An annular solar eclipse occurred at the Moon's ascending node of orbit on Saturday, May 31, 2003, with a magnitude of 0.9384. 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. Occurring about 2.6 days after apogee (on May 28, 2003, at 14:00 UTC), the Moon's apparent diameter was smaller.

Annularity was visible across central Greenland, the Faroe Islands, Iceland, Jan Mayen and northern Scotland. A partial eclipse was visible for parts of Eastern Europe, North Asia, West Asia, Middle East, Alaska, Greenland, and northwestern Canada.

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. However, viewing parties in Orkney saw "just another grey morning in the far north of Scotland". 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). A partial eclipse was observed in large parts of Asia, the Middle East, and Europe, including Greece.

Images

Animated path

Eclipse timing

Places experiencing annular eclipse

Solar Eclipse of May 31, 2003(Local Times)
Country or territoryCity or placeStart of partial eclipseStart of annular eclipseMaximum eclipseEnd of annular eclipseEnd of partial eclipseDuration of annularity (min:s)Duration of eclipse (hr:min)Maximum coverage
United KingdomFort William04:38:23 (sunrise)04:44:4904:45:1704:45:4305:42:150:541:0488.04%
United KingdomInverness04:29:58 (sunrise)04:44:5904:45:3204:46:0605:42:501:071:1388.08%
United KingdomPortree04:38:20 (sunrise)04:45:4404:46:4204:47:4005:43:421:561:0588.05%
United KingdomKirkwall04:12:41 (sunrise)04:45:5404:46:4304:47:3105:44:381:371:3288.16%
United KingdomLerwick03:54:39 (sunrise)04:46:3704:47:1604:47:5605:45:481:191:5188.23%
United KingdomStornoway04:32:53 (sunrise)04:46:3804:47:4904:48:5905:45:002:211:1288.08%
Faroe IslandsTórshavn03:56:52 (sunrise)04:51:1804:52:5204:54:2605:51:063:081:5488.22%
Faroe IslandsKlaksvík03:56:4204:51:2904:53:0304:54:3605:51:223:071:5888.23%
IcelandHöfn03:04:1303:58:3804:00:2604:02:1304:58:143:351:5488.20%
IcelandEgilsstaðir03:04:3303:59:2304:01:1004:02:5704:59:243:341:5588.25%
IcelandKirkjubæjarklaustur03:17:13 (sunrise)03:59:4604:01:3404:03:2204:58:553:361:4288.15%
IcelandVestmannaeyjar03:31:27 (sunrise)04:00:4504:02:3204:04:2004:59:323:351:2888.11%
IcelandHúsavík03:07:0404:01:5504:03:4304:05:3005:01:513:351:5588.25%
IcelandAkureyri03:07:1504:01:5504:03:4304:05:3105:01:403:361:5488.23%
IcelandReykjavík03:26:44 (sunrise)04:02:3004:04:1804:06:0605:01:213:361:3588.12%
IcelandKeflavík03:31:38 (sunrise)04:02:4404:04:3104:06:1905:01:283:351:3088.11%
IcelandBorgarnes03:19:07 (sunrise)04:02:5504:04:4204:06:3005:31:533:351:4388.14%
Svalbard and Jan MayenJan Mayen05:06:3606:04:3806:05:4106:06:4507:06:242:072:0088.54%
IcelandHólmavík03:09:3304:03:5904:05:4704:07:3505:03:213:361:5488.19%
IcelandÍsafjörður03:10:4404:05:1204:07:0004:08:4805:04:333:361:5488.19%
GreenlandIttoqqortoormiit03:13:1304:09:2504:11:0804:12:5005:10:163:251:5788.39%
GreenlandDaneborg01:15:2102:14:1202:14:4802:15:2403:15:231:122:0088.56%
GreenlandTasiilaq01:59:07 (sunrise)02:13:4302:15:3102:17:1803:11:433:351:1388.06%
GreenlandSummit Camp01:23:0902:19:4102:21:0702:22:3403:19:482:531:5788.37%
GreenlandKangerlussuaq02:00:21 (sunrise)02:23:1402:25:3902:26:2203:20:463:081:2088.06%
GreenlandIlulissat01:29:3802:24:3502:26:0102:27:2803:22:482:531:5388.16%
GreenlandAasiaat01:30:4202:25:3002:26:5302:28:1503:23:232:451:5388.13%
GreenlandUummannaq01:30:1802:26:0302:27:1502:28:2603:24:312:231:5488.22%
GreenlandQeqertarsuaq01:31:0602:26:1302:27:2902:28:4603:24:112:331:5388.15%
References:

