A partial solar eclipse occurred at the Moon's descending node of orbit between Wednesday, October 13 and Thursday, October 14, 2004,[1][2][3] with a magnitude of 0.9282. 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.
| Solar eclipse of October 14, 2004 | |
|---|---|
 Map | |
| Type of eclipse | |
| Nature | Partial |
| Gamma | 1.0348 |
| Magnitude | 0.9282 |
| Maximum eclipse | |
| Coordinates | 61°12′N 153°42′W / 61.2°N 153.7°W |
| Times (UTC) | |
| Greatest eclipse | 3:00:23 |
| References | |
| Saros | 124 (54 of 73) |
| Catalog # (SE5000) | 9518 |
A partial eclipse was visible for parts of eastern Russia, Mongolia, northeastern China, Korea, Japan, Hawaii, and western Alaska.
Images
edit
Animated path
Eclipse details
editShown 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.[4]
| Event | Time (UTC) |
|---|---|
| First Penumbral External Contact | 2004 October 14 at 00:55:42.4 UTC |
| Equatorial Conjunction | 2004 October 14 at 02:01:31.9 UTC |
| Ecliptic Conjunction | 2004 October 14 at 02:49:19.6 UTC |
| Greatest Eclipse | 2004 October 14 at 03:00:23.0 UTC |
| Last Penumbral External Contact | 2004 October 14 at 05:05:22.2 UTC |
| Parameter | Value |
|---|---|
| Eclipse Magnitude | 0.92826 |
| Eclipse Obscuration | 0.90617 |
| Gamma | 1.03481 |
| Sun Right Ascension | 13h18m00.5s |
| Sun Declination | -08°14'10.7" |
| Sun Semi-Diameter | 16'02.2" |
| Sun Equatorial Horizontal Parallax | 08.8" |
| Moon Right Ascension | 13h19m53.4s |
| Moon Declination | -07°20'43.5" |
| Moon Semi-Diameter | 15'55.4" |
| Moon Equatorial Horizontal Parallax | 0°58'26.4" |
| ΔT | 64.6 s |
Eclipse season
editThis 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.
| October 14 Descending node (new moon) |
October 28 Ascending node (full moon) |
|---|---|
| Partial solar eclipse Solar Saros 124 |
Total lunar eclipse Lunar Saros 136 |
Related eclipses
editEclipses in 2004
edit- A partial solar eclipse on April 19.
- A total lunar eclipse on May 4.
- A partial solar eclipse on October 14.
- A total lunar eclipse on October 28.
Metonic
edit- Preceded by: Solar eclipse of December 25, 2000
- Followed by: Solar eclipse of August 1, 2008
Tzolkinex
edit- Preceded by: Solar eclipse of September 2, 1997
- Followed by: Solar eclipse of November 25, 2011
Half-Saros
edit- Preceded by: Lunar eclipse of October 8, 1995
- Followed by: Lunar eclipse of October 18, 2013
Tritos
edit- Preceded by: Solar eclipse of November 13, 1993
- Followed by: Solar eclipse of September 13, 2015
Solar Saros 124
edit- Preceded by: Solar eclipse of October 3, 1986
- Followed by: Solar eclipse of October 25, 2022
Inex
edit- Preceded by: Solar eclipse of November 3, 1975
- Followed by: Solar eclipse of September 23, 2033
Triad
edit- Preceded by: Solar eclipse of December 14, 1917
- Followed by: Solar eclipse of August 15, 2091
Solar eclipses of 2004–2007
editThis 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.[5]
| Solar eclipse series sets from 2004 to 2007 | ||||||
|---|---|---|---|---|---|---|
| Ascending node | Descending node | |||||
| Saros | Map | Gamma | Saros | Map | Gamma | |
| 119 | April 19, 2004 Partial |
−1.13345 | 124 | October 14, 2004 Partial |
1.03481 | |
| 129 Partial in Naiguatá, Venezuela |
April 8, 2005 Hybrid |
−0.34733 | 134 Annularity in Madrid, Spain |
October 3, 2005 Annular |
0.33058 | |
| 139 Totality in Side, Turkey |
March 29, 2006 Total |
0.38433 | 144 Partial in São Paulo, Brazil |
September 22, 2006 Annular |
−0.40624 | |
| 149 Partial in Jaipur, India |
March 19, 2007 Partial |
1.07277 | 154 Partial in Córdoba, Argentina |
September 11, 2007 Partial |
−1.12552 | |
Saros 124
