Solar eclipse of September 22, 2006

Last updated
Solar eclipse of September 22, 2006
Helder da Rocha - Partial solar eclipse (by-sa).jpg
Partial from São Paulo, Brazil
SE2006Sep22A.png
Map
Type of eclipse
NatureAnnular
Gamma −0.4062
Magnitude 0.9352
Maximum eclipse
Duration429 s (7 min 9 s)
Coordinates 20°36′S9°06′W / 20.6°S 9.1°W / -20.6; -9.1
Max. width of band261 km (162 mi)
Times (UTC)
Greatest eclipse11:41:16
References
Saros 144 (16 of 70)
Catalog # (SE5000) 9522

An annular solar eclipse occurred at the Moon's descending node of orbit on Friday, September 22, 2006, [1] [2] [3] with a magnitude of 0.9352. 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 only about 5 hours after apogee (on September 22, 2006, at 6:20 UTC), the Moon's apparent diameter was smaller. [4]

Contents

The path of annularity of this eclipse passed through Guyana, Suriname, French Guiana, the northern tip of Roraima and Amapá of Brazil, and the southern Atlantic. A partial eclipse was visible for parts of South America, West Africa, Southern Africa, the Antarctic Peninsula, and east Antarctica.

Images

SE2006Sep22A.gif
Animated path

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. [5]

September 22, 2006 Solar Eclipse Times
EventTime (UTC)
First Penumbral External Contact2006 September 22 at 08:41:01.9 UTC
First Umbral External Contact2006 September 22 at 09:49:37.0 UTC
First Central Line2006 September 22 at 09:52:37.2 UTC
First Umbral Internal Contact2006 September 22 at 09:55:38.2 UTC
First Penumbral Internal Contact2006 September 22 at 11:24:51.6 UTC
Greatest Duration2006 September 22 at 11:40:28.6 UTC
Greatest Eclipse2006 September 22 at 11:41:16.4 UTC
Ecliptic Conjunction2006 September 22 at 11:46:08.5 UTC
Last Penumbral Internal Contact2006 September 22 at 11:57:02.3 UTC
Equatorial Conjunction2006 September 22 at 12:08:15.8 UTC
Last Umbral Internal Contact2006 September 22 at 13:26:37.6 UTC
Last Central Line2006 September 22 at 13:29:39.0 UTC
Last Umbral External Contact2006 September 22 at 13:32:39.5 UTC
Last Penumbral External Contact2006 September 22 at 14:41:20.1 UTC
September 22, 2006 Solar Eclipse Parameters
ParameterValue
Eclipse Magnitude0.93517
Eclipse Obscuration0.87455
Gamma−0.40624
Sun Right Ascension11h57m32.9s
Sun Declination+00°15'56.9"
Sun Semi-Diameter15'56.1"
Sun Equatorial Horizontal Parallax08.8"
Moon Right Ascension11h56m50.2s
Moon Declination-00°03'07.8"
Moon Semi-Diameter14'41.9"
Moon Equatorial Horizontal Parallax0°53'56.7"
ΔT65.0 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 September 2006
September 7
Ascending node (full moon)
September 22
Descending node (new moon)
Lunar eclipse chart close-2006Sep07.png SE2006Sep22A.png
Partial lunar eclipse
Lunar Saros 118
Annular solar eclipse
Solar Saros 144

Eclipses in 2006

Metonic

Tzolkinex

Half-Saros

Tritos

Solar Saros 144

Inex

Triad

Solar eclipses of 2004–2007

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]

Solar eclipse series sets from 2004 to 2007
Ascending node Descending node
SarosMapGammaSarosMapGamma
119 April 19, 2004
SE2004Apr19P.png
Partial
−1.13345124 October 14, 2004
SE2004Oct14P.png
Partial
1.03481
129
Solar eclipse at sunset (2937676527) (cropped).jpg
Partial in Naiguatá, Venezuela
April 8, 2005
SE2005Apr08H.png
Hybrid
−0.34733134
Ecl-ann.jpg
Annularity in Madrid, Spain
October 3, 2005
SE2005Oct03A.png
Annular
0.33058
139
Diamondring-eclipse-March03-29-2006.jpg
Totality in Side, Turkey
March 29, 2006
SE2006Mar29T.png
Total
0.38433144
Helder da Rocha - Partial solar eclipse (by-sa).jpg
Partial in São Paulo, Brazil
September 22, 2006
SE2006Sep22A.png
Annular
−0.40624
149
Solar Eclipse (3445953058) (cropped).jpg
Partial in Jaipur, India
March 19, 2007
SE2007Mar19P.png
Partial
1.07277154
Eclipse solar 01 (1360685468) (cropped).jpg
Partial in Córdoba, Argentina
September 11, 2007
SE2007Sep11P.png
Partial
−1.12552

Saros 144

This eclipse is a part of Saros series 144, repeating every 18 years, 11 days, and containing 70 events. The series started with a partial solar eclipse on April 11, 1736. It contains annular eclipses from July 7, 1880 through August 27, 2565. There are no hybrid or total eclipses in this set. The series ends at member 70 as a partial eclipse on May 5, 2980. 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 51 at 9 minutes, 52 seconds on December 29, 2168. All eclipses in this series occur at the Moon’s descending node of orbit. [7]

Series members 5–26 occur between 1801 and 2200:
567
SE1808May25P.png
May 25, 1808
SE1826Jun05P.png
June 5, 1826
SE1844Jun16P.png
June 16, 1844
8910
SE1862Jun27P.png
June 27, 1862
SE1880Jul07A.png
July 7, 1880
SE1898Jul18A.png
July 18, 1898
111213
SE1916Jul30A.png
July 30, 1916
SE1934Aug10A.png
August 10, 1934
SE1952Aug20A.png
August 20, 1952
141516
SE1970Aug31A.png
August 31, 1970
SE1988Sep11A.png
September 11, 1988
SE2006Sep22A.png
September 22, 2006
171819
SE2024Oct02A.png
October 2, 2024
SE2042Oct14A.png
October 14, 2042
SE2060Oct24A.png
October 24, 2060
202122
SE2078Nov04A.png
November 4, 2078
SE2096Nov15A.png
November 15, 2096
SE2114Nov27A.png
November 27, 2114
232425
SE2132Dec07A.png
December 7, 2132
SE2150Dec19A.png
December 19, 2150
SE2168Dec29A.png
December 29, 2168
26
SE2187Jan09A.png
January 9, 2187

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 descending node.

21 eclipse events between July 11, 1953 and July 11, 2029
July 10–11April 29–30February 15–16December 4September 21–23
116118120122124
SE1953Jul11P.png
July 11, 1953
SE1957Apr30A.png
April 30, 1957
SE1961Feb15T.png
February 15, 1961
SE1964Dec04P.png
December 4, 1964
SE1968Sep22T.png
September 22, 1968
126128130132134
SE1972Jul10T.png
July 10, 1972
SE1976Apr29A.png
April 29, 1976
SE1980Feb16T.png
February 16, 1980
SE1983Dec04A.png
December 4, 1983
SE1987Sep23A.png
September 23, 1987
136138140142144
SE1991Jul11T.png
July 11, 1991
SE1995Apr29A.png
April 29, 1995
SE1999Feb16A.png
February 16, 1999
SE2002Dec04T.png
December 4, 2002
SE2006Sep22A.png
September 22, 2006
146148150152154
SE2010Jul11T.png
July 11, 2010
SE2014Apr29A.png
April 29, 2014
SE2018Feb15P.png
February 15, 2018
SE2021Dec04T.png
December 4, 2021
SE2025Sep21P.png
September 21, 2025
156
SE2029Jul11P.png
July 11, 2029

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.

