Solar eclipse of February 5, 2000

Summary

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.

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

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

  • http://eclipse.gsfc.nasa.gov/SEplot/SEplot1951/SE2000Feb05P.GIF