Solar eclipse of July 3, 2084

Solar eclipse of July 3, 2084
Map
Type of eclipse
Nature	Annular
Gamma	0.8208
Magnitude	0.9421
Maximum eclipse
Duration	265 s (4 min 25 s)
Coordinates	75°N 169.1°W / 75; -169.1
Max. width of band	377 km (234 mi)
Times (UTC)
Greatest eclipse	1:50:26
References
Saros	128 (62 of 73)
Catalog # (SE5000)	9697

An annular solar eclipse will occur on Monday, July 3, 2084. 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 kilometers wide.

An annular eclipse will start in European Russia north-east of Moscow (passing through Yaroslavl, Vologda and Syktyvkar), will cross Arctic Ocean, Alaska, west part of Canada and will finish in the United States, crossing north-western states (Washington, Oregon, Wyoming, California, Nevada and Utah) respectively.

Related eclipses

Solar eclipses 2083–2087

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.

The partial solar eclipses on February 16, 2083 and August 13, 2083 occur in the previous lunar year eclipse set, and the partial solar eclipses on May 2, 2087 and October 26, 2087 occur in the next lunar year eclipse set.

Solar eclipse series sets from 2083 to 2087
Descending node				Ascending node
Saros	Map	Gamma		Saros	Map	Gamma
118	July 15, 2083 Partial	1.5465		123	January 7, 2084 Partial	−1.0715
128	July 3, 2084 Annular	0.8208		133	December 27, 2084 Total	−0.4094
138	June 22, 2085 Annular	0.0452		143	December 16, 2085 Annular	0.2786
148	June 11, 2086 Total	−0.7215		153	December 6, 2086 Partial	1.0194
158	June 1, 2087 Partial	−1.4186

Saros 128

This eclipse is a part of Saros series 128, repeating every 18 years, 11 days, and containing 73 events. The series started with a partial solar eclipse on August 29, 984 AD. It contains total eclipses from May 16, 1417 through June 18, 1471; hybrid eclipses from June 28, 1489 through July 31, 1543; and annular eclipses from August 11, 1561 through July 25, 2120. The series ends at member 73 as a partial eclipse on November 1, 2282. 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 27 at 1 minutes, 45 seconds on June 7, 1453, and the longest duration of annularity was produced by member 48 at 8 minutes, 35 seconds on February 1, 1832. All eclipses in this series occur at the Moon’s descending node of orbit.

Series members 47–68 occur between 1801 and 2200:
47	48	49
January 21, 1814	February 1, 1832	February 12, 1850
50	51	52
February 23, 1868	March 5, 1886	March 17, 1904
53	54	55
March 28, 1922	April 7, 1940	April 19, 1958
56	57	58
April 29, 1976	May 10, 1994	May 20, 2012
59	60	61
June 1, 2030	June 11, 2048	June 22, 2066
62	63	64
July 3, 2084	July 15, 2102	July 25, 2120
65	66	67
August 5, 2138	August 16, 2156	August 27, 2174
68
September 6, 2192

References

• Earth visibility chart and eclipse statistics Eclipse Predictions by Fred Espenak, NASA/GSFC
  • Google interactive map
  • Besselian elements