Series members between 1801 and 2200
SE1810Apr04A.gif
April 4, 1810
(Saros 126)
SE1821Mar04T.gif
March 4, 1821
(Saros 127)
SE1832Feb01A.gif
February 1, 1832
(Saros 128)
SE1842Dec31A.gif
December 31, 1842
(Saros 129)
SE1853Nov30T.png
November 30, 1853
(Saros 130)
SE1864Oct30A.gif
October 30, 1864
(Saros 131)
SE1875Sep29A.gif
September 29, 1875
(Saros 132)
SE1886Aug29T.png
August 29, 1886
(Saros 133)
SE1897Jul29A.gif
July 29, 1897
(Saros 134)
SE1908Jun28A.png
June 28, 1908
(Saros 135)
SE1919May29T.png
May 29, 1919
(Saros 136)
SE1930Apr28H.png
April 28, 1930
(Saros 137)
SE1941Mar27A.png
March 27, 1941
(Saros 138)
SE1952Feb25T.png
February 25, 1952
(Saros 139)
SE1963Jan25A.png
January 25, 1963
(Saros 140)
SE1973Dec24A.png
December 24, 1973
(Saros 141)
SE1984Nov22T.png
November 22, 1984
(Saros 142)
SE1995Oct24T.png
October 24, 1995
(Saros 143)
SE2006Sep22A.png
September 22, 2006
(Saros 144)
SE2017Aug21T.png
August 21, 2017
(Saros 145)
SE2028Jul22T.png
July 22, 2028
(Saros 146)
SE2039Jun21A.png
June 21, 2039
(Saros 147)
SE2050May20H.png
May 20, 2050
(Saros 148)
SE2061Apr20T.png
April 20, 2061
(Saros 149)
SE2072Mar19P.png
March 19, 2072
(Saros 150)
SE2083Feb16P.png
February 16, 2083
(Saros 151)
SE2094Jan16T.png
January 16, 2094
(Saros 152)
Saros153 14van70 SE2104Dec17A.jpg
December 17, 2104
(Saros 153)
SE2115Nov16A.png
November 16, 2115
(Saros 154)
SE2126Oct16T.png
October 16, 2126
(Saros 155)
Saros156 08van69 SE2137Sep15P.jpg
September 15, 2137
(Saros 156)
Saros157 06van70 SE2148Aug14P.jpg
August 14, 2148
(Saros 157)
Saros158 06van70 SE2159Jul15P.jpg
July 15, 2159
(Saros 158)
Saros159 03van70 SE2170Jun14P.jpg
June 14, 2170
(Saros 159)
Saros160 01van71 SE2181May13P.jpg
May 13, 2181
(Saros 160)
Saros161 02van72 SE2192Apr12P.jpg
April 12, 2192
(Saros 161)

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
SE1804Feb11H.png
February 11, 1804
(Saros 137)
SE1833Jan20A.gif
January 20, 1833
(Saros 138)
SE1861Dec31T.gif
December 31, 1861
(Saros 139)
SE1890Dec12H.gif
December 12, 1890
(Saros 140)
SE1919Nov22A.png
November 22, 1919
(Saros 141)
SE1948Nov01T.png
November 1, 1948
(Saros 142)
SE1977Oct12T.png
October 12, 1977
(Saros 143)
SE2006Sep22A.png
September 22, 2006
(Saros 144)
SE2035Sep02T.png
September 2, 2035
(Saros 145)
SE2064Aug12T.png
August 12, 2064
(Saros 146)
SE2093Jul23A.png
July 23, 2093
(Saros 147)
Saros148 27van75 SE2122Jul04T.jpg
July 4, 2122
(Saros 148)
Saros149 28van71 SE2151Jun14T.jpg
June 14, 2151
(Saros 149)
Saros150 26van71 SE2180May24A.jpg
May 24, 2180
(Saros 150)

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References

  1. "September 22, 2006 Annular Solar Eclipse". timeanddate. Retrieved 11 August 2024.
  2. "An eclipse's effect". The Gazette. 2006-09-23. p. 11. Retrieved 2023-10-25 via Newspapers.com.
  3. "StarTales". Arizona Daily Sun. 2006-09-22. p. 8. Retrieved 2023-10-25 via Newspapers.com.
  4. "Moon Distances for London, United Kingdom, England". timeanddate. Retrieved 11 August 2024.
  5. "Annular Solar Eclipse of 2006 Sep 22". EclipseWise.com. Retrieved 11 August 2024.
  6. 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.
  7. "NASA - Catalog of Solar Eclipses of Saros 144". eclipse.gsfc.nasa.gov.

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