Solar eclipse of September 2, 2035

Last updated
Solar eclipse of September 2, 2035
SE2035Sep02T.png
Map
Type of eclipse
NatureTotal
Gamma 0.3727
Magnitude 1.032
Maximum eclipse
Duration174 s (2 min 54 s)
Coordinates 29°06′N158°00′E / 29.1°N 158°E / 29.1; 158
Max. width of band116 km (72 mi)
Times (UTC)
Greatest eclipse1:56:46
References
Saros 145 (23 of 77)
Catalog # (SE5000) 9586

A total solar eclipse will occur at the Moon's ascending node of orbit between Saturday, September 1 and 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 August 30, 2035, at 3:35 UTC), the Moon's apparent diameter will be larger. [2]

Contents

Totality will be visible from parts of northern China, North Korea, and Japan. A partial eclipse will be visible for most of Asia, northern Oceania, Hawaii, southwest Alaska, and the western United States.

Visibility

Animation of the eclipse shadow. The dot in the center represents the path of totality. SE2035Sep02T.gif
Animation of the eclipse shadow. The dot in the center represents the path of totality.

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]

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]

September 2, 2035 Solar Eclipse Times
EventTime (UTC)
First Penumbral External Contact2035 September 01 at 23:16:45.8 UTC
First Umbral External Contact2035 September 02 at 00:17:05.5 UTC
First Central Line2035 September 02 at 00:17:36.1 UTC
First Umbral Internal Contact2035 September 02 at 00:18:06.7 UTC
First Penumbral Internal Contact2035 September 02 at 01:28:48.7 UTC
Equatorial Conjunction2035 September 02 at 01:45:01.1 UTC
Greatest Duration2035 September 02 at 01:53:17.4 UTC
Greatest Eclipse2035 September 02 at 01:56:46.3 UTC
Ecliptic Conjunction2035 September 02 at 02:00:44.2 UTC
Last Penumbral Internal Contact2035 September 02 at 02:25:01.7 UTC
Last Umbral Internal Contact2035 September 02 at 03:35:37.6 UTC
Last Central Line2035 September 02 at 03:36:05.7 UTC
Last Umbral External Contact2035 September 02 at 03:36:33.8 UTC
Last Penumbral External Contact2035 September 02 at 04:36:57.8 UTC
September 2, 2035 Solar Eclipse Parameters
ParameterValue
Eclipse Magnitude1.03204
Eclipse Obscuration1.06510
Gamma0.37273
Sun Right Ascension10h44m07.3s
Sun Declination+08°01'09.8"
Sun Semi-Diameter15'50.9"
Sun Equatorial Horizontal Parallax08.7"
Moon Right Ascension10h44m32.4s
Moon Declination+08°22'14.7"
Moon Semi-Diameter16'06.4"
Moon Equatorial Horizontal Parallax0°59'06.9"
ΔT76.4 s

Eclipse season

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.

Eclipse season of August–September 2035
August 19
Descending node (full moon)
September 2
Ascending node (new moon)
Lunar eclipse chart close-2035Aug19.png SE2035Sep02T.png
Partial lunar eclipse
Lunar Saros 119
Total solar eclipse
Solar Saros 145