editThis eclipse is a part of Saros series 124, repeating every 18 years, 11 days, and containing 73 events. The series started with a partial solar eclipse on March 6, 1049. It contains total eclipses from June 12, 1211 through September 22, 1968, and a hybrid eclipse on October 3, 1986. There are no annular eclipses in this set. The series ends at member 73 as a partial eclipse on May 11, 2347. 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 39 at 5 minutes, 46 seconds on May 3, 1734. All eclipses in this series occur at the Moon’s descending node of orbit.[6]
| Series members 43–64 occur between 1801 and 2200: | ||
|---|---|---|
| 43 | 44 | 45 |
June 16, 1806 |
June 26, 1824 |
July 8, 1842 |
| 46 | 47 | 48 |
July 18, 1860 |
July 29, 1878 |
August 9, 1896 |
| 49 | 50 | 51 |
August 21, 1914 |
August 31, 1932 |
September 12, 1950 |
| 52 | 53 | 54 |
September 22, 1968 |
October 3, 1986 |
October 14, 2004 |
| 55 | 56 | 57 |
October 25, 2022 |
November 4, 2040 |
November 16, 2058 |
| 58 | 59 | 60 |
November 26, 2076 |
December 7, 2094 |
December 19, 2112 |
| 61 | 62 | 63 |
December 30, 2130 |
January 9, 2149 |
January 21, 2167 |
| 64 | ||
January 31, 2185 | ||
Metonic series
editThe 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 May 21, 1993 and May 20, 2069 | ||||
|---|---|---|---|---|
| May 20–21 | March 9 | December 25–26 | October 13–14 | August 1–2 |
| 118 | 120 | 122 | 124 | 126 |
May 21, 1993 |
March 9, 1997 |
December 25, 2000 |
October 14, 2004 |
August 1, 2008 |
| 128 | 130 | 132 | 134 | 136 |
May 20, 2012 |
March 9, 2016 |
December 26, 2019 |
October 14, 2023 |
August 2, 2027 |
| 138 | 140 | 142 | 144 | 146 |
May 21, 2031 |
March 9, 2035 |
December 26, 2038 |
October 14, 2042 |
August 2, 2046 |
| 148 | 150 | 152 | 154 | 156 |
May 20, 2050 |
March 9, 2054 |
December 26, 2057 |
October 13, 2061 |
August 2, 2065 |
| 158 | ||||
May 20, 2069 | ||||
Tritos series
editThis 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 | ||||
|---|---|---|---|---|
March 25, 1819 (Saros 107) |
February 23, 1830 (Saros 108) |
January 22, 1841 (Saros 109) |
November 21, 1862 (Saros 111) | |
August 20, 1895 (Saros 114) |
July 21, 1906 (Saros 115) |
June 19, 1917 (Saros 116) | ||
May 19, 1928 (Saros 117) |
April 19, 1939 (Saros 118) |
March 18, 1950 (Saros 119) |
February 15, 1961 (Saros 120) |
January 16, 1972 (Saros 121) |
December 15, 1982 (Saros 122) |
November 13, 1993 (Saros 123) |
October 14, 2004 (Saros 124) |
September 13, 2015 (Saros 125) |
August 12, 2026 (Saros 126) |
July 13, 2037 (Saros 127) |
June 11, 2048 (Saros 128) |
May 11, 2059 (Saros 129) |
April 11, 2070 (Saros 130) |
March 10, 2081 (Saros 131) |
February 7, 2092 (Saros 132) |
January 8, 2103 (Saros 133) |
December 8, 2113 (Saros 134) |
November 6, 2124 (Saros 135) |
October 7, 2135 (Saros 136) |
September 6, 2146 (Saros 137) |
August 5, 2157 (Saros 138) |
July 5, 2168 (Saros 139) |
June 5, 2179 (Saros 140) |
May 4, 2190 (Saros 141) |
Inex series
editThis 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 | ||
|---|---|---|
March 4, 1802 (Saros 117) |
February 12, 1831 (Saros 118) |
January 23, 1860 (Saros 119) |
January 1, 1889 (Saros 120) |
December 14, 1917 (Saros 121) |
November 23, 1946 (Saros 122) |
November 3, 1975 (Saros 123) |
October 14, 2004 (Saros 124) |
September 23, 2033 (Saros 125) |
September 3, 2062 (Saros 126) |
August 15, 2091 (Saros 127) |
July 25, 2120 (Saros 128) |
July 5, 2149 (Saros 129) |
June 16, 2178 (Saros 130) |
|
References
edit- ^ "October 14, 2004 Partial Solar Eclipse". timeanddate. Retrieved 11 August 2024.
- ^ "'Almost eclipse' will be in this afternoon's sky". Pacific Daily News. 2004-10-14. p. 37. Retrieved 2023-10-25 – via Newspapers.com.
- ^ "Sky Watch". Albuquerque Journal. 2004-10-13. p. 22. Retrieved 2023-10-25 – via Newspapers.com.
- ^ "Partial Solar Eclipse of 2004 Oct 14". EclipseWise.com. Retrieved 11 August 2024.
- ^ 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 124". eclipse.gsfc.nasa.gov.
External links
editPhotos:
- Spaceweather.com eclipse gallery
- Partial Solar Eclipse on October 14, 2004[permanent dead link], Nagoya, Aichi, Japan by Toshimi Taki
- Report (0,371 max.phase) from Khabarovsk, Russia