Solar eclipse of September 2, 2035
Template:Short description Script error: No such module "Solar eclipse". A total solar eclipse will occur at the Moon's ascending node of orbit on Sunday, September 2, 2035,[1] with a magnitude of 1.032. 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. Occurring about 2.9 days after perigee (on Thursday, August 30, 2035, at 3:35 UTC), the Moon's apparent diameter will be larger.[2]
Totality will be visible from parts of northern China, North Korea, the extreme northern tip of South Korea (Goseong County, Gangwon Province) and Japan. A partial eclipse will be visible for most of Asia, northern Oceania, Hawaii, southwest Alaska, and the western United States.
Visibility
The path of totality will cross two Asian capital cities, Beijing, China and Pyongyang, North Korea, and will pass north of a third, Tokyo, Japan.[3]
In popular culture
The 2035 eclipse is the setting of the 2003 video game Castlevania: Aria of Sorrow. Dracula's castle is located inside the solar eclipse, having been sealed there in 1999.
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.[4]
| Event | Time (UTC) |
|---|---|
| First Penumbral External Contact | 2035 September 1 at 23:16:45.8 UTC |
| First Umbral External Contact | 2035 September 2 at 00:17:05.5 UTC |
| First Central Line | 2035 September 2 at 00:17:36.1 UTC |
| First Umbral Internal Contact | 2035 September 2 at 00:18:06.7 UTC |
| First Penumbral Internal Contact | 2035 September 2 at 01:28:48.7 UTC |
| Equatorial Conjunction | 2035 September 2 at 01:45:01.1 UTC |
| Greatest Duration | 2035 September 2 at 01:53:17.4 UTC |
| Greatest Eclipse | 2035 September 2 at 01:56:46.3 UTC |
| Ecliptic Conjunction | 2035 September 2 at 02:00:44.2 UTC |
| Last Penumbral Internal Contact | 2035 September 2 at 02:25:01.7 UTC |
| Last Umbral Internal Contact | 2035 September 2 at 03:35:37.6 UTC |
| Last Central Line | 2035 September 2 at 03:36:05.7 UTC |
| Last Umbral External Contact | 2035 September 2 at 03:36:33.8 UTC |
| Last Penumbral External Contact | 2035 September 2 at 04:36:57.8 UTC |
| Parameter | Value |
|---|---|
| Eclipse Magnitude | 1.03204 |
| Eclipse Obscuration | 1.06510 |
| Gamma | 0.37273 |
| Sun Right Ascension | 10h44m07.3s |
| Sun Declination | +08°01'09.8" |
| Sun Semi-Diameter | 15'50.9" |
| Sun Equatorial Horizontal Parallax | 08.7" |
| Moon Right Ascension | 10h44m32.4s |
| Moon Declination | +08°22'14.7" |
| Moon Semi-Diameter | 16'06.4" |
| Moon Equatorial Horizontal Parallax | 0°59'06.9" |
| ΔT | 76.4 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.