Eclipses in 2035

Metonic

Tzolkinex

Half-Saros

Tritos

Solar Saros 145

Inex

Triad

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
SarosMapGammaSarosMapGamma
120 March 30, 2033
SE2033Mar30T.png
Total
0.9778125 September 23, 2033
SE2033Sep23P.png
Partial
−1.1583
130 March 20, 2034
SE2034Mar20T.png
Total
0.2894135 September 12, 2034
SE2034Sep12A.png
Annular
−0.3936
140 March 9, 2035
SE2035Mar09A.png
Annular
−0.4368145 September 2, 2035
SE2035Sep02T.png
Total
0.3727
150 February 27, 2036
SE2036Feb27P.png
Partial
−1.1942155 August 21, 2036
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:
101112
SE1801Apr13P.png
April 13, 1801
SE1819Apr24P.png
April 24, 1819
SE1837May04P.png
May 4, 1837
131415
SE1855May16P.png
May 16, 1855
SE1873May26P.png
May 26, 1873
SE1891Jun06A.png
June 6, 1891
161718
SE1909Jun17H.png
June 17, 1909
SE1927Jun29T.png
June 29, 1927
1945Jul09T.png
July 9, 1945
192021
SE1963Jul20T.png
July 20, 1963
SE1981Jul31T.png
July 31, 1981
SE1999Aug11T.png
August 11, 1999
222324
SE2017Aug21T.png
August 21, 2017
SE2035Sep02T.png
September 2, 2035
SE2053Sep12T.png
September 12, 2053
252627
SE2071Sep23T.png
September 23, 2071
SE2089Oct04T.png
October 4, 2089
SE2107Oct16T.png
October 16, 2107
282930
SE2125Oct26T.png
October 26, 2125
SE2143Nov07T.png
November 7, 2143
SE2161Nov17T.png
November 17, 2161
3132
SE2179Nov28T.png
November 28, 2179
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 21April 8–9January 26November 13–14September 1–2
117119121123125
SE1982Jun21P.png
June 21, 1982
SE1986Apr09P.png
April 9, 1986
SE1990Jan26A.png
January 26, 1990
SE1993Nov13P.png
November 13, 1993
SE1997Sep02P.png
September 2, 1997
127129131133135
SE2001Jun21T.png
June 21, 2001
SE2005Apr08H.png
April 8, 2005
SE2009Jan26A.png
January 26, 2009
SE2012Nov13T.png
November 13, 2012
SE2016Sep01A.png
September 1, 2016
137139141143145
SE2020Jun21A.png
June 21, 2020
SE2024Apr08T.png
April 8, 2024
SE2028Jan26A.png
January 26, 2028
SE2031Nov14H.png
November 14, 2031
SE2035Sep02T.png
September 2, 2035
147149151153155
SE2039Jun21A.png
June 21, 2039
SE2043Apr09T.png
April 9, 2043
SE2047Jan26P.png
January 26, 2047
SE2050Nov14P.png
November 14, 2050
SE2054Sep02P.png
September 2, 2054
157
SE2058Jun21P.png
June 21, 2058

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.

Series members between 1801 and 2200
SE1806Jun16T.png
June 16, 1806
(Saros 124)
SE1817May16A.gif
May 16, 1817
(Saros 125)
Saros126 37van72 SE1828Apr14H.jpg
April 14, 1828
(Saros 126)
SE1839Mar15T.gif
March 15, 1839
(Saros 127)
SE1850Feb12A.gif
February 12, 1850
(Saros 128)
SE1861Jan11A.gif
January 11, 1861
(Saros 129)
SE1871Dec12T.png
December 12, 1871
(Saros 130)
SE1882Nov10A.gif
November 10, 1882
(Saros 131)
SE1893Oct09A.gif
October 9, 1893
(Saros 132)
SE1904Sep09T.png
September 9, 1904
(Saros 133)
SE1915Aug10A.png
August 10, 1915
(Saros 134)
SE1926Jul09A.png
July 9, 1926
(Saros 135)
SE1937Jun08T.png
June 8, 1937
(Saros 136)
SE1948May09A.png
May 9, 1948
(Saros 137)
SE1959Apr08A.png
April 8, 1959
(Saros 138)
SE1970Mar07T.png
March 7, 1970
(Saros 139)
SE1981Feb04A.png
February 4, 1981
(Saros 140)
SE1992Jan04A.png
January 4, 1992
(Saros 141)
SE2002Dec04T.png
December 4, 2002
(Saros 142)
SE2013Nov03H.png
November 3, 2013
(Saros 143)
SE2024Oct02A.png
October 2, 2024
(Saros 144)
SE2035Sep02T.png
September 2, 2035
(Saros 145)
SE2046Aug02T.png
August 2, 2046
(Saros 146)
SE2057Jul01A.png
July 1, 2057
(Saros 147)
SE2068May31T.png
May 31, 2068
(Saros 148)
SE2079May01T.png
May 1, 2079
(Saros 149)
SE2090Mar31P.png
March 31, 2090
(Saros 150)
SE2101Feb28A.png
February 28, 2101
(Saros 151)
Saros152 18van70 SE2112Jan29T.jpg
January 29, 2112
(Saros 152)
Saros153 15van70 SE2122Dec28A.jpg
December 28, 2122
(Saros 153)
Saros154 13van71 SE2133Nov26A.jpg
November 26, 2133
(Saros 154)
Saros155 13van71 SE2144Oct26T.jpg
October 26, 2144
(Saros 155)
Saros156 09van69 SE2155Sep26A.jpg
September 26, 2155
(Saros 156)
SE2166Aug25A.png
August 25, 2166
(Saros 157)
Saros158 07van70 SE2177Jul25P.jpg
July 25, 2177
(Saros 158)
Saros159 04van70 SE2188Jun24P.jpg
June 24, 2188
(Saros 159)
Saros160 02van71 SE2199May24P.jpg
May 24, 2199
(Saros 160)