Places experiencing partial eclipse

Solar Eclipse of May 31, 2003(Local Times)
Country or territoryCity or placeStart of partial eclipseMaximum eclipseEnd of partial eclipseDuration of eclipse (hr:min)Maximum coverage
BulgariaSofia05:52:12 (sunrise)06:08:2607:06:051:1466.28%
RomaniaBucharest05:35:09 (sunrise)06:09:2807:08:181:3366.76%
SerbiaBelgrade04:56:20 (sunrise)05:13:0806:11:021:1570.47%
Bosnia and HerzegovinaSarajevo05:08:01 (sunrise)05:16:5406:10:121:0269.08%
UkraineKyiv05:19:2706:17:1207:19:012:0070.28%
CroatiaZagreb05:10:35 (sunrise)05:17:1406:14:381:0473.87%
HungaryBudapest04:51:42 (sunrise)05:17:4906:16:211:2574.13%
SloveniaLjubljana05:15:34 (sunrise)05:19:1006:15:421:0074.76%
SlovakiaBratislava04:56:45 (sunrise)05:19:5306:18:151:2275.76%
AustriaVienna04:59:28 (sunrise)05:20:2306:18:381:1976.17%
PolandWarsaw04:27:1105:24:0406:24:281:5777.38%
BelarusMinsk05:25:4806:24:1207:26:262:0175.00%
Czech RepublicPrague04:58:58 (sunrise)05:24:1306:22:401:2478.78%
RussiaMoscow06:24:2307:24:5608:29:492:0569.86%
LithuaniaVilnius05:28:0406:26:2107:28:192:0076.85%
GermanyBerlin04:51:04 (sunrise)05:28:2106:27:181:3681.15%
LatviaRiga05:31:5506:30:4107:33:012:0178.89%
NetherlandsAmsterdam05:25:44 (sunrise)05:33:0906:30:301:0584.09%
DenmarkCopenhagen04:36:4905:33:3106:33:121:5883.46%
EstoniaTallinn05:35:1706:34:5307:37:572:0379.80%
FinlandHelsinki05:36:1806:36:0807:39:252:0380.01%
SwedenStockholm04:38:2405:36:5806:38:402:0082.90%
LuxembourgLuxembourg05:34:18 (sunrise)05:38:3706:25:290:5169.58%
BelgiumBrussels05:35:37 (sunrise)05:39:4606:28:190:5373.33%
NorwayOslo04:43:1605:40:5706:41:251:5885.86%
United KingdomEdinburgh04:36:46 (sunrise)04:42:5705:39:591:0387.74%
United KingdomLondon04:50:16 (sunrise)04:57:2605:31:370:4146.99%
GreenlandDanmarkshavn03:16:5004:17:1805:18:502:0287.68%
GreenlandPituffik00:37:1701:36:3902:35:541:5985.09%
CanadaPond Inlet23:43:3400:41:3301:39:081:5684.31%
References:

Gallery

Eclipse details

Shown below are two tables displaying details about this particular solar eclipse. The first table outlines times at which the Moon's penumbra or umbra attains the specific parameter, and the second table describes various other parameters pertaining to this eclipse.

May 31, 2003 Solar Eclipse Times
EventTime (UTC)
First Penumbral External Contact2003 May 31 at 01:47:21.0 UTC
First Umbral External Contact2003 May 31 at 03:45:50.6 UTC
First Central Line2003 May 31 at 04:03:10.1 UTC
Greatest Duration2003 May 31 at 04:08:58.5 UTC
Greatest Eclipse2003 May 31 at 04:09:22.5 UTC
Last Central Line2003 May 31 at 04:15:15.4 UTC
Ecliptic Conjunction2003 May 31 at 04:20:57.2 UTC
Last Umbral External Contact2003 May 31 at 04:32:33.6 UTC
Equatorial Conjunction2003 May 31 at 04:39:20.5 UTC
Last Penumbral External Contact2003 May 31 at 06:31:08.5 UTC
May 31, 2003 Solar Eclipse Parameters
ParameterValue
Eclipse Magnitude0.93842
Eclipse Obscuration0.88064
Gamma0.99597
Sun Right Ascension04h30m33.5s
Sun Declination+21°50'57.1"
Sun Semi-Diameter15'46.5"
Sun Equatorial Horizontal Parallax08.7"
Moon Right Ascension04h29m35.5s
Moon Declination+22°43'13.1"
Moon Semi-Diameter14'48.1"
Moon Equatorial Horizontal Parallax0°54'19.3"
ΔT64.5 s

Eclipse season

This eclipse is part of an eclipse season, a period, roughly every six months, when eclipses occur. Only two (or occasionally three) eclipse seasons occur each year, and each season lasts about 35 days and repeats just short of six months (173 days) later; thus two full eclipse seasons always occur each year. Either two or three eclipses happen each eclipse season. In the sequence below, each eclipse is separated by a fortnight.

