Solar eclipse of August 3, 2054

Solar eclipse of August 3, 2054
Map
Type of eclipse
NaturePartial
Gamma−1.4941
Magnitude0.0655
Maximum eclipse
Coordinates69°48′S 121°18′W / 69.8°S 121.3°W / -69.8; -121.3
Times (UTC)
Greatest eclipse18:04:02
References
Saros117 (71 of 71)
Catalog # (SE5000)9629

A partial solar eclipse will occur at the Moon's ascending node of orbit on Monday, August 3, 2054,[1] with a magnitude of 0.0655. 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 partial solar eclipse occurs in the polar regions of the Earth when the center of the Moon's shadow misses the Earth.

The partial solar eclipse will be visible for a very small part of Antarctica. This event will be the 71st and final event in Solar Saros 117.

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.[2]

August 3, 2054 Solar Eclipse Times
Event Time (UTC)
First Penumbral External Contact 2054 August 03 at 17:30:57.7 UTC
Ecliptic Conjunction 2054 August 03 at 17:49:29.6 UTC
Greatest Eclipse 2054 August 03 at 18:04:02.1 UTC
Equatorial Conjunction 2054 August 03 at 18:32:59.0 UTC
Last Penumbral External Contact 2054 August 03 at 18:36:52.3 UTC
August 3, 2054 Solar Eclipse Parameters
Parameter Value
Eclipse Magnitude 0.06558
Eclipse Obscuration 0.02025
Gamma −1.49414
Sun Right Ascension 08h56m24.5s
Sun Declination +17°17'09.2"
Sun Semi-Diameter 15'45.7"
Sun Equatorial Horizontal Parallax 08.7"
Moon Right Ascension 08h55m14.2s
Moon Declination +15°47'22.5"
Moon Semi-Diameter 16'41.7"
Moon Equatorial Horizontal Parallax 1°01'16.5"
ΔT 86.9 s

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. The first and last eclipse in this sequence is separated by one synodic month.

Eclipse season of August–September 2054
August 3
Ascending node (new moon)
 August 18
Descending node (full moon)
 September 2
Ascending node (new moon)
Partial solar eclipse
Solar Saros 117		 Total lunar eclipse
Lunar Saros 129		 Partial solar eclipse
Solar Saros 155

Eclipses in 2054

Metonic

Tzolkinex

Tritos

Solar Saros 117

Inex

Triad

Solar eclipses of 2054–2058

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.[3]

The partial solar eclipses on March 9, 2054 and September 2, 2054 occur in the previous lunar year eclipse set, and the partial solar eclipses on May 22, 2058 and November 16, 2058 occur in the next lunar year eclipse set.

Solar eclipse series sets from 2054 to 2058
Ascending node   Descending node
Saros Map Gamma Saros Map Gamma
117 August 3, 2054

Partial 		−1.4941 122 January 27, 2055

Partial 		1.155
127 July 24, 2055

Total 		−0.8012 132 January 16, 2056

Annular 		0.4199
137 July 12, 2056

Annular 		−0.0426 142 January 5, 2057

Total 		−0.2837
147 July 1, 2057

Annular 		0.7455 152 December 26, 2057

Total 		−0.9405
157 June 21, 2058

Partial 		1.4869

Saros 117

This eclipse is a part of Saros series 117, repeating every 18 years, 11 days, and containing 71 events. The series started with a partial solar eclipse on June 24, 792 AD. It contains annular eclipses from September 18, 936 AD through May 14, 1333; hybrid eclipses from May 25, 1351 through July 8, 1423; and total eclipses from July 18, 1441 through May 19, 1928. The series ends at member 71 as a partial eclipse on August 3, 2054. 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 16 at 9 minutes, 26 seconds on December 3, 1062, and the longest duration of totality was produced by member 62 at 4 minutes, 19 seconds on April 26, 1892. All eclipses in this series occur at the Moon’s ascending node of orbit.[4]

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.

23 eclipse events between August 3, 2054 and October 16, 2145
August 3–4 May 22–24 March 10–11 December 27–29 October 14–16
117 119 121 123 125

August 3, 2054
May 22, 2058
March 11, 2062
December 27, 2065
October 15, 2069
127 129 131 133 135

August 3, 2073
May 22, 2077
March 10, 2081
December 27, 2084
October 14, 2088
137 139 141 143 145

August 3, 2092
May 22, 2096
March 10, 2100
December 29, 2103
October 16, 2107
147 149 151 153 155

August 4, 2111
May 24, 2115
March 11, 2119
December 28, 2122
October 16, 2126
157 159 161 163 165

August 4, 2130
May 23, 2134
October 16, 2145

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 2054 and 2200

August 3, 2054
(Saros 117)
July 3, 2065
(Saros 118)
June 1, 2076
(Saros 119)
May 2, 2087
(Saros 120)
April 1, 2098
(Saros 121)

March 1, 2109
(Saros 122)
January 30, 2120
(Saros 123)
December 30, 2130
(Saros 124)
November 28, 2141
(Saros 125)
October 28, 2152
(Saros 126)

September 28, 2163
(Saros 127)
August 27, 2174
(Saros 128)
July 26, 2185
(Saros 129)
June 26, 2196
(Saros 130)

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.

The partial solar eclipses on January 12, 1823 (part of Saros 109) and December 2, 1880 (part of Saros 111) are also a part of this series but are not included in the table below.

Series members between 2054 and 2200

August 3, 2054
(Saros 117)
July 15, 2083
(Saros 118)
June 24, 2112
(Saros 119)

June 4, 2141
(Saros 120)
May 16, 2170
(Saros 121)
April 25, 2199
(Saros 122)

References

  1. ^ "August 3, 2054 Partial Solar Eclipse". timeanddate. Retrieved 15 August 2024.
  2. ^ "Partial Solar Eclipse of 2054 Aug 03". EclipseWise.com. Retrieved 15 August 2024.
  3. ^ 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.
  4. ^ "NASA - Catalog of Solar Eclipses of Saros 117". eclipse.gsfc.nasa.gov.

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