Solar eclipse of February 5, 2000

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Solar eclipse of February 5, 2000
Map
Type of eclipse
NaturePartial
Gamma−1.2233
Magnitude0.5795
Maximum eclipse
Coordinates70°12′S 134°06′E / 70.2°S 134.1°E / -70.2; 134.1
Times (UTC)
Greatest eclipse12:50:27
References
Saros150 (16 of 71)
Catalog # (SE5000)9507

A partial solar eclipse occurred on 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.

Images[edit]

Related eclipses[edit]

Eclipses of 2000[edit]

Solar eclipses 1997–2000[edit]

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 to 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 150[edit]

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[edit]

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 11-12 June 30-July 1 April 17-19 February 4-5 November 22-23
114 116 118 120 122

September 12, 1931

June 30, 1935

April 19, 1939

February 4, 1943

November 23, 1946
124 126 128 130 132

September 12, 1950

June 30, 1954

April 19, 1958

February 5, 1962

November 23, 1965
134 136 138 140 142

September 11, 1969

June 30, 1973

April 18, 1977

February 4, 1981

November 22, 1984
144 146 148 150 152

September 11, 1988

June 30, 1992

April 17, 1996

February 5, 2000

November 23, 2003
154 156

September 11, 2007

July 1, 2011

References[edit]

  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.

External links[edit]