| August 19 Descending node (full moon) |
September 2 Ascending node (new moon) |
|---|---|
| File:Lunar eclipse chart close-2035Aug19.png | File:SE2035Sep02T.png |
| Partial lunar eclipse Lunar Saros 119 |
Total solar eclipse Solar Saros 145 |
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 November 14, 2031
- Followed by: Solar eclipse of June 21, 2039
Tzolkinex
- Preceded by: Solar eclipse of July 22, 2028
- Followed by: Solar eclipse of October 14, 2042
Half-Saros
- Preceded by: Lunar eclipse of August 28, 2026
- Followed by: Lunar eclipse of September 7, 2044
Tritos
- Preceded by: Solar eclipse of October 2, 2024
- Followed by: Solar eclipse of August 2, 2046
Solar Saros 145
- Preceded by: Solar eclipse of August 21, 2017
- Followed by: Solar eclipse of September 12, 2053
Inex
- Preceded by: Solar eclipse of September 22, 2006
- Followed by: Solar eclipse of August 12, 2064
Triad
- Preceded by: Solar eclipse of November 1, 1948
- Followed by: Solar eclipse of July 4, 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.[5]
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 145
This eclipse is a part of Saros series 145, repeating every 18 years, 11 days, and containing 77 events. The series started with a partial solar eclipse on January 4, 1639. It contains an annular eclipse on June 6, 1891; a hybrid eclipse on June 17, 1909; and total eclipses from June 29, 1927 through September 9, 2648. The series ends at member 77 as a partial eclipse on April 17, 3009. 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 annularity was produced by member 15 at 6 seconds (by default) on June 6, 1891, and the longest duration of totality will be produced by member 50 at 7 minutes, 12 seconds on June 25, 2522. All eclipses in this series occur at the Moon’s ascending node of orbit.[6]
| Series members 10–32 occur between 1801 and 2200: | ||
|---|---|---|
| 10 | 11 | 12 |
| File:SE1801Apr13P.png April 13, 1801 |
File:SE1819Apr24P.png April 24, 1819 |
File:SE1837May04P.png May 4, 1837 |
| 13 | 14 | 15 |
| File:SE1855May16P.png May 16, 1855 |
File:SE1873May26P.png May 26, 1873 |
File:SE1891Jun06A.png June 6, 1891 |
| 16 | 17 | 18 |
| File:SE1909Jun17H.png June 17, 1909 |
File:SE1927Jun29T.png June 29, 1927 |
File:1945Jul09T.png July 9, 1945 |
| 19 | 20 | 21 |
| File:SE1963Jul20T.png July 20, 1963 |
File:SE1981Jul31T.png July 31, 1981 |
File:SE1999Aug11T.png August 11, 1999 |
| 22 | 23 | 24 |
| File:SE2017Aug21T.png August 21, 2017 |
File:SE2035Sep02T.png September 2, 2035 |
File:SE2053Sep12T.png September 12, 2053 |
| 25 | 26 | 27 |
| File:SE2071Sep23T.png September 23, 2071 |
File:SE2089Oct04T.png October 4, 2089 |
File:SE2107Oct16T.png October 16, 2107 |
| 28 | 29 | 30 |
| File:SE2125Oct26T.png October 26, 2125 |
File:SE2143Nov07T.png November 7, 2143 |
File:SE2161Nov17T.png November 17, 2161 |
| 31 | 32 | |
| File:SE2179Nov28T.png November 28, 2179 |
File:SE2197Dec09T.png December 9, 2197 | |
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 ascending node.
| 21 eclipse events between June 21, 1982 and June 21, 2058 | ||||
|---|---|---|---|---|
| June 21 | April 8–9 | January 26 | November 13–14 | September 1–2 |
| 117 | 119 | 121 | 123 | 125 |
| File:SE1982Jun21P.png June 21, 1982 |
File:SE1986Apr09P.png April 9, 1986 |
File:SE1990Jan26A.png January 26, 1990 |
File:SE1993Nov13P.png November 13, 1993 |
File:SE1997Sep02P.png September 2, 1997 |
| 127 | 129 | 131 | 133 | 135 |
| File:SE2001Jun21T.png June 21, 2001 |
File:SE2005Apr08H.png April 8, 2005 |
File:SE2009Jan26A.png January 26, 2009 |
File:SE2012Nov13T.png November 13, 2012 |
File:SE2016Sep01A.png September 1, 2016 |
| 137 | 139 | 141 | 143 | 145 |
| File:SE2020Jun21A.png June 21, 2020 |
File:SE2024Apr08T.png April 8, 2024 |
File:SE2028Jan26A.png January 26, 2028 |
File:SE2031Nov14H.png November 14, 2031 |
File:SE2035Sep02T.png September 2, 2035 |
| 147 | 149 | 151 | 153 | 155 |
| File:SE2039Jun21A.png June 21, 2039 |
File:SE2043Apr09T.png April 9, 2043 |
File:SE2047Jan26P.png January 26, 2047 |
File:SE2050Nov14P.png November 14, 2050 |
File:SE2054Sep02P.png September 2, 2054 |
| 157 | ||||
| File:SE2058Jun21P.png June 21, 2058 | ||||
Tritos series
Template:Solar Tritos series 2002 December 4
Inex series
Template:Solar Inex series 2006 September 22
References
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External links
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