Inex series

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
SE1804Feb11H.png
February 11, 1804
(Saros 137)
SE1833Jan20A.gif
January 20, 1833
(Saros 138)
SE1861Dec31T.gif
December 31, 1861
(Saros 139)
SE1890Dec12H.gif
December 12, 1890
(Saros 140)
SE1919Nov22A.png
November 22, 1919
(Saros 141)
SE1948Nov01T.png
November 1, 1948
(Saros 142)
SE1977Oct12T.png
October 12, 1977
(Saros 143)
SE2006Sep22A.png
September 22, 2006
(Saros 144)
SE2035Sep02T.png
September 2, 2035
(Saros 145)
SE2064Aug12T.png
August 12, 2064
(Saros 146)
SE2093Jul23A.png
July 23, 2093
(Saros 147)
Saros148 27van75 SE2122Jul04T.jpg
July 4, 2122
(Saros 148)
Saros149 28van71 SE2151Jun14T.jpg
June 14, 2151
(Saros 149)
Saros150 26van71 SE2180May24A.jpg
May 24, 2180
(Saros 150)

Related Research Articles

<span class="mw-page-title-main">Solar eclipse of August 24, 2063</span> Total eclipse

A total solar eclipse will occur at the Moon's descending node of orbit on Friday, August 24, 2063, with a magnitude of 1.075. 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.

<span class="mw-page-title-main">Solar eclipse of April 20, 2042</span> Total eclipse

A total solar eclipse will occur at the Moon's ascending node of orbit between Saturday, April 19 and Sunday, April 20, 2042, with a magnitude of 1.0614. 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 only about 21 hours after perigee, the Moon's apparent diameter will be larger.

<span class="mw-page-title-main">Solar eclipse of July 22, 2028</span> Total eclipse

A total solar eclipse will occur at the Moon's descending node of orbit on Saturday, July 22, 2028, with a magnitude of 1.056. 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 1.8 days before perigee, the Moon's apparent diameter will be larger.

<span class="mw-page-title-main">Solar eclipse of February 17, 2026</span> Future annular solar eclipse

An annular solar eclipse will occur at the Moon’s ascending node of orbit on Tuesday, February 17, 2026, with a magnitude of 0.963. 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 6.8 days after apogee and 7.5 days before perigee.

<span class="mw-page-title-main">Solar eclipse of November 14, 2031</span> Total eclipse

A total solar eclipse will occur at the Moon's ascending node of orbit on Friday, November 14, 2031, with a magnitude of 1.0106. It is a hybrid event, with portions of its central path near sunrise and sunset 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. Occurring about 3.1 days before perigee, the Moon's apparent diameter will be larger.

<span class="mw-page-title-main">Solar eclipse of March 9, 2035</span> Future annular 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, 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 and 5.1 days before perigee.

<span class="mw-page-title-main">Solar eclipse of December 26, 2038</span> Total eclipse

A total solar eclipse will occur at the Moon's descending node of orbit between Saturday, December 25 and Sunday, December 26, 2038, with a magnitude of 1.0268. 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 1.7 days after perigee, the Moon's apparent diameter will be larger.

