Summary
An annular solar eclipse occurred at the Moon's ascending node of the orbit on Saturday, May 31, 2003. 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 across central Greenland, the Faroe Islands, Iceland, Jan Mayen and northern Scotland. Partiality was visible throughout Europe, Asia, and far northwestern Canada.
| Solar eclipse of May 31, 2003 | |
|---|---|
 Annular from Culloden, Scotland | |
 Map | |
| Type of eclipse | |
| Nature | Annular |
| Gamma | 0.996 |
| Magnitude | 0.9384 |
| Maximum eclipse | |
| Duration | 217 s (3 min 37 s) |
| Coordinates | 66°36′N 24°30′W / 66.6°N 24.5°W |
| Max. width of band | - km |
| Times (UTC) | |
| Greatest eclipse | 4:09:22 |
| References | |
| Saros | 147 (22 of 80) |
| Catalog # (SE5000) | 9515 |
People from around the world traveled to see the eclipse from the small portion of Britain from which it could be seen, with the Independent saying: "A timely gap in the clouds was all it took to make the arduous journey to the northernmost reaches of Scotland worthwhile". In the village of Durness, the eclipse was observed by Patrick Moore and Brian May.[1] [2] However, viewing parties in Orkney saw "just another grey morning in the far north of Scotland".[3][4] In India, hundreds of thousands of Hindus carried out a tradition of bathing in sacred rivers during the eclipse, with queues as long as 3 mi (4.8 km).[4] A partial eclipse was observed in large parts of Asia, the middle East, and Europe, including Greece.[5]
Images edit
-
Chassepierre, Belgium -
From Belfort, France -
Wonneberg, Germany -
From Oria, Italy -
From Venice, Italy -
Willeskop, Netherlands -
From Oslo, Norway -
From Ringerike, Norway -
Grantown-on-Spey, Scotland
Related eclipses edit
Eclipses of 2003 edit
- A total lunar eclipse on May 16.
- An annular solar eclipse (one limit) on May 31.
- A total lunar eclipse on November 9.
- A total solar eclipse on November 23.
Solar eclipses 2000–2003 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.[6]
Partial solar eclipses on February 5, 2000 and July 31, 2000 occur in the previous lunar year set.
| Ascending node | Descending node | |||||
|---|---|---|---|---|---|---|
| Saros | Map | Gamma | Saros | Map | Gamma | |
| 117 | 2000 July 01 Partial (south) |
−1.28214 | 122 | 2000 December 25 Partial (north) |
1.13669 | |
127 Totality from Lusaka, Zambia |
2001 June 21 Total |
−0.57013 | 132 Partial from Minneapolis, MN |
2001 December 14 Annular |
0.40885 | |
137 Partial from Los Angeles, CA |
2002 June 10 Annular |
0.19933 | 142 Totality from Woomera |
2002 December 04 Total |
−0.30204 | |
147 Culloden, Scotland |
2003 May 31 Annular |
0.99598 | 152 | 2003 November 23 Total |
−0.96381 | |
Saros 147 edit
Solar saros 147, repeating every about 18 years and 11 days, contains 80 events. The series started with a partial solar eclipse on October 12, 1624. It has annular eclipses from May 31, 2003, to July 31, 2706. There are no total eclipses in this series. The series ends at member 80 as a partial eclipse on February 24, 3049. The longest annular eclipse will be on November 21, 2291, at 9 minutes and 41 seconds.[7]
| Series members 17–27 occur between 1901 and 2100: | ||||
|---|---|---|---|---|
| 17 | 18 | 19 | ||
 April 6, 1913 |
 April 18, 1931 |
 April 28, 1949 | ||
| 20 | 21 | 22 | ||
 May 9, 1967 |
 May 19, 1985 |
May 31, 2003 23 24 25  June 10, 2021 |
 June 21, 2039 |
 July 1, 2057 |
| 26 | 27 | |||
 July 13, 2075 |
 July 23, 2093 | |||
Tritos series edit
This eclipse is a part of a tritos cycle, repeating at alternating nodes every 135 synodic months (≈ 3986.63 days, or 11 years minus 1 month). Their appearance and longitude are irregular due to a lack of synchronization with the anomalistic month (period of perigee), but groupings of 3 tritos cycles (≈ 33 years minus 3 months) come close (≈ 434.044 anomalistic months), so eclipses are similar in these groupings.
