Solar eclipse of March 9, 2035
Template:Short description Script error: No such module "Solar eclipse". An annular solar eclipse will occur at the Moon's descending node of orbit between Friday, March 9 and Saturday, March 10, 2035,[1] 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. The Moon's apparent diameter will be near the average diameter because it will occur 7.6 days after apogee (on March 2, 2035, at 9:30 UTC) and 5.1 days before perigee (on March 15, 2035, at 1:40 UTC).[2]
Annularity will be visible for parts of New Zealand. A partial eclipse will be visible for parts of Australia, Oceania, Antarctica, and central Mexico.
Images
File:SE2035Mar09A.gif
Animated path
Eclipse details
Shown below are two tables displaying details about this particular solar eclipse. The first table outlines times at which the moon's penumbra or umbra attains the specific parameter, and the second table describes various other parameters pertaining to this eclipse.[3]
| Event | Time (UTC) |
|---|---|
| First Penumbral External Contact | 2035 March 9 at 20:22:04.1 UTC |
| First Umbral External Contact | 2035 March 9 at 21:26:19.2 UTC |
| First Central Line | 2035 March 9 at 21:27:07.8 UTC |
| Greatest Duration | 2035 March 9 at 21:27:07.8 UTC |
| First Umbral Internal Contact | 2035 March 9 at 21:27:56.5 UTC |
| Equatorial Conjunction | 2035 March 9 at 22:50:50.5 UTC |
| First Penumbral Internal Contact | 2035 March 9 at 22:57:05.1 UTC |
| Greatest Eclipse | 2035 March 9 at 23:05:53.6 UTC |
| Ecliptic Conjunction | 2035 March 9 at 23:10:39.6 UTC |
| Last Penumbral Internal Contact | 2035 March 9 at 23:15:08.3 UTC |
| Last Umbral Internal Contact | 2035 March 10 at 00:44:04.1 UTC |
| Last Central Line | 2035 March 10 at 00:44:49.7 UTC |
| Last Umbral External Contact | 2035 March 10 at 00:45:35.2 UTC |
| Last Penumbral External Contact | 2035 March 10 at 01:49:43.7 UTC |
| Parameter | Value |
|---|---|
| Eclipse Magnitude | 0.99191 |
| Eclipse Obscuration | 0.98388 |
| Gamma | −0.43679 |
| Sun Right Ascension | 23h20m17.6s |
| Sun Declination | -04°16'22.2" |
| Sun Semi-Diameter | 16'06.5" |
| Sun Equatorial Horizontal Parallax | 08.9" |
| Moon Right Ascension | 23h20m47.9s |
| Moon Declination | -04°40'23.8" |
| Moon Semi-Diameter | 15'44.9" |
| Moon Equatorial Horizontal Parallax | 0°57'47.9" |
| ΔT | 76.2 s |
Eclipse season
Script error: No such module "Labelled list hatnote". This eclipse is part of an eclipse season, a period, roughly every six months, when eclipses occur. Only two (or occasionally three) eclipse seasons occur each year, and each season lasts about 35 days and repeats just short of six months (173 days) later; thus two full eclipse seasons always occur each year. Either two or three eclipses happen each eclipse season. In the sequence below, each eclipse is separated by a fortnight.
| February 22 Ascending node (full moon) |
March 9 Descending node (new moon) |
|---|---|
| File:Lunar eclipse chart close-2035Feb22.png | File:SE2035Mar09A.png |
| Penumbral lunar eclipse Lunar Saros 114 |
Annular solar eclipse Solar Saros 140 |
Related eclipses
Eclipses in 2035
- A penumbral lunar eclipse on February 22.
- An annular solar eclipse on March 9.
- A partial lunar eclipse on August 19.
- A total solar eclipse on September 2.
Metonic
- Preceded by: Solar eclipse of May 21, 2031
- Followed by: Solar eclipse of December 26, 2038
Tzolkinex
- Preceded by: Solar eclipse of January 26, 2028
- Followed by: Solar eclipse of April 20, 2042
Half-Saros
- Preceded by: Lunar eclipse of March 3, 2026
- Followed by: Lunar eclipse of March 13, 2044
Tritos
- Preceded by: Solar eclipse of April 8, 2024
- Followed by: Solar eclipse of February 5, 2046
Solar Saros 140
- Preceded by: Solar eclipse of February 26, 2017
- Followed by: Solar eclipse of March 20, 2053
Inex
- Preceded by: Solar eclipse of March 29, 2006
- Followed by: Solar eclipse of February 17, 2064
Triad
- Preceded by: Solar eclipse of May 9, 1948
- Followed by: Solar eclipse of January 8, 2122
Solar eclipses of 2033–2036
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.[4]
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 File:SE2033Mar30T.png Total |
0.9778 | 125 | September 23, 2033 File:SE2033Sep23P.png Partial |
−1.1583 | |
| 130 | March 20, 2034 File:SE2034Mar20T.png Total |
0.2894 | 135 | September 12, 2034 File:SE2034Sep12A.png Annular |
−0.3936 | |
| 140 | March 9, 2035 File:SE2035Mar09A.png Annular |
−0.4368 | 145 | September 2, 2035 File:SE2035Sep02T.png Total |
0.3727 | |
| 150 | February 27, 2036 File:SE2036Feb27P.png Partial |
−1.1942 | 155 | August 21, 2036 File:SE2036Aug21P.png Partial |
1.0825 | |
Saros 140
Template:Solar Saros series 140
Metonic series
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.
| 21 eclipse events between May 21, 1993 and May 20, 2069 | ||||
|---|---|---|---|---|
| May 20–21 | March 9 | December 25–26 | October 13–14 | August 1–2 |
| 118 | 120 | 122 | 124 | 126 |
| File:SE1993May21P.png May 21, 1993 |
File:SE1997Mar09T.png March 9, 1997 |
File:SE2000Dec25P.png December 25, 2000 |
File:SE2004Oct14P.png October 14, 2004 |
File:SE2008Aug01T.png August 1, 2008 |
| 128 | 130 | 132 | 134 | 136 |
| File:SE2012May20A.png May 20, 2012 |
File:SE2016Mar09T.png March 9, 2016 |
File:SE2019Dec26A.png December 26, 2019 |
File:SE2023Oct14A.png October 14, 2023 |
File:SE2027Aug02T.png August 2, 2027 |
| 138 | 140 | 142 | 144 | 146 |
| File:SE2031May21A.png May 21, 2031 |
File:SE2035Mar09A.png March 9, 2035 |
File:SE2038Dec26T.png December 26, 2038 |
File:SE2042Oct14A.png October 14, 2042 |
File:SE2046Aug02T.png August 2, 2046 |
| 148 | 150 | 152 | 154 | 156 |
| File:SE2050May20H.png May 20, 2050 |
File:SE2054Mar09P.png March 9, 2054 |
File:SE2057Dec26T.png December 26, 2057 |
File:SE2061Oct13A.png October 13, 2061 |
File:SE2065Aug02P.png August 2, 2065 |
| 158 | ||||
| File:SE2069May20P.png May 20, 2069 | ||||
Tritos series
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.
Inex series
Template:Solar Inex series 2006 March 29
References
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External links
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