Solar eclipse of February 16, 1999
Solar eclipse of February 16, 1999 | |
---|---|
Type of eclipse | |
Nature | Annular |
Gamma | −0.4726 |
Magnitude | 0.9928 |
Maximum eclipse | |
Duration | 40 s (0 min 40 s) |
Coordinates | 39°48′S 93°54′E / 39.8°S 93.9°E |
Max. width of band | 29 km (18 mi) |
Times (UTC) | |
Greatest eclipse | 6:34:38 |
References | |
Saros | 140 (28 of 71) |
Catalog # (SE5000) | 9505 |
An annular solar eclipse occurred at the Moon’s descending node of orbit on Tuesday, February 16, 1999, with a magnitude of 0.9928. 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 the southern Indian Ocean including the Prince Edward Islands, South Africa (the northern part of Marion Island and the whole Prince Edward Island), and Australia.
Images[edit]
Related eclipses[edit]
Eclipses in 1999[edit]
- A penumbral lunar eclipse on January 31, 1999.
- An annular solar eclipse on February 16, 1999.
- A partial lunar eclipse on July 28, 1999.
- A total solar eclipse on August 11, 1999.
Metonic[edit]
- Preceded by: Solar eclipse of April 29, 1995
- Followed by: Solar eclipse of December 4, 2002
Tzolkinex[edit]
- Preceded by: Solar eclipse of January 4, 1992
- Followed by: Solar eclipse of March 29, 2006
Half-Saros[edit]
- Preceded by: Lunar eclipse of February 9, 1990
- Followed by: Lunar eclipse of February 21, 2008
Tritos[edit]
- Preceded by: Solar eclipse of March 18, 1988
- Followed by: Solar eclipse of January 15, 2010
Solar Saros 140[edit]
- Preceded by: Solar eclipse of February 4, 1981
- Followed by: Solar eclipse of February 26, 2017
Inex[edit]
- Preceded by: Solar eclipse of March 7, 1970
- Followed by: Solar eclipse of January 26, 2028
Triad[edit]
- Preceded by: Solar eclipse of April 17, 1912
- Followed by: Solar eclipse of December 16, 2085
Solar eclipses of 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]
The partial solar eclipses on July 1, 2000 and December 25, 2000 occur in the next lunar year eclipse set.
Solar eclipse series sets from 1997 to 2000 | ||||||
---|---|---|---|---|---|---|
Descending node | Ascending node | |||||
Saros | Map | Gamma | Saros | Map | Gamma | |
120 Totality in Chita, Russia |
March 9, 1997 Total |
0.9183 | 125 | September 2, 1997 Partial |
−1.0352 | |
130 Totality near Guadeloupe |
February 26, 1998 Total |
0.2391 | 135 | August 22, 1998 Annular |
−0.2644 | |
140 | February 16, 1999 Annular |
−0.4726 | 145 Totality in France |
August 11, 1999 Total |
0.5062 | |
150 | February 5, 2000 Partial |
−1.2233 | 155 | July 31, 2000 Partial |
1.2166 |
Saros 140[edit]
This eclipse is a part of Saros series 140, repeating every 18 years, 11 days, and containing 71 events. The series started with a partial solar eclipse on April 16, 1512. It contains total eclipses from July 21, 1656 through November 9, 1836; hybrid eclipses from November 20, 1854 through December 23, 1908; and annular eclipses from January 3, 1927 through December 7, 2485. The series ends at member 71 as a partial eclipse on June 1, 2774. Its eclipses are tabulated in three columns; every third eclipse in the same column is one exeligmos apart, so they all cast shadows over approximately the same parts of the Earth.
The longest duration of totality was produced by member 11 at 4 minutes, 10 seconds on August 12, 1692, and the longest duration of annularity will be produced by member 53 at 7 minutes, 35 seconds on November 15, 2449. All eclipses in this series occur at the Moon’s descending node of orbit.[2]
Series members 18–39 occur between 1801 and 2200: | ||
---|---|---|
18 | 19 | 20 |
October 29, 1818 |
November 9, 1836 |
November 20, 1854 |
21 | 22 | 23 |
November 30, 1872 |
December 12, 1890 |
December 23, 1908 |
24 | 25 | 26 |
January 3, 1927 |
January 14, 1945 |
January 25, 1963 |
27 | 28 | 29 |
February 4, 1981 |
February 16, 1999 |
February 26, 2017 |
30 | 31 | 32 |
March 9, 2035 |
March 20, 2053 |
March 31, 2071 |
33 | 34 | 35 |
April 10, 2089 |
April 23, 2107 |
May 3, 2125 |
36 | 37 | 38 |
May 14, 2143 |
May 25, 2161 |
June 5, 2179 |
39 | ||
June 15, 2197 |
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.
21 eclipse events, progressing from north to south between July 11, 1953 and July 11, 2029 | ||||
---|---|---|---|---|
July 10–12 | April 29–30 | February 15–16 | December 4–5 | September 21–23 |
116 | 118 | 120 | 122 | 124 |
July 11, 1953 |
April 30, 1957 |
February 15, 1961 |
December 4, 1964 |
September 22, 1968 |
126 | 128 | 130 | 132 | 134 |
July 10, 1972 |
April 29, 1976 |
February 16, 1980 |
December 4, 1983 |
September 23, 1987 |
136 | 138 | 140 | 142 | 144 |
July 11, 1991 |
April 29, 1995 |
February 16, 1999 |
December 4, 2002 |
September 22, 2006 |
146 | 148 | 150 | 152 | 154 |
July 11, 2010 |
April 29, 2014 |
February 15, 2018 |
December 4, 2021 |
September 21, 2025 |
156 | 158 | 160 | 162 | 164 |
July 11, 2029 |
Notes[edit]
- ^ 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.
- ^ "NASA - Catalog of Solar Eclipses of Saros 140". eclipse.gsfc.nasa.gov.
References[edit]
- Earth visibility chart and eclipse statistics Eclipse Predictions by Fred Espenak, NASA/GSFC