Eclipse season of May 2003
May 16 Descending node (full moon)May 31 Ascending node (new moon)
Total lunar eclipse Lunar Saros 121Annular solar eclipse Solar Saros 147

Related eclipses

Eclipses in 2003

Metonic

Tzolkinex

Half-Saros

Tritos

Solar Saros 147

Inex

Triad

Solar eclipses of 2000–2003

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.

The partial solar eclipses on February 5, 2000 and July 31, 2000 occur in the previous lunar year eclipse set.

Solar eclipse series sets from 2000 to 2003
Ascending nodeDescending node
SarosMapGammaSarosMapGamma
117July 1, 2000 Partial−1.28214122 Partial projection in Minneapolis, MN, USADecember 25, 2000 Partial1.13669
127 Totality in Lusaka, ZambiaJune 21, 2001 Total−0.57013132 Partial in Minneapolis, MN, USADecember 14, 2001 Annular0.40885
137 Partial in Los Angeles, CA, USAJune 10, 2002 Annular0.19933142 Totality in Woomera, South AustraliaDecember 4, 2002 Total−0.30204
147 Annularity in Culloden, ScotlandMay 31, 2003 Annular0.99598152November 23, 2003 Total−0.96381

Saros 147

This eclipse is a part of Saros series 147, repeating every 18 years, 11 days, and containing 80 events. The series started with a partial solar eclipse on October 12, 1624. It contains annular eclipses from May 31, 2003 through July 31, 2706. There are no hybrid or total eclipses in this set. The series ends at member 80 as a partial eclipse on February 24, 3049. 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 annularity will be produced by member 38 at 9 minutes, 41 seconds on November 21, 2291. All eclipses in this series occur at the Moon’s ascending node of orbit.

Series members 11–32 occur between 1801 and 2200:
111213
January 30, 1805February 11, 1823February 21, 1841
141516
March 4, 1859March 15, 1877March 26, 1895
171819
April 6, 1913April 18, 1931April 28, 1949
202122
May 9, 1967May 19, 1985May 31, 2003
232425
June 10, 2021June 21, 2039July 1, 2057
262728
July 13, 2075July 23, 2093August 4, 2111
293031
August 15, 2129August 26, 2147September 5, 2165
32
September 16, 2183

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 ascending node.

22 eclipse events between January 5, 1935 and August 11, 2018
January 4–5October 23–24August 10–12May 30–31March 18–19
111113115117119
January 5, 1935August 12, 1942May 30, 1946March 18, 1950
121123125127129
January 5, 1954October 23, 1957August 11, 1961May 30, 1965March 18, 1969
131133135137139
January 4, 1973October 23, 1976August 10, 1980May 30, 1984March 18, 1988
141143145147149
January 4, 1992October 24, 1995August 11, 1999May 31, 2003March 19, 2007
151153155
January 4, 2011October 23, 2014August 11, 2018

Tritos series

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.

The partial solar eclipses on December 18, 2188 (part of Saros 164) and November 18, 2199 (part of Saros 165) are also a part of this series but are not included in the table below.

Series members between 1801 and 2134
December 10, 1806 (Saros 129)November 9, 1817 (Saros 130)October 9, 1828 (Saros 131)September 7, 1839 (Saros 132)August 7, 1850 (Saros 133)
July 8, 1861 (Saros 134)June 6, 1872 (Saros 135)May 6, 1883 (Saros 136)April 6, 1894 (Saros 137)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)August 24, 2101 (Saros 156)July 23, 2112 (Saros 157)June 23, 2123 (Saros 158)
May 23, 2134 (Saros 159)

Inex series

This eclipse is a part of the long period inex cycle, repeating at alternating nodes, every 358 synodic months (≈ 10,571.95 days, or 29 years minus 20 days). Their appearance and longitude are irregular due to a lack of synchronization with the anomalistic month (period of perigee). However, groupings of 3 inex cycles (≈ 87 years minus 2 months) comes close (≈ 1,151.02 anomalistic months), so eclipses are similar in these groupings.

Series members between 1801 and 2200
September 28, 1829 (Saros 141)September 7, 1858 (Saros 142)August 19, 1887 (Saros 143)
July 30, 1916 (Saros 144)July 9, 1945 (Saros 145)June 20, 1974 (Saros 146)
May 31, 2003 (Saros 147)May 9, 2032 (Saros 148)April 20, 2061 (Saros 149)
March 31, 2090 (Saros 150)March 11, 2119 (Saros 151)February 19, 2148 (Saros 152)
January 29, 2177 (Saros 153)

See also

Notes

External links

Photos: