Solar eclipse of September 2, 2035

Total eclipse
Map
Gamma	0.3727
Magnitude	1.032
Maximum eclipse
Duration	174 s (2 min 54 s)
Coordinates	29°06′N158°00′E / 29.1°N 158°E /29.1; 158
Max. width of band	116 km (72 mi)
Times (UTC)
Greatest eclipse	1:56:46
References
Saros	145 (23 of 77)
Catalog # (SE5000)	9586
←March 9, 2035 February 27, 2036 →

A totalsolar eclipse will occur at the Moon'sascending node of orbit between Saturday, September 1, and Sunday, September 2, 2035,^[1] with amagnitude of 1.032. Asolar eclipse occurs when theMoon passes betweenEarth and theSun, thereby totally or partly obscuring the image of the Sun for a viewer on Earth. A total solar eclipse occurs when the Moon'sapparent 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 afterperigee (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 northernChina,North Korea, the extreme northern tip ofSouth Korea (Goseong County, Gangwon Province) andJapan. A partial eclipse will be visible for most ofAsia, northernOceania,Hawaii, southwestAlaska, and the westernUnited States.

The path of totality will cross two Asian capital cities,Beijing,China andPyongyang,North Korea, and will pass north of a third,Tokyo, Japan.^[3]

Solar Eclipse of September 2, 2035
(Local Times)

Country or territory	City or place	Start of partial eclipse	Start of total eclipse	Maximum eclipse	End of total eclipse	End of partial eclipse	Duration of totality (min:s)	Duration of eclipse (hr:min)	Maximum magnitude
China	Baotou	07:22:14	08:27:38	08:28:05	08:28:31	09:41:06	0:53	2:19	1.0022
China	Datong	07:23:05	08:29:52	08:30:39	08:31:26	09:45:42	1:34	2:23	1.0072
China	Beijing	07:24:29	08:32:50	08:33:37	08:34:25	09:50:22	1:35	2:26	1.0067
China	Tangshan	07:25:18	08:35:00	08:35:24	08:35:49	09:53:13	0:49	2:28	1.0016
China	Qinhuangdao	07:26:24	08:36:13	08:37:11	08:38:09	09:55:36	1:56	2:29	1.0129
North Korea	Pyongyang	08:30:28	09:43:54	09:44:48	09:45:41	11:06:42	1:47	2:36	1.0066
North Korea	Kaechon	08:31:00	09:44:56	09:45:12	09:45:28	11:06:47	0:32	2:36	1.0008
North Korea	Wonsan	08:32:04	09:46:12	09:47:15	09:48:19	11:09:50	2:07	2:38	1.0107
Japan	Toyama	08:42:11	10:03:01	10:03:41	10:04:22	11:31:11	1:21	2:49	1.0027
Japan	Nagano	08:43:32	10:04:25	10:05:34	10:06:43	11:33:19	2:18	2:50	1.0088
Japan	Utsunomiya	08:45:56	10:07:37	10:08:52	10:10:07	11:36:58	2:30	2:51	1.0111
References:[1]

Solar Eclipse of September 2, 2035
(Local Times)

Country or territory	City or place	Start of partial eclipse	Maximum eclipse	End of partial eclipse	Duration of eclipse (hr:min)	Maximum coverage
Bangladesh	Dhaka	05:40:21 (sunrise)	06:08:22	07:04:18	1:24	42.63%
Nepal	Kathmandu	05:42:48 (sunrise)	05:54:36	06:52:16	1:09	59.65%
Bhutan	Thimphu	05:40:41 (sunrise)	06:09:50	07:08:57	1:28	56.70%
Vietnam	Hanoi	06:22:43	07:15:28	08:14:25	1:52	29.04%
Kazakhstan	Almaty	05:17:03 (sunrise)	05:21:05	06:18:42	1:02	81.69%
China	Ürümqi	07:33:33 (sunrise)	08:21:23	09:23:03	1:50	84.51%
Hong Kong	Hong Kong	07:25:44	08:24:49	09:31:28	2:06	33.33%
Kyrgyzstan	Bishkek	06:26:47 (sunrise)	06:29:44	07:18:00	0:51	73.71%
India	New Delhi	05:59:32 (sunrise)	06:01:58	06:36:23	0:37	44.05%
Mongolia	Ulaanbaatar	07:29:42	08:32:14	09:40:14	2:11	73.91%
Russia	Omsk	06:13:53 (sunrise)	06:33:38	07:24:46	1:11	43.67%
China	Tianjin	07:24:22	08:34:02	09:51:29	2:27	98.52%
Russia	Irkutsk	07:36:02	08:35:14	09:38:51	2:03	58.89%
Taiwan	Taipei	07:28:27	08:36:04	09:52:27	2:24	45.05%
China	Shanghai	07:25:05	08:36:33	09:56:58	2:32	68.81%
China	Dalian	07:27:06	08:39:12	09:59:06	2:32	99.06%
Uzbekistan	Andijan	05:38:03 (sunrise)	05:40:53	06:16:16	0:38	52.03%
Pakistan	Lahore	05:38:48 (sunrise)	05:41:19	06:09:03	0:30	35.93%
North Korea	Nampo	08:29:59	09:44:12	11:06:05	2:36	99.78%
Pakistan	Islamabad	05:41:58 (sunrise)	05:44:46	06:10:52	0:29	34.03%
South Korea	Seoul	08:30:48	09:46:12	11:09:22	2:39	96.56%
North Korea	Hamhung	08:32:38	09:47:37	11:09:47	2:37	98.97%
Russia	Vladivostok	09:39:31	10:54:47	12:15:52	2:36	84.48%
Japan	Tokyo	08:45:32	10:08:49	11:37:27	2:52	99.52%
Russia	Yuzhno-Sakhalinsk	10:56:49	12:11:27	13:28:58	2:32	62.64%
United States Minor Outlying Islands	Wake Island	12:57:25	14:31:02	15:55:09	2:58	86.78%
United States Minor Outlying Islands	Midway Atoll[a]	14:24:10	15:43:42	16:54:41	2:31	63.95%
Marshall Islands	Majuro	13:36:02	15:00:29	16:14:31	2:38	55.37%
United States	Honolulu[a]	16:08:13	17:14:18	18:13:15	2:05	59.85%
Kiribati	Kiritimati	16:30:49	17:36:30	18:33:34 (sunset)	2:03	78.67%
References:[1]

