Solar eclipse of September 2, 1997

Last updated
Solar eclipse of September 2, 1997
SE1997Sep02P.png
Map
Type of eclipse
NaturePartial
Gamma -1.0352
Magnitude 0.8988
Maximum eclipse
Coordinates 71°48′S114°18′E / 71.8°S 114.3°E / -71.8; 114.3
Times (UTC)
Greatest eclipse0:04:48
References
Saros 125 (53 of 73)
Catalog # (SE5000) 9502

A partial solar eclipse occurred on Tuesday, September 2, 1997. 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.

Contents

The exact time of the greatest eclipse took place on Tuesday, September 2, 1997, at 12:03:45.6 a.m. UTC, but occurring only 0.9 days before apogee (Apogee on Tuesday, September 2, 1997, at 09:16 p.m. UTC), the Moon's apparent diameter was 6.5% smaller than average, and the Moon's distance from the Earth was 406,216 km (252,411 mi).

Images

SE1997Sep02P.gif

Eclipses of 1997

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. [1]

Solar eclipse series sets from 1997–2000
Ascending node Descending node
SarosMapGammaSarosMapGamma
120
Total solar eclipse of March 9 1997.jpg
Chita, Russia
1997 March 09
SE1997Mar09T.png
Total
0.91830125 1997 September 02
SE1997Sep02P.png
Partial (south)
-1.03521
130
Ecl002-2 (4321047401).jpg
Total eclipse near Guadeloupe
1998 February 26
SE1998Feb26T.png
Total
0.23909135 1998 August 22
SE1998Aug22A.png
Annular
-0.26441
140 1999 February 16
SE1999Feb16A.png
Annular
-0.47260145
Solar eclipse 1999 4.jpg
Totality from France
1999 August 11
SE1999Aug11T.png
Total
0.50623
150 2000 February 05
SE2000Feb05P.png
Partial (south)
-1.22325155 2000 July 31
SE2000Jul31P.png
Partial (north)
1.21664

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

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 June 21, 1982, and June 21, 2058
June 21April 8–9January 26November 13–14September 1–2
107109111113115
June 21, 1963April 9, 1967January 26, 1971November 14, 1974September 2, 1978
117119121123125
SE1982Jun21P.png
June 21, 1982
SE1986Apr09P.png
April 9, 1986
SE1990Jan26A.png
January 26, 1990
SE1993Nov13P.png
November 13, 1993
SE1997Sep02P.png
September 2, 1997
127129131133135
SE2001Jun21T.png
June 21, 2001
SE2005Apr08H.png
April 8, 2005
SE2009Jan26A.png
January 26, 2009
SE2012Nov13T.png
November 13, 2012
SE2016Sep01A.png
September 1, 2016
137139141143145
SE2020Jun21A.png
June 21, 2020
SE2024Apr08T.png
April 8, 2024
SE2028Jan26A.png
January 26, 2028
SE2031Nov14H.png
November 14, 2031
SE2035Sep02T.png
September 2, 2035
147149151153155
SE2039Jun21A.png
June 21, 2039
SE2043Apr09T.png
April 9, 2043
SE2047Jan26P.png
January 26, 2047
SE2050Nov14P.png
November 14, 2050
SE2054Sep02P.png
September 2, 2054
157
SE2058Jun21P.png
June 21, 2058

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References

  1. 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.

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