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Solar eclipse of August 22, 1998

From Wikipedia, the free encyclopedia

Solar eclipse of August 22, 1998
Map
Type of eclipse
NatureAnnular
Gamma−0.2644
Magnitude0.9734
Maximum eclipse
Duration194 sec (3 m 14 s)
Coordinates3°00′S 145°24′E / 3°S 145.4°E / -3; 145.4
Max. width of band99 km (62 mi)
Times (UTC)
Greatest eclipse2:07:11
References
Saros135 (38 of 71)
Catalog # (SE5000)9504

An annular solar eclipse occurred at the Moon’s ascending node of the orbit on August 22, 1998. 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. Annularity was visible in Indonesia, Malaysia, Papua New Guinea, Solomon Islands (Bellona Island and Rennell Island) and Vanuatu. Occurring only 5.2 days before apogee (Apogee on August 27, 1998), the Moon’s apparent diameter was 3.6% smaller than average.[1] [2] [3]

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Transcription

Images

Related eclipses

Eclipses of 1998

Solar eclipses 1997–2000

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.[4]

Solar eclipse series sets from 1997–2000
Descending node   Ascending node
Saros Map Gamma Saros Map Gamma
120

Chita, Russia
1997 March 09

Total
0.91830 125 1997 September 02

Partial (south)
−1.03521
130

Total eclipse near Guadeloupe
1998 February 26

Total
0.23909 135 1998 August 22

Annular
−0.26441
140 1999 February 16

Annular
−0.47260 145

Totality from France
1999 August 11

Total
0.50623
150 2000 February 05

Partial (south)
−1.22325 155 2000 July 31

Partial (north)
1.21664

Partial solar eclipses on July 1, 2000 and December 25, 2000 occur in the next lunar year eclipse set.

Saros 135

It is a part of Saros cycle 135, repeating every 18 years, 11 days, containing 71 events. The series started with partial solar eclipse on July 5, 1331. It contains annular eclipses from October 21, 1511, through February 24, 2305, hybrid eclipses on March 8, 2323, and March 18, 2341, and total eclipses from March 29, 2359, through May 22, 2449. The series ends at member 71 as a partial eclipse on August 17, 2593. The longest duration of totality will be 2 minutes, 27 seconds on May 12, 2431.

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, progressing from south to north between June 10, 1964, and August 21, 2036
June 10–11 March 27–29 January 15–16 November 3 August 21–22
117 119 121 123 125

June 10, 1964

March 28, 1968

January 16, 1972

November 3, 1975

August 22, 1979
127 129 131 133 135

June 11, 1983

March 29, 1987

January 15, 1991

November 3, 1994

August 22, 1998
137 139 141 143 145

June 10, 2002

March 29, 2006

January 15, 2010

November 3, 2013

August 21, 2017
147 149 151 153 155

June 10, 2021

March 29, 2025

January 14, 2029

November 3, 2032

August 21, 2036

Notes

  1. ^ "Clouds may put eclipse in shade". The Sydney Morning Herald. Sydney, New South Wales, New South Wales, Australia. 1998-08-22. p. 5. Retrieved 2023-10-21 – via Newspapers.com.
  2. ^ "Saturday". Newsday (Suffolk Edition). 1998-08-19. p. 114. Retrieved 2023-10-21 – via Newspapers.com.
  3. ^ "Eclipse Aug. 23". Mitchell Tribune. 1998-08-05. p. 12. Retrieved 2023-10-21 – via Newspapers.com.
  4. ^ 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.

References

Photos:

This page was last edited on 21 October 2023, at 02:03
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