Solar eclipse of March 9, 2035
Solar eclipse of March 9, 2035 | |
---|---|
Type of eclipse | |
Nature | Annular |
Gamma | −0.4368 |
Magnitude | 0.9919 |
Maximum eclipse | |
Duration | 48 s (0 min 48 s) |
Coordinates | 29°00′S 154°54′W / 29°S 154.9°W |
Max. width of band | 31 km (19 mi) |
Times (UTC) | |
Greatest eclipse | 23:05:54 |
References | |
Saros | 140 (30 of 71) |
Catalog # (SE5000) | 9585 |
An annular solar eclipse will occur at the Moon's descending node of orbit on Friday, March 9, 2035, with a magnitude of 0.9919. 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.
Images[edit]
Related eclipses[edit]
Eclipses of 2035[edit]
- A penumbral lunar eclipse on February 22, 2035.
- An annular solar eclipse on March 9, 2035.
- A partial lunar eclipse on August 19, 2035.
- A total solar eclipse on September 2, 2035.
Metonic[edit]
- Preceded by: Solar eclipse of May 21, 2031
- Followed by: Solar eclipse of December 26, 2038
Tzolkinex[edit]
- Preceded by: Solar eclipse of January 26, 2028
- Followed by: Solar eclipse of April 20, 2042
Half-Saros[edit]
- Preceded by: Lunar eclipse of March 3, 2026
- Followed by: Lunar eclipse of March 13, 2044
Tritos[edit]
- Preceded by: Solar eclipse of April 8, 2024
- Followed by: Solar eclipse of February 5, 2046
Solar Saros 140[edit]
- Preceded by: Solar eclipse of February 26, 2017
- Followed by: Solar eclipse of March 20, 2053
Inex[edit]
- Preceded by: Solar eclipse of March 29, 2006
- Followed by: Solar eclipse of February 17, 2064
Triad[edit]
- Preceded by: Solar eclipse of May 9, 1948
- Followed by: Solar eclipse of January 8, 2122
Solar eclipses of 2033–2036[edit]
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 partial solar eclipse on July 23, 2036 occurs in the next lunar year eclipse set.
Solar eclipse series sets from 2033 to 2036 | ||||||
---|---|---|---|---|---|---|
Descending node | Ascending node | |||||
Saros | Map | Gamma | Saros | Map | Gamma | |
120 | March 30, 2033 Total |
0.9778 | 125 | September 23, 2033 Partial |
−1.1583 | |
130 | March 20, 2034 Total |
0.2894 | 135 | September 12, 2034 Annular |
−0.3936 | |
140 | March 9, 2035 Annular |
−0.4368 | 145 | September 2, 2035 Total |
0.3727 | |
150 | February 27, 2036 Partial |
−1.1942 | 155 | August 21, 2036 Partial |
1.0825 |
Saros 140[edit]
This eclipse is a part of Saros series 140, repeating every 18 years, 11 days, and containing 71 events. The series started with a partial solar eclipse on April 16, 1512. It contains total eclipses from July 21, 1656 through November 9, 1836; hybrid eclipses from November 20, 1854 through December 23, 1908; and annular eclipses from January 3, 1927 through December 7, 2485. The series ends at member 71 as a partial eclipse on June 1, 2774. 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 11 at 4 minutes, 10 seconds on August 12, 1692, and the longest duration of annularity will be produced by member 53 at 7 minutes, 35 seconds on November 15, 2449. All eclipses in this series occur at the Moon’s descending node of orbit.[2]
Series members 18–39 occur between 1801 and 2200: | ||
---|---|---|
18 | 19 | 20 |
October 29, 1818 |
November 9, 1836 |
November 20, 1854 |
21 | 22 | 23 |
November 30, 1872 |
December 12, 1890 |
December 23, 1908 |
24 | 25 | 26 |
January 3, 1927 |
January 14, 1945 |
January 25, 1963 |
27 | 28 | 29 |
February 4, 1981 |
February 16, 1999 |
February 26, 2017 |
30 | 31 | 32 |
March 9, 2035 |
March 20, 2053 |
March 31, 2071 |
33 | 34 | 35 |
April 10, 2089 |
April 23, 2107 |
May 3, 2125 |
36 | 37 | 38 |
May 14, 2143 |
May 25, 2161 |
June 5, 2179 |
39 | ||
June 15, 2197 |
Tritos series[edit]
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 2100 | |||
---|---|---|---|
December 21, 1805 (Saros 119) |
November 19, 1816 (Saros 120) |
October 20, 1827 (Saros 121) | |
