Solar eclipse of September 2, 2035

{{Short description|Total eclipse}}

{{Infobox solar eclipse|2035Sep02

| previous = Solar eclipse of March 9, 2035

| next = Solar eclipse of February 27, 2036

}}

A total solar eclipse will occur at the Moon's ascending node of orbit on Sunday, September 2, 2035,{{cite web|title=September 1–2, 2035 Total Solar Eclipse|url=https://www.timeanddate.com/eclipse/solar/2035-september-2|publisher=timeanddate|access-date=14 August 2024}} 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.{{cite web|title=Moon Distances for London, United Kingdom, England|url=https://www.timeanddate.com/astronomy/moon/distance.html?year=2035&n=136|publisher=timeanddate|access-date=14 August 2024}}

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

File:SE2035Sep02T.gif

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.{{cite news|last1=Kennedy|first1=Kelsey|title=If You Missed This Year's Eclipse, Chase Another|url=https://www.atlasobscura.com/articles/upcoming-solar-eclipses-dates-places|access-date=December 12, 2017|work=Atlas Obscura|date=August 21, 2017|language=en}}

{{clear}}

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.{{cite web|title=Total Solar Eclipse of 2035 Sep 02|url=https://eclipsewise.com/solar/SEprime/2001-2100/SE2035Sep02Tprime.html|publisher=EclipseWise.com|access-date=14 August 2024}}

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|+September 2, 2035 Solar Eclipse Times

! Event

! Time (UTC)

First Penumbral External Contact

| 2035 September 01 at 23:16:45.8 UTC

First Umbral External Contact

| 2035 September 02 at 00:17:05.5 UTC

First Central Line

| 2035 September 02 at 00:17:36.1 UTC

First Umbral Internal Contact

| 2035 September 02 at 00:18:06.7 UTC

First Penumbral Internal Contact

| 2035 September 02 at 01:28:48.7 UTC

Equatorial Conjunction

| 2035 September 02 at 01:45:01.1 UTC

Greatest Duration

| 2035 September 02 at 01:53:17.4 UTC

Greatest Eclipse

| 2035 September 02 at 01:56:46.3 UTC

Ecliptic Conjunction

| 2035 September 02 at 02:00:44.2 UTC

Last Penumbral Internal Contact

| 2035 September 02 at 02:25:01.7 UTC

Last Umbral Internal Contact

| 2035 September 02 at 03:35:37.6 UTC

Last Central Line

| 2035 September 02 at 03:36:05.7 UTC

Last Umbral External Contact

| 2035 September 02 at 03:36:33.8 UTC

Last Penumbral External Contact

| 2035 September 02 at 04:36:57.8 UTC

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|+September 2, 2035 Solar Eclipse Parameters

! 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

{{clear}}

Eclipse season

{{See also|Eclipse cycle}}

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.

class="wikitable"

|+ Eclipse season of August–September 2035

! August 19
Descending node (full moon)
!! September 2
Ascending node (new moon)

200px200px
align=center

| Partial lunar eclipse
Lunar Saros 119

Total solar eclipse
Solar Saros 145

Related eclipses

= Eclipses in 2035 =

= Metonic =

= Tzolkinex =

= Half-Saros =

= Tritos =

= Solar Saros 145 =

= Inex =

= Triad =

= Solar eclipses of 2033–2036 =

{{Solar eclipse set 2033–2036}}

= Saros 145 =

{{Solar Saros series 145}}

= Metonic series =

{{Solar Metonic series 1982–2058}}

= Tritos series =

{{Solar Tritos series 2002 December 4}}

= Inex series =

{{Solar Inex series 2006 September 22}}

References

{{reflist}}

{{commons category|Solar eclipse of 2035 September 2}}