular eclipse will cover only 93.71% of the Sun in a very broad path, 262 km wide at maximum, and will last 7 minutes and 54 seconds. Occurring only 4 days after apogee, the Moon's apparent diameter is smaller.
An annular solar eclipse will occur at the Moon's ascending node of orbit on Sunday, September 22, 2052, 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. 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 Saturday, July 13, 2075, with a magnitude of 0.9467. 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.
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 ascending node of orbit on Thursday, March 21, 2080, with a magnitude of 0.8734. 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 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 descending node of orbit on Monday, July 3, 2084, with a magnitude of 0.9421. 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.
A total solar eclipse occurred at the Moon's descending node of orbit on Wednesday, December 23, 1908, with a magnitude of 1.0024. It was a hybrid event, with only a fraction of its path as total, and longer sections at the start and end as an annular eclipse. 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. Annularity was visible from Chile, Argentina, Uruguay and southern Brazil, while totality was visible only from southern Atlantic Ocean with no land.
An annular solar eclipse occurred at the Moon's ascending node of orbit on Sunday, June 28, 1908, with a magnitude of 0.9655. 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 occurred at the Moon's ascending node of orbit on Monday, April 28, 1930, with a magnitude of 1.0003. It was a hybrid event, with only a fraction of its path as total, and longer sections at the start and end as an annular eclipse. 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 partial solar eclipse occurred at the Moon's descending node of orbit on Sunday, October 11, 1931, with a magnitude of 0.9005. 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 event was visible as a partial solar eclipse from southern South America, and parts of Antarctica.
A total solar eclipse occurred at the Moon's ascending node of orbit on Thursday, October 12, 1939, with a magnitude of 1.0266. 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.