Solar eclipse of February 5, 2000

Last updated
Solar eclipse of February 5, 2000
SE2000Feb05P.png
Map
Type of eclipse
NaturePartial
Gamma -1.2233
Magnitude 0.5795
Maximum eclipse
Coordinates 70°12′S134°06′E / 70.2°S 134.1°E / -70.2; 134.1
Times (UTC)
Greatest eclipse12:50:27
References
Saros 150 (16 of 71)
Catalog # (SE5000) 9507

A partial solar eclipse occurred on Saturday, February 5, 2000. 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. It was only visible over Antarctica.

Contents

The exact time of the greatest eclipse took place on February 5, 2000, at 12:49:23.1 p.m. UTC, but occurring only 4.5 days after apogee (Apogee on Tuesday, February 1, 2000, at 01:19 a.m. UTC), the Moon's apparent diameter was 4.5% smaller than average, and the Moon's distance from the Earth was 397,705 km (247,122 mi).

Images

SE2000Feb05P.gif

Eclipses of 2000

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.

Saros 150

It is a part of Saros cycle 150, repeating every 18 years, 11 days, containing 71 events. The series started with partial solar eclipse on August 24, 1729. It contains annular eclipses from April 22, 2126 through June 22, 2829. There are no total eclipses in this series. The series ends at member 71 as a partial eclipse on September 29, 2991. The longest duration of annularity will be 9 minutes, 58 seconds on December 19, 2522.

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 descending node.

22 eclipse events between September 12, 1931 and July 1, 2011.
September 11-12June 30-July 1April 17-19February 4-5November 22-23
114116118120122
SE1931Sep12P.png
September 12, 1931
SE1935Jun30P.png
June 30, 1935
SE1939Apr19A.png
April 19, 1939
SE1943Feb04T.png
February 4, 1943
SE1946Nov23P.png
November 23, 1946
124126128130132
SE1950Sep12T.png
September 12, 1950
SE1954Jun30T.png
June 30, 1954
SE1958Apr19A.png
April 19, 1958
SE1962Feb05T.png
February 5, 1962
SE1965Nov23A.png
November 23, 1965
134136138140142
SE1969Sep11A.png
September 11, 1969
SE1973Jun30T.png
June 30, 1973
SE1977Apr18A.png
April 18, 1977
SE1981Feb04A.png
February 4, 1981
SE1984Nov22T.png
November 22, 1984
144146148150152
SE1988Sep11A.png
September 11, 1988
SE1992Jun30T.png
June 30, 1992
SE1996Apr17P.png
April 17, 1996
SE2000Feb05P.png
February 5, 2000
SE2003Nov23T.png
November 23, 2003
154156
SE2007Sep11P.png
September 11, 2007
SE2011Jul01P.png
July 1, 2011

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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.