| Series members between 1901 and 2100 | |||
|---|---|---|---|
 March 6, 1905 (Saros 138) |
 February 3, 1916 (Saros 139) |
 January 3, 1927 (Saros 140) | |
 December 2, 1937 (Saros 141) |
 November 1, 1948 (Saros 142) |
 October 2, 1959 (Saros 143) | |
 August 31, 1970 (Saros 144) |
 July 31, 1981 (Saros 145) |
 June 30, 1992 (Saros 146) | |
| May 31, 2003 (Saros 147) |
 April 29, 2014 (Saros 148) |
 March 29, 2025 (Saros 149) | |
 February 27, 2036 (Saros 150) |
 January 26, 2047 (Saros 151) |
 December 26, 2057 (Saros 152) | |
 November 24, 2068 (Saros 153) |
 October 24, 2079 (Saros 154) |
 September 23, 2090 (Saros 155) |
|
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 ascending node.
| 22 eclipse events between January 5, 1935 and August 11, 2018 | ||||
|---|---|---|---|---|
| January 4-5 | October 23-24 | August 10-12 | May 30-31 | March 18-19 |
| 111 | 113 | 115 | 117 | 119 |
 January 5, 1935 |
 August 12, 1942 |
 May 30, 1946 |
 March 18, 1950 | |
| 121 | 123 | 125 | 127 | 129 |
 January 5, 1954 |
 October 23, 1957 |
 August 11, 1961 |
 May 30, 1965 |
 March 18, 1969 |
| 131 | 133 | 135 | 137 | 139 |
 January 4, 1973 |
 October 23, 1976 |
 August 10, 1980 |
 May 30, 1984 |
 March 18, 1988 |
| 141 | 143 | 145 | 147 | 149 |
 January 4, 1992 |
 October 24, 1995 |
 August 11, 1999 |
May 31, 2003  March 19, 2007 | |
| 151 | 153 | 155 | ||
 January 4, 2011 |
 October 23, 2014 |
 August 11, 2018 |
||
See also edit
Notes edit
- ^ "Circle of light that set the cash tills ringing". The Independent. London, Greater London, England. 2003-06-01. p. 17. Retrieved 2023-10-15 – via Newspapers.com.
- ^ "Moon is a star for one day". The Observer. London, Greater London, England. 2003-06-01. p. 1. Retrieved 2023-10-15 – via Newspapers.com.
- ^ "Great party, shame about the eclipse". The Observer. London, Greater London, England. 2003-06-01. p. 7. Retrieved 2023-10-15 – via Newspapers.com.
- ^ a b "Eclipse draws watchers in north nations". Florida Today. 2003-06-01. p. 49. Retrieved 2023-10-25 – via Newspapers.com.
- ^ "Eclipse is partly sunny". Omaha World-Herald. 2003-06-01. p. 13. Retrieved 2023-10-25 – via Newspapers.com.
- ^ 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.
- ^ Saros Series Catalog of Solar Eclipses NASA Eclipse Web Site.
References edit
- Earth visibility chart and eclipse statistics Eclipse Predictions by Fred Espenak, NASA/GSFC
- Google interactive map
- Besselian elements
Photos:
- Spaceweather.com solar eclipse gallery
- Czech Republic. Prof. Druckmüller's eclipse photography site
- Eclipse in the Mist, APOD 6/4/2003, Dawn partial from Charneux, Belgium
- Ring of Fire from Cape Wrath, APOD 6/5/2003, Annular eclipse from Cape Wrath, northwestern coast of Scotland
- Sun, Moon, Hot Air Balloon, APOD 6/6/2003, partial eclipse from Bonn, Germany
- Clouds and the Moon Move to Block the Sun, APOD 6/18/2003, partial eclipse from Vienna, Austria
- Photos of solar eclipse around the world