September 18, 1838 (Saros 122) |
August 18, 1849 (Saros 123) |
July 18, 1860 (Saros 124) | |
June 18, 1871 (Saros 125) |
May 17, 1882 (Saros 126) |
April 16, 1893 (Saros 127) | |
March 17, 1904 (Saros 128) |
February 14, 1915 (Saros 129) |
January 14, 1926 (Saros 130) | |
December 13, 1936 (Saros 131) |
November 12, 1947 (Saros 132) |
October 12, 1958 (Saros 133) | |
September 11, 1969 (Saros 134) |
August 10, 1980 (Saros 135) |
July 11, 1991 (Saros 136) | |
June 10, 2002 (Saros 137) |
May 10, 2013 (Saros 138) |
April 8, 2024 (Saros 139) | |
March 9, 2035 (Saros 140) |
February 5, 2046 (Saros 141) |
January 5, 2057 (Saros 142) | |
December 6, 2067 (Saros 143) |
November 4, 2078 (Saros 144) |
October 4, 2089 (Saros 145) | |
September 4, 2100 (Saros 146) |
In the 22nd century:
- Solar saros 147: annular solar eclipse of August 4, 2111
- Solar saros 148: total solar eclipse of July 4, 2122
- Solar saros 149: total solar eclipse of June 3, 2133
- Solar saros 150: annular solar eclipse of May 3, 2144
- Solar saros 151: annular solar eclipse of April 2, 2155
- Solar saros 152: total solar eclipse of March 2, 2166
- Solar saros 153: annular solar eclipse of January 29, 2177
- Solar saros 154: annular solar eclipse of December 29, 2187
- Solar saros 155: total solar eclipse of November 28, 2198
In the 23rd century:
- Solar saros 156: annular solar eclipse of October 29, 2209
- Solar saros 157: annular solar eclipse of September 27, 2220
- Solar saros 158: total solar eclipse of August 28, 2231
- Solar saros 159: partial solar eclipse of July 28, 2242
- Solar saros 160: partial solar eclipse of June 26, 2253
- Solar saros 161: partial solar eclipse of May 26, 2264
- Solar saros 162: partial solar eclipse of April 26, 2275
- Solar saros 163: partial solar eclipse of March 25, 2286
- Solar saros 164: partial solar eclipse of February 22, 2297
Inex series[edit]
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.
Inex series members between 1901 and 2100: | ||
---|---|---|
May 29, 1919 (Saros 136) |
May 9, 1948 (Saros 137) |
April 18, 1977 (Saros 138) |
March 29, 2006 (Saros 139) |
March 9, 2035 (Saros 140) |
February 17, 2064 (Saros 141) |
January 27, 2093 (Saros 142) |
Metonic series[edit]
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.[3]
Octon series with 21 events between May 21, 1993 and August 2, 2065 | ||||
---|---|---|---|---|
May 20–21 | March 8–9 | December 25–26 | October 13–14 | August 1–2 |
98 | 100 | 102 | 104 | 106 |
May 21, 1955 | March 9, 1959 | December 26, 1962 | October 14, 1966 | August 2, 1970 |
108 | 110 | 112 | 114 | 116 |
May 21, 1974 | March 9, 1978 | December 26, 1981 | October 14, 1985 | August 1, 1989 |
118 | 120 | 122 | 124 | 126 |
May 21, 1993 |
March 9, 1997 |
December 25, 2000 |
October 14, 2004 |
August 1, 2008 |
128 | 130 | 132 | 134 | 136 |
May 20, 2012 |
March 9, 2016 |
December 26, 2019 |
October 14, 2023 |
August 2, 2027 |
138 | 140 | 142 | 144 | 146 |
May 21, 2031 |
March 9, 2035 |
December 26, 2038 |
October 14, 2042 |
August 2, 2046 |
148 | 150 | 152 | 154 | 156 |
May 20, 2050 |
March 9, 2054 |
December 26, 2057 |
October 13, 2061 |
August 2, 2065 |
158 | 160 | 162 | 164 | 166 |
May 20, 2069 |
March 8, 2073 | December 26, 2076 | October 13, 2080 | August 1, 2084 |
References[edit]
- ^ van Gent, R.H. "Solar- and Lunar-Eclipse Predictions from Antiquity to the Present". A Catalogue of Eclipse Cycles. Utrecht University. Retrieved 6 October 2018.
- ^ "NASA - Catalog of Solar Eclipses of Saros 140". eclipse.gsfc.nasa.gov.
- ^ Note S1: Eclipses & Predictions in Freeth, Tony (2014). "Eclipse Prediction on the Ancient Greek Astronomical Calculating Machine Known as the Antikythera Mechanism". PLOS ONE. 9 (7): e103275. Bibcode:2014PLoSO...9j3275F. doi:10.1371/journal.pone.0103275. PMC 4116162. PMID 25075747.