Solar eclipse of July 2, 2019

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Template:Short description Script error: No such module "Solar eclipse". A total solar eclipse occurred at the Moon's ascending node of orbit on Tuesday, July 2, 2019,[1][2][3][4][5] with a magnitude of 1.0459. A total solar eclipse occurs when the Moon's apparent diameter is larger than the Sun's and the apparent path of the Sun and Moon intersect, blocking all direct sunlight and turning daylight into darkness; the Sun appears to be black with a halo around it. 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 before perigee (on July 5, 2019, at 6:00 UTC), the Moon's apparent diameter was larger.[6]

Totality was visible from the southern Pacific Ocean east of New Zealand to the Pitcairn Islands and the Tuamotu Archipelago and finally reaching the Coquimbo Region in Chile and central Argentina near sunset, with the maximum of 4 minutes 33 seconds visible from the Pacific Ocean. A partial eclipse was visible for parts of eastern Oceania, South America, and southern Central America. A total solar eclipse crossed a similar region of the Earth about a year and a half later on December 14, 2020.

List of major cities in the path of totality

Images

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Visibility

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.

Following the North American solar eclipse of August 21, 2017, Astronomers Without Borders collected eclipse glasses for redistribution to Latin America and Asia for the 2019 eclipses.[8]

Totality travelled over areas with low levels of humidity and light pollution, allowing for very good observations. Several major observatories experienced totality, including the European Southern Observatory.[9][10]

Oeno Island

The first land surface and the only Pacific island from which totality was visible is Oeno Island, an uninhabited atoll in the Pitcairn Islands.[10]

Chile

Totality was visible in a large portion of Coquimbo Region and small parts of Atacama Region. Cities in the path included La Serena and La Higuera. Approximately 300,000 people visited La Serena to view the event.[9] Tickets to view the eclipse from the European Southern Observatory were sold for US$2000 each.[10]

Argentina

Totality was visible in the provinces of San Juan, La Rioja, San Luis, Córdoba, Santa Fe, and Buenos Aires. Cities in the path included San Juan and Río Cuarto.[10] The path of totality finished at the Samborombon Bay, where the eclipsed sunset was observed from San Clemente del Tuyu.

Gallery

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.[11]

July 2, 2019 Solar Eclipse Times
Event Time (UTC)
First Penumbral External Contact 2019 July 2 at 16:56:22.9 UTC
First Umbral External Contact 2019 July 2 at 18:02:19.5 UTC
First Central Line 2019 July 2 at 18:03:29.5 UTC
First Umbral Internal Contact 2019 July 2 at 18:04:39.8 UTC
Ecliptic Conjunction 2019 July 2 at 19:17:21.9 UTC
Equatorial Conjunction 2019 July 2 at 19:22:51.0 UTC
Greatest Eclipse 2019 July 2 at 19:24:07.5 UTC
Greatest Duration 2019 July 2 at 19:25:18.8 UTC
Last Umbral Internal Contact 2019 July 2 at 20:43:33.5 UTC
Last Central Line 2019 July 2 at 20:44:46.0 UTC
Last Umbral External Contact 2019 July 2 at 20:45:58.2 UTC
Last Penumbral External Contact 2019 July 2 at 21:51:48.1 UTC
July 2, 2019 Solar Eclipse Parameters
Parameter Value
Eclipse Magnitude 1.04593
Eclipse Obscuration 1.09398
Gamma −0.64656
Sun Right Ascension 06h46m14.8s
Sun Declination +23°00'36.4"
Sun Semi-Diameter 15'43.8"
Sun Equatorial Horizontal Parallax 08.6"
Moon Right Ascension 06h46m17.9s
Moon Declination +22°22'09.2"
Moon Semi-Diameter 16'14.9"
Moon Equatorial Horizontal Parallax 0°59'37.8"
ΔT 69.6 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.

Eclipse season of July 2019
July 2
Ascending node (new moon)
July 16
Descending node (full moon)
File:SE2019Jul02T.png File:Lunar eclipse chart close-2019Jul16.png
Total solar eclipse
Solar Saros 127
Partial lunar eclipse
Lunar Saros 139

Related eclipses

Eclipses in 2019

Metonic

Tzolkinex

Half-Saros

Tritos

Solar Saros 127

Inex

Triad

Solar eclipses of 2018–2021

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.[12]

The partial solar eclipses on February 15, 2018 and August 11, 2018 occur in the previous lunar year eclipse set.

