Solar eclipse of July 2, 2019

Last updated
Solar eclipse of July 2, 2019
20190702 Totality LaSerena Chile.jpg
Totality viewed from La Serena, Chile
SE2019Jul02T.png
Map
Type of eclipse
NatureTotal
Gamma −0.6466
Magnitude 1.0459
Maximum eclipse
Duration273 s (4 min 33 s)
Coordinates 17°24′S109°00′W / 17.4°S 109°W / -17.4; -109
Max. width of band201 km (125 mi)
Times (UTC)
Greatest eclipse19:24:08
References
Saros 127 (58 of 82)
Catalog # (SE5000) 9551

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]

Contents

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

SE2019Jul02T.gif
Animated path
July 2, 2019 Total Solar Eclipse from GOES-East.gif
Geostationary satellite view of the eclipse by NOAA's GOES East. Hurricane Barbara can also be seen in the northern hemisphere.

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.

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
EventTime (UTC)
First Penumbral External Contact2019 July 02 at 16:56:22.9 UTC
First Umbral External Contact2019 July 02 at 18:02:19.5 UTC
First Central Line2019 July 02 at 18:03:29.5 UTC
First Umbral Internal Contact2019 July 02 at 18:04:39.8 UTC
Ecliptic Conjunction2019 July 02 at 19:17:21.9 UTC
Equatorial Conjunction2019 July 02 at 19:22:51.0 UTC
Greatest Eclipse2019 July 02 at 19:24:07.5 UTC
Greatest Duration2019 July 02 at 19:25:18.8 UTC
Last Umbral Internal Contact2019 July 02 at 20:43:33.5 UTC
Last Central Line2019 July 02 at 20:44:46.0 UTC
Last Umbral External Contact2019 July 02 at 20:45:58.2 UTC
Last Penumbral External Contact2019 July 02 at 21:51:48.1 UTC
July 2, 2019 Solar Eclipse Parameters
ParameterValue
Eclipse Magnitude1.04593
Eclipse Obscuration1.09398
Gamma−0.64656
Sun Right Ascension06h46m14.8s
Sun Declination+23°00'36.4"
Sun Semi-Diameter15'43.8"
Sun Equatorial Horizontal Parallax08.6"
Moon Right Ascension06h46m17.9s
Moon Declination+22°22'09.2"
Moon Semi-Diameter16'14.9"
Moon Equatorial Horizontal Parallax0°59'37.8"
ΔT69.6 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 July 2019
July 2
Ascending node (new moon)
July 16
Descending node (full moon)
SE2019Jul02T.png Lunar eclipse chart close-2019Jul16.png
Total solar eclipse
Solar Saros 127
Partial lunar eclipse
Lunar Saros 139

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
SarosMapGammaSarosMapGamma
117
Eclipse (41629136430).jpg
Partial in Melbourne, Australia
July 13, 2018
SE2018Jul13P.png
Partial
−1.35423122
Solar eclipse of January 6, 2019 in Nakhodka, Primorsky Krai.jpg
Partial in Nakhodka, Russia
January 6, 2019
SE2019Jan06P.png
Partial
1.14174
127
20190702 Totality LaSerena Chile.jpg
Totality in La Serena, Chile
July 2, 2019
SE2019Jul02T.png
Total
−0.64656132
Annular Solar Eclipse in Jaffna - 26 December 2019 (1).jpg
Annularity in Jaffna, Sri Lanka
December 26, 2019
SE2019Dec26A.png
Annular
0.41351
137
Solar eclipse of 21 June 2020 in Beigang, Yunlin, Taiwan.jpg
Annularity in Beigang, Yunlin, Taiwan
June 21, 2020
SE2020Jun21A.png
Annular
0.12090142
Eclipse total Gorbea 2020.jpg
Totality in Gorbea, Chile
December 14, 2020
SE2020Dec14T.png
Total
−0.29394
147
Partial Solar Eclipse, 10 June 2021 (51237879346) (cropped).jpg
Partial in Halifax, Canada
June 10, 2021
SE2021Jun10A.png
Annular
0.91516152
Royal Navy sailors observed 2021 partial solar eclipse off South Georgia (cropped).jpg
From HMS Protector off South Georgia
December 4, 2021
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:
464748
SE1803Feb21T.png
February 21, 1803
SE1821Mar04T.gif
March 4, 1821
SE1839Mar15T.gif
March 15, 1839
495051
SE1857Mar25T.gif
March 25, 1857
SE1875Apr06T.png
April 6, 1875
SE1893Apr16T.png
April 16, 1893
525354
SE1911Apr28T.png
April 28, 1911
SE1929May09T.png
May 9, 1929
SE1947May20T.png
May 20, 1947
555657
SE1965May30T.png
May 30, 1965
SE1983Jun11T.png
June 11, 1983
SE2001Jun21T.png
June 21, 2001
585960
SE2019Jul02T.png
July 2, 2019
SE2037Jul13T.png
July 13, 2037
SE2055Jul24T.png
July 24, 2055
616263
SE2073Aug03T.png
August 3, 2073
SE2091Aug15T.png
August 15, 2091
Saros127 63van82 SE2109Aug26P.jpg
August 26, 2109
646566
Saros127 64van82 SE2127Sep06P.jpg
September 6, 2127
Saros127 65van82 SE2145Sep16P.jpg
September 16, 2145
Saros127 66van82 SE2163Sep28P.jpg
September 28, 2163
6768
Saros127 67van82 SE2181Oct08P.jpg
October 8, 2181
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 1–2April 19–20February 5–7November 24–25September 12–13
117119121123125
SE2000Jul01P.png
July 1, 2000
SE2004Apr19P.png
April 19, 2004
SE2008Feb07A.png
February 7, 2008
SE2011Nov25P.png
November 25, 2011
SE2015Sep13P.png
September 13, 2015
127129131133135
SE2019Jul02T.png
July 2, 2019
SE2023Apr20H.png
April 20, 2023
SE2027Feb06A.png
February 6, 2027
SE2030Nov25T.png
November 25, 2030
SE2034Sep12A.png
September 12, 2034
137139141143145
SE2038Jul02A.png
July 2, 2038
SE2042Apr20T.png
April 20, 2042
SE2046Feb05A.png
February 5, 2046
SE2049Nov25H.png
November 25, 2049
SE2053Sep12T.png
September 12, 2053
147149151153155
SE2057Jul01A.png
July 1, 2057
SE2061Apr20T.png
April 20, 2061
SE2065Feb05P.png
February 5, 2065
SE2068Nov24P.png
November 24, 2068
SE2072Sep12T.png
September 12, 2072
157
SE2076Jul01P.png
July 1, 2076