<span class="mw-page-title-main">Solar eclipse of February 28, 2044</span> Future annular solar eclipse

An annular solar eclipse will occur at the Moon's ascending node of orbit on Sunday, February 28, 2044, with a magnitude of 0.96. 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. Occurring about 6.7 days after apogee, the Moon's apparent diameter will be smaller.

<span class="mw-page-title-main">Solar eclipse of August 2, 2046</span> Total eclipse

A total solar eclipse will occur at the Moon's descending node of orbit on Thursday, August 2, 2046, with a magnitude of 1.0531. 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 greater than the Sun's, blocking all direct sunlight. 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 days before perigee, the Moon's apparent diameter will be larger.

<span class="mw-page-title-main">Solar eclipse of November 1, 1948</span> Total eclipse

A total solar eclipse occurred at the Moon's descending node of orbit on Monday, November 1, 1948, with a magnitude of 1.0231. 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 2.4 days after perigee, the Moon's apparent diameter was larger.

<span class="mw-page-title-main">Solar eclipse of September 22, 2052</span> Future annular solar eclipse

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.

<span class="mw-page-title-main">Solar eclipse of September 12, 2053</span> Total eclipse

A total solar eclipse will take place at the Moon's ascending node of orbit on Friday, September 12, 2053, with a magnitude of 1.0328. 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.

<span class="mw-page-title-main">Solar eclipse of March 20, 2053</span> Future annular solar eclipse

An annular solar eclipse will occur at the Moon's descending node of orbit on Thursday, March 20, 2053, 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.

<span class="mw-page-title-main">Solar eclipse of August 12, 2064</span> Total eclipse

A total solar eclipse will occur at the Moon's descending node of orbit on Tuesday, August 12, 2064, with a magnitude of 1.0495. 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. This eclipse will pass through the Chilean cities of Valparaíso and the capital Santiago.

<span class="mw-page-title-main">Solar eclipse of February 17, 2064</span> Future annular solar eclipse

An annular solar eclipse will occur at the Moon's ascending node of orbit on Sunday, February 17, 2064, with a magnitude of 0.9262. 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.

<span class="mw-page-title-main">Solar eclipse of September 23, 2071</span> Total eclipse

A total solar eclipse will occur at the Moon's ascending node of orbit on Wednesday, September 23, 2071, with a magnitude of 1.0333. 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.

<span class="mw-page-title-main">Solar eclipse of August 24, 2082</span> Total eclipse

A total solar eclipse will occur at the Moon's descending node of orbit on Monday, August 24, 2082, with a magnitude of 1.0452. 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.

<span class="mw-page-title-main">Solar eclipse of April 21, 2088</span> Total eclipse

A total solar eclipse will occur at the Moon's descending node of orbit on Wednesday, April 21, 2088, with a magnitude of 1.0474. 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.

<span class="mw-page-title-main">Solar eclipse of October 12, 1939</span> Total eclipse

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. Occurring about 1.8 days after perigee, the Moon's apparent diameter was larger.

<span class="mw-page-title-main">Solar eclipse of October 1, 1921</span> Total eclipse

A total solar eclipse occurred at the Moon's ascending node of orbit on Saturday, October 1, 1921, with a magnitude of 1.0293. 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 1.9 days after perigee, the Moon's apparent diameter was larger.

References

  1. "September 1–2, 2035 Total Solar Eclipse". timeanddate. Retrieved 14 August 2024.
  2. "Moon Distances for London, United Kingdom, England". timeanddate. Retrieved 14 August 2024.
  3. Kennedy, Kelsey (August 21, 2017). "If You Missed This Year's Eclipse, Chase Another". Atlas Obscura. Retrieved December 12, 2017.
  4. "Total Solar Eclipse of 2035 Sep 02". EclipseWise.com. Retrieved 14 August 2024.
  5. 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.
  6. "NASA - Catalog of Solar Eclipses of Saros 145". eclipse.gsfc.nasa.gov.