Solar eclipse series sets from 2018 to 2021
Ascending node   Descending node
Saros Map Gamma Saros Map Gamma
117
File:Eclipse (41629136430).jpg
Partial in Melbourne, Australia
July 13, 2018
File:SE2018Jul13P.png
Partial
−1.35423 122
File:Solar eclipse of January 6, 2019 in Nakhodka, Primorsky Krai.jpg
Partial in Nakhodka, Russia
January 6, 2019
File:SE2019Jan06P.png
Partial
1.14174
127
File:20190702 Totality LaSerena Chile.jpg
Totality in La Serena, Chile
July 2, 2019
File:SE2019Jul02T.png
Total
−0.64656 132
File:Annular Solar Eclipse in Jaffna - 26 December 2019 (1).jpg
Annularity in Jaffna, Sri Lanka
December 26, 2019
File:SE2019Dec26A.png
Annular
0.41351
137
File:Solar eclipse of 21 June 2020 in Beigang, Yunlin, Taiwan.jpg
Annularity in Beigang, Yunlin, Taiwan
June 21, 2020
File:SE2020Jun21A.png
Annular
0.12090 142
File:Eclipse total Gorbea 2020.jpg
Totality in Gorbea, Chile
December 14, 2020
File:SE2020Dec14T.png
Total
−0.29394
147
File:Partial Solar Eclipse, 10 June 2021 (51237879346) (cropped).jpg
Partial in Halifax, Canada
June 10, 2021
File:SE2021Jun10A.png
Annular
0.91516 152
File:Royal Navy sailors observed 2021 partial solar eclipse off South Georgia (cropped).jpg
From HMS Protector off South Georgia
December 4, 2021
File:SE2021Dec04T.png
Total
−0.95261

Saros 127

This eclipse is a part of Saros series 127, repeating every 18 years, 11 days, and containing 82 events. The series started with a partial solar eclipse on October 10, 991 AD. It contains total eclipses from May 14, 1352 through August 15, 2091. There are no annular or hybrid eclipses in this set. The series ends at member 82 as a partial eclipse on March 21, 2452. 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 totality was produced by member 31 at 5 minutes, 40 seconds on August 30, 1532. All eclipses in this series occur at the Moon’s ascending node of orbit.[13]

Series members 46–68 occur between 1801 and 2200:
46 47 48
File:SE1803Feb21T.png
February 21, 1803
File:SE1821Mar04T.gif
March 4, 1821
File:SE1839Mar15T.gif
March 15, 1839
49 50 51
File:SE1857Mar25T.gif
March 25, 1857
File:SE1875Apr06T.png
April 6, 1875
File:SE1893Apr16T.png
April 16, 1893
52 53 54
File:SE1911Apr28T.png
April 28, 1911
File:SE1929May09T.png
May 9, 1929
File:SE1947May20T.png
May 20, 1947
55 56 57
File:SE1965May30T.png
May 30, 1965
File:SE1983Jun11T.png
June 11, 1983
File:SE2001Jun21T.png
June 21, 2001
58 59 60
File:SE2019Jul02T.png
July 2, 2019
File:SE2037Jul13T.png
July 13, 2037
File:SE2055Jul24T.png
July 24, 2055
61 62 63
File:SE2073Aug03T.png
August 3, 2073
File:SE2091Aug15T.png
August 15, 2091
File:Saros127 63van82 SE2109Aug26P.jpg
August 26, 2109
64 65 66
File:Saros127 64van82 SE2127Sep06P.jpg
September 6, 2127
File:Saros127 65van82 SE2145Sep16P.jpg
September 16, 2145
File:Saros127 66van82 SE2163Sep28P.jpg
September 28, 2163
67 68
File:Saros127 67van82 SE2181Oct08P.jpg
October 8, 2181
File:Saros127 68van82 SE2199Oct19P.jpg
October 19, 2199

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 July 1, 2000 and July 1, 2076
July 1–2 April 19–20 February 5–7 November 24–25 September 12–13
117 119 121 123 125
File:SE2000Jul01P.png
July 1, 2000
File:SE2004Apr19P.png
April 19, 2004
File:SE2008Feb07A.png
February 7, 2008
File:SE2011Nov25P.png
November 25, 2011
File:SE2015Sep13P.png
September 13, 2015
127 129 131 133 135
File:SE2019Jul02T.png
July 2, 2019
File:SE2023Apr20H.png
April 20, 2023
File:SE2027Feb06A.png
February 6, 2027
File:SE2030Nov25T.png
November 25, 2030
File:SE2034Sep12A.png
September 12, 2034
137 139 141 143 145
File:SE2038Jul02A.png
July 2, 2038
File:SE2042Apr20T.png
April 20, 2042
File:SE2046Feb05A.png
February 5, 2046
File:SE2049Nov25H.png
November 25, 2049
File:SE2053Sep12T.png
September 12, 2053
147 149 151 153 155
File:SE2057Jul01A.png
July 1, 2057
File:SE2061Apr20T.png
April 20, 2061
File:SE2065Feb05P.png
February 5, 2065
File:SE2068Nov24P.png
November 24, 2068
File:SE2072Sep12T.png
September 12, 2072
157
File:SE2076Jul01P.png
July 1, 2076

Tritos series

Template:Solar Tritos series 2008 August 1

Inex series

Template:Solar Inex series 2019 July 2

References

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Additional sources

External links

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