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
SE1801Mar14P.png
March 14, 1801
(Saros 107)
SE1812Feb12P.gif
February 12, 1812
(Saros 108)
SE1823Jan12P.gif
January 12, 1823
(Saros 109)
SE1844Nov10P.gif
November 10, 1844
(Saros 111)
SE1877Aug09P.gif
August 9, 1877
(Saros 114)
SE1888Jul09P.gif
July 9, 1888
(Saros 115)
SE1899Jun08P.gif
June 8, 1899
(Saros 116)
SE1910May09T.png
May 9, 1910
(Saros 117)
SE1921Apr08A.png
April 8, 1921
(Saros 118)
SE1932Mar07A.png
March 7, 1932
(Saros 119)
SE1943Feb04T.png
February 4, 1943
(Saros 120)
SE1954Jan05A.png
January 5, 1954
(Saros 121)
SE1964Dec04P.png
December 4, 1964
(Saros 122)
SE1975Nov03P.png
November 3, 1975
(Saros 123)
SE1986Oct03H.png
October 3, 1986
(Saros 124)
SE1997Sep02P.png
September 2, 1997
(Saros 125)
SE2008Aug01T.png
August 1, 2008
(Saros 126)
SE2019Jul02T.png
July 2, 2019
(Saros 127)
SE2030Jun01A.png
June 1, 2030
(Saros 128)
SE2041Apr30T.png
April 30, 2041
(Saros 129)
SE2052Mar30T.png
March 30, 2052
(Saros 130)
SE2063Feb28A.png
February 28, 2063
(Saros 131)
SE2074Jan27A.png
January 27, 2074
(Saros 132)
SE2084Dec27T.png
December 27, 2084
(Saros 133)
SE2095Nov27A.png
November 27, 2095
(Saros 134)
SE2106Oct26A.png
October 26, 2106
(Saros 135)
SE2117Sep26T.png
September 26, 2117
(Saros 136)
SE2128Aug25A.png
August 25, 2128
(Saros 137)
SE2139Jul25A.png
July 25, 2139
(Saros 138)
SE2150Jun25T.png
June 25, 2150
(Saros 139)
SE2161May25A.png
May 25, 2161
(Saros 140)
SE2172Apr23A.png
April 23, 2172
(Saros 141)
SE2183Mar23T.png
March 23, 2183
(Saros 142)
SE2194Feb21A.png
February 21, 2194
(Saros 143)

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
SE1816Nov19T.png
November 19, 1816
(Saros 120)
SE1845Oct30H.png
October 30, 1845
(Saros 121)
SE1874Oct10An.gif
October 10, 1874
(Saros 122)
SE1903Sep21T.png
September 21, 1903
(Saros 123)
SE1932Aug31T.png
August 31, 1932
(Saros 124)
SE1961Aug11A.png
August 11, 1961
(Saros 125)
SE1990Jul22T.png
July 22, 1990
(Saros 126)
SE2019Jul02T.png
July 2, 2019
(Saros 127)
SE2048Jun11A.png
June 11, 2048
(Saros 128)
SE2077May22T.png
May 22, 2077
(Saros 129)
SE2106May03T.png
May 3, 2106
(Saros 130)
SE2135Apr13A.png
April 13, 2135
(Saros 131)
SE2164Mar23H.png
March 23, 2164
(Saros 132)
SE2193Mar03T.png
March 3, 2193
(Saros 133)

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<span class="mw-page-title-main">Solar eclipse of January 3, 1927</span> 20th-century annular solar eclipse

An annular solar eclipse occurred at the Moon's descending node of orbit between Monday, January 3 and Tuesday, January 4, 1927, with a magnitude of 0.9995. 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 was near the average diameter because it occurred 8.6 days after apogee and 3.3 days before perigee.

<span class="mw-page-title-main">Solar eclipse of August 21, 1914</span> Total eclipse

A total solar eclipse occurred at the Moon's descending node of orbit on Friday, August 21, 1914, 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. Occurring about 2.7 days before perigee, the Moon's apparent diameter was larger.

References

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  2. "Chileans, Argentines see total solar eclipse". Albany Democrat-Herald. 2019-07-03. p. B7. Retrieved 2023-10-27 via Newspapers.com.
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Additional sources