The 2035 eclipse is the setting of the 2003 video gameCastlevania: Aria of Sorrow. Dracula's castle is located inside the solar eclipse, having been sealed there in1999.

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]

This eclipse is part of aneclipse 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 afortnight.

Eclipse season of August–September 2035

August 19 Descending node (full moon)	September 2 Ascending node (new moon)
Partial lunar eclipse Lunar Saros 119	Total solar eclipse Solar Saros 145

• 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.

• Preceded by:Solar eclipse of November 14, 2031
• Followed by:Solar eclipse of June 21, 2039

• Preceded by:Solar eclipse of July 22, 2028
• Followed by:Solar eclipse of October 14, 2042

• Preceded by:Lunar eclipse of August 28, 2026
• Followed by:Lunar eclipse of September 7, 2044

• Preceded by:Solar eclipse of October 2, 2024
• Followed by:Solar eclipse of August 2, 2046

• Preceded by:Solar eclipse of August 21, 2017
• Followed by:Solar eclipse of September 12, 2053

• Preceded by:Solar eclipse of September 22, 2006
• Followed by:Solar eclipse of August 12, 2064

• Preceded by:Solar eclipse of November 1, 1948
• Followed by:Solar eclipse of July 4, 2122

This eclipse is a member of asemester series. An eclipse in a semester series of solar eclipses repeats approximately every 177 days and 4 hours (a semester) at alternatingnodes of the Moon's orbit.^[5]

The partial solar eclipse onJuly 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

This eclipse is a part ofSaros series 145, repeating every 18 years, 11 days, and containing 77 events. The series started with a partial solar eclipse onJanuary 4, 1639. It contains an annular eclipse on June 6, 1891; a hybrid eclipse onJune 17, 1909; and total eclipses fromJune 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 oneexeligmos 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’sascending node of orbit.^[6]

Series members 10–32 occur between 1801 and 2200:
10	11	12
April 13, 1801	April 24, 1819	May 4, 1837
13	14	15
May 16, 1855	May 26, 1873	June 6, 1891
16	17	18
June 17, 1909	June 29, 1927	July 9, 1945
19	20	21
July 20, 1963	July 31, 1981	August 11, 1999
22	23	24
August 21, 2017	September 2, 2035	September 12, 2053
25	26	27
September 23, 2071	October 4, 2089	October 16, 2107
28	29	30
October 26, 2125	November 7, 2143	November 17, 2161
31	32
November 28, 2179	December 9, 2197

Themetonic 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
June 21, 1982	April 9, 1986	January 26, 1990	November 13, 1993	September 2, 1997
127	129	131	133	135
June 21, 2001	April 8, 2005	January 26, 2009	November 13, 2012	September 1, 2016
137	139	141	143	145
June 21, 2020	April 8, 2024	January 26, 2028	November 14, 2031	September 2, 2035
147	149	151	153	155
June 21, 2039	April 9, 2043	January 26, 2047	November 14, 2050	September 2, 2054
157
June 21, 2058

This eclipse is a part of atritos cycle, repeating at alternating nodes every 135synodic months (≈ 3986.63 days, or 11 years minus 1 month). Their appearance and longitude are irregular due to a lack of synchronization with theanomalistic 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 2200
June 16, 1806 (Saros 124)	May 16, 1817 (Saros 125)	April 14, 1828 (Saros 126)	March 15, 1839 (Saros 127)	February 12, 1850 (Saros 128)
January 11, 1861 (Saros 129)	December 12, 1871 (Saros 130)	November 10, 1882 (Saros 131)	October 9, 1893 (Saros 132)	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)	February 28, 2101 (Saros 151)	January 29, 2112 (Saros 152)	December 28, 2122 (Saros 153)
November 26, 2133 (Saros 154)	October 26, 2144 (Saros 155)	September 26, 2155 (Saros 156)	August 25, 2166 (Saros 157)	July 25, 2177 (Saros 158)
June 24, 2188 (Saros 159)	May 24, 2199 (Saros 160)

This eclipse is a part of the long periodinex cycle, repeating at alternating nodes, every 358synodic months (≈ 10,571.95 days, or 29 years minus 20 days). Their appearance and longitude are irregular due to a lack of synchronization with theanomalistic 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
February 11, 1804 (Saros 137)	January 20, 1833 (Saros 138)	December 31, 1861 (Saros 139)
December 12, 1890 (Saros 140)	November 22, 1919 (Saros 141)	November 1, 1948 (Saros 142)
October 12, 1977 (Saros 143)	September 22, 2006 (Saros 144)	September 2, 2035 (Saros 145)
August 12, 2064 (Saros 146)	July 23, 2093 (Saros 147)	July 4, 2122 (Saros 148)
June 14, 2151 (Saros 149)	May 24, 2180 